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	<updated>2026-04-14T22:13:48Z</updated>
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	<entry>
		<id>https://globalmeteornetwork.org//wiki/index.php?title=Installing_OS_onto_a_Raspberry_Pi&amp;diff=856</id>
		<title>Installing OS onto a Raspberry Pi</title>
		<link rel="alternate" type="text/html" href="https://globalmeteornetwork.org//wiki/index.php?title=Installing_OS_onto_a_Raspberry_Pi&amp;diff=856"/>
		<updated>2025-11-03T21:38:42Z</updated>

		<summary type="html">&lt;p&gt;MeteorsABQ: /* Flash the image onto a microSD card or a USB flash drive */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt; Ahoj! In this section, you will flash (or install if you wish) an OS Linux onto your SD card or USB flash key and boot your Raspberry Pi for the first time.&lt;br /&gt;
&lt;br /&gt;
= Install the OS by flashing the image =&lt;br /&gt;
&lt;br /&gt;
== Flash the image onto a microSD card or a USB flash drive ==&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The process is the same for types of storage; only the target differs.&lt;br /&gt;
&lt;br /&gt;
1. Download the appropriate image for your Raspberry Pi model, and save it on your PC in any directory.&lt;br /&gt;
* If you have &#039;&#039;&#039;Raspberry Pi 4B&#039;&#039;&#039;, we recommend you download [https://globalmeteornetwork.org/projects/sd_card_images/RMS_RPi4Bullseye_image_20250429.img.xz this image]. &lt;br /&gt;
: This image is based on &#039;&#039;&#039;Bullseye&#039;&#039;&#039; 64-bit.&lt;br /&gt;
* If you have &#039;&#039;&#039;Raspberry Pi 5&#039;&#039;&#039;, download [https://globalmeteornetwork.org/projects/sd_card_images/RMS_RPi5Bookworm_image_20240910.img.xz this image]. &lt;br /&gt;
: This image is based on &#039;&#039;&#039;Bookworm&#039;&#039;&#039; 64-bit, and it is the only image that works with Raspberry Pi 5.&lt;br /&gt;
: Additional documentation for Bookworm RMS can be found in wiki section 2.3 &amp;quot;Advanced RMS installations and multi-camera support&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; You can use this download for Raspberry Pi 4B, but some functions may not work, such as the RTC module, and you must install &#039;&#039;&#039;AnyDesk&#039;&#039;&#039;. At this time, we see no advantage in running this image on Raspberry Pi 4B.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;For archive uses&#039;&#039;&#039;, you can download the previous 32-bit image for Raspberry Pi 4B, which is based on &#039;&#039;&#039;Buster&#039;&#039;&#039; 32-bit [https://globalmeteornetwork.org/projects/sd_card_images/RMS_RPi4_image_20230804.img.xz image]. We do not support this image, so you should use it only if you really need it and know what you are doing.&lt;br /&gt;
&lt;br /&gt;
: If you encounter problems with any of the images, contact the Technical Support group at https://globalmeteornetwork.groups.io/g/techsupport. &lt;br /&gt;
: &#039;&#039;&#039;TIP:&#039;&#039;&#039; [https://globalmeteornetwork.org/wiki/index.php?title=Images_checksums Here], you will see a list of checksums and sizes of images.&lt;br /&gt;
&lt;br /&gt;
2. Download &#039;&#039;&#039;[https://www.balena.io/etcher/ balenaEtcher]&#039;&#039;&#039;.&lt;br /&gt;
:  The process shown here uses &#039;&#039;&#039;balenaEtcher&#039;&#039;&#039; because it is the simplest tool for beginners. If you are familiar with a different USB flashing utility (such as, &#039;&#039;&#039;Rufu&#039;&#039;&#039; or &#039;&#039;&#039;Raspberry Pi Imager&#039;&#039;&#039;), feel free to use these. It these alternatives do not work for you, use &#039;&#039;&#039;balenaEtcher&#039;&#039;&#039; and the process documented here.&lt;br /&gt;
:  If you use &#039;&#039;&#039;RPi imager&#039;&#039;&#039;, select &#039;&#039;Custom&#039;&#039; for the OS, then select the image you downloaded. You also can configure the hostname, wifi details, and ssh key details with &#039;&#039;&#039;Custom Settings&#039;&#039;&#039;. &lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; DO NOT change the username and password. These are embedded in the image. &lt;br /&gt;
3. Insert a microSD card or a USB flash disk into your PC and note the letter it was assigned.&lt;br /&gt;
&lt;br /&gt;
4. Run &#039;&#039;&#039;balenaEtcher&#039;&#039;&#039;, then flash the image file onto your microSD card/USB flash drive.&lt;br /&gt;
&lt;br /&gt;
5. Select &#039;&#039;Flash from file&#039;&#039;, then find the image file and select it. &lt;br /&gt;
&lt;br /&gt;
6. Select your USB flash drive as the &#039;&#039;Target&#039;&#039;. &lt;br /&gt;
:  Even though the system disks are hidden, they usually verify the name, letter, and size of your USB flash drive to verify you chose the correct target. &lt;br /&gt;
7. Click &#039;&#039;Flash&#039;&#039; once again to verify the target and confirm it, then wait for the process to finish. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; If you see an error, you may need to run &#039;&#039;&#039;balenaEtcher&#039;&#039;&#039; as administrator.&lt;br /&gt;
8. Eject the USB flash drive in Windows, then remove microSD card/USB flash drive.&lt;br /&gt;
&lt;br /&gt;
9. Insert the microSD card/USB flash drive into your Raspberry Pi.&lt;br /&gt;
: Raspberry Pi should already be connected to a TV or monitor, a keyboard, and mouse connected. &lt;br /&gt;
: If a TV or monitor is not connected, refer to &#039;&#039;&#039;[[#Booting without a TV/Monitor|these instructions]]&#039;&#039;&#039;.&lt;br /&gt;
10. Wait for the boot. &lt;br /&gt;
: If the boot takes too long to begin, refer to the next section. If the Pi booted successfully, follow the on-screen instructions. &lt;br /&gt;
&lt;br /&gt;
: This is what the selection should look like:&lt;br /&gt;
[[File:BalenaEtcher_selection.png|center]]&lt;br /&gt;
&lt;br /&gt;
: This is what the process should look like:&lt;br /&gt;
[[File:BalenaEtcher_process.png|center]]&lt;br /&gt;
&lt;br /&gt;
== Pre-2021 Raspberry Pi 4 bootloader update - USB flash drive ONLY ==&lt;br /&gt;
&lt;br /&gt;
If you encountered a problem booting Raspberry Pi 4 from a USB device (common for all USB devices, not only flash disks), the most probable reason is that your Raspberry Pi 4 is from an older batch and you must update its bootloader. &lt;br /&gt;
&lt;br /&gt;
The procedure is simple, and you need a small capacity, blank microSD card to store about 1MB of data. The process is nicely described in &#039;&#039;&#039;[https://www.raspberrypi.com/documentation/computers/raspberry-pi.html#updating-the-bootloader the raspberry pi official documentation]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; If you are looking for an extensive USB booting guide, click &#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Booting_from_a_USB_device here]&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
The preinstalled RMS software images incorporate an auto-update feature, which updates the RMS software to the current release whenever you boot Raspberry Pi RMS. Your station always runs the most recent set of updates! &lt;br /&gt;
&lt;br /&gt;
== The first boot ==&lt;br /&gt;
&lt;br /&gt;
This is how the first boot of RMS linux looks:&lt;br /&gt;
[[File:The_first_boot_raspi.png|1500px|center]]&lt;br /&gt;
&lt;br /&gt;
Now is a good time to send an email to &#039;&#039;&#039;denis.vida@gmail.com&#039;&#039;&#039;. Include a short introduction that includes your country, then tell him you are building a camera and you need a station code. You use a station code when you set up the RMS software, after your camera is fully installed and positioned.&lt;br /&gt;
&lt;br /&gt;
= (Optional) Install the software from scratch =&lt;br /&gt;
This installation is for users who want to complete more advanced tasks. If you the procedure in the previous section, do not continue with the sections that follow.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; When you set up a Raspberry Pi, you should use the prebuilt image, which includes all necessary software installed and ready to use. If you decide to install the software on the RPi from scratch, follow the instructions on &#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Advanced_RMS_installations_and_Multi-camera_support this page]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
Next, you will focus your camera and assemble the bits and pieces for the first test. &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_-_The_complete_how-to Back to the signpost page.]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
= Boot without a TV or monitor =&lt;br /&gt;
If you do not have a TV or monitor connected to the Pi when you set it up, you must use &#039;&#039;&#039;VNC&#039;&#039;&#039;, a remote-access tool. &lt;br /&gt;
&lt;br /&gt;
1. After you burn the microSD card, insert it into the Pi and switch on the power.&lt;br /&gt;
: You should see the lights on the Pi flicker for a minute or two. If the lights do not flicker, it is possible the microSD card image did not properly burn. &lt;br /&gt;
&lt;br /&gt;
2. If the lights flicker as ecpected, wait at least three minutes after the lights stop flickering before you proceed.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; There are several stages to the initial boot, so it will take a while.&lt;br /&gt;
&lt;br /&gt;
3. While you wait, download &#039;&#039;&#039;[https://www.realvnc.com/en/connect/download/viewer/ VNC Viewer]&#039;&#039;&#039;.&lt;br /&gt;
: You do not need to create an account or subscribe, so ignore the buttons and links. After a few seconds, the download will start. &lt;br /&gt;
&lt;br /&gt;
4. To connect to the Pi using VNC, you must know either its name or its IP address.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; If you did not set the hostname when you burned the microSD card, (this is an option available in Raspberry Pi Imager), its name is probably &#039;&#039;raspberrypi&#039;&#039;. &lt;br /&gt;
: To find its IP address using the manufacturer name, run &#039;&#039;&#039;[https://www.advanced-ip-scanner.com/ Advanced IP Scanner]&#039;&#039;&#039;. This tool starts with Raspberry Pifind.&lt;br /&gt;
&lt;br /&gt;
5. Open &#039;&#039;&#039;VNC Viewer&#039;&#039;&#039; and enter the name or IP address into the box at the top.&lt;br /&gt;
: After a few seconds, you see a login dialog box. &lt;br /&gt;
&lt;br /&gt;
6. The default username is &#039;&#039;&#039;rms&#039;&#039;&#039; and the initial password is &#039;&#039;&#039;rmsraspberry&#039;&#039;&#039;. Change these credentials as soon as you log in. &lt;br /&gt;
&lt;br /&gt;
: Now, you should now see the Pi desktop and the &#039;&#039;&#039;RMS_FirstBoot&#039;&#039;&#039; window.&lt;/div&gt;</summary>
		<author><name>MeteorsABQ</name></author>
	</entry>
	<entry>
		<id>https://globalmeteornetwork.org//wiki/index.php?title=Installing_OS_onto_a_Raspberry_Pi&amp;diff=855</id>
		<title>Installing OS onto a Raspberry Pi</title>
		<link rel="alternate" type="text/html" href="https://globalmeteornetwork.org//wiki/index.php?title=Installing_OS_onto_a_Raspberry_Pi&amp;diff=855"/>
		<updated>2025-11-03T21:36:35Z</updated>

		<summary type="html">&lt;p&gt;MeteorsABQ: /* Flash the image onto a microSD card or a USB flash drive */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt; Ahoj! In this section, you will flash (or install if you wish) an OS Linux onto your SD card or USB flash key and boot your Raspberry Pi for the first time.&lt;br /&gt;
&lt;br /&gt;
= Install the OS by flashing the image =&lt;br /&gt;
&lt;br /&gt;
== Flash the image onto a microSD card or a USB flash drive ==&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The process is the same for types of storage; only the target differs.&lt;br /&gt;
&lt;br /&gt;
1. Download the appropriate image for your Raspberry Pi model, and save it on your PC in any directory.&lt;br /&gt;
* If you have &#039;&#039;&#039;Raspberry Pi 4B&#039;&#039;&#039;, we recommend you download [https://globalmeteornetwork.org/projects/sd_card_images/RMS_RPi4Bullseye_image_20250429.img.xz this image]. &lt;br /&gt;
: This image is based on &#039;&#039;&#039;Bullseye&#039;&#039;&#039; 64-bit.&lt;br /&gt;
* If you have &#039;&#039;&#039;Raspberry Pi 5&#039;&#039;&#039;, download [https://globalmeteornetwork.org/projects/sd_card_images/RMS_RPi5Bookworm_image_20240910.img.xz this image]. &lt;br /&gt;
: This image is based on &#039;&#039;&#039;Bookworm&#039;&#039;&#039; 64-bit, and it is the only image that works with Raspberry Pi 5.&lt;br /&gt;
: Additional documentation for Bookworm RMS can be found in wiki section 2.3 &amp;quot;Advanced RMS installations and multi-camera support&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; You can use this download for Raspberry Pi 4B, but some functions do not work, such as the RTC module, and you must install &#039;&#039;&#039;AnyDesk&#039;&#039;&#039;. At this time, we see no advantage in running this image on Raspberry Pi 4B.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;For archive uses&#039;&#039;&#039;, you can download the previous 32-bit image for Raspberry Pi 4B, which is based on &#039;&#039;&#039;Buster&#039;&#039;&#039; 32-bit [https://globalmeteornetwork.org/projects/sd_card_images/RMS_RPi4_image_20230804.img.xz image]. We do not support this image, so you should use it only if you really need it and know what you are doing.&lt;br /&gt;
&lt;br /&gt;
: If you encounter problems with any of the images, contact the Technical Support group at https://globalmeteornetwork.groups.io/g/techsupport. &lt;br /&gt;
: &#039;&#039;&#039;TIP:&#039;&#039;&#039; [https://globalmeteornetwork.org/wiki/index.php?title=Images_checksums Here], you will see a list of checksums and sizes of images.&lt;br /&gt;
&lt;br /&gt;
2. Download &#039;&#039;&#039;[https://www.balena.io/etcher/ balenaEtcher]&#039;&#039;&#039;.&lt;br /&gt;
:  The process shown here uses &#039;&#039;&#039;balenaEtcher&#039;&#039;&#039; because it is the simplest tool for beginners. If you are familiar with a different USB flashing utility (such as, &#039;&#039;&#039;Rufu&#039;&#039;&#039; or &#039;&#039;&#039;Raspberry Pi Imager&#039;&#039;&#039;), feel free to use these. It these alternatives do not work for you, use &#039;&#039;&#039;balenaEtcher&#039;&#039;&#039; and the process documented here.&lt;br /&gt;
:  If you use &#039;&#039;&#039;RPi imager&#039;&#039;&#039;, select &#039;&#039;Custom&#039;&#039; for the OS, then select the image you downloaded. You also can configure the hostname, wifi details, and ssh key details with &#039;&#039;&#039;Custom Settings&#039;&#039;&#039;. &lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; DO NOT change the username and password. These are embedded in the image. &lt;br /&gt;
3. Insert a microSD card or a USB flash disk into your PC and note the letter it was assigned.&lt;br /&gt;
&lt;br /&gt;
4. Run &#039;&#039;&#039;balenaEtcher&#039;&#039;&#039;, then flash the image file onto your microSD card/USB flash drive.&lt;br /&gt;
&lt;br /&gt;
5. Select &#039;&#039;Flash from file&#039;&#039;, then find the image file and select it. &lt;br /&gt;
&lt;br /&gt;
6. Select your USB flash drive as the &#039;&#039;Target&#039;&#039;. &lt;br /&gt;
:  Even though the system disks are hidden, they usually verify the name, letter, and size of your USB flash drive to verify you chose the correct target. &lt;br /&gt;
7. Click &#039;&#039;Flash&#039;&#039; once again to verify the target and confirm it, then wait for the process to finish. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; If you see an error, you may need to run &#039;&#039;&#039;balenaEtcher&#039;&#039;&#039; as administrator.&lt;br /&gt;
8. Eject the USB flash drive in Windows, then remove microSD card/USB flash drive.&lt;br /&gt;
&lt;br /&gt;
9. Insert the microSD card/USB flash drive into your Raspberry Pi.&lt;br /&gt;
: Raspberry Pi should already be connected to a TV or monitor, a keyboard, and mouse connected. &lt;br /&gt;
: If a TV or monitor is not connected, refer to &#039;&#039;&#039;[[#Booting without a TV/Monitor|these instructions]]&#039;&#039;&#039;.&lt;br /&gt;
10. Wait for the boot. &lt;br /&gt;
: If the boot takes too long to begin, refer to the next section. If the Pi booted successfully, follow the on-screen instructions. &lt;br /&gt;
&lt;br /&gt;
: This is what the selection should look like:&lt;br /&gt;
[[File:BalenaEtcher_selection.png|center]]&lt;br /&gt;
&lt;br /&gt;
: This is what the process should look like:&lt;br /&gt;
[[File:BalenaEtcher_process.png|center]]&lt;br /&gt;
&lt;br /&gt;
== Pre-2021 Raspberry Pi 4 bootloader update - USB flash drive ONLY ==&lt;br /&gt;
&lt;br /&gt;
If you encountered a problem booting Raspberry Pi 4 from a USB device (common for all USB devices, not only flash disks), the most probable reason is that your Raspberry Pi 4 is from an older batch and you must update its bootloader. &lt;br /&gt;
&lt;br /&gt;
The procedure is simple, and you need a small capacity, blank microSD card to store about 1MB of data. The process is nicely described in &#039;&#039;&#039;[https://www.raspberrypi.com/documentation/computers/raspberry-pi.html#updating-the-bootloader the raspberry pi official documentation]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; If you are looking for an extensive USB booting guide, click &#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Booting_from_a_USB_device here]&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
The preinstalled RMS software images incorporate an auto-update feature, which updates the RMS software to the current release whenever you boot Raspberry Pi RMS. Your station always runs the most recent set of updates! &lt;br /&gt;
&lt;br /&gt;
== The first boot ==&lt;br /&gt;
&lt;br /&gt;
This is how the first boot of RMS linux looks:&lt;br /&gt;
[[File:The_first_boot_raspi.png|1500px|center]]&lt;br /&gt;
&lt;br /&gt;
Now is a good time to send an email to &#039;&#039;&#039;denis.vida@gmail.com&#039;&#039;&#039;. Include a short introduction that includes your country, then tell him you are building a camera and you need a station code. You use a station code when you set up the RMS software, after your camera is fully installed and positioned.&lt;br /&gt;
&lt;br /&gt;
= (Optional) Install the software from scratch =&lt;br /&gt;
This installation is for users who want to complete more advanced tasks. If you the procedure in the previous section, do not continue with the sections that follow.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; When you set up a Raspberry Pi, you should use the prebuilt image, which includes all necessary software installed and ready to use. If you decide to install the software on the RPi from scratch, follow the instructions on &#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Advanced_RMS_installations_and_Multi-camera_support this page]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
Next, you will focus your camera and assemble the bits and pieces for the first test. &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_-_The_complete_how-to Back to the signpost page.]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
= Boot without a TV or monitor =&lt;br /&gt;
If you do not have a TV or monitor connected to the Pi when you set it up, you must use &#039;&#039;&#039;VNC&#039;&#039;&#039;, a remote-access tool. &lt;br /&gt;
&lt;br /&gt;
1. After you burn the microSD card, insert it into the Pi and switch on the power.&lt;br /&gt;
: You should see the lights on the Pi flicker for a minute or two. If the lights do not flicker, it is possible the microSD card image did not properly burn. &lt;br /&gt;
&lt;br /&gt;
2. If the lights flicker as ecpected, wait at least three minutes after the lights stop flickering before you proceed.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; There are several stages to the initial boot, so it will take a while.&lt;br /&gt;
&lt;br /&gt;
3. While you wait, download &#039;&#039;&#039;[https://www.realvnc.com/en/connect/download/viewer/ VNC Viewer]&#039;&#039;&#039;.&lt;br /&gt;
: You do not need to create an account or subscribe, so ignore the buttons and links. After a few seconds, the download will start. &lt;br /&gt;
&lt;br /&gt;
4. To connect to the Pi using VNC, you must know either its name or its IP address.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; If you did not set the hostname when you burned the microSD card, (this is an option available in Raspberry Pi Imager), its name is probably &#039;&#039;raspberrypi&#039;&#039;. &lt;br /&gt;
: To find its IP address using the manufacturer name, run &#039;&#039;&#039;[https://www.advanced-ip-scanner.com/ Advanced IP Scanner]&#039;&#039;&#039;. This tool starts with Raspberry Pifind.&lt;br /&gt;
&lt;br /&gt;
5. Open &#039;&#039;&#039;VNC Viewer&#039;&#039;&#039; and enter the name or IP address into the box at the top.&lt;br /&gt;
: After a few seconds, you see a login dialog box. &lt;br /&gt;
&lt;br /&gt;
6. The default username is &#039;&#039;&#039;rms&#039;&#039;&#039; and the initial password is &#039;&#039;&#039;rmsraspberry&#039;&#039;&#039;. Change these credentials as soon as you log in. &lt;br /&gt;
&lt;br /&gt;
: Now, you should now see the Pi desktop and the &#039;&#039;&#039;RMS_FirstBoot&#039;&#039;&#039; window.&lt;/div&gt;</summary>
		<author><name>MeteorsABQ</name></author>
	</entry>
	<entry>
		<id>https://globalmeteornetwork.org//wiki/index.php?title=Main_Page&amp;diff=854</id>
		<title>Main Page</title>
		<link rel="alternate" type="text/html" href="https://globalmeteornetwork.org//wiki/index.php?title=Main_Page&amp;diff=854"/>
		<updated>2025-11-03T21:20:17Z</updated>

		<summary type="html">&lt;p&gt;MeteorsABQ: /* Advanced RMS installations and multi-camera support */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Welcome to the Global Meteor Network wiki page!&lt;br /&gt;
&lt;br /&gt;
The Global Meteor Network (GMN) is a world-wide organization of amateur and professional astronomers. The goal is to observe the night sky using low-light video cameras and produce meteor trajectories in a coordinated network of recording stations. Here, you can find information about the purpose and structure of the GMN, and how to assemble and operate your own meteor camera. You also will discover how to contribute to the development of RMS (the GMN software) and how your observations as a citizen scientist contribute to the ongoing understanding of our solar system&#039;s formation and evolution. &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;If you are here to find out how to build and set up a camera from scratch, jump ahead to [https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_-_The_complete_how-to this] section!&amp;lt;/span&amp;gt;&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;For German speakers, there is &amp;quot;Build camera from scratch&amp;quot; documentation written by students of [https://fsg-preetz.de/ Friedrich-Schiller-Gymnasium in Preetz] available [http://wiki.linux-astronomie.de/doku.php?id=ceres here]. This version is maintained by Friedrich-Schiller-Gymnasium in Preetz. &amp;lt;/span&amp;gt;&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Global Meteor Network overview ==&lt;br /&gt;
&lt;br /&gt;
===  [https://globalmeteornetwork.org/?page_id=141 Our mission] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=363 A brief history of the Global Meteor Network] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://www.youtube.com/watch?v=MAGq-XqD5Po Video introduction - Overview of the Global Meteor Network (IMC2020)] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://youtu.be/oM7lfQ4nmyw Video overview - Meteor tracking and the GMN from Astro Imaging Channel presentation] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/data/ Some &#039;live&#039; GMN data products] ===&lt;br /&gt;
&lt;br /&gt;
== Meteor detection station ==&lt;br /&gt;
&lt;br /&gt;
What is an RMS GMN station? An RMS-based GMN station consists of a Raspberry Pi (RPi) single board computer, a low light level security video camera, the RMS software, and a connection to the Internet via Wifi. The camera is securely mounted in a weatherproof housing, pointed at the sky, and connected to the RPi with a Power Over Ethernet (POE) cable. To be a part of the GMN network, you need a fairly powerful Raspberry Pi (Pi 4, 5, or better) and a reasonably fast Internet connection. The internet connection is required only for data upload to a central server each morning and to provide automatic updates for the RMS software. &lt;br /&gt;
&lt;br /&gt;
Nightly, the RPi records video from the camera shortly after local sunset, then continuously compressing and storing the video data on a local SSD drive. Each morning before sunrise, when capture is complete, the RPi analyzes the video and extracts  meteor observations from the previous night. These extracted video clips of detected meteors are archived and then uploaded to a server. On a &#039;busy&#039; night, the clips can total hundreds of megabytes as a result of a heavy meteor shower or a night with a lot of false detections. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Continuous progress is being made on the detection software to filter out false detections. &lt;br /&gt;
&lt;br /&gt;
The server finds meteors that were observed from more than one station, which allows the server to triangulate meteor trails in 3D and calculate the orbits of the meteors.&lt;br /&gt;
&lt;br /&gt;
=== What do I need? ===&lt;br /&gt;
&lt;br /&gt;
You need a Raspberry Pi compluter, RMS software, and a camera kit. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; We strongly recommend the Pi 4 or 5 model. &lt;br /&gt;
The software can run on a Pi3, but it is much slower and it is no longer supported. A list with everything you need is available here: [https://globalmeteornetwork.org/wiki/index.php?title=Shopping_list_and_tools_needed page].&lt;br /&gt;
&lt;br /&gt;
You can run multiple cameras on a Linux PC, and details are available &#039;&#039;&#039;[https://docs.google.com/document/d/16PSFi8RAqbenPdluhulCRaIenOkEzgs5piUhkX3yaOc/edit here]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== How do I obtain a camera? ===&lt;br /&gt;
There are two options - buy a camera or build a camera.&lt;br /&gt;
&lt;br /&gt;
==== Buy a Camera ====&lt;br /&gt;
You can buy a camera and prebuilt Pi, and ready to install. Cameras are available from several suppliers, as well as the Croatian Meteor Network, as explained here: [https://globalmeteornetwork.org/?page_id=136 this page]. &lt;br /&gt;
If you are in the UK, you can contact the UK Meteor network for advice. [https://ukmeteornetwork.org/ UK Meteor Network].&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; As of 2024, UK Meteor network can no longer sell cameras directly.&lt;br /&gt;
&lt;br /&gt;
==== Build your own from scratch ====&lt;br /&gt;
This option requires an intermediate level of DIY skills and familiarity with the Raspberry Pi, but do not be put off. The instructions are comprehensive and, if you get stuck, you can ask for advice in the forum here: &#039;&#039;&#039;[https://groups.io/g/globalmeteornetwork groups.io]&#039;&#039;&#039; forum.&lt;br /&gt;
&lt;br /&gt;
You can find out more about this option here: &#039;&#039;&#039;[[Build &amp;amp; Install &amp;amp; Setup your camera - The complete how-to]]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== Advanced RMS installations and multi-camera support ===&lt;br /&gt;
If you would like to explore advanced RMS installation options for various platforms or run multiple cameras on a single Linux computer, complete information is available on &#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Advanced_RMS_installations_and_Multi-camera_support this page]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
If you plan to run RMS software on the Raspberry Pi 4 or 5, the best supported and easiest solution is our prepared image. Complete information is available in an &#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_-_The_complete_how-to extensive guide]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
If you want to run single or multiple cameras on the Raspberry Pi 5, please see the Bookworm RMS MultiCamPi documentation in this &#039;&#039;&#039;[https://drive.google.com/file/d/1XOsnDGLC1tGNRsZ4Ojy7axPP9hulgUJt/view?usp=sharing pdf file]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== Can I use a commercial all-sky camera? ===&lt;br /&gt;
&lt;br /&gt;
Generally, this is not a good idea because these cameras lack sufficient sensitivity. More information is available here: &#039;&#039;&#039;[https://globalmeteornetwork.org/?p=163 See this recent experiment]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Operate and maintain your GMN station ==&lt;br /&gt;
&lt;br /&gt;
=== Overview ===&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; GMS is a nascent operation, so you may share some of our growing pains if you choose to be involved. We are constantly solving bugs and making improvements, which is an opportunity for you to help if you have programming skills! The workload of day-to-day operation can be non-zero, and may require some of your time.&lt;br /&gt;
&lt;br /&gt;
Ideally, you should monitor your RMS Pi systems daily to identify freezes, glitches, or other problems. For example, you may see birds nesting or soiling the camera window, someone may unintentionally unplug the power cord, or animals (mice, cats, or dogs) may chew on the camera Ethernet cable. Although we make constant progress, the GMS network is not yet a &#039;power up and forget about it&#039; system. &lt;br /&gt;
&lt;br /&gt;
By its nature, the GMS network is staffed by lots of people who are willing to help newcomers get started. Here are some suggestions for daily operation of your RMS camera.&lt;br /&gt;
&lt;br /&gt;
=== What does the meteor camera do over the course of 24 hours? ===&lt;br /&gt;
&lt;br /&gt;
The RMS python-based system calculates the sundown to sunrise interval, and schedules video camera capture all night. Based on the video camera and capabilities of the Pi, the camera captures at least 25 frames per second between evening and morning twilight. During each nightly continuous image capture, the station processes captured image data and idenitfies frames that contain a minimum number of stars (usually around 20) that are worth reviewing for meteor detections. When data capture is complete, the station begins processing all frames it flagged with possible detections, then refines the astrometric accuracy of every positive detection. Using the station plate parameters (platepar) calibration file, processing iterates to find the best astrometry and photometry solution for each detected meteor. After this process analyzes each detection, summary files are created. &lt;br /&gt;
&lt;br /&gt;
The summary files include many types of information.&lt;br /&gt;
* Text file data presentation in several widely accepted formats (such as &#039;&#039;CAMS&#039;&#039; and &#039;&#039;UFOorbit&#039;&#039;).&lt;br /&gt;
* Graphic plots of detection frequencies throughout the night.&lt;br /&gt;
* Plot of all detections, showing any identified radiants.&lt;br /&gt;
* Plots of photometry, astrometry, and camera pointing drift in arc minutes throughout the course of the night as the mount or building flexes.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039;  Detailed information about plots is available here: &#039;&#039;&#039;[https://docs.google.com/document/d/132aHGn0QPzhpVN2s2n6FT6rJn39LAsPkchWJqXQb8Qk/edit?usp=sharing Explanation of GMN plots]&#039;&#039;&#039;&lt;br /&gt;
* Thumbnail images of detections.&lt;br /&gt;
* Thumbnail images of data captured throughout the night.&lt;br /&gt;
* Single image with all detections stacked together.&lt;br /&gt;
* Single image with all captured images stacked together.&lt;br /&gt;
* Flat file for correcting images.&lt;br /&gt;
* An &#039;&#039;.mp4&#039;&#039; movie time lapse of the night&#039;s captured images.&lt;br /&gt;
* Meteor shower flux charts, if specific showers are detected.&lt;br /&gt;
* Observation summary data of hardware and data recording characteristics.&lt;br /&gt;
 &lt;br /&gt;
When you click a meteor track, its data displays in the lower data window. Ultimately, all results are combined into a single compressed archive that automatically uploads each morning to the central server. &lt;br /&gt;
&lt;br /&gt;
Each morning, you can review the result files on the RPi and copy anything you want to your computer or tablet.&lt;br /&gt;
&lt;br /&gt;
===Archive data ===&lt;br /&gt;
&lt;br /&gt;
Your primary scientific data is automatically uploaded to the central server every morning after data processing is complete. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; When the night&#039;s results are uploaded, RMS purges the oldest data to free up space for the next night&#039;s run. As a result, you may want to copy some of the data to a PC, NAS, or the cloud for further analysis.&lt;br /&gt;
:       You should consider backing up the content of &#039;&#039;&#039;~/RMS_data/ArchivedFiles&#039;&#039;&#039;, which holds individual files and data that RMS determined were probably meteors. &lt;br /&gt;
&lt;br /&gt;
Details about backing up data is beyond the scope of the GMN Wiki. Tools such as Robocopy for Windows and rsync for Linux/MacOS are ideal, and they can &#039;mirror&#039; data across a network. Help to configure these tools is available in the &#039;&#039;&#039;Globalmeteornetwork&#039;&#039;&#039; group on &#039;&#039;&#039;groups.io&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
In addition, we added some automated tools that can help you back up data to a thumb drive inserted into the RPi. Assistance about these tools also is available in the &#039;&#039;&#039;Globalmeteornetwork&#039;&#039;&#039; group on &#039;&#039;&#039;groups.io&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
===Backup and restore the configuration and RSA keys===&lt;br /&gt;
&lt;br /&gt;
:&#039;&#039;&#039;NOTE:&#039;&#039;&#039; If you are on an older Buster image, you must replace username &#039;&#039;rms&#039;&#039; with username &#039;&#039;pi&#039;&#039;. For example, enter &#039;&#039;/home/pi&#039;&#039; instead of &#039;&#039;/home/rms&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
To determine which username to use, run &lt;br /&gt;
::&#039;&#039;ls /home/rms home/pi&#039;&#039;&lt;br /&gt;
to display the username that is your home directory.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Back up the configuration&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
1. Open a terminal and run the command  &#039;&#039;Scripts/RMS_Backup.sh&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
: A compressed &#039;&#039;.zip&#039;&#039; file, with all important configuration files and keys, is created in your user home directory with the prefix &#039;&#039;RMS_Backup&#039;&#039; and the &#039;&#039;.zip&#039;&#039; extension. &lt;br /&gt;
: For example, &#039;&#039;/home/rms/RMS_Backup_XX0001_2023-01-28.zip&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
2. Copy the &#039;&#039;.zip&#039;&#039; file to a safe place outside RPi. &lt;br /&gt;
&lt;br /&gt;
: Later, it will be useful to restore the system in case of failure. The &#039;&#039;.zip&#039;&#039; file contains the RSA public and private keys used to contact GMN servers, so keep it secret.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Restore the configuration&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
1. Unzip the backup file in any folder on the RPi.&lt;br /&gt;
&lt;br /&gt;
2. Copy the files &#039;&#039;.config&#039;&#039;, &#039;&#039;platepar_cmn2010.cal&#039;&#039;, and &#039;&#039;mask.bmp&#039;&#039; to the folder &#039;&#039;/home/rms/source/RMS/&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
3. Copy the files &#039;&#039;id_rsa&#039;&#039; and &#039;&#039;id_rsa.pub&#039;&#039; to the folder &#039;&#039;/home/rms/.ssh/&#039;&#039;, as shown in this example:&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;cp .config platepar_cmn2010.cal mask.bmp /home/rms/source/RMS/&#039;&#039;&lt;br /&gt;
: &#039;&#039;cp id_rsa id_rsa.pub /home/rms/.ssh/&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
4. To make sure that permission bits in the RSA key files are correct, enter:&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;chmod 400 ~/.ssh/id_rsa*&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== View the data ===&lt;br /&gt;
&lt;br /&gt;
To view data, you can use &#039;&#039;&#039;CMN_binViewer&#039;&#039;&#039; software [https://github.com/CroatianMeteorNetwork/cmn_binviewer], which is included in the RMS SD image. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; There also is a Windows version [https://github.com/CroatianMeteorNetwork/cmn_binviewer/releases] you can install.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; You can open images in astronomical FITS viewers, such as &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039; or &#039;&#039;&#039;Pixinsight&#039;&#039;&#039;, but what you see may be surprising. For example, in &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039;, the image is upside down, which is an artefact of how the software reads the image. &lt;br /&gt;
&lt;br /&gt;
In space, there is no &#039;up&#039; or &#039;down&#039;, so the FITS specification does not dictate if pixel (0,0) is at a specific corner. Some software, notably &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039;, specifies the top left corner as the origin location, which causes terrestrial images  to display vertically mirrored.&lt;br /&gt;
&lt;br /&gt;
=== Tools and utilities ===&lt;br /&gt;
&lt;br /&gt;
There are many tools available.&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;&#039;[https://www.realvnc.com/en/connect/download/viewer/ RealVNC]&#039;&#039;&#039;, &#039;&#039;&#039;[https://www.nomachine.com/ NoMachine]&#039;&#039;&#039;, &#039;&#039;&#039;[https://anydesk.com/en AnyDesk]&#039;&#039;&#039;, or &#039;&#039;&#039;[https://rustdesk.com/ RustDesk]&#039;&#039;&#039; remote connect tools provide station access from anywhere. Access to your station from outside your network is enabled by an OpenVPN connection address that is available to meteor stations.&lt;br /&gt;
: With &#039;&#039;&#039;VNC&#039;&#039;&#039; and &#039;&#039;&#039;Teamviewer&#039;&#039;&#039;, you can create an account and team on their websites, and then remotely access your station. &lt;br /&gt;
* &#039;&#039;&#039;Samba&#039;&#039;&#039; data directory access allows you to copy data results directly from your RPi to your computer or tablet.&lt;br /&gt;
* &#039;&#039;&#039;[https://github.com/CroatianMeteorNetwork/cmn_binviewer CMN_binViewer]&#039;&#039;&#039; allows you to view standard FITS image files that contain meteor detections. It runs on the RPi, and it can run under Windows.&lt;br /&gt;
* &#039;&#039;&#039;[https://sonotaco.com/soft/e_index.html UFO Orbit]&#039;&#039;&#039; allows you to process data from multiple stations, and generate unified radiants of two or more stations that see the same meteor. &#039;&#039;&#039;[https://sonotaco.com/soft/e_index.html UFO Orbit]&#039;&#039;&#039; can plot the shared object ground path and orbital characteristics, and it can output a summary file of all objects seen by more than one station.&lt;br /&gt;
* RMS software can be installed under Windows to allow much of the RMS python-based code to run on your computer. This means you can run RMS against meteor station data that was transferred to your computer from the RPi.&lt;br /&gt;
&lt;br /&gt;
You also can run RMS python jobs on the RPi to sample captured image files, and then condense them into an &#039;&#039;.mp4&#039;&#039; video. Sometimes, these videos are mesmerizing summaries that can run for more than two minutes of winter time data.&lt;br /&gt;
&lt;br /&gt;
== What can I do with my GMN station? ==&lt;br /&gt;
&lt;br /&gt;
=== Use SkyFit2 for astrometric and photometric calibration + Manually reduce observations of fireballs and compute their trajectories ===&lt;br /&gt;
* &#039;&#039;&#039;[https://www.youtube.com/watch?v=ao3J9Jf0iLQ Updated 2023 video tutorial]&#039;&#039;&#039;&lt;br /&gt;
* &#039;&#039;&#039;[https://www.youtube.com/watch?v=MOjb3qxDlX4 Old 2021 video tutorial]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/fov3d/ Generate a Google Earth KML file to show your station&#039;s field of view] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=253 Use the UFO Orbit program to estimate meteor trajectories] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=221 Urban meteor observing] ===&lt;br /&gt;
&lt;br /&gt;
== Data analysis with SkyFit2 ==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SkyFit2&#039;&#039;&#039;, a program in the RMS library, allows you to analyze optical meteor data in most of the optical formats in current use. The program supports popular video formats (&#039;&#039;.mp4&#039;&#039;, &#039;&#039;.avi&#039;&#039;, and &#039;&#039;.mkv&#039;&#039;), sequences of static images, and single images with shutter breaks.&lt;br /&gt;
&lt;br /&gt;
A &#039;&#039;&#039;[https://www.youtube.com/watch?v=ao3J9Jf0iLQ video tutorial]&#039;&#039;&#039; explains how to useg &#039;&#039;&#039;SkyFit2&#039;&#039;&#039; to run astrometric and photometric calibrations on GMN data, and it can manually reduce observations of fireballs and compute their trajectories.&lt;br /&gt;
&lt;br /&gt;
A more detailed description of &#039;&#039;&#039;SkyFit2&#039;&#039;&#039; is available on the &#039;&#039;&#039;[[SkyFit2|SkyFit2]]&#039;&#039;&#039; page.&lt;br /&gt;
&lt;br /&gt;
== FAQ ==&lt;br /&gt;
&lt;br /&gt;
=== What should I back up when I re-flash an SD card or a USB disk? ===&lt;br /&gt;
&lt;br /&gt;
You should backup the &#039;&#039;.config&#039;&#039;, platepar, and mask files that are in the RMS source directory, plus the entire content of the hidden directory &#039;&#039;/home/pi/.ssh&#039;&#039;. Refer to the section titled, &#039;&#039;&#039;Back up the configuration&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
If your SD card or USB disk fails or becomes corrupted, you can fetch the config files from the server because they are uploaded every day, together with the data.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The content of &#039;&#039;.ssh&#039;&#039; is essential for connection to the server, so you also must save these files. &lt;br /&gt;
&lt;br /&gt;
After you set up a new SD card or USB disk, return the files to their original location.&lt;br /&gt;
&lt;br /&gt;
=== What are the values in the &#039;&#039;FTPdetectinfo_*&#039;&#039;  file designated as hnr mle bin Pix/fm Rho Phi? ===&lt;br /&gt;
&lt;br /&gt;
Some of these values (hnr mle bin) are not used in RMS but they are used in CAMS, so their presence is to conform to the standard. As a result, these values are all zeros. &lt;br /&gt;
&lt;br /&gt;
There are other values:&lt;br /&gt;
* Pix/fm is the average angular speed of the meteor, in pixels, per frame.&lt;br /&gt;
* Rho, Phi are parameters that define the line of the meteor in polar coordinates, see this &#039;&#039;&#039;[https://en.wikipedia.org/wiki/Hough_transform#Theory page]&#039;&#039;&#039; for more detail. &lt;br /&gt;
: &#039;&#039;Rho&#039;&#039; is the distance of the line from the center of the image.&lt;br /&gt;
: &#039;&#039;Phi&#039;&#039; is the angle of the line, as measured from the positive direction of the Y axis. (Basically, this is a line from the center of the image to the top of the image.) The positive angles are measured clockwise, although the CAMS standard may define these parameters a bit differently, with the Y axis flipped.&lt;br /&gt;
The &#039;&#039;intensity&#039;&#039; is the sum of all pixel intensities of the meteor on a given frame. &lt;br /&gt;
&lt;br /&gt;
For example, you could represent an area around the meteor on a given frame, as shown in the figure, where the numbers are pixel intensities on an 8-bit image (so they can range from 0 to 255) and the pixel values inside the red boundary represent the meteor blob on the frame. The result? The intensity is the sum of all numbers inside the red boundary. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Later, this value is used to compute the magnitude.&lt;br /&gt;
&lt;br /&gt;
[[File:Intensity_sum.png |Intensity_sum.png ]]&lt;br /&gt;
&lt;br /&gt;
The magnitude is computed as&lt;br /&gt;
: &#039;&#039;mag = -2.5*log10(intensity sum) + photometric_offset&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
To estimate the photometric offset in &#039;&#039;&#039;SkyFit&#039;&#039;&#039;, fit the line with slope -2.5 through pairs of known magnitudes of stars and logartihms of their pixel intensity sum. Fundamentally, the photometric offset is the intercept of that line. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The constant slope of -2.5 comes from the &#039;&#039;&#039;[https://en.wikipedia.org/wiki/Apparent_magnitude#Calculations Definition of stellar magnitudes]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== GMN data policy ==&lt;br /&gt;
&lt;br /&gt;
The Global Meteor Network produces three levels of data products.&lt;br /&gt;
* Level 1 - The lowest level data (as close to &#039;raw&#039; as possible) are the FF image and FR video files saved to the RPi by the capture code and the fireball detector.&lt;br /&gt;
* Level 2 - Data is used in three ways:&lt;br /&gt;
:* The meteor detector extracts positional and brightness information of individual meteors (&#039;&#039;FTPdetectinfo&#039;&#039; file). &lt;br /&gt;
:* Images are used for astrometric and photometric calibration (platepar file). &lt;br /&gt;
:* Meteor and star detections are used to generate a range of plots, such as the single-station shower association graph and the camera drift graph. The calibrated meteor measurements are uploaded to the GMN server, together with the raw images of individual meteors.&lt;br /&gt;
* Level 3 - Software on the server correlates individual observations and computes multi-station meteor trajectories, which are published daily on the &#039;&#039;&#039;GMN [https://globalmeteornetwork.org/data/ Data website]&#039;&#039;&#039;. This data is made public under the &#039;&#039;&#039;[https://creativecommons.org/licenses/by/4.0/ CC BY 4.0 license]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
Operators of individual GMN stations exclusively own the Level 1 and Level 2 data their stations produce. In practice, this means they are free to share this data with other meteor networks if they wish. The data that is uploaded to the GMN server is not shared publicly or with other parties without the operator&#039;s consent. However, the data may be used internally by the GMN coordinators to manually produce other data products, such as the trajectory of a meteorite dropping fireball or an analysis of a meteor shower. &lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; All station operators are credited for their data in all GMN publications.&lt;br /&gt;
&lt;br /&gt;
== GMN Plots and Images Explained ==&lt;br /&gt;
&lt;br /&gt;
This document explains the data summaries produced on your system and displayed on the GMN Weblog every morning &#039;&#039;&#039;[https://docs.google.com/document/d/132aHGn0QPzhpVN2s2n6FT6rJn39LAsPkchWJqXQb8Qk/edit?pli=1&amp;amp;tab=t.0 GMN Plots and Images]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;[https://IstraStream.com IstraStream.com]&#039;&#039;&#039; was an independent hosting site primarily intended for cameras sold by IstraStream. In mid-2023, Istrastream stopped listing camera image output and the IstraStream data display was replaced with the &#039;&#039;&#039;[https://globalmeteornetwork.org/weblog/ GMN weblog]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== For more information ==&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?page_id=43 Contact the Global Meteor Network] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://groups.io/g/globalmeteornetwork Join the Global Meteor Network Forum] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://github.com/markmac99/ukmon-pitools/wiki UK Meteor Network Wiki]===&lt;br /&gt;
This wiki has numerous FAQs and tips on maintaining, monitoring and managing your system, and several explainers such as how to calibrate and create a mask, how to copy data and so forth. &lt;br /&gt;
&lt;br /&gt;
=== Important GMN resources ===&lt;br /&gt;
&lt;br /&gt;
There are two additional web pages you should know about.&lt;br /&gt;
&lt;br /&gt;
* The &#039;&#039;&#039;[https://globalmeteornetwork.org/status GMN status page]&#039;&#039;&#039; provides access to the &#039;&#039;&#039;[https://globalmeteornetwork.org/weblog/ GMN weblog]&#039;&#039;&#039;.&lt;br /&gt;
* A mapping utility website that is directly derived from GMN data: &#039;&#039;&#039;[https://tammojan.github.io/meteormap Meteor map]&#039;&#039;&#039;.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; This map takes quite a while to load. When you review the map, you must scroll down to see the full power of the data display.&lt;br /&gt;
&lt;br /&gt;
=== GMN talks ===&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=_tV7WBo0RrQ 2025 GMN Meeting Session 1 (February 2025)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=z23aJeIg7wo 2025 GMN Meeting Session 2 (February 2025)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/playlist?list=PLmQ5Bvz4ACYJLYfswIeAipapoeGeI6QWy GMN talk for Society for Astronomical Sciences workshop 2024 (The first 3 videos)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=juOvRTtoqhs 2024 GMN Meeting Session 1 (February 2024)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=MXhVIxrz2ks 2024 GMN Meeting Session 2 (February 2024)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=IfUyCHjMATc 2023 GMN Meeting Session 1 (February 2023)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=I78KwF5-1GE 2023 GMN Meeting Session 2 (February 2023)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=wDdrG_FCyGk 2022 GMN Meeting Session 1 (February 2022)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=j_75CDPzjI4 2022 GMN Meeting Session 2 (February 2022)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=f6x9_WCVphY GMN talk at the European Space Agency&#039;s Fireball Workshop (June 2021)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=QXBTLPnPDWs 2021 GMN Meeting] - [https://www.dropbox.com/sh/ia9vagug5lxm8k9/AAB_i_1jcWThUdAHO_2gF_Ksa?dl=0 Link to slides]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=MAGq-XqD5Po Overview of the GMN - IMC2020 (September 2020)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=oM7lfQ4nmyw Overview of the GMN, Astro Imaging Channel presentation (May 2020)]&lt;br /&gt;
&lt;br /&gt;
=== GMN-related publications ===&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2206.11365 Vida, D., Blaauw Erskine, R. C., Brown, P. G., Kambulow, J., Campbell-Brown, M., &amp;amp; Mazur, M. J. (2022). Computing optical meteor flux using global meteor network data. Monthly Notices of the Royal Astronomical Society, 515(2), 2322-2339.]&lt;br /&gt;
&lt;br /&gt;
: [https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stab2557/6368869 Moorhead, A. V., Clements, T., &amp;amp; Vida, D. (2021). Meteor shower radiant dispersions in Global Meteor Network data. Monthly Notices of the Royal Astronomical Society, 508(1), 326-339.]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2107.12335 Vida, D., Šegon, D., Gural, P. S., Brown, P. G., McIntyre, M. J., Dijkema, T. J., Pavletić, L., Kukić, P., Mazur, M.J., Eschman, P., Roggemans, P., Merlak, A., &amp;amp; Zubović, D. (2021). The Global Meteor Network–Methodology and first results. Monthly Notices of the Royal Astronomical Society, 506(4), 5046-5074.]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2003.05458/ Moorhead, A. V., Clements, T. D., &amp;amp; Vida, D. (2020). Realistic gravitational focusing of meteoroid streams. Monthly Notices of the Royal Astronomical Society, 494(2), 2982-2994.] &lt;br /&gt;
&lt;br /&gt;
: [https://globalmeteornetwork.org/wordpress/wp-content/uploads/2018/11/Kukic-et-al-2018-Rolling-shutter.pdf  Kukić, P., Gural, P., Vida, D., Šegon, D. &amp;amp; Merlak, A. (2018) Correction for meteor centroids observed using rolling shutter cameras. WGN, Journal of the International Meteor Organization, 46:5, 154-118.]&lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/2018_WGN___RMS_sun_skirter_final.pdf  Vida, D., Mazur, M. J., Šegon, D., Kukić, P., &amp;amp; Merlak, A. (2018). Compressive strength of a skirting Daytime Arietid-first science results from low-cost Raspberry Pi-based meteor stations. WGN, Journal of the International Meteor Organization, 46, 113-118.] &lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/pdf/1911.02979.pdf Vida, D., Gural, P., Brown, P., Campbell-Brown, M., Wiegert, P. (2019) Estimating trajectories of meteors: an observational Monte Carlo approach - I. Theory. arXiv:1911.02979v4 [astro-ph.EP] 21 Apr 2020]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/pdf/1911.11734.pdf Vida, D., Gural, P., Brown, P., Campbell-Brown, M., Wiegert, P. (2019) Estimating trajectories of meteors: an observational Monte Carlo approach - II. Results. arXiv:1911.11734v1 [astro-ph.EP] 26 Novr 2019]&lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/2018_WGN___RMS_first_results-final.pdf Vida, D., Mazur, M. J., Šegon, D., Zubović, D., Kukić, P., Parag, F., &amp;amp; Macan, A. (2018). First results of a Raspberry Pi based meteor camera system. WGN, Journal of the International Meteor Organization, 46, 71-78.] &lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/Vida_IMC2016_proceedings_final.pdf Vida, D., Zubović, D., Šegon, D., Gural, P., &amp;amp; Cupec, R. (2016). Open-source meteor detection software for low-cost single-board computers. In Proceedings of the International Meteor Conference (IMC2016), Egmond, The Netherlands (pp. 2-5).] &lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/Zubovic_IMC2015_priceedings_final.pdf Zubović, D., Vida, D., Gural, P., &amp;amp; Šegon, D. (2015). Advances in the development of a low-cost video meteor station. In Proceedings of the International Meteor Conference, Mistelbach, Austria (pp. 27-30).]&lt;/div&gt;</summary>
		<author><name>MeteorsABQ</name></author>
	</entry>
	<entry>
		<id>https://globalmeteornetwork.org//wiki/index.php?title=Main_Page&amp;diff=853</id>
		<title>Main Page</title>
		<link rel="alternate" type="text/html" href="https://globalmeteornetwork.org//wiki/index.php?title=Main_Page&amp;diff=853"/>
		<updated>2025-11-03T21:19:26Z</updated>

		<summary type="html">&lt;p&gt;MeteorsABQ: /* Advanced RMS installations and multi-camera support */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Welcome to the Global Meteor Network wiki page!&lt;br /&gt;
&lt;br /&gt;
The Global Meteor Network (GMN) is a world-wide organization of amateur and professional astronomers. The goal is to observe the night sky using low-light video cameras and produce meteor trajectories in a coordinated network of recording stations. Here, you can find information about the purpose and structure of the GMN, and how to assemble and operate your own meteor camera. You also will discover how to contribute to the development of RMS (the GMN software) and how your observations as a citizen scientist contribute to the ongoing understanding of our solar system&#039;s formation and evolution. &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;If you are here to find out how to build and set up a camera from scratch, jump ahead to [https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_-_The_complete_how-to this] section!&amp;lt;/span&amp;gt;&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;For German speakers, there is &amp;quot;Build camera from scratch&amp;quot; documentation written by students of [https://fsg-preetz.de/ Friedrich-Schiller-Gymnasium in Preetz] available [http://wiki.linux-astronomie.de/doku.php?id=ceres here]. This version is maintained by Friedrich-Schiller-Gymnasium in Preetz. &amp;lt;/span&amp;gt;&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Global Meteor Network overview ==&lt;br /&gt;
&lt;br /&gt;
===  [https://globalmeteornetwork.org/?page_id=141 Our mission] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=363 A brief history of the Global Meteor Network] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://www.youtube.com/watch?v=MAGq-XqD5Po Video introduction - Overview of the Global Meteor Network (IMC2020)] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://youtu.be/oM7lfQ4nmyw Video overview - Meteor tracking and the GMN from Astro Imaging Channel presentation] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/data/ Some &#039;live&#039; GMN data products] ===&lt;br /&gt;
&lt;br /&gt;
== Meteor detection station ==&lt;br /&gt;
&lt;br /&gt;
What is an RMS GMN station? An RMS-based GMN station consists of a Raspberry Pi (RPi) single board computer, a low light level security video camera, the RMS software, and a connection to the Internet via Wifi. The camera is securely mounted in a weatherproof housing, pointed at the sky, and connected to the RPi with a Power Over Ethernet (POE) cable. To be a part of the GMN network, you need a fairly powerful Raspberry Pi (Pi 4, 5, or better) and a reasonably fast Internet connection. The internet connection is required only for data upload to a central server each morning and to provide automatic updates for the RMS software. &lt;br /&gt;
&lt;br /&gt;
Nightly, the RPi records video from the camera shortly after local sunset, then continuously compressing and storing the video data on a local SSD drive. Each morning before sunrise, when capture is complete, the RPi analyzes the video and extracts  meteor observations from the previous night. These extracted video clips of detected meteors are archived and then uploaded to a server. On a &#039;busy&#039; night, the clips can total hundreds of megabytes as a result of a heavy meteor shower or a night with a lot of false detections. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Continuous progress is being made on the detection software to filter out false detections. &lt;br /&gt;
&lt;br /&gt;
The server finds meteors that were observed from more than one station, which allows the server to triangulate meteor trails in 3D and calculate the orbits of the meteors.&lt;br /&gt;
&lt;br /&gt;
=== What do I need? ===&lt;br /&gt;
&lt;br /&gt;
You need a Raspberry Pi compluter, RMS software, and a camera kit. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; We strongly recommend the Pi 4 or 5 model. &lt;br /&gt;
The software can run on a Pi3, but it is much slower and it is no longer supported. A list with everything you need is available here: [https://globalmeteornetwork.org/wiki/index.php?title=Shopping_list_and_tools_needed page].&lt;br /&gt;
&lt;br /&gt;
You can run multiple cameras on a Linux PC, and details are available &#039;&#039;&#039;[https://docs.google.com/document/d/16PSFi8RAqbenPdluhulCRaIenOkEzgs5piUhkX3yaOc/edit here]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== How do I obtain a camera? ===&lt;br /&gt;
There are two options - buy a camera or build a camera.&lt;br /&gt;
&lt;br /&gt;
==== Buy a Camera ====&lt;br /&gt;
You can buy a camera and prebuilt Pi, and ready to install. Cameras are available from several suppliers, as well as the Croatian Meteor Network, as explained here: [https://globalmeteornetwork.org/?page_id=136 this page]. &lt;br /&gt;
If you are in the UK, you can contact the UK Meteor network for advice. [https://ukmeteornetwork.org/ UK Meteor Network].&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; As of 2024, UK Meteor network can no longer sell cameras directly.&lt;br /&gt;
&lt;br /&gt;
==== Build your own from scratch ====&lt;br /&gt;
This option requires an intermediate level of DIY skills and familiarity with the Raspberry Pi, but do not be put off. The instructions are comprehensive and, if you get stuck, you can ask for advice in the forum here: &#039;&#039;&#039;[https://groups.io/g/globalmeteornetwork groups.io]&#039;&#039;&#039; forum.&lt;br /&gt;
&lt;br /&gt;
You can find out more about this option here: &#039;&#039;&#039;[[Build &amp;amp; Install &amp;amp; Setup your camera - The complete how-to]]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== Advanced RMS installations and multi-camera support ===&lt;br /&gt;
If you would like to explore advanced RMS installation options for various platforms or run multiple cameras on a single Linux computer, complete information is available on &#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Advanced_RMS_installations_and_Multi-camera_support this page]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
If you plan to run RMS software on the Raspberry Pi 4 or 5, the best supported and easiest solution is our prepared image. Complete information is available in an &#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_-_The_complete_how-to extensive guide]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
If you want to run single or multiple cameras on the Raspberry Pi 5, please see the MultiCamPi documentation in this &#039;&#039;&#039;[https://drive.google.com/file/d/1XOsnDGLC1tGNRsZ4Ojy7axPP9hulgUJt/view?usp=sharing pdf file]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== Can I use a commercial all-sky camera? ===&lt;br /&gt;
&lt;br /&gt;
Generally, this is not a good idea because these cameras lack sufficient sensitivity. More information is available here: &#039;&#039;&#039;[https://globalmeteornetwork.org/?p=163 See this recent experiment]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Operate and maintain your GMN station ==&lt;br /&gt;
&lt;br /&gt;
=== Overview ===&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; GMS is a nascent operation, so you may share some of our growing pains if you choose to be involved. We are constantly solving bugs and making improvements, which is an opportunity for you to help if you have programming skills! The workload of day-to-day operation can be non-zero, and may require some of your time.&lt;br /&gt;
&lt;br /&gt;
Ideally, you should monitor your RMS Pi systems daily to identify freezes, glitches, or other problems. For example, you may see birds nesting or soiling the camera window, someone may unintentionally unplug the power cord, or animals (mice, cats, or dogs) may chew on the camera Ethernet cable. Although we make constant progress, the GMS network is not yet a &#039;power up and forget about it&#039; system. &lt;br /&gt;
&lt;br /&gt;
By its nature, the GMS network is staffed by lots of people who are willing to help newcomers get started. Here are some suggestions for daily operation of your RMS camera.&lt;br /&gt;
&lt;br /&gt;
=== What does the meteor camera do over the course of 24 hours? ===&lt;br /&gt;
&lt;br /&gt;
The RMS python-based system calculates the sundown to sunrise interval, and schedules video camera capture all night. Based on the video camera and capabilities of the Pi, the camera captures at least 25 frames per second between evening and morning twilight. During each nightly continuous image capture, the station processes captured image data and idenitfies frames that contain a minimum number of stars (usually around 20) that are worth reviewing for meteor detections. When data capture is complete, the station begins processing all frames it flagged with possible detections, then refines the astrometric accuracy of every positive detection. Using the station plate parameters (platepar) calibration file, processing iterates to find the best astrometry and photometry solution for each detected meteor. After this process analyzes each detection, summary files are created. &lt;br /&gt;
&lt;br /&gt;
The summary files include many types of information.&lt;br /&gt;
* Text file data presentation in several widely accepted formats (such as &#039;&#039;CAMS&#039;&#039; and &#039;&#039;UFOorbit&#039;&#039;).&lt;br /&gt;
* Graphic plots of detection frequencies throughout the night.&lt;br /&gt;
* Plot of all detections, showing any identified radiants.&lt;br /&gt;
* Plots of photometry, astrometry, and camera pointing drift in arc minutes throughout the course of the night as the mount or building flexes.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039;  Detailed information about plots is available here: &#039;&#039;&#039;[https://docs.google.com/document/d/132aHGn0QPzhpVN2s2n6FT6rJn39LAsPkchWJqXQb8Qk/edit?usp=sharing Explanation of GMN plots]&#039;&#039;&#039;&lt;br /&gt;
* Thumbnail images of detections.&lt;br /&gt;
* Thumbnail images of data captured throughout the night.&lt;br /&gt;
* Single image with all detections stacked together.&lt;br /&gt;
* Single image with all captured images stacked together.&lt;br /&gt;
* Flat file for correcting images.&lt;br /&gt;
* An &#039;&#039;.mp4&#039;&#039; movie time lapse of the night&#039;s captured images.&lt;br /&gt;
* Meteor shower flux charts, if specific showers are detected.&lt;br /&gt;
* Observation summary data of hardware and data recording characteristics.&lt;br /&gt;
 &lt;br /&gt;
When you click a meteor track, its data displays in the lower data window. Ultimately, all results are combined into a single compressed archive that automatically uploads each morning to the central server. &lt;br /&gt;
&lt;br /&gt;
Each morning, you can review the result files on the RPi and copy anything you want to your computer or tablet.&lt;br /&gt;
&lt;br /&gt;
===Archive data ===&lt;br /&gt;
&lt;br /&gt;
Your primary scientific data is automatically uploaded to the central server every morning after data processing is complete. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; When the night&#039;s results are uploaded, RMS purges the oldest data to free up space for the next night&#039;s run. As a result, you may want to copy some of the data to a PC, NAS, or the cloud for further analysis.&lt;br /&gt;
:       You should consider backing up the content of &#039;&#039;&#039;~/RMS_data/ArchivedFiles&#039;&#039;&#039;, which holds individual files and data that RMS determined were probably meteors. &lt;br /&gt;
&lt;br /&gt;
Details about backing up data is beyond the scope of the GMN Wiki. Tools such as Robocopy for Windows and rsync for Linux/MacOS are ideal, and they can &#039;mirror&#039; data across a network. Help to configure these tools is available in the &#039;&#039;&#039;Globalmeteornetwork&#039;&#039;&#039; group on &#039;&#039;&#039;groups.io&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
In addition, we added some automated tools that can help you back up data to a thumb drive inserted into the RPi. Assistance about these tools also is available in the &#039;&#039;&#039;Globalmeteornetwork&#039;&#039;&#039; group on &#039;&#039;&#039;groups.io&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
===Backup and restore the configuration and RSA keys===&lt;br /&gt;
&lt;br /&gt;
:&#039;&#039;&#039;NOTE:&#039;&#039;&#039; If you are on an older Buster image, you must replace username &#039;&#039;rms&#039;&#039; with username &#039;&#039;pi&#039;&#039;. For example, enter &#039;&#039;/home/pi&#039;&#039; instead of &#039;&#039;/home/rms&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
To determine which username to use, run &lt;br /&gt;
::&#039;&#039;ls /home/rms home/pi&#039;&#039;&lt;br /&gt;
to display the username that is your home directory.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Back up the configuration&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
1. Open a terminal and run the command  &#039;&#039;Scripts/RMS_Backup.sh&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
: A compressed &#039;&#039;.zip&#039;&#039; file, with all important configuration files and keys, is created in your user home directory with the prefix &#039;&#039;RMS_Backup&#039;&#039; and the &#039;&#039;.zip&#039;&#039; extension. &lt;br /&gt;
: For example, &#039;&#039;/home/rms/RMS_Backup_XX0001_2023-01-28.zip&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
2. Copy the &#039;&#039;.zip&#039;&#039; file to a safe place outside RPi. &lt;br /&gt;
&lt;br /&gt;
: Later, it will be useful to restore the system in case of failure. The &#039;&#039;.zip&#039;&#039; file contains the RSA public and private keys used to contact GMN servers, so keep it secret.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Restore the configuration&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
1. Unzip the backup file in any folder on the RPi.&lt;br /&gt;
&lt;br /&gt;
2. Copy the files &#039;&#039;.config&#039;&#039;, &#039;&#039;platepar_cmn2010.cal&#039;&#039;, and &#039;&#039;mask.bmp&#039;&#039; to the folder &#039;&#039;/home/rms/source/RMS/&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
3. Copy the files &#039;&#039;id_rsa&#039;&#039; and &#039;&#039;id_rsa.pub&#039;&#039; to the folder &#039;&#039;/home/rms/.ssh/&#039;&#039;, as shown in this example:&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;cp .config platepar_cmn2010.cal mask.bmp /home/rms/source/RMS/&#039;&#039;&lt;br /&gt;
: &#039;&#039;cp id_rsa id_rsa.pub /home/rms/.ssh/&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
4. To make sure that permission bits in the RSA key files are correct, enter:&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;chmod 400 ~/.ssh/id_rsa*&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== View the data ===&lt;br /&gt;
&lt;br /&gt;
To view data, you can use &#039;&#039;&#039;CMN_binViewer&#039;&#039;&#039; software [https://github.com/CroatianMeteorNetwork/cmn_binviewer], which is included in the RMS SD image. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; There also is a Windows version [https://github.com/CroatianMeteorNetwork/cmn_binviewer/releases] you can install.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; You can open images in astronomical FITS viewers, such as &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039; or &#039;&#039;&#039;Pixinsight&#039;&#039;&#039;, but what you see may be surprising. For example, in &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039;, the image is upside down, which is an artefact of how the software reads the image. &lt;br /&gt;
&lt;br /&gt;
In space, there is no &#039;up&#039; or &#039;down&#039;, so the FITS specification does not dictate if pixel (0,0) is at a specific corner. Some software, notably &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039;, specifies the top left corner as the origin location, which causes terrestrial images  to display vertically mirrored.&lt;br /&gt;
&lt;br /&gt;
=== Tools and utilities ===&lt;br /&gt;
&lt;br /&gt;
There are many tools available.&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;&#039;[https://www.realvnc.com/en/connect/download/viewer/ RealVNC]&#039;&#039;&#039;, &#039;&#039;&#039;[https://www.nomachine.com/ NoMachine]&#039;&#039;&#039;, &#039;&#039;&#039;[https://anydesk.com/en AnyDesk]&#039;&#039;&#039;, or &#039;&#039;&#039;[https://rustdesk.com/ RustDesk]&#039;&#039;&#039; remote connect tools provide station access from anywhere. Access to your station from outside your network is enabled by an OpenVPN connection address that is available to meteor stations.&lt;br /&gt;
: With &#039;&#039;&#039;VNC&#039;&#039;&#039; and &#039;&#039;&#039;Teamviewer&#039;&#039;&#039;, you can create an account and team on their websites, and then remotely access your station. &lt;br /&gt;
* &#039;&#039;&#039;Samba&#039;&#039;&#039; data directory access allows you to copy data results directly from your RPi to your computer or tablet.&lt;br /&gt;
* &#039;&#039;&#039;[https://github.com/CroatianMeteorNetwork/cmn_binviewer CMN_binViewer]&#039;&#039;&#039; allows you to view standard FITS image files that contain meteor detections. It runs on the RPi, and it can run under Windows.&lt;br /&gt;
* &#039;&#039;&#039;[https://sonotaco.com/soft/e_index.html UFO Orbit]&#039;&#039;&#039; allows you to process data from multiple stations, and generate unified radiants of two or more stations that see the same meteor. &#039;&#039;&#039;[https://sonotaco.com/soft/e_index.html UFO Orbit]&#039;&#039;&#039; can plot the shared object ground path and orbital characteristics, and it can output a summary file of all objects seen by more than one station.&lt;br /&gt;
* RMS software can be installed under Windows to allow much of the RMS python-based code to run on your computer. This means you can run RMS against meteor station data that was transferred to your computer from the RPi.&lt;br /&gt;
&lt;br /&gt;
You also can run RMS python jobs on the RPi to sample captured image files, and then condense them into an &#039;&#039;.mp4&#039;&#039; video. Sometimes, these videos are mesmerizing summaries that can run for more than two minutes of winter time data.&lt;br /&gt;
&lt;br /&gt;
== What can I do with my GMN station? ==&lt;br /&gt;
&lt;br /&gt;
=== Use SkyFit2 for astrometric and photometric calibration + Manually reduce observations of fireballs and compute their trajectories ===&lt;br /&gt;
* &#039;&#039;&#039;[https://www.youtube.com/watch?v=ao3J9Jf0iLQ Updated 2023 video tutorial]&#039;&#039;&#039;&lt;br /&gt;
* &#039;&#039;&#039;[https://www.youtube.com/watch?v=MOjb3qxDlX4 Old 2021 video tutorial]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/fov3d/ Generate a Google Earth KML file to show your station&#039;s field of view] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=253 Use the UFO Orbit program to estimate meteor trajectories] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=221 Urban meteor observing] ===&lt;br /&gt;
&lt;br /&gt;
== Data analysis with SkyFit2 ==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SkyFit2&#039;&#039;&#039;, a program in the RMS library, allows you to analyze optical meteor data in most of the optical formats in current use. The program supports popular video formats (&#039;&#039;.mp4&#039;&#039;, &#039;&#039;.avi&#039;&#039;, and &#039;&#039;.mkv&#039;&#039;), sequences of static images, and single images with shutter breaks.&lt;br /&gt;
&lt;br /&gt;
A &#039;&#039;&#039;[https://www.youtube.com/watch?v=ao3J9Jf0iLQ video tutorial]&#039;&#039;&#039; explains how to useg &#039;&#039;&#039;SkyFit2&#039;&#039;&#039; to run astrometric and photometric calibrations on GMN data, and it can manually reduce observations of fireballs and compute their trajectories.&lt;br /&gt;
&lt;br /&gt;
A more detailed description of &#039;&#039;&#039;SkyFit2&#039;&#039;&#039; is available on the &#039;&#039;&#039;[[SkyFit2|SkyFit2]]&#039;&#039;&#039; page.&lt;br /&gt;
&lt;br /&gt;
== FAQ ==&lt;br /&gt;
&lt;br /&gt;
=== What should I back up when I re-flash an SD card or a USB disk? ===&lt;br /&gt;
&lt;br /&gt;
You should backup the &#039;&#039;.config&#039;&#039;, platepar, and mask files that are in the RMS source directory, plus the entire content of the hidden directory &#039;&#039;/home/pi/.ssh&#039;&#039;. Refer to the section titled, &#039;&#039;&#039;Back up the configuration&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
If your SD card or USB disk fails or becomes corrupted, you can fetch the config files from the server because they are uploaded every day, together with the data.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The content of &#039;&#039;.ssh&#039;&#039; is essential for connection to the server, so you also must save these files. &lt;br /&gt;
&lt;br /&gt;
After you set up a new SD card or USB disk, return the files to their original location.&lt;br /&gt;
&lt;br /&gt;
=== What are the values in the &#039;&#039;FTPdetectinfo_*&#039;&#039;  file designated as hnr mle bin Pix/fm Rho Phi? ===&lt;br /&gt;
&lt;br /&gt;
Some of these values (hnr mle bin) are not used in RMS but they are used in CAMS, so their presence is to conform to the standard. As a result, these values are all zeros. &lt;br /&gt;
&lt;br /&gt;
There are other values:&lt;br /&gt;
* Pix/fm is the average angular speed of the meteor, in pixels, per frame.&lt;br /&gt;
* Rho, Phi are parameters that define the line of the meteor in polar coordinates, see this &#039;&#039;&#039;[https://en.wikipedia.org/wiki/Hough_transform#Theory page]&#039;&#039;&#039; for more detail. &lt;br /&gt;
: &#039;&#039;Rho&#039;&#039; is the distance of the line from the center of the image.&lt;br /&gt;
: &#039;&#039;Phi&#039;&#039; is the angle of the line, as measured from the positive direction of the Y axis. (Basically, this is a line from the center of the image to the top of the image.) The positive angles are measured clockwise, although the CAMS standard may define these parameters a bit differently, with the Y axis flipped.&lt;br /&gt;
The &#039;&#039;intensity&#039;&#039; is the sum of all pixel intensities of the meteor on a given frame. &lt;br /&gt;
&lt;br /&gt;
For example, you could represent an area around the meteor on a given frame, as shown in the figure, where the numbers are pixel intensities on an 8-bit image (so they can range from 0 to 255) and the pixel values inside the red boundary represent the meteor blob on the frame. The result? The intensity is the sum of all numbers inside the red boundary. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Later, this value is used to compute the magnitude.&lt;br /&gt;
&lt;br /&gt;
[[File:Intensity_sum.png |Intensity_sum.png ]]&lt;br /&gt;
&lt;br /&gt;
The magnitude is computed as&lt;br /&gt;
: &#039;&#039;mag = -2.5*log10(intensity sum) + photometric_offset&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
To estimate the photometric offset in &#039;&#039;&#039;SkyFit&#039;&#039;&#039;, fit the line with slope -2.5 through pairs of known magnitudes of stars and logartihms of their pixel intensity sum. Fundamentally, the photometric offset is the intercept of that line. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The constant slope of -2.5 comes from the &#039;&#039;&#039;[https://en.wikipedia.org/wiki/Apparent_magnitude#Calculations Definition of stellar magnitudes]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== GMN data policy ==&lt;br /&gt;
&lt;br /&gt;
The Global Meteor Network produces three levels of data products.&lt;br /&gt;
* Level 1 - The lowest level data (as close to &#039;raw&#039; as possible) are the FF image and FR video files saved to the RPi by the capture code and the fireball detector.&lt;br /&gt;
* Level 2 - Data is used in three ways:&lt;br /&gt;
:* The meteor detector extracts positional and brightness information of individual meteors (&#039;&#039;FTPdetectinfo&#039;&#039; file). &lt;br /&gt;
:* Images are used for astrometric and photometric calibration (platepar file). &lt;br /&gt;
:* Meteor and star detections are used to generate a range of plots, such as the single-station shower association graph and the camera drift graph. The calibrated meteor measurements are uploaded to the GMN server, together with the raw images of individual meteors.&lt;br /&gt;
* Level 3 - Software on the server correlates individual observations and computes multi-station meteor trajectories, which are published daily on the &#039;&#039;&#039;GMN [https://globalmeteornetwork.org/data/ Data website]&#039;&#039;&#039;. This data is made public under the &#039;&#039;&#039;[https://creativecommons.org/licenses/by/4.0/ CC BY 4.0 license]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
Operators of individual GMN stations exclusively own the Level 1 and Level 2 data their stations produce. In practice, this means they are free to share this data with other meteor networks if they wish. The data that is uploaded to the GMN server is not shared publicly or with other parties without the operator&#039;s consent. However, the data may be used internally by the GMN coordinators to manually produce other data products, such as the trajectory of a meteorite dropping fireball or an analysis of a meteor shower. &lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; All station operators are credited for their data in all GMN publications.&lt;br /&gt;
&lt;br /&gt;
== GMN Plots and Images Explained ==&lt;br /&gt;
&lt;br /&gt;
This document explains the data summaries produced on your system and displayed on the GMN Weblog every morning &#039;&#039;&#039;[https://docs.google.com/document/d/132aHGn0QPzhpVN2s2n6FT6rJn39LAsPkchWJqXQb8Qk/edit?pli=1&amp;amp;tab=t.0 GMN Plots and Images]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;[https://IstraStream.com IstraStream.com]&#039;&#039;&#039; was an independent hosting site primarily intended for cameras sold by IstraStream. In mid-2023, Istrastream stopped listing camera image output and the IstraStream data display was replaced with the &#039;&#039;&#039;[https://globalmeteornetwork.org/weblog/ GMN weblog]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== For more information ==&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?page_id=43 Contact the Global Meteor Network] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://groups.io/g/globalmeteornetwork Join the Global Meteor Network Forum] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://github.com/markmac99/ukmon-pitools/wiki UK Meteor Network Wiki]===&lt;br /&gt;
This wiki has numerous FAQs and tips on maintaining, monitoring and managing your system, and several explainers such as how to calibrate and create a mask, how to copy data and so forth. &lt;br /&gt;
&lt;br /&gt;
=== Important GMN resources ===&lt;br /&gt;
&lt;br /&gt;
There are two additional web pages you should know about.&lt;br /&gt;
&lt;br /&gt;
* The &#039;&#039;&#039;[https://globalmeteornetwork.org/status GMN status page]&#039;&#039;&#039; provides access to the &#039;&#039;&#039;[https://globalmeteornetwork.org/weblog/ GMN weblog]&#039;&#039;&#039;.&lt;br /&gt;
* A mapping utility website that is directly derived from GMN data: &#039;&#039;&#039;[https://tammojan.github.io/meteormap Meteor map]&#039;&#039;&#039;.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; This map takes quite a while to load. When you review the map, you must scroll down to see the full power of the data display.&lt;br /&gt;
&lt;br /&gt;
=== GMN talks ===&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=_tV7WBo0RrQ 2025 GMN Meeting Session 1 (February 2025)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=z23aJeIg7wo 2025 GMN Meeting Session 2 (February 2025)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/playlist?list=PLmQ5Bvz4ACYJLYfswIeAipapoeGeI6QWy GMN talk for Society for Astronomical Sciences workshop 2024 (The first 3 videos)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=juOvRTtoqhs 2024 GMN Meeting Session 1 (February 2024)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=MXhVIxrz2ks 2024 GMN Meeting Session 2 (February 2024)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=IfUyCHjMATc 2023 GMN Meeting Session 1 (February 2023)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=I78KwF5-1GE 2023 GMN Meeting Session 2 (February 2023)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=wDdrG_FCyGk 2022 GMN Meeting Session 1 (February 2022)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=j_75CDPzjI4 2022 GMN Meeting Session 2 (February 2022)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=f6x9_WCVphY GMN talk at the European Space Agency&#039;s Fireball Workshop (June 2021)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=QXBTLPnPDWs 2021 GMN Meeting] - [https://www.dropbox.com/sh/ia9vagug5lxm8k9/AAB_i_1jcWThUdAHO_2gF_Ksa?dl=0 Link to slides]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=MAGq-XqD5Po Overview of the GMN - IMC2020 (September 2020)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=oM7lfQ4nmyw Overview of the GMN, Astro Imaging Channel presentation (May 2020)]&lt;br /&gt;
&lt;br /&gt;
=== GMN-related publications ===&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2206.11365 Vida, D., Blaauw Erskine, R. C., Brown, P. G., Kambulow, J., Campbell-Brown, M., &amp;amp; Mazur, M. J. (2022). Computing optical meteor flux using global meteor network data. Monthly Notices of the Royal Astronomical Society, 515(2), 2322-2339.]&lt;br /&gt;
&lt;br /&gt;
: [https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stab2557/6368869 Moorhead, A. V., Clements, T., &amp;amp; Vida, D. (2021). Meteor shower radiant dispersions in Global Meteor Network data. Monthly Notices of the Royal Astronomical Society, 508(1), 326-339.]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2107.12335 Vida, D., Šegon, D., Gural, P. S., Brown, P. G., McIntyre, M. J., Dijkema, T. J., Pavletić, L., Kukić, P., Mazur, M.J., Eschman, P., Roggemans, P., Merlak, A., &amp;amp; Zubović, D. (2021). The Global Meteor Network–Methodology and first results. Monthly Notices of the Royal Astronomical Society, 506(4), 5046-5074.]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2003.05458/ Moorhead, A. V., Clements, T. D., &amp;amp; Vida, D. (2020). Realistic gravitational focusing of meteoroid streams. Monthly Notices of the Royal Astronomical Society, 494(2), 2982-2994.] &lt;br /&gt;
&lt;br /&gt;
: [https://globalmeteornetwork.org/wordpress/wp-content/uploads/2018/11/Kukic-et-al-2018-Rolling-shutter.pdf  Kukić, P., Gural, P., Vida, D., Šegon, D. &amp;amp; Merlak, A. (2018) Correction for meteor centroids observed using rolling shutter cameras. WGN, Journal of the International Meteor Organization, 46:5, 154-118.]&lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/2018_WGN___RMS_sun_skirter_final.pdf  Vida, D., Mazur, M. J., Šegon, D., Kukić, P., &amp;amp; Merlak, A. (2018). Compressive strength of a skirting Daytime Arietid-first science results from low-cost Raspberry Pi-based meteor stations. WGN, Journal of the International Meteor Organization, 46, 113-118.] &lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/pdf/1911.02979.pdf Vida, D., Gural, P., Brown, P., Campbell-Brown, M., Wiegert, P. (2019) Estimating trajectories of meteors: an observational Monte Carlo approach - I. Theory. arXiv:1911.02979v4 [astro-ph.EP] 21 Apr 2020]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/pdf/1911.11734.pdf Vida, D., Gural, P., Brown, P., Campbell-Brown, M., Wiegert, P. (2019) Estimating trajectories of meteors: an observational Monte Carlo approach - II. Results. arXiv:1911.11734v1 [astro-ph.EP] 26 Novr 2019]&lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/2018_WGN___RMS_first_results-final.pdf Vida, D., Mazur, M. J., Šegon, D., Zubović, D., Kukić, P., Parag, F., &amp;amp; Macan, A. (2018). First results of a Raspberry Pi based meteor camera system. WGN, Journal of the International Meteor Organization, 46, 71-78.] &lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/Vida_IMC2016_proceedings_final.pdf Vida, D., Zubović, D., Šegon, D., Gural, P., &amp;amp; Cupec, R. (2016). Open-source meteor detection software for low-cost single-board computers. In Proceedings of the International Meteor Conference (IMC2016), Egmond, The Netherlands (pp. 2-5).] &lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/Zubovic_IMC2015_priceedings_final.pdf Zubović, D., Vida, D., Gural, P., &amp;amp; Šegon, D. (2015). Advances in the development of a low-cost video meteor station. In Proceedings of the International Meteor Conference, Mistelbach, Austria (pp. 27-30).]&lt;/div&gt;</summary>
		<author><name>MeteorsABQ</name></author>
	</entry>
	<entry>
		<id>https://globalmeteornetwork.org//wiki/index.php?title=Main_Page&amp;diff=852</id>
		<title>Main Page</title>
		<link rel="alternate" type="text/html" href="https://globalmeteornetwork.org//wiki/index.php?title=Main_Page&amp;diff=852"/>
		<updated>2025-11-03T21:18:14Z</updated>

		<summary type="html">&lt;p&gt;MeteorsABQ: /* Advanced RMS installations and multi-camera support */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Welcome to the Global Meteor Network wiki page!&lt;br /&gt;
&lt;br /&gt;
The Global Meteor Network (GMN) is a world-wide organization of amateur and professional astronomers. The goal is to observe the night sky using low-light video cameras and produce meteor trajectories in a coordinated network of recording stations. Here, you can find information about the purpose and structure of the GMN, and how to assemble and operate your own meteor camera. You also will discover how to contribute to the development of RMS (the GMN software) and how your observations as a citizen scientist contribute to the ongoing understanding of our solar system&#039;s formation and evolution. &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;If you are here to find out how to build and set up a camera from scratch, jump ahead to [https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_-_The_complete_how-to this] section!&amp;lt;/span&amp;gt;&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;For German speakers, there is &amp;quot;Build camera from scratch&amp;quot; documentation written by students of [https://fsg-preetz.de/ Friedrich-Schiller-Gymnasium in Preetz] available [http://wiki.linux-astronomie.de/doku.php?id=ceres here]. This version is maintained by Friedrich-Schiller-Gymnasium in Preetz. &amp;lt;/span&amp;gt;&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Global Meteor Network overview ==&lt;br /&gt;
&lt;br /&gt;
===  [https://globalmeteornetwork.org/?page_id=141 Our mission] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=363 A brief history of the Global Meteor Network] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://www.youtube.com/watch?v=MAGq-XqD5Po Video introduction - Overview of the Global Meteor Network (IMC2020)] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://youtu.be/oM7lfQ4nmyw Video overview - Meteor tracking and the GMN from Astro Imaging Channel presentation] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/data/ Some &#039;live&#039; GMN data products] ===&lt;br /&gt;
&lt;br /&gt;
== Meteor detection station ==&lt;br /&gt;
&lt;br /&gt;
What is an RMS GMN station? An RMS-based GMN station consists of a Raspberry Pi (RPi) single board computer, a low light level security video camera, the RMS software, and a connection to the Internet via Wifi. The camera is securely mounted in a weatherproof housing, pointed at the sky, and connected to the RPi with a Power Over Ethernet (POE) cable. To be a part of the GMN network, you need a fairly powerful Raspberry Pi (Pi 4, 5, or better) and a reasonably fast Internet connection. The internet connection is required only for data upload to a central server each morning and to provide automatic updates for the RMS software. &lt;br /&gt;
&lt;br /&gt;
Nightly, the RPi records video from the camera shortly after local sunset, then continuously compressing and storing the video data on a local SSD drive. Each morning before sunrise, when capture is complete, the RPi analyzes the video and extracts  meteor observations from the previous night. These extracted video clips of detected meteors are archived and then uploaded to a server. On a &#039;busy&#039; night, the clips can total hundreds of megabytes as a result of a heavy meteor shower or a night with a lot of false detections. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Continuous progress is being made on the detection software to filter out false detections. &lt;br /&gt;
&lt;br /&gt;
The server finds meteors that were observed from more than one station, which allows the server to triangulate meteor trails in 3D and calculate the orbits of the meteors.&lt;br /&gt;
&lt;br /&gt;
=== What do I need? ===&lt;br /&gt;
&lt;br /&gt;
You need a Raspberry Pi compluter, RMS software, and a camera kit. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; We strongly recommend the Pi 4 or 5 model. &lt;br /&gt;
The software can run on a Pi3, but it is much slower and it is no longer supported. A list with everything you need is available here: [https://globalmeteornetwork.org/wiki/index.php?title=Shopping_list_and_tools_needed page].&lt;br /&gt;
&lt;br /&gt;
You can run multiple cameras on a Linux PC, and details are available &#039;&#039;&#039;[https://docs.google.com/document/d/16PSFi8RAqbenPdluhulCRaIenOkEzgs5piUhkX3yaOc/edit here]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== How do I obtain a camera? ===&lt;br /&gt;
There are two options - buy a camera or build a camera.&lt;br /&gt;
&lt;br /&gt;
==== Buy a Camera ====&lt;br /&gt;
You can buy a camera and prebuilt Pi, and ready to install. Cameras are available from several suppliers, as well as the Croatian Meteor Network, as explained here: [https://globalmeteornetwork.org/?page_id=136 this page]. &lt;br /&gt;
If you are in the UK, you can contact the UK Meteor network for advice. [https://ukmeteornetwork.org/ UK Meteor Network].&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; As of 2024, UK Meteor network can no longer sell cameras directly.&lt;br /&gt;
&lt;br /&gt;
==== Build your own from scratch ====&lt;br /&gt;
This option requires an intermediate level of DIY skills and familiarity with the Raspberry Pi, but do not be put off. The instructions are comprehensive and, if you get stuck, you can ask for advice in the forum here: &#039;&#039;&#039;[https://groups.io/g/globalmeteornetwork groups.io]&#039;&#039;&#039; forum.&lt;br /&gt;
&lt;br /&gt;
You can find out more about this option here: &#039;&#039;&#039;[[Build &amp;amp; Install &amp;amp; Setup your camera - The complete how-to]]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== Advanced RMS installations and multi-camera support ===&lt;br /&gt;
If you would like to explore advanced RMS installation options for various platforms or run multiple cameras on a single Linux computer, complete information is available on &#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Advanced_RMS_installations_and_Multi-camera_support this page]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
If you plan to run RMS software on the Raspberry Pi 4 or 5, the best supported and easiest solution is our prepared image. Complete information is available in an &#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_-_The_complete_how-to extensive guide]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
If you want to run Multiple cameras on the Raspberry Pi 5, please see the MultiCamPi documentation in this &#039;&#039;&#039;[https://drive.google.com/file/d/1XOsnDGLC1tGNRsZ4Ojy7axPP9hulgUJt/view?usp=sharing pdf file]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== Can I use a commercial all-sky camera? ===&lt;br /&gt;
&lt;br /&gt;
Generally, this is not a good idea because these cameras lack sufficient sensitivity. More information is available here: &#039;&#039;&#039;[https://globalmeteornetwork.org/?p=163 See this recent experiment]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Operate and maintain your GMN station ==&lt;br /&gt;
&lt;br /&gt;
=== Overview ===&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; GMS is a nascent operation, so you may share some of our growing pains if you choose to be involved. We are constantly solving bugs and making improvements, which is an opportunity for you to help if you have programming skills! The workload of day-to-day operation can be non-zero, and may require some of your time.&lt;br /&gt;
&lt;br /&gt;
Ideally, you should monitor your RMS Pi systems daily to identify freezes, glitches, or other problems. For example, you may see birds nesting or soiling the camera window, someone may unintentionally unplug the power cord, or animals (mice, cats, or dogs) may chew on the camera Ethernet cable. Although we make constant progress, the GMS network is not yet a &#039;power up and forget about it&#039; system. &lt;br /&gt;
&lt;br /&gt;
By its nature, the GMS network is staffed by lots of people who are willing to help newcomers get started. Here are some suggestions for daily operation of your RMS camera.&lt;br /&gt;
&lt;br /&gt;
=== What does the meteor camera do over the course of 24 hours? ===&lt;br /&gt;
&lt;br /&gt;
The RMS python-based system calculates the sundown to sunrise interval, and schedules video camera capture all night. Based on the video camera and capabilities of the Pi, the camera captures at least 25 frames per second between evening and morning twilight. During each nightly continuous image capture, the station processes captured image data and idenitfies frames that contain a minimum number of stars (usually around 20) that are worth reviewing for meteor detections. When data capture is complete, the station begins processing all frames it flagged with possible detections, then refines the astrometric accuracy of every positive detection. Using the station plate parameters (platepar) calibration file, processing iterates to find the best astrometry and photometry solution for each detected meteor. After this process analyzes each detection, summary files are created. &lt;br /&gt;
&lt;br /&gt;
The summary files include many types of information.&lt;br /&gt;
* Text file data presentation in several widely accepted formats (such as &#039;&#039;CAMS&#039;&#039; and &#039;&#039;UFOorbit&#039;&#039;).&lt;br /&gt;
* Graphic plots of detection frequencies throughout the night.&lt;br /&gt;
* Plot of all detections, showing any identified radiants.&lt;br /&gt;
* Plots of photometry, astrometry, and camera pointing drift in arc minutes throughout the course of the night as the mount or building flexes.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039;  Detailed information about plots is available here: &#039;&#039;&#039;[https://docs.google.com/document/d/132aHGn0QPzhpVN2s2n6FT6rJn39LAsPkchWJqXQb8Qk/edit?usp=sharing Explanation of GMN plots]&#039;&#039;&#039;&lt;br /&gt;
* Thumbnail images of detections.&lt;br /&gt;
* Thumbnail images of data captured throughout the night.&lt;br /&gt;
* Single image with all detections stacked together.&lt;br /&gt;
* Single image with all captured images stacked together.&lt;br /&gt;
* Flat file for correcting images.&lt;br /&gt;
* An &#039;&#039;.mp4&#039;&#039; movie time lapse of the night&#039;s captured images.&lt;br /&gt;
* Meteor shower flux charts, if specific showers are detected.&lt;br /&gt;
* Observation summary data of hardware and data recording characteristics.&lt;br /&gt;
 &lt;br /&gt;
When you click a meteor track, its data displays in the lower data window. Ultimately, all results are combined into a single compressed archive that automatically uploads each morning to the central server. &lt;br /&gt;
&lt;br /&gt;
Each morning, you can review the result files on the RPi and copy anything you want to your computer or tablet.&lt;br /&gt;
&lt;br /&gt;
===Archive data ===&lt;br /&gt;
&lt;br /&gt;
Your primary scientific data is automatically uploaded to the central server every morning after data processing is complete. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; When the night&#039;s results are uploaded, RMS purges the oldest data to free up space for the next night&#039;s run. As a result, you may want to copy some of the data to a PC, NAS, or the cloud for further analysis.&lt;br /&gt;
:       You should consider backing up the content of &#039;&#039;&#039;~/RMS_data/ArchivedFiles&#039;&#039;&#039;, which holds individual files and data that RMS determined were probably meteors. &lt;br /&gt;
&lt;br /&gt;
Details about backing up data is beyond the scope of the GMN Wiki. Tools such as Robocopy for Windows and rsync for Linux/MacOS are ideal, and they can &#039;mirror&#039; data across a network. Help to configure these tools is available in the &#039;&#039;&#039;Globalmeteornetwork&#039;&#039;&#039; group on &#039;&#039;&#039;groups.io&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
In addition, we added some automated tools that can help you back up data to a thumb drive inserted into the RPi. Assistance about these tools also is available in the &#039;&#039;&#039;Globalmeteornetwork&#039;&#039;&#039; group on &#039;&#039;&#039;groups.io&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
===Backup and restore the configuration and RSA keys===&lt;br /&gt;
&lt;br /&gt;
:&#039;&#039;&#039;NOTE:&#039;&#039;&#039; If you are on an older Buster image, you must replace username &#039;&#039;rms&#039;&#039; with username &#039;&#039;pi&#039;&#039;. For example, enter &#039;&#039;/home/pi&#039;&#039; instead of &#039;&#039;/home/rms&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
To determine which username to use, run &lt;br /&gt;
::&#039;&#039;ls /home/rms home/pi&#039;&#039;&lt;br /&gt;
to display the username that is your home directory.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Back up the configuration&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
1. Open a terminal and run the command  &#039;&#039;Scripts/RMS_Backup.sh&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
: A compressed &#039;&#039;.zip&#039;&#039; file, with all important configuration files and keys, is created in your user home directory with the prefix &#039;&#039;RMS_Backup&#039;&#039; and the &#039;&#039;.zip&#039;&#039; extension. &lt;br /&gt;
: For example, &#039;&#039;/home/rms/RMS_Backup_XX0001_2023-01-28.zip&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
2. Copy the &#039;&#039;.zip&#039;&#039; file to a safe place outside RPi. &lt;br /&gt;
&lt;br /&gt;
: Later, it will be useful to restore the system in case of failure. The &#039;&#039;.zip&#039;&#039; file contains the RSA public and private keys used to contact GMN servers, so keep it secret.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Restore the configuration&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
1. Unzip the backup file in any folder on the RPi.&lt;br /&gt;
&lt;br /&gt;
2. Copy the files &#039;&#039;.config&#039;&#039;, &#039;&#039;platepar_cmn2010.cal&#039;&#039;, and &#039;&#039;mask.bmp&#039;&#039; to the folder &#039;&#039;/home/rms/source/RMS/&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
3. Copy the files &#039;&#039;id_rsa&#039;&#039; and &#039;&#039;id_rsa.pub&#039;&#039; to the folder &#039;&#039;/home/rms/.ssh/&#039;&#039;, as shown in this example:&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;cp .config platepar_cmn2010.cal mask.bmp /home/rms/source/RMS/&#039;&#039;&lt;br /&gt;
: &#039;&#039;cp id_rsa id_rsa.pub /home/rms/.ssh/&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
4. To make sure that permission bits in the RSA key files are correct, enter:&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;chmod 400 ~/.ssh/id_rsa*&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== View the data ===&lt;br /&gt;
&lt;br /&gt;
To view data, you can use &#039;&#039;&#039;CMN_binViewer&#039;&#039;&#039; software [https://github.com/CroatianMeteorNetwork/cmn_binviewer], which is included in the RMS SD image. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; There also is a Windows version [https://github.com/CroatianMeteorNetwork/cmn_binviewer/releases] you can install.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; You can open images in astronomical FITS viewers, such as &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039; or &#039;&#039;&#039;Pixinsight&#039;&#039;&#039;, but what you see may be surprising. For example, in &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039;, the image is upside down, which is an artefact of how the software reads the image. &lt;br /&gt;
&lt;br /&gt;
In space, there is no &#039;up&#039; or &#039;down&#039;, so the FITS specification does not dictate if pixel (0,0) is at a specific corner. Some software, notably &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039;, specifies the top left corner as the origin location, which causes terrestrial images  to display vertically mirrored.&lt;br /&gt;
&lt;br /&gt;
=== Tools and utilities ===&lt;br /&gt;
&lt;br /&gt;
There are many tools available.&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;&#039;[https://www.realvnc.com/en/connect/download/viewer/ RealVNC]&#039;&#039;&#039;, &#039;&#039;&#039;[https://www.nomachine.com/ NoMachine]&#039;&#039;&#039;, &#039;&#039;&#039;[https://anydesk.com/en AnyDesk]&#039;&#039;&#039;, or &#039;&#039;&#039;[https://rustdesk.com/ RustDesk]&#039;&#039;&#039; remote connect tools provide station access from anywhere. Access to your station from outside your network is enabled by an OpenVPN connection address that is available to meteor stations.&lt;br /&gt;
: With &#039;&#039;&#039;VNC&#039;&#039;&#039; and &#039;&#039;&#039;Teamviewer&#039;&#039;&#039;, you can create an account and team on their websites, and then remotely access your station. &lt;br /&gt;
* &#039;&#039;&#039;Samba&#039;&#039;&#039; data directory access allows you to copy data results directly from your RPi to your computer or tablet.&lt;br /&gt;
* &#039;&#039;&#039;[https://github.com/CroatianMeteorNetwork/cmn_binviewer CMN_binViewer]&#039;&#039;&#039; allows you to view standard FITS image files that contain meteor detections. It runs on the RPi, and it can run under Windows.&lt;br /&gt;
* &#039;&#039;&#039;[https://sonotaco.com/soft/e_index.html UFO Orbit]&#039;&#039;&#039; allows you to process data from multiple stations, and generate unified radiants of two or more stations that see the same meteor. &#039;&#039;&#039;[https://sonotaco.com/soft/e_index.html UFO Orbit]&#039;&#039;&#039; can plot the shared object ground path and orbital characteristics, and it can output a summary file of all objects seen by more than one station.&lt;br /&gt;
* RMS software can be installed under Windows to allow much of the RMS python-based code to run on your computer. This means you can run RMS against meteor station data that was transferred to your computer from the RPi.&lt;br /&gt;
&lt;br /&gt;
You also can run RMS python jobs on the RPi to sample captured image files, and then condense them into an &#039;&#039;.mp4&#039;&#039; video. Sometimes, these videos are mesmerizing summaries that can run for more than two minutes of winter time data.&lt;br /&gt;
&lt;br /&gt;
== What can I do with my GMN station? ==&lt;br /&gt;
&lt;br /&gt;
=== Use SkyFit2 for astrometric and photometric calibration + Manually reduce observations of fireballs and compute their trajectories ===&lt;br /&gt;
* &#039;&#039;&#039;[https://www.youtube.com/watch?v=ao3J9Jf0iLQ Updated 2023 video tutorial]&#039;&#039;&#039;&lt;br /&gt;
* &#039;&#039;&#039;[https://www.youtube.com/watch?v=MOjb3qxDlX4 Old 2021 video tutorial]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/fov3d/ Generate a Google Earth KML file to show your station&#039;s field of view] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=253 Use the UFO Orbit program to estimate meteor trajectories] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=221 Urban meteor observing] ===&lt;br /&gt;
&lt;br /&gt;
== Data analysis with SkyFit2 ==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SkyFit2&#039;&#039;&#039;, a program in the RMS library, allows you to analyze optical meteor data in most of the optical formats in current use. The program supports popular video formats (&#039;&#039;.mp4&#039;&#039;, &#039;&#039;.avi&#039;&#039;, and &#039;&#039;.mkv&#039;&#039;), sequences of static images, and single images with shutter breaks.&lt;br /&gt;
&lt;br /&gt;
A &#039;&#039;&#039;[https://www.youtube.com/watch?v=ao3J9Jf0iLQ video tutorial]&#039;&#039;&#039; explains how to useg &#039;&#039;&#039;SkyFit2&#039;&#039;&#039; to run astrometric and photometric calibrations on GMN data, and it can manually reduce observations of fireballs and compute their trajectories.&lt;br /&gt;
&lt;br /&gt;
A more detailed description of &#039;&#039;&#039;SkyFit2&#039;&#039;&#039; is available on the &#039;&#039;&#039;[[SkyFit2|SkyFit2]]&#039;&#039;&#039; page.&lt;br /&gt;
&lt;br /&gt;
== FAQ ==&lt;br /&gt;
&lt;br /&gt;
=== What should I back up when I re-flash an SD card or a USB disk? ===&lt;br /&gt;
&lt;br /&gt;
You should backup the &#039;&#039;.config&#039;&#039;, platepar, and mask files that are in the RMS source directory, plus the entire content of the hidden directory &#039;&#039;/home/pi/.ssh&#039;&#039;. Refer to the section titled, &#039;&#039;&#039;Back up the configuration&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
If your SD card or USB disk fails or becomes corrupted, you can fetch the config files from the server because they are uploaded every day, together with the data.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The content of &#039;&#039;.ssh&#039;&#039; is essential for connection to the server, so you also must save these files. &lt;br /&gt;
&lt;br /&gt;
After you set up a new SD card or USB disk, return the files to their original location.&lt;br /&gt;
&lt;br /&gt;
=== What are the values in the &#039;&#039;FTPdetectinfo_*&#039;&#039;  file designated as hnr mle bin Pix/fm Rho Phi? ===&lt;br /&gt;
&lt;br /&gt;
Some of these values (hnr mle bin) are not used in RMS but they are used in CAMS, so their presence is to conform to the standard. As a result, these values are all zeros. &lt;br /&gt;
&lt;br /&gt;
There are other values:&lt;br /&gt;
* Pix/fm is the average angular speed of the meteor, in pixels, per frame.&lt;br /&gt;
* Rho, Phi are parameters that define the line of the meteor in polar coordinates, see this &#039;&#039;&#039;[https://en.wikipedia.org/wiki/Hough_transform#Theory page]&#039;&#039;&#039; for more detail. &lt;br /&gt;
: &#039;&#039;Rho&#039;&#039; is the distance of the line from the center of the image.&lt;br /&gt;
: &#039;&#039;Phi&#039;&#039; is the angle of the line, as measured from the positive direction of the Y axis. (Basically, this is a line from the center of the image to the top of the image.) The positive angles are measured clockwise, although the CAMS standard may define these parameters a bit differently, with the Y axis flipped.&lt;br /&gt;
The &#039;&#039;intensity&#039;&#039; is the sum of all pixel intensities of the meteor on a given frame. &lt;br /&gt;
&lt;br /&gt;
For example, you could represent an area around the meteor on a given frame, as shown in the figure, where the numbers are pixel intensities on an 8-bit image (so they can range from 0 to 255) and the pixel values inside the red boundary represent the meteor blob on the frame. The result? The intensity is the sum of all numbers inside the red boundary. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Later, this value is used to compute the magnitude.&lt;br /&gt;
&lt;br /&gt;
[[File:Intensity_sum.png |Intensity_sum.png ]]&lt;br /&gt;
&lt;br /&gt;
The magnitude is computed as&lt;br /&gt;
: &#039;&#039;mag = -2.5*log10(intensity sum) + photometric_offset&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
To estimate the photometric offset in &#039;&#039;&#039;SkyFit&#039;&#039;&#039;, fit the line with slope -2.5 through pairs of known magnitudes of stars and logartihms of their pixel intensity sum. Fundamentally, the photometric offset is the intercept of that line. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The constant slope of -2.5 comes from the &#039;&#039;&#039;[https://en.wikipedia.org/wiki/Apparent_magnitude#Calculations Definition of stellar magnitudes]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== GMN data policy ==&lt;br /&gt;
&lt;br /&gt;
The Global Meteor Network produces three levels of data products.&lt;br /&gt;
* Level 1 - The lowest level data (as close to &#039;raw&#039; as possible) are the FF image and FR video files saved to the RPi by the capture code and the fireball detector.&lt;br /&gt;
* Level 2 - Data is used in three ways:&lt;br /&gt;
:* The meteor detector extracts positional and brightness information of individual meteors (&#039;&#039;FTPdetectinfo&#039;&#039; file). &lt;br /&gt;
:* Images are used for astrometric and photometric calibration (platepar file). &lt;br /&gt;
:* Meteor and star detections are used to generate a range of plots, such as the single-station shower association graph and the camera drift graph. The calibrated meteor measurements are uploaded to the GMN server, together with the raw images of individual meteors.&lt;br /&gt;
* Level 3 - Software on the server correlates individual observations and computes multi-station meteor trajectories, which are published daily on the &#039;&#039;&#039;GMN [https://globalmeteornetwork.org/data/ Data website]&#039;&#039;&#039;. This data is made public under the &#039;&#039;&#039;[https://creativecommons.org/licenses/by/4.0/ CC BY 4.0 license]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
Operators of individual GMN stations exclusively own the Level 1 and Level 2 data their stations produce. In practice, this means they are free to share this data with other meteor networks if they wish. The data that is uploaded to the GMN server is not shared publicly or with other parties without the operator&#039;s consent. However, the data may be used internally by the GMN coordinators to manually produce other data products, such as the trajectory of a meteorite dropping fireball or an analysis of a meteor shower. &lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; All station operators are credited for their data in all GMN publications.&lt;br /&gt;
&lt;br /&gt;
== GMN Plots and Images Explained ==&lt;br /&gt;
&lt;br /&gt;
This document explains the data summaries produced on your system and displayed on the GMN Weblog every morning &#039;&#039;&#039;[https://docs.google.com/document/d/132aHGn0QPzhpVN2s2n6FT6rJn39LAsPkchWJqXQb8Qk/edit?pli=1&amp;amp;tab=t.0 GMN Plots and Images]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;[https://IstraStream.com IstraStream.com]&#039;&#039;&#039; was an independent hosting site primarily intended for cameras sold by IstraStream. In mid-2023, Istrastream stopped listing camera image output and the IstraStream data display was replaced with the &#039;&#039;&#039;[https://globalmeteornetwork.org/weblog/ GMN weblog]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== For more information ==&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?page_id=43 Contact the Global Meteor Network] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://groups.io/g/globalmeteornetwork Join the Global Meteor Network Forum] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://github.com/markmac99/ukmon-pitools/wiki UK Meteor Network Wiki]===&lt;br /&gt;
This wiki has numerous FAQs and tips on maintaining, monitoring and managing your system, and several explainers such as how to calibrate and create a mask, how to copy data and so forth. &lt;br /&gt;
&lt;br /&gt;
=== Important GMN resources ===&lt;br /&gt;
&lt;br /&gt;
There are two additional web pages you should know about.&lt;br /&gt;
&lt;br /&gt;
* The &#039;&#039;&#039;[https://globalmeteornetwork.org/status GMN status page]&#039;&#039;&#039; provides access to the &#039;&#039;&#039;[https://globalmeteornetwork.org/weblog/ GMN weblog]&#039;&#039;&#039;.&lt;br /&gt;
* A mapping utility website that is directly derived from GMN data: &#039;&#039;&#039;[https://tammojan.github.io/meteormap Meteor map]&#039;&#039;&#039;.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; This map takes quite a while to load. When you review the map, you must scroll down to see the full power of the data display.&lt;br /&gt;
&lt;br /&gt;
=== GMN talks ===&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=_tV7WBo0RrQ 2025 GMN Meeting Session 1 (February 2025)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=z23aJeIg7wo 2025 GMN Meeting Session 2 (February 2025)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/playlist?list=PLmQ5Bvz4ACYJLYfswIeAipapoeGeI6QWy GMN talk for Society for Astronomical Sciences workshop 2024 (The first 3 videos)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=juOvRTtoqhs 2024 GMN Meeting Session 1 (February 2024)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=MXhVIxrz2ks 2024 GMN Meeting Session 2 (February 2024)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=IfUyCHjMATc 2023 GMN Meeting Session 1 (February 2023)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=I78KwF5-1GE 2023 GMN Meeting Session 2 (February 2023)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=wDdrG_FCyGk 2022 GMN Meeting Session 1 (February 2022)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=j_75CDPzjI4 2022 GMN Meeting Session 2 (February 2022)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=f6x9_WCVphY GMN talk at the European Space Agency&#039;s Fireball Workshop (June 2021)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=QXBTLPnPDWs 2021 GMN Meeting] - [https://www.dropbox.com/sh/ia9vagug5lxm8k9/AAB_i_1jcWThUdAHO_2gF_Ksa?dl=0 Link to slides]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=MAGq-XqD5Po Overview of the GMN - IMC2020 (September 2020)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=oM7lfQ4nmyw Overview of the GMN, Astro Imaging Channel presentation (May 2020)]&lt;br /&gt;
&lt;br /&gt;
=== GMN-related publications ===&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2206.11365 Vida, D., Blaauw Erskine, R. C., Brown, P. G., Kambulow, J., Campbell-Brown, M., &amp;amp; Mazur, M. J. (2022). Computing optical meteor flux using global meteor network data. Monthly Notices of the Royal Astronomical Society, 515(2), 2322-2339.]&lt;br /&gt;
&lt;br /&gt;
: [https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stab2557/6368869 Moorhead, A. V., Clements, T., &amp;amp; Vida, D. (2021). Meteor shower radiant dispersions in Global Meteor Network data. Monthly Notices of the Royal Astronomical Society, 508(1), 326-339.]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2107.12335 Vida, D., Šegon, D., Gural, P. S., Brown, P. G., McIntyre, M. J., Dijkema, T. J., Pavletić, L., Kukić, P., Mazur, M.J., Eschman, P., Roggemans, P., Merlak, A., &amp;amp; Zubović, D. (2021). The Global Meteor Network–Methodology and first results. Monthly Notices of the Royal Astronomical Society, 506(4), 5046-5074.]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2003.05458/ Moorhead, A. V., Clements, T. D., &amp;amp; Vida, D. (2020). Realistic gravitational focusing of meteoroid streams. Monthly Notices of the Royal Astronomical Society, 494(2), 2982-2994.] &lt;br /&gt;
&lt;br /&gt;
: [https://globalmeteornetwork.org/wordpress/wp-content/uploads/2018/11/Kukic-et-al-2018-Rolling-shutter.pdf  Kukić, P., Gural, P., Vida, D., Šegon, D. &amp;amp; Merlak, A. (2018) Correction for meteor centroids observed using rolling shutter cameras. WGN, Journal of the International Meteor Organization, 46:5, 154-118.]&lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/2018_WGN___RMS_sun_skirter_final.pdf  Vida, D., Mazur, M. J., Šegon, D., Kukić, P., &amp;amp; Merlak, A. (2018). Compressive strength of a skirting Daytime Arietid-first science results from low-cost Raspberry Pi-based meteor stations. WGN, Journal of the International Meteor Organization, 46, 113-118.] &lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/pdf/1911.02979.pdf Vida, D., Gural, P., Brown, P., Campbell-Brown, M., Wiegert, P. (2019) Estimating trajectories of meteors: an observational Monte Carlo approach - I. Theory. arXiv:1911.02979v4 [astro-ph.EP] 21 Apr 2020]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/pdf/1911.11734.pdf Vida, D., Gural, P., Brown, P., Campbell-Brown, M., Wiegert, P. (2019) Estimating trajectories of meteors: an observational Monte Carlo approach - II. Results. arXiv:1911.11734v1 [astro-ph.EP] 26 Novr 2019]&lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/2018_WGN___RMS_first_results-final.pdf Vida, D., Mazur, M. J., Šegon, D., Zubović, D., Kukić, P., Parag, F., &amp;amp; Macan, A. (2018). First results of a Raspberry Pi based meteor camera system. WGN, Journal of the International Meteor Organization, 46, 71-78.] &lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/Vida_IMC2016_proceedings_final.pdf Vida, D., Zubović, D., Šegon, D., Gural, P., &amp;amp; Cupec, R. (2016). Open-source meteor detection software for low-cost single-board computers. In Proceedings of the International Meteor Conference (IMC2016), Egmond, The Netherlands (pp. 2-5).] &lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/Zubovic_IMC2015_priceedings_final.pdf Zubović, D., Vida, D., Gural, P., &amp;amp; Šegon, D. (2015). Advances in the development of a low-cost video meteor station. In Proceedings of the International Meteor Conference, Mistelbach, Austria (pp. 27-30).]&lt;/div&gt;</summary>
		<author><name>MeteorsABQ</name></author>
	</entry>
	<entry>
		<id>https://globalmeteornetwork.org//wiki/index.php?title=Installation_for_Linux&amp;diff=850</id>
		<title>Installation for Linux</title>
		<link rel="alternate" type="text/html" href="https://globalmeteornetwork.org//wiki/index.php?title=Installation_for_Linux&amp;diff=850"/>
		<updated>2025-10-27T20:40:32Z</updated>

		<summary type="html">&lt;p&gt;MeteorsABQ: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;=== Installation for Linux ===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
To streamline the maintenance of these scripts as the RMS codebase evolves, the installation code for Linux was moved to the &#039;&#039;MultiCam&#039;&#039; directory maintained in the RMS github pages.&lt;br /&gt;
&lt;br /&gt;
For a single station, use the multi-cam instructions. The script will install RMS, then prompt you for input.&lt;br /&gt;
&lt;br /&gt;
1. Do you wish to configure some stations?&lt;br /&gt;
&lt;br /&gt;
2. Enter &#039;&#039;N&#039;&#039; or &#039;&#039;n&#039;&#039; to exit the script.  &lt;br /&gt;
&lt;br /&gt;
   The script will exit and leave you at the default shell prompt with RMS installed. The default camera configuration location is &#039;&#039;~/source/RMS&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Detailed instructions are available &#039;&#039;&#039;[https://drive.google.com/file/d/1-vJLYypFWx72TFqbBHQbXK2LhfWIwDP1/view?usp=sharing here].&#039;&#039;&#039;&lt;/div&gt;</summary>
		<author><name>MeteorsABQ</name></author>
	</entry>
	<entry>
		<id>https://globalmeteornetwork.org//wiki/index.php?title=Advanced_RMS_installations_and_Multi-camera_support&amp;diff=849</id>
		<title>Advanced RMS installations and Multi-camera support</title>
		<link rel="alternate" type="text/html" href="https://globalmeteornetwork.org//wiki/index.php?title=Advanced_RMS_installations_and_Multi-camera_support&amp;diff=849"/>
		<updated>2025-10-22T16:08:58Z</updated>

		<summary type="html">&lt;p&gt;MeteorsABQ: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;= Advanced RMS installations and multi-camera support  =&lt;br /&gt;
&lt;br /&gt;
When you set up a Raspberry Pi, it is receommended that you use the prebuilt image. This image includes an installation of all necessary software and it is ready to use. If you are convinced that you want to install RPi from scratch, use the process that follows.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; This process is intended for users who want to tackle more advanced tasks. If you completed the previous section, do not attempt the instructions that follow.&lt;br /&gt;
&lt;br /&gt;
== Install Raspberry Pi 4 ==&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;WARNING:&#039;&#039;&#039; This installation process is not recommended. If you insist on completing this procedure, use the image &#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Installing_OS_onto_a_Raspberry_Pi here]&#039;&#039;&#039; and follow the detailed instructions at these links:&lt;br /&gt;
* &#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Pi4_with_Raspbian_Bookworm Bookworm]&#039;&#039;&#039; &lt;br /&gt;
* &#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Pi4_with_Raspbian_Bullseye Bullseye]&#039;&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; We also no longer recommend using &#039;&#039;&#039;Buster&#039;&#039;&#039;, but the legacy instructions are available &#039;&#039;&#039;[https://docs.google.com/document/d/19ImeNqBTD1ml2iisp5y7CjDrRV33wBeF9rtx3mIVjh4/edit?usp=sharing here]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Installation for Linux ==&lt;br /&gt;
&lt;br /&gt;
Detailed instructions are available &#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Installation_for_Linux here]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Linux GUI and multi-camera support ==&lt;br /&gt;
&lt;br /&gt;
Detailed instructions are available &#039;&#039;&#039;[https://drive.google.com/file/d/1-vJLYypFWx72TFqbBHQbXK2LhfWIwDP1/view?usp=sharing here]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Installation for Windows ==&lt;br /&gt;
Data capture does not work under windows. However, you can use other tools on your PC. You can run &#039;&#039;&#039;SkyFit2&#039;&#039;&#039; to calibrate your camera to the sky, or you can use the &#039;&#039;BatchFFToImage&#039;&#039; script to convert data to &#039;&#039;.jpeg&#039;&#039; format to share on social media. &lt;br /&gt;
&lt;br /&gt;
Click &#039;&#039;&#039;[[Windows_Installation|here]]&#039;&#039;&#039; for detailed instructions. This process was tested on Windows 10 64-bit, but it should work with any Windows version where &#039;&#039;&#039;git&#039;&#039;&#039; and &#039;&#039;&#039;Anaconda&#039;&#039;&#039; are available. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;Aside:&#039;&#039;&#039; If you are a Windows expert, feel free to investigate why data capture does not work. If you are able to determine the cause of the problem and its solution, contact one of the Administrators on this wiki.&lt;br /&gt;
&lt;br /&gt;
== Installation for MacOS ==&lt;br /&gt;
As with Windows, installation for MacOS is useful if you want to analyze the data offline. To install  the software for MacOS, follow the instructions &#039;&#039;&#039;[[MacOS_Install | here]]&#039;&#039;&#039;.&lt;/div&gt;</summary>
		<author><name>MeteorsABQ</name></author>
	</entry>
	<entry>
		<id>https://globalmeteornetwork.org//wiki/index.php?title=Main_Page&amp;diff=848</id>
		<title>Main Page</title>
		<link rel="alternate" type="text/html" href="https://globalmeteornetwork.org//wiki/index.php?title=Main_Page&amp;diff=848"/>
		<updated>2025-10-02T21:06:57Z</updated>

		<summary type="html">&lt;p&gt;MeteorsABQ: /* GMN talks */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Welcome to the Global Meteor Network wiki page!&lt;br /&gt;
&lt;br /&gt;
The Global Meteor Network (GMN) is a world-wide organization of amateur and professional astronomers. The goal is to observe the night sky using low-light video cameras and produce meteor trajectories in a coordinated network of recording stations. Here, you can find information about the purpose and structure of the GMN, and how to assemble and operate your own meteor camera. You also will discover how to contribute to the development of RMS (the GMN software) and how your observations as a citizen scientist contribute to the ongoing understanding of our solar system&#039;s formation and evolution. &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;If you are here to find out how to build and set up a camera from scratch, jump ahead to [https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_-_The_complete_how-to this] section!&amp;lt;/span&amp;gt;&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;For German speakers, there is &amp;quot;Build camera from scratch&amp;quot; documentation written by students of [https://fsg-preetz.de/ Friedrich-Schiller-Gymnasium in Preetz] available [http://wiki.linux-astronomie.de/doku.php?id=ceres here]. This version is maintained by Friedrich-Schiller-Gymnasium in Preetz. &amp;lt;/span&amp;gt;&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Global Meteor Network overview ==&lt;br /&gt;
&lt;br /&gt;
===  [https://globalmeteornetwork.org/?page_id=141 Our mission] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=363 A brief history of the Global Meteor Network] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://www.youtube.com/watch?v=MAGq-XqD5Po Video introduction - Overview of the Global Meteor Network (IMC2020)] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://youtu.be/oM7lfQ4nmyw Video overview - Meteor tracking and the GMN from Astro Imaging Channel presentation] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/data/ Some &#039;live&#039; GMN data products] ===&lt;br /&gt;
&lt;br /&gt;
== Meteor detection station ==&lt;br /&gt;
&lt;br /&gt;
What is an RMS GMN station? An RMS-based GMN station consists of a Raspberry Pi (RPi) single board computer, a low light level security video camera, the RMS software, and a connection to the Internet via Wifi. The camera is securely mounted in a weatherproof housing, pointed at the sky, and connected to the RPi with a Power Over Ethernet (POE) cable. To be a part of the GMN network, you need a fairly powerful Raspberry Pi (Pi 4, 5, or better) and a reasonably fast Internet connection. The internet connection is required only for data upload to a central server each morning and to provide automatic updates for the RMS software. &lt;br /&gt;
&lt;br /&gt;
Nightly, the RPi records video from the camera shortly after local sunset, then continuously compressing and storing the video data on a local SSD drive. Each morning before sunrise, when capture is complete, the RPi analyzes the video and extracts  meteor observations from the previous night. These extracted video clips of detected meteors are archived and then uploaded to a server. On a &#039;busy&#039; night, the clips can total hundreds of megabytes as a result of a heavy meteor shower or a night with a lot of false detections. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Continuous progress is being made on the detection software to filter out false detections. &lt;br /&gt;
&lt;br /&gt;
The server finds meteors that were observed from more than one station, which allows the server to triangulate meteor trails in 3D and calculate the orbits of the meteors.&lt;br /&gt;
&lt;br /&gt;
=== What do I need? ===&lt;br /&gt;
&lt;br /&gt;
You need a Raspberry Pi compluter, RMS software, and a camera kit. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; We strongly recommend the Pi 4 or 5 model. &lt;br /&gt;
The software can run on a Pi3, but it is much slower and it is no longer supported. A list with everything you need is available here: [https://globalmeteornetwork.org/wiki/index.php?title=Shopping_list_and_tools_needed page].&lt;br /&gt;
&lt;br /&gt;
You can run multiple cameras on a Linux PC, and details are available &#039;&#039;&#039;[https://docs.google.com/document/d/16PSFi8RAqbenPdluhulCRaIenOkEzgs5piUhkX3yaOc/edit here]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== How do I obtain a camera? ===&lt;br /&gt;
There are two options - buy a camera or build a camera.&lt;br /&gt;
&lt;br /&gt;
==== Buy a Camera ====&lt;br /&gt;
You can buy a camera and prebuilt Pi, and ready to install. Cameras are available from several suppliers, as well as the Croatian Meteor Network, as explained here: [https://globalmeteornetwork.org/?page_id=136 this page]. &lt;br /&gt;
If you are in the UK, you can contact the UK Meteor network for advice. [https://ukmeteornetwork.org/ UK Meteor Network].&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; As of 2024, UK Meteor network can no longer sell cameras directly.&lt;br /&gt;
&lt;br /&gt;
==== Build your own from scratch ====&lt;br /&gt;
This option requires an intermediate level of DIY skills and familiarity with the Raspberry Pi, but do not be put off. The instructions are comprehensive and, if you get stuck, you can ask for advice in the forum here: &#039;&#039;&#039;[https://groups.io/g/globalmeteornetwork groups.io]&#039;&#039;&#039; forum.&lt;br /&gt;
&lt;br /&gt;
You can find out more about this option here: &#039;&#039;&#039;[[Build &amp;amp; Install &amp;amp; Setup your camera - The complete how-to]]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== Advanced RMS installations and multi-camera support ===&lt;br /&gt;
If you would like to explore advanced RMS installation options for various platforms or run multiple cameras on a single Linux computer, complete information is available on &#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Advanced_RMS_installations_and_Multi-camera_support this page]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
If you plan to run RMS software on the Raspberry Pi 4 or 5, the best supported and easiest solution is our prepared image. Complete information is available in an &#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_- Extensive how-to guide]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== Can I use a commercial all-sky camera? ===&lt;br /&gt;
&lt;br /&gt;
Generally, this is not a good idea because these cameras lack sufficient sensitivity. More information is available here: &#039;&#039;&#039;[https://globalmeteornetwork.org/?p=163 See this recent experiment]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Operate and maintain your GMN station ==&lt;br /&gt;
&lt;br /&gt;
=== Overview ===&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; GMS is a nascent operation, so you may share some of our growing pains if you choose to be involved. We are constantly solving bugs and making improvements, which is an opportunity for you to help if you have programming skills! The workload of day-to-day operation can be non-zero, and may require some of your time.&lt;br /&gt;
&lt;br /&gt;
Ideally, you should monitor your RMS Pi systems daily to identify freezes, glitches, or other problems. For example, you may see birds nesting or soiling the camera window, someone may unintentionally unplug the power cord, or animals (mice, cats, or dogs) may chew on the camera Ethernet cable. Although we make constant progress, the GMS network is not yet a &#039;power up and forget about it&#039; system. &lt;br /&gt;
&lt;br /&gt;
By its nature, the GMS network is staffed by lots of people who are willing to help newcomers get started. Here are some suggestions for daily operation of your RMS camera.&lt;br /&gt;
&lt;br /&gt;
=== What does the meteor camera do over the course of 24 hours? ===&lt;br /&gt;
&lt;br /&gt;
The RMS python-based system calculates the sundown to sunrise interval, and schedules video camera capture all night. Based on the video camera and capabilities of the Pi, the camera captures at least 25 frames per second between evening and morning twilight. During each nightly continuous image capture, the station processes captured image data and idenitfies frames that contain a minimum number of stars (usually around 20) that are worth reviewing for meteor detections. When data capture is complete, the station begins processing all frames it flagged with possible detections, then refines the astrometric accuracy of every positive detection. Using the station plate parameters (platepar) calibration file, processing iterates to find the best astrometry and photometry solution for each detected meteor. After this process analyzes each detection, summary files are created. &lt;br /&gt;
&lt;br /&gt;
The summary files include many types of information.&lt;br /&gt;
* Text file data presentation in several widely accepted formats (such as &#039;&#039;CAMS&#039;&#039; and &#039;&#039;UFOorbit&#039;&#039;).&lt;br /&gt;
* Graphic plots of detection frequencies throughout the night.&lt;br /&gt;
* Plot of all detections, showing any identified radiants.&lt;br /&gt;
* Plots of photometry, astrometry, and camera pointing drift in arc minutes throughout the course of the night as the mount or building flexes.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039;  Detailed information about plots is available here: &#039;&#039;&#039;[https://docs.google.com/document/d/132aHGn0QPzhpVN2s2n6FT6rJn39LAsPkchWJqXQb8Qk/edit?usp=sharing Explanation of GMN plots]&#039;&#039;&#039;&lt;br /&gt;
* Thumbnail images of detections.&lt;br /&gt;
* Thumbnail images of data captured throughout the night.&lt;br /&gt;
* Single image with all detections stacked together.&lt;br /&gt;
* Single image with all captured images stacked together.&lt;br /&gt;
* Flat file for correcting images.&lt;br /&gt;
* An &#039;&#039;.mp4&#039;&#039; movie time lapse of the night&#039;s captured images.&lt;br /&gt;
* Meteor shower flux charts, if specific showers are detected.&lt;br /&gt;
* Observation summary data of hardware and data recording characteristics.&lt;br /&gt;
 &lt;br /&gt;
When you click a meteor track, its data displays in the lower data window. Ultimately, all results are combined into a single compressed archive that automatically uploads each morning to the central server. &lt;br /&gt;
&lt;br /&gt;
Each morning, you can review the result files on the RPi and copy anything you want to your computer or tablet.&lt;br /&gt;
&lt;br /&gt;
===Archive data ===&lt;br /&gt;
&lt;br /&gt;
Your primary scientific data is automatically uploaded to the central server every morning after data processing is complete. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; When the night&#039;s results are uploaded, RMS purges the oldest data to free up space for the next night&#039;s run. As a result, you may want to copy some of the data to a PC, NAS, or the cloud for further analysis.&lt;br /&gt;
:       You should consider backing up the content of &#039;&#039;&#039;~/RMS_data/ArchivedFiles&#039;&#039;&#039;, which holds individual files and data that RMS determined were probably meteors. &lt;br /&gt;
&lt;br /&gt;
Details about backing up data is beyond the scope of the GMN Wiki. Tools such as Robocopy for Windows and rsync for Linux/MacOS are ideal, and they can &#039;mirror&#039; data across a network. Help to configure these tools is available in the &#039;&#039;&#039;Globalmeteornetwork&#039;&#039;&#039; group on &#039;&#039;&#039;groups.io&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
In addition, we added some automated tools that can help you back up data to a thumb drive inserted into the RPi. Assistance about these tools also is available in the &#039;&#039;&#039;Globalmeteornetwork&#039;&#039;&#039; group on &#039;&#039;&#039;groups.io&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
===Backup and restore the configuration and RSA keys===&lt;br /&gt;
&lt;br /&gt;
:&#039;&#039;&#039;NOTE:&#039;&#039;&#039; If you are on an older Buster image, you must replace username &#039;&#039;rms&#039;&#039; with username &#039;&#039;pi&#039;&#039;. For example, enter &#039;&#039;/home/pi&#039;&#039; instead of &#039;&#039;/home/rms&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
To determine which username to use, run &lt;br /&gt;
::&#039;&#039;ls /home/rms home/pi&#039;&#039;&lt;br /&gt;
to display the username that is your home directory.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Back up the configuration&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
1. Open a terminal and run the command  &#039;&#039;Scripts/RMS_Backup.sh&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
: A compressed &#039;&#039;.zip&#039;&#039; file, with all important configuration files and keys, is created in your user home directory with the prefix &#039;&#039;RMS_Backup&#039;&#039; and the &#039;&#039;.zip&#039;&#039; extension. &lt;br /&gt;
: For example, &#039;&#039;/home/rms/RMS_Backup_XX0001_2023-01-28.zip&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
2. Copy the &#039;&#039;.zip&#039;&#039; file to a safe place outside RPi. &lt;br /&gt;
&lt;br /&gt;
: Later, it will be useful to restore the system in case of failure. The &#039;&#039;.zip&#039;&#039; file contains the RSA public and private keys used to contact GMN servers, so keep it secret.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Restore the configuration&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
1. Unzip the backup file in any folder on the RPi.&lt;br /&gt;
&lt;br /&gt;
2. Copy the files &#039;&#039;.config&#039;&#039;, &#039;&#039;platepar_cmn2010.cal&#039;&#039;, and &#039;&#039;mask.bmp&#039;&#039; to the folder &#039;&#039;/home/rms/source/RMS/&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
3. Copy the files &#039;&#039;id_rsa&#039;&#039; and &#039;&#039;id_rsa.pub&#039;&#039; to the folder &#039;&#039;/home/rms/.ssh/&#039;&#039;, as shown in this example:&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;cp .config platepar_cmn2010.cal mask.bmp /home/rms/source/RMS/&#039;&#039;&lt;br /&gt;
: &#039;&#039;cp id_rsa id_rsa.pub /home/rms/.ssh/&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
4. To make sure that permission bits in the RSA key files are correct, enter:&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;chmod 400 ~/.ssh/id_rsa*&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== View the data ===&lt;br /&gt;
&lt;br /&gt;
To view data, you can use &#039;&#039;&#039;CMN_binViewer&#039;&#039;&#039; software [https://github.com/CroatianMeteorNetwork/cmn_binviewer], which is included in the RMS SD image. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; There also is a Windows version [https://github.com/CroatianMeteorNetwork/cmn_binviewer/releases] you can install.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; You can open images in astronomical FITS viewers, such as &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039; or &#039;&#039;&#039;Pixinsight&#039;&#039;&#039;, but what you see may be surprising. For example, in &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039;, the image is upside down, which is an artefact of how the software reads the image. &lt;br /&gt;
&lt;br /&gt;
In space, there is no &#039;up&#039; or &#039;down&#039;, so the FITS specification does not dictate if pixel (0,0) is at a specific corner. Some software, notably &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039;, specifies the top left corner as the origin location, which causes terrestrial images  to display vertically mirrored.&lt;br /&gt;
&lt;br /&gt;
=== Tools and utilities ===&lt;br /&gt;
&lt;br /&gt;
There are many tools available.&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;&#039;[https://www.realvnc.com/en/connect/download/viewer/ RealVNC]&#039;&#039;&#039;, &#039;&#039;&#039;[https://www.nomachine.com/ NoMachine]&#039;&#039;&#039;, &#039;&#039;&#039;[https://anydesk.com/en AnyDesk]&#039;&#039;&#039;, or &#039;&#039;&#039;[https://rustdesk.com/ RustDesk]&#039;&#039;&#039; remote connect tools provide station access from anywhere. Access to your station from outside your network is enabled by an OpenVPN connection address that is available to meteor stations.&lt;br /&gt;
: With &#039;&#039;&#039;VNC&#039;&#039;&#039; and &#039;&#039;&#039;Teamviewer&#039;&#039;&#039;, you can create an account and team on their websites, and then remotely access your station. &lt;br /&gt;
* &#039;&#039;&#039;Samba&#039;&#039;&#039; data directory access allows you to copy data results directly from your RPi to your computer or tablet.&lt;br /&gt;
* &#039;&#039;&#039;[https://github.com/CroatianMeteorNetwork/cmn_binviewer CMN_binViewer]&#039;&#039;&#039; allows you to view standard FITS image files that contain meteor detections. It runs on the RPi, and it can run under Windows.&lt;br /&gt;
* &#039;&#039;&#039;[https://sonotaco.com/soft/e_index.html UFO Orbit]&#039;&#039;&#039; allows you to process data from multiple stations, and generate unified radiants of two or more stations that see the same meteor. &#039;&#039;&#039;[https://sonotaco.com/soft/e_index.html UFO Orbit]&#039;&#039;&#039; can plot the shared object ground path and orbital characteristics, and it can output a summary file of all objects seen by more than one station.&lt;br /&gt;
* RMS software can be installed under Windows to allow much of the RMS python-based code to run on your computer. This means you can run RMS against meteor station data that was transferred to your computer from the RPi.&lt;br /&gt;
&lt;br /&gt;
You also can run RMS python jobs on the RPi to sample captured image files, and then condense them into an &#039;&#039;.mp4&#039;&#039; video. Sometimes, these videos are mesmerizing summaries that can run for more than two minutes of winter time data.&lt;br /&gt;
&lt;br /&gt;
== What can I do with my GMN station? ==&lt;br /&gt;
&lt;br /&gt;
=== Use SkyFit2 for astrometric and photometric calibration + Manually reduce observations of fireballs and compute their trajectories ===&lt;br /&gt;
* &#039;&#039;&#039;[https://www.youtube.com/watch?v=ao3J9Jf0iLQ Updated 2023 video tutorial]&#039;&#039;&#039;&lt;br /&gt;
* &#039;&#039;&#039;[https://www.youtube.com/watch?v=MOjb3qxDlX4 Old 2021 video tutorial]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/fov3d/ Generate a Google Earth KML file to show your station&#039;s field of view] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=253 Use the UFO Orbit program to estimate meteor trajectories] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=221 Urban meteor observing] ===&lt;br /&gt;
&lt;br /&gt;
== Data analysis with SkyFit2 ==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SkyFit2&#039;&#039;&#039;, a program in the RMS library, allows you to analyze optical meteor data in most of the optical formats in current use. The program supports popular video formats (&#039;&#039;.mp4&#039;&#039;, &#039;&#039;.avi&#039;&#039;, and &#039;&#039;.mkv&#039;&#039;), sequences of static images, and single images with shutter breaks.&lt;br /&gt;
&lt;br /&gt;
A &#039;&#039;&#039;[https://www.youtube.com/watch?v=ao3J9Jf0iLQ video tutorial]&#039;&#039;&#039; explains how to useg &#039;&#039;&#039;SkyFit2&#039;&#039;&#039; to run astrometric and photometric calibrations on GMN data, and it can manually reduce observations of fireballs and compute their trajectories.&lt;br /&gt;
&lt;br /&gt;
A more detailed description of &#039;&#039;&#039;SkyFit2&#039;&#039;&#039; is available on the &#039;&#039;&#039;[[SkyFit2|SkyFit2]]&#039;&#039;&#039; page.&lt;br /&gt;
&lt;br /&gt;
== FAQ ==&lt;br /&gt;
&lt;br /&gt;
=== What should I back up when I re-flash an SD card or a USB disk? ===&lt;br /&gt;
&lt;br /&gt;
You should backup the &#039;&#039;.config&#039;&#039;, platepar, and mask files that are in the RMS source directory, plus the entire content of the hidden directory &#039;&#039;/home/pi/.ssh&#039;&#039;. Refer to the section titled, &#039;&#039;&#039;Back up the configuration&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
If your SD card or USB disk fails or becomes corrupted, you can fetch the config files from the server because they are uploaded every day, together with the data.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The content of &#039;&#039;.ssh&#039;&#039; is essential for connection to the server, so you also must save these files. &lt;br /&gt;
&lt;br /&gt;
After you set up a new SD card or USB disk, return the files to their original location.&lt;br /&gt;
&lt;br /&gt;
=== What are the values in the &#039;&#039;FTPdetectinfo_*&#039;&#039;  file designated as hnr mle bin Pix/fm Rho Phi? ===&lt;br /&gt;
&lt;br /&gt;
Some of these values (hnr mle bin) are not used in RMS but they are used in CAMS, so their presence is to conform to the standard. As a result, these values are all zeros. &lt;br /&gt;
&lt;br /&gt;
There are other values:&lt;br /&gt;
* Pix/fm is the average angular speed of the meteor, in pixels, per frame.&lt;br /&gt;
* Rho, Phi are parameters that define the line of the meteor in polar coordinates, see this &#039;&#039;&#039;[https://en.wikipedia.org/wiki/Hough_transform#Theory page]&#039;&#039;&#039; for more detail. &lt;br /&gt;
: &#039;&#039;Rho&#039;&#039; is the distance of the line from the center of the image.&lt;br /&gt;
: &#039;&#039;Phi&#039;&#039; is the angle of the line, as measured from the positive direction of the Y axis. (Basically, this is a line from the center of the image to the top of the image.) The positive angles are measured clockwise, although the CAMS standard may define these parameters a bit differently, with the Y axis flipped.&lt;br /&gt;
The &#039;&#039;intensity&#039;&#039; is the sum of all pixel intensities of the meteor on a given frame. &lt;br /&gt;
&lt;br /&gt;
For example, you could represent an area around the meteor on a given frame, as shown in the figure, where the numbers are pixel intensities on an 8-bit image (so they can range from 0 to 255) and the pixel values inside the red boundary represent the meteor blob on the frame. The result? The intensity is the sum of all numbers inside the red boundary. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Later, this value is used to compute the magnitude.&lt;br /&gt;
&lt;br /&gt;
[[File:Intensity_sum.png |Intensity_sum.png ]]&lt;br /&gt;
&lt;br /&gt;
The magnitude is computed as&lt;br /&gt;
: &#039;&#039;mag = -2.5*log10(intensity sum) + photometric_offset&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
To estimate the photometric offset in &#039;&#039;&#039;SkyFit&#039;&#039;&#039;, fit the line with slope -2.5 through pairs of known magnitudes of stars and logartihms of their pixel intensity sum. Fundamentally, the photometric offset is the intercept of that line. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The constant slope of -2.5 comes from the &#039;&#039;&#039;[https://en.wikipedia.org/wiki/Apparent_magnitude#Calculations Definition of stellar magnitudes]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== GMN data policy ==&lt;br /&gt;
&lt;br /&gt;
The Global Meteor Network produces three levels of data products.&lt;br /&gt;
* Level 1 - The lowest level data (as close to &#039;raw&#039; as possible) are the FF image and FR video files saved to the RPi by the capture code and the fireball detector.&lt;br /&gt;
* Level 2 - Data is used in three ways:&lt;br /&gt;
:* The meteor detector extracts positional and brightness information of individual meteors (&#039;&#039;FTPdetectinfo&#039;&#039; file). &lt;br /&gt;
:* Images are used for astrometric and photometric calibration (platepar file). &lt;br /&gt;
:* Meteor and star detections are used to generate a range of plots, such as the single-station shower association graph and the camera drift graph. The calibrated meteor measurements are uploaded to the GMN server, together with the raw images of individual meteors.&lt;br /&gt;
* Level 3 - Software on the server correlates individual observations and computes multi-station meteor trajectories, which are published daily on the &#039;&#039;&#039;GMN [https://globalmeteornetwork.org/data/ Data website]&#039;&#039;&#039;. This data is made public under the &#039;&#039;&#039;[https://creativecommons.org/licenses/by/4.0/ CC BY 4.0 license]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
Operators of individual GMN stations exclusively own the Level 1 and Level 2 data their stations produce. In practice, this means they are free to share this data with other meteor networks if they wish. The data that is uploaded to the GMN server is not shared publicly or with other parties without the operator&#039;s consent. However, the data may be used internally by the GMN coordinators to manually produce other data products, such as the trajectory of a meteorite dropping fireball or an analysis of a meteor shower. &lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; All station operators are credited for their data in all GMN publications.&lt;br /&gt;
&lt;br /&gt;
== GMN Plots and Images Explained ==&lt;br /&gt;
&lt;br /&gt;
This document explains the data summaries produced on your system and displayed on the GMN Weblog every morning &#039;&#039;&#039;[https://docs.google.com/document/d/132aHGn0QPzhpVN2s2n6FT6rJn39LAsPkchWJqXQb8Qk/edit?pli=1&amp;amp;tab=t.0 GMN Plots and Images]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;[https://IstraStream.com IstraStream.com]&#039;&#039;&#039; was an independent hosting site primarily intended for cameras sold by IstraStream. In mid-2023, Istrastream stopped listing camera image output and the IstraStream data display was replaced with the &#039;&#039;&#039;[https://globalmeteornetwork.org/weblog/ GMN weblog]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== For more information ==&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?page_id=43 Contact the Global Meteor Network] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://groups.io/g/globalmeteornetwork Join the Global Meteor Network Forum] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://github.com/markmac99/ukmon-pitools/wiki UK Meteor Network Wiki]===&lt;br /&gt;
This wiki has numerous FAQs and tips on maintaining, monitoring and managing your system, and several explainers such as how to calibrate and create a mask, how to copy data and so forth. &lt;br /&gt;
&lt;br /&gt;
=== Important GMN resources ===&lt;br /&gt;
&lt;br /&gt;
There are two additional web pages you should know about.&lt;br /&gt;
&lt;br /&gt;
* The &#039;&#039;&#039;[https://globalmeteornetwork.org/status GMN status page]&#039;&#039;&#039; provides access to the &#039;&#039;&#039;[https://globalmeteornetwork.org/weblog/ GMN weblog]&#039;&#039;&#039;.&lt;br /&gt;
* A mapping utility website that is directly derived from GMN data: &#039;&#039;&#039;[https://tammojan.github.io/meteormap Meteor map]&#039;&#039;&#039;.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; This map takes quite a while to load. When you review the map, you must scroll down to see the full power of the data display.&lt;br /&gt;
&lt;br /&gt;
=== GMN talks ===&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=_tV7WBo0RrQ 2025 GMN Meeting Session 1 (February 2025)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=z23aJeIg7wo 2025 GMN Meeting Session 2 (February 2025)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/playlist?list=PLmQ5Bvz4ACYJLYfswIeAipapoeGeI6QWy GMN talk for Society for Astronomical Sciences workshop 2024 (The first 3 videos)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=juOvRTtoqhs 2024 GMN Meeting Session 1 (February 2024)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=MXhVIxrz2ks 2024 GMN Meeting Session 2 (February 2024)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=IfUyCHjMATc 2023 GMN Meeting Session 1 (February 2023)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=I78KwF5-1GE 2023 GMN Meeting Session 2 (February 2023)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=wDdrG_FCyGk 2022 GMN Meeting Session 1 (February 2022)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=j_75CDPzjI4 2022 GMN Meeting Session 2 (February 2022)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=f6x9_WCVphY GMN talk at the European Space Agency&#039;s Fireball Workshop (June 2021)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=QXBTLPnPDWs 2021 GMN Meeting] - [https://www.dropbox.com/sh/ia9vagug5lxm8k9/AAB_i_1jcWThUdAHO_2gF_Ksa?dl=0 Link to slides]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=MAGq-XqD5Po Overview of the GMN - IMC2020 (September 2020)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=oM7lfQ4nmyw Overview of the GMN, Astro Imaging Channel presentation (May 2020)]&lt;br /&gt;
&lt;br /&gt;
=== GMN-related publications ===&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2206.11365 Vida, D., Blaauw Erskine, R. C., Brown, P. G., Kambulow, J., Campbell-Brown, M., &amp;amp; Mazur, M. J. (2022). Computing optical meteor flux using global meteor network data. Monthly Notices of the Royal Astronomical Society, 515(2), 2322-2339.]&lt;br /&gt;
&lt;br /&gt;
: [https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stab2557/6368869 Moorhead, A. V., Clements, T., &amp;amp; Vida, D. (2021). Meteor shower radiant dispersions in Global Meteor Network data. Monthly Notices of the Royal Astronomical Society, 508(1), 326-339.]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2107.12335 Vida, D., Šegon, D., Gural, P. S., Brown, P. G., McIntyre, M. J., Dijkema, T. J., Pavletić, L., Kukić, P., Mazur, M.J., Eschman, P., Roggemans, P., Merlak, A., &amp;amp; Zubović, D. (2021). The Global Meteor Network–Methodology and first results. Monthly Notices of the Royal Astronomical Society, 506(4), 5046-5074.]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2003.05458/ Moorhead, A. V., Clements, T. D., &amp;amp; Vida, D. (2020). Realistic gravitational focusing of meteoroid streams. Monthly Notices of the Royal Astronomical Society, 494(2), 2982-2994.] &lt;br /&gt;
&lt;br /&gt;
: [https://globalmeteornetwork.org/wordpress/wp-content/uploads/2018/11/Kukic-et-al-2018-Rolling-shutter.pdf  Kukić, P., Gural, P., Vida, D., Šegon, D. &amp;amp; Merlak, A. (2018) Correction for meteor centroids observed using rolling shutter cameras. WGN, Journal of the International Meteor Organization, 46:5, 154-118.]&lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/2018_WGN___RMS_sun_skirter_final.pdf  Vida, D., Mazur, M. J., Šegon, D., Kukić, P., &amp;amp; Merlak, A. (2018). Compressive strength of a skirting Daytime Arietid-first science results from low-cost Raspberry Pi-based meteor stations. WGN, Journal of the International Meteor Organization, 46, 113-118.] &lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/pdf/1911.02979.pdf Vida, D., Gural, P., Brown, P., Campbell-Brown, M., Wiegert, P. (2019) Estimating trajectories of meteors: an observational Monte Carlo approach - I. Theory. arXiv:1911.02979v4 [astro-ph.EP] 21 Apr 2020]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/pdf/1911.11734.pdf Vida, D., Gural, P., Brown, P., Campbell-Brown, M., Wiegert, P. (2019) Estimating trajectories of meteors: an observational Monte Carlo approach - II. Results. arXiv:1911.11734v1 [astro-ph.EP] 26 Novr 2019]&lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/2018_WGN___RMS_first_results-final.pdf Vida, D., Mazur, M. J., Šegon, D., Zubović, D., Kukić, P., Parag, F., &amp;amp; Macan, A. (2018). First results of a Raspberry Pi based meteor camera system. WGN, Journal of the International Meteor Organization, 46, 71-78.] &lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/Vida_IMC2016_proceedings_final.pdf Vida, D., Zubović, D., Šegon, D., Gural, P., &amp;amp; Cupec, R. (2016). Open-source meteor detection software for low-cost single-board computers. In Proceedings of the International Meteor Conference (IMC2016), Egmond, The Netherlands (pp. 2-5).] &lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/Zubovic_IMC2015_priceedings_final.pdf Zubović, D., Vida, D., Gural, P., &amp;amp; Šegon, D. (2015). Advances in the development of a low-cost video meteor station. In Proceedings of the International Meteor Conference, Mistelbach, Austria (pp. 27-30).]&lt;/div&gt;</summary>
		<author><name>MeteorsABQ</name></author>
	</entry>
	<entry>
		<id>https://globalmeteornetwork.org//wiki/index.php?title=Main_Page&amp;diff=847</id>
		<title>Main Page</title>
		<link rel="alternate" type="text/html" href="https://globalmeteornetwork.org//wiki/index.php?title=Main_Page&amp;diff=847"/>
		<updated>2025-10-02T21:05:38Z</updated>

		<summary type="html">&lt;p&gt;MeteorsABQ: /* GMN talks */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Welcome to the Global Meteor Network wiki page!&lt;br /&gt;
&lt;br /&gt;
The Global Meteor Network (GMN) is a world-wide organization of amateur and professional astronomers. The goal is to observe the night sky using low-light video cameras and produce meteor trajectories in a coordinated network of recording stations. Here, you can find information about the purpose and structure of the GMN, and how to assemble and operate your own meteor camera. You also will discover how to contribute to the development of RMS (the GMN software) and how your observations as a citizen scientist contribute to the ongoing understanding of our solar system&#039;s formation and evolution. &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;If you are here to find out how to build and set up a camera from scratch, jump ahead to [https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_-_The_complete_how-to this] section!&amp;lt;/span&amp;gt;&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;For German speakers, there is &amp;quot;Build camera from scratch&amp;quot; documentation written by students of [https://fsg-preetz.de/ Friedrich-Schiller-Gymnasium in Preetz] available [http://wiki.linux-astronomie.de/doku.php?id=ceres here]. This version is maintained by Friedrich-Schiller-Gymnasium in Preetz. &amp;lt;/span&amp;gt;&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Global Meteor Network overview ==&lt;br /&gt;
&lt;br /&gt;
===  [https://globalmeteornetwork.org/?page_id=141 Our mission] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=363 A brief history of the Global Meteor Network] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://www.youtube.com/watch?v=MAGq-XqD5Po Video introduction - Overview of the Global Meteor Network (IMC2020)] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://youtu.be/oM7lfQ4nmyw Video overview - Meteor tracking and the GMN from Astro Imaging Channel presentation] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/data/ Some &#039;live&#039; GMN data products] ===&lt;br /&gt;
&lt;br /&gt;
== Meteor detection station ==&lt;br /&gt;
&lt;br /&gt;
What is an RMS GMN station? An RMS-based GMN station consists of a Raspberry Pi (RPi) single board computer, a low light level security video camera, the RMS software, and a connection to the Internet via Wifi. The camera is securely mounted in a weatherproof housing, pointed at the sky, and connected to the RPi with a Power Over Ethernet (POE) cable. To be a part of the GMN network, you need a fairly powerful Raspberry Pi (Pi 4, 5, or better) and a reasonably fast Internet connection. The internet connection is required only for data upload to a central server each morning and to provide automatic updates for the RMS software. &lt;br /&gt;
&lt;br /&gt;
Nightly, the RPi records video from the camera shortly after local sunset, then continuously compressing and storing the video data on a local SSD drive. Each morning before sunrise, when capture is complete, the RPi analyzes the video and extracts  meteor observations from the previous night. These extracted video clips of detected meteors are archived and then uploaded to a server. On a &#039;busy&#039; night, the clips can total hundreds of megabytes as a result of a heavy meteor shower or a night with a lot of false detections. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Continuous progress is being made on the detection software to filter out false detections. &lt;br /&gt;
&lt;br /&gt;
The server finds meteors that were observed from more than one station, which allows the server to triangulate meteor trails in 3D and calculate the orbits of the meteors.&lt;br /&gt;
&lt;br /&gt;
=== What do I need? ===&lt;br /&gt;
&lt;br /&gt;
You need a Raspberry Pi compluter, RMS software, and a camera kit. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; We strongly recommend the Pi 4 or 5 model. &lt;br /&gt;
The software can run on a Pi3, but it is much slower and it is no longer supported. A list with everything you need is available here: [https://globalmeteornetwork.org/wiki/index.php?title=Shopping_list_and_tools_needed page].&lt;br /&gt;
&lt;br /&gt;
You can run multiple cameras on a Linux PC, and details are available &#039;&#039;&#039;[https://docs.google.com/document/d/16PSFi8RAqbenPdluhulCRaIenOkEzgs5piUhkX3yaOc/edit here]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== How do I obtain a camera? ===&lt;br /&gt;
There are two options - buy a camera or build a camera.&lt;br /&gt;
&lt;br /&gt;
==== Buy a Camera ====&lt;br /&gt;
You can buy a camera and prebuilt Pi, and ready to install. Cameras are available from several suppliers, as well as the Croatian Meteor Network, as explained here: [https://globalmeteornetwork.org/?page_id=136 this page]. &lt;br /&gt;
If you are in the UK, you can contact the UK Meteor network for advice. [https://ukmeteornetwork.org/ UK Meteor Network].&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; As of 2024, UK Meteor network can no longer sell cameras directly.&lt;br /&gt;
&lt;br /&gt;
==== Build your own from scratch ====&lt;br /&gt;
This option requires an intermediate level of DIY skills and familiarity with the Raspberry Pi, but do not be put off. The instructions are comprehensive and, if you get stuck, you can ask for advice in the forum here: &#039;&#039;&#039;[https://groups.io/g/globalmeteornetwork groups.io]&#039;&#039;&#039; forum.&lt;br /&gt;
&lt;br /&gt;
You can find out more about this option here: &#039;&#039;&#039;[[Build &amp;amp; Install &amp;amp; Setup your camera - The complete how-to]]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== Advanced RMS installations and multi-camera support ===&lt;br /&gt;
If you would like to explore advanced RMS installation options for various platforms or run multiple cameras on a single Linux computer, complete information is available on &#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Advanced_RMS_installations_and_Multi-camera_support this page]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
If you plan to run RMS software on the Raspberry Pi 4 or 5, the best supported and easiest solution is our prepared image. Complete information is available in an &#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_- Extensive how-to guide]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== Can I use a commercial all-sky camera? ===&lt;br /&gt;
&lt;br /&gt;
Generally, this is not a good idea because these cameras lack sufficient sensitivity. More information is available here: &#039;&#039;&#039;[https://globalmeteornetwork.org/?p=163 See this recent experiment]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Operate and maintain your GMN station ==&lt;br /&gt;
&lt;br /&gt;
=== Overview ===&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; GMS is a nascent operation, so you may share some of our growing pains if you choose to be involved. We are constantly solving bugs and making improvements, which is an opportunity for you to help if you have programming skills! The workload of day-to-day operation can be non-zero, and may require some of your time.&lt;br /&gt;
&lt;br /&gt;
Ideally, you should monitor your RMS Pi systems daily to identify freezes, glitches, or other problems. For example, you may see birds nesting or soiling the camera window, someone may unintentionally unplug the power cord, or animals (mice, cats, or dogs) may chew on the camera Ethernet cable. Although we make constant progress, the GMS network is not yet a &#039;power up and forget about it&#039; system. &lt;br /&gt;
&lt;br /&gt;
By its nature, the GMS network is staffed by lots of people who are willing to help newcomers get started. Here are some suggestions for daily operation of your RMS camera.&lt;br /&gt;
&lt;br /&gt;
=== What does the meteor camera do over the course of 24 hours? ===&lt;br /&gt;
&lt;br /&gt;
The RMS python-based system calculates the sundown to sunrise interval, and schedules video camera capture all night. Based on the video camera and capabilities of the Pi, the camera captures at least 25 frames per second between evening and morning twilight. During each nightly continuous image capture, the station processes captured image data and idenitfies frames that contain a minimum number of stars (usually around 20) that are worth reviewing for meteor detections. When data capture is complete, the station begins processing all frames it flagged with possible detections, then refines the astrometric accuracy of every positive detection. Using the station plate parameters (platepar) calibration file, processing iterates to find the best astrometry and photometry solution for each detected meteor. After this process analyzes each detection, summary files are created. &lt;br /&gt;
&lt;br /&gt;
The summary files include many types of information.&lt;br /&gt;
* Text file data presentation in several widely accepted formats (such as &#039;&#039;CAMS&#039;&#039; and &#039;&#039;UFOorbit&#039;&#039;).&lt;br /&gt;
* Graphic plots of detection frequencies throughout the night.&lt;br /&gt;
* Plot of all detections, showing any identified radiants.&lt;br /&gt;
* Plots of photometry, astrometry, and camera pointing drift in arc minutes throughout the course of the night as the mount or building flexes.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039;  Detailed information about plots is available here: &#039;&#039;&#039;[https://docs.google.com/document/d/132aHGn0QPzhpVN2s2n6FT6rJn39LAsPkchWJqXQb8Qk/edit?usp=sharing Explanation of GMN plots]&#039;&#039;&#039;&lt;br /&gt;
* Thumbnail images of detections.&lt;br /&gt;
* Thumbnail images of data captured throughout the night.&lt;br /&gt;
* Single image with all detections stacked together.&lt;br /&gt;
* Single image with all captured images stacked together.&lt;br /&gt;
* Flat file for correcting images.&lt;br /&gt;
* An &#039;&#039;.mp4&#039;&#039; movie time lapse of the night&#039;s captured images.&lt;br /&gt;
* Meteor shower flux charts, if specific showers are detected.&lt;br /&gt;
* Observation summary data of hardware and data recording characteristics.&lt;br /&gt;
 &lt;br /&gt;
When you click a meteor track, its data displays in the lower data window. Ultimately, all results are combined into a single compressed archive that automatically uploads each morning to the central server. &lt;br /&gt;
&lt;br /&gt;
Each morning, you can review the result files on the RPi and copy anything you want to your computer or tablet.&lt;br /&gt;
&lt;br /&gt;
===Archive data ===&lt;br /&gt;
&lt;br /&gt;
Your primary scientific data is automatically uploaded to the central server every morning after data processing is complete. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; When the night&#039;s results are uploaded, RMS purges the oldest data to free up space for the next night&#039;s run. As a result, you may want to copy some of the data to a PC, NAS, or the cloud for further analysis.&lt;br /&gt;
:       You should consider backing up the content of &#039;&#039;&#039;~/RMS_data/ArchivedFiles&#039;&#039;&#039;, which holds individual files and data that RMS determined were probably meteors. &lt;br /&gt;
&lt;br /&gt;
Details about backing up data is beyond the scope of the GMN Wiki. Tools such as Robocopy for Windows and rsync for Linux/MacOS are ideal, and they can &#039;mirror&#039; data across a network. Help to configure these tools is available in the &#039;&#039;&#039;Globalmeteornetwork&#039;&#039;&#039; group on &#039;&#039;&#039;groups.io&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
In addition, we added some automated tools that can help you back up data to a thumb drive inserted into the RPi. Assistance about these tools also is available in the &#039;&#039;&#039;Globalmeteornetwork&#039;&#039;&#039; group on &#039;&#039;&#039;groups.io&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
===Backup and restore the configuration and RSA keys===&lt;br /&gt;
&lt;br /&gt;
:&#039;&#039;&#039;NOTE:&#039;&#039;&#039; If you are on an older Buster image, you must replace username &#039;&#039;rms&#039;&#039; with username &#039;&#039;pi&#039;&#039;. For example, enter &#039;&#039;/home/pi&#039;&#039; instead of &#039;&#039;/home/rms&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
To determine which username to use, run &lt;br /&gt;
::&#039;&#039;ls /home/rms home/pi&#039;&#039;&lt;br /&gt;
to display the username that is your home directory.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Back up the configuration&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
1. Open a terminal and run the command  &#039;&#039;Scripts/RMS_Backup.sh&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
: A compressed &#039;&#039;.zip&#039;&#039; file, with all important configuration files and keys, is created in your user home directory with the prefix &#039;&#039;RMS_Backup&#039;&#039; and the &#039;&#039;.zip&#039;&#039; extension. &lt;br /&gt;
: For example, &#039;&#039;/home/rms/RMS_Backup_XX0001_2023-01-28.zip&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
2. Copy the &#039;&#039;.zip&#039;&#039; file to a safe place outside RPi. &lt;br /&gt;
&lt;br /&gt;
: Later, it will be useful to restore the system in case of failure. The &#039;&#039;.zip&#039;&#039; file contains the RSA public and private keys used to contact GMN servers, so keep it secret.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Restore the configuration&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
1. Unzip the backup file in any folder on the RPi.&lt;br /&gt;
&lt;br /&gt;
2. Copy the files &#039;&#039;.config&#039;&#039;, &#039;&#039;platepar_cmn2010.cal&#039;&#039;, and &#039;&#039;mask.bmp&#039;&#039; to the folder &#039;&#039;/home/rms/source/RMS/&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
3. Copy the files &#039;&#039;id_rsa&#039;&#039; and &#039;&#039;id_rsa.pub&#039;&#039; to the folder &#039;&#039;/home/rms/.ssh/&#039;&#039;, as shown in this example:&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;cp .config platepar_cmn2010.cal mask.bmp /home/rms/source/RMS/&#039;&#039;&lt;br /&gt;
: &#039;&#039;cp id_rsa id_rsa.pub /home/rms/.ssh/&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
4. To make sure that permission bits in the RSA key files are correct, enter:&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;chmod 400 ~/.ssh/id_rsa*&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== View the data ===&lt;br /&gt;
&lt;br /&gt;
To view data, you can use &#039;&#039;&#039;CMN_binViewer&#039;&#039;&#039; software [https://github.com/CroatianMeteorNetwork/cmn_binviewer], which is included in the RMS SD image. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; There also is a Windows version [https://github.com/CroatianMeteorNetwork/cmn_binviewer/releases] you can install.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; You can open images in astronomical FITS viewers, such as &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039; or &#039;&#039;&#039;Pixinsight&#039;&#039;&#039;, but what you see may be surprising. For example, in &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039;, the image is upside down, which is an artefact of how the software reads the image. &lt;br /&gt;
&lt;br /&gt;
In space, there is no &#039;up&#039; or &#039;down&#039;, so the FITS specification does not dictate if pixel (0,0) is at a specific corner. Some software, notably &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039;, specifies the top left corner as the origin location, which causes terrestrial images  to display vertically mirrored.&lt;br /&gt;
&lt;br /&gt;
=== Tools and utilities ===&lt;br /&gt;
&lt;br /&gt;
There are many tools available.&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;&#039;[https://www.realvnc.com/en/connect/download/viewer/ RealVNC]&#039;&#039;&#039;, &#039;&#039;&#039;[https://www.nomachine.com/ NoMachine]&#039;&#039;&#039;, &#039;&#039;&#039;[https://anydesk.com/en AnyDesk]&#039;&#039;&#039;, or &#039;&#039;&#039;[https://rustdesk.com/ RustDesk]&#039;&#039;&#039; remote connect tools provide station access from anywhere. Access to your station from outside your network is enabled by an OpenVPN connection address that is available to meteor stations.&lt;br /&gt;
: With &#039;&#039;&#039;VNC&#039;&#039;&#039; and &#039;&#039;&#039;Teamviewer&#039;&#039;&#039;, you can create an account and team on their websites, and then remotely access your station. &lt;br /&gt;
* &#039;&#039;&#039;Samba&#039;&#039;&#039; data directory access allows you to copy data results directly from your RPi to your computer or tablet.&lt;br /&gt;
* &#039;&#039;&#039;[https://github.com/CroatianMeteorNetwork/cmn_binviewer CMN_binViewer]&#039;&#039;&#039; allows you to view standard FITS image files that contain meteor detections. It runs on the RPi, and it can run under Windows.&lt;br /&gt;
* &#039;&#039;&#039;[https://sonotaco.com/soft/e_index.html UFO Orbit]&#039;&#039;&#039; allows you to process data from multiple stations, and generate unified radiants of two or more stations that see the same meteor. &#039;&#039;&#039;[https://sonotaco.com/soft/e_index.html UFO Orbit]&#039;&#039;&#039; can plot the shared object ground path and orbital characteristics, and it can output a summary file of all objects seen by more than one station.&lt;br /&gt;
* RMS software can be installed under Windows to allow much of the RMS python-based code to run on your computer. This means you can run RMS against meteor station data that was transferred to your computer from the RPi.&lt;br /&gt;
&lt;br /&gt;
You also can run RMS python jobs on the RPi to sample captured image files, and then condense them into an &#039;&#039;.mp4&#039;&#039; video. Sometimes, these videos are mesmerizing summaries that can run for more than two minutes of winter time data.&lt;br /&gt;
&lt;br /&gt;
== What can I do with my GMN station? ==&lt;br /&gt;
&lt;br /&gt;
=== Use SkyFit2 for astrometric and photometric calibration + Manually reduce observations of fireballs and compute their trajectories ===&lt;br /&gt;
* &#039;&#039;&#039;[https://www.youtube.com/watch?v=ao3J9Jf0iLQ Updated 2023 video tutorial]&#039;&#039;&#039;&lt;br /&gt;
* &#039;&#039;&#039;[https://www.youtube.com/watch?v=MOjb3qxDlX4 Old 2021 video tutorial]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/fov3d/ Generate a Google Earth KML file to show your station&#039;s field of view] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=253 Use the UFO Orbit program to estimate meteor trajectories] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=221 Urban meteor observing] ===&lt;br /&gt;
&lt;br /&gt;
== Data analysis with SkyFit2 ==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SkyFit2&#039;&#039;&#039;, a program in the RMS library, allows you to analyze optical meteor data in most of the optical formats in current use. The program supports popular video formats (&#039;&#039;.mp4&#039;&#039;, &#039;&#039;.avi&#039;&#039;, and &#039;&#039;.mkv&#039;&#039;), sequences of static images, and single images with shutter breaks.&lt;br /&gt;
&lt;br /&gt;
A &#039;&#039;&#039;[https://www.youtube.com/watch?v=ao3J9Jf0iLQ video tutorial]&#039;&#039;&#039; explains how to useg &#039;&#039;&#039;SkyFit2&#039;&#039;&#039; to run astrometric and photometric calibrations on GMN data, and it can manually reduce observations of fireballs and compute their trajectories.&lt;br /&gt;
&lt;br /&gt;
A more detailed description of &#039;&#039;&#039;SkyFit2&#039;&#039;&#039; is available on the &#039;&#039;&#039;[[SkyFit2|SkyFit2]]&#039;&#039;&#039; page.&lt;br /&gt;
&lt;br /&gt;
== FAQ ==&lt;br /&gt;
&lt;br /&gt;
=== What should I back up when I re-flash an SD card or a USB disk? ===&lt;br /&gt;
&lt;br /&gt;
You should backup the &#039;&#039;.config&#039;&#039;, platepar, and mask files that are in the RMS source directory, plus the entire content of the hidden directory &#039;&#039;/home/pi/.ssh&#039;&#039;. Refer to the section titled, &#039;&#039;&#039;Back up the configuration&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
If your SD card or USB disk fails or becomes corrupted, you can fetch the config files from the server because they are uploaded every day, together with the data.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The content of &#039;&#039;.ssh&#039;&#039; is essential for connection to the server, so you also must save these files. &lt;br /&gt;
&lt;br /&gt;
After you set up a new SD card or USB disk, return the files to their original location.&lt;br /&gt;
&lt;br /&gt;
=== What are the values in the &#039;&#039;FTPdetectinfo_*&#039;&#039;  file designated as hnr mle bin Pix/fm Rho Phi? ===&lt;br /&gt;
&lt;br /&gt;
Some of these values (hnr mle bin) are not used in RMS but they are used in CAMS, so their presence is to conform to the standard. As a result, these values are all zeros. &lt;br /&gt;
&lt;br /&gt;
There are other values:&lt;br /&gt;
* Pix/fm is the average angular speed of the meteor, in pixels, per frame.&lt;br /&gt;
* Rho, Phi are parameters that define the line of the meteor in polar coordinates, see this &#039;&#039;&#039;[https://en.wikipedia.org/wiki/Hough_transform#Theory page]&#039;&#039;&#039; for more detail. &lt;br /&gt;
: &#039;&#039;Rho&#039;&#039; is the distance of the line from the center of the image.&lt;br /&gt;
: &#039;&#039;Phi&#039;&#039; is the angle of the line, as measured from the positive direction of the Y axis. (Basically, this is a line from the center of the image to the top of the image.) The positive angles are measured clockwise, although the CAMS standard may define these parameters a bit differently, with the Y axis flipped.&lt;br /&gt;
The &#039;&#039;intensity&#039;&#039; is the sum of all pixel intensities of the meteor on a given frame. &lt;br /&gt;
&lt;br /&gt;
For example, you could represent an area around the meteor on a given frame, as shown in the figure, where the numbers are pixel intensities on an 8-bit image (so they can range from 0 to 255) and the pixel values inside the red boundary represent the meteor blob on the frame. The result? The intensity is the sum of all numbers inside the red boundary. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Later, this value is used to compute the magnitude.&lt;br /&gt;
&lt;br /&gt;
[[File:Intensity_sum.png |Intensity_sum.png ]]&lt;br /&gt;
&lt;br /&gt;
The magnitude is computed as&lt;br /&gt;
: &#039;&#039;mag = -2.5*log10(intensity sum) + photometric_offset&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
To estimate the photometric offset in &#039;&#039;&#039;SkyFit&#039;&#039;&#039;, fit the line with slope -2.5 through pairs of known magnitudes of stars and logartihms of their pixel intensity sum. Fundamentally, the photometric offset is the intercept of that line. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The constant slope of -2.5 comes from the &#039;&#039;&#039;[https://en.wikipedia.org/wiki/Apparent_magnitude#Calculations Definition of stellar magnitudes]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== GMN data policy ==&lt;br /&gt;
&lt;br /&gt;
The Global Meteor Network produces three levels of data products.&lt;br /&gt;
* Level 1 - The lowest level data (as close to &#039;raw&#039; as possible) are the FF image and FR video files saved to the RPi by the capture code and the fireball detector.&lt;br /&gt;
* Level 2 - Data is used in three ways:&lt;br /&gt;
:* The meteor detector extracts positional and brightness information of individual meteors (&#039;&#039;FTPdetectinfo&#039;&#039; file). &lt;br /&gt;
:* Images are used for astrometric and photometric calibration (platepar file). &lt;br /&gt;
:* Meteor and star detections are used to generate a range of plots, such as the single-station shower association graph and the camera drift graph. The calibrated meteor measurements are uploaded to the GMN server, together with the raw images of individual meteors.&lt;br /&gt;
* Level 3 - Software on the server correlates individual observations and computes multi-station meteor trajectories, which are published daily on the &#039;&#039;&#039;GMN [https://globalmeteornetwork.org/data/ Data website]&#039;&#039;&#039;. This data is made public under the &#039;&#039;&#039;[https://creativecommons.org/licenses/by/4.0/ CC BY 4.0 license]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
Operators of individual GMN stations exclusively own the Level 1 and Level 2 data their stations produce. In practice, this means they are free to share this data with other meteor networks if they wish. The data that is uploaded to the GMN server is not shared publicly or with other parties without the operator&#039;s consent. However, the data may be used internally by the GMN coordinators to manually produce other data products, such as the trajectory of a meteorite dropping fireball or an analysis of a meteor shower. &lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; All station operators are credited for their data in all GMN publications.&lt;br /&gt;
&lt;br /&gt;
== GMN Plots and Images Explained ==&lt;br /&gt;
&lt;br /&gt;
This document explains the data summaries produced on your system and displayed on the GMN Weblog every morning &#039;&#039;&#039;[https://docs.google.com/document/d/132aHGn0QPzhpVN2s2n6FT6rJn39LAsPkchWJqXQb8Qk/edit?pli=1&amp;amp;tab=t.0 GMN Plots and Images]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;[https://IstraStream.com IstraStream.com]&#039;&#039;&#039; was an independent hosting site primarily intended for cameras sold by IstraStream. In mid-2023, Istrastream stopped listing camera image output and the IstraStream data display was replaced with the &#039;&#039;&#039;[https://globalmeteornetwork.org/weblog/ GMN weblog]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== For more information ==&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?page_id=43 Contact the Global Meteor Network] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://groups.io/g/globalmeteornetwork Join the Global Meteor Network Forum] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://github.com/markmac99/ukmon-pitools/wiki UK Meteor Network Wiki]===&lt;br /&gt;
This wiki has numerous FAQs and tips on maintaining, monitoring and managing your system, and several explainers such as how to calibrate and create a mask, how to copy data and so forth. &lt;br /&gt;
&lt;br /&gt;
=== Important GMN resources ===&lt;br /&gt;
&lt;br /&gt;
There are two additional web pages you should know about.&lt;br /&gt;
&lt;br /&gt;
* The &#039;&#039;&#039;[https://globalmeteornetwork.org/status GMN status page]&#039;&#039;&#039; provides access to the &#039;&#039;&#039;[https://globalmeteornetwork.org/weblog/ GMN weblog]&#039;&#039;&#039;.&lt;br /&gt;
* A mapping utility website that is directly derived from GMN data: &#039;&#039;&#039;[https://tammojan.github.io/meteormap Meteor map]&#039;&#039;&#039;.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; This map takes quite a while to load. When you review the map, you must scroll down to see the full power of the data display.&lt;br /&gt;
&lt;br /&gt;
=== GMN talks ===&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/playlist?list=PLmQ5Bvz4ACYJLYfswIeAipapoeGeI6QWy GMN talk for Society for Astronomical Sciences workshop 2024 (The first 3 videos)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=_tV7WBo0RrQ 2025 GMN Meeting Session 1 (February 2025)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=z23aJeIg7wo 2025 GMN Meeting Session 2 (February 2025)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=juOvRTtoqhs 2024 GMN Meeting Session 1 (February 2024)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=MXhVIxrz2ks 2024 GMN Meeting Session 2 (February 2024)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=IfUyCHjMATc 2023 GMN Meeting Session 1 (February 2023)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=I78KwF5-1GE 2023 GMN Meeting Session 2 (February 2023)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=wDdrG_FCyGk 2022 GMN Meeting Session 1 (February 2022)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=j_75CDPzjI4 2022 GMN Meeting Session 2 (February 2022)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=f6x9_WCVphY GMN talk at the European Space Agency&#039;s Fireball Workshop (June 2021)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=QXBTLPnPDWs 2021 GMN Meeting] - [https://www.dropbox.com/sh/ia9vagug5lxm8k9/AAB_i_1jcWThUdAHO_2gF_Ksa?dl=0 Link to slides]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=MAGq-XqD5Po Overview of the GMN - IMC2020 (September 2020)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=oM7lfQ4nmyw Overview of the GMN, Astro Imaging Channel presentation (May 2020)]&lt;br /&gt;
&lt;br /&gt;
=== GMN-related publications ===&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2206.11365 Vida, D., Blaauw Erskine, R. C., Brown, P. G., Kambulow, J., Campbell-Brown, M., &amp;amp; Mazur, M. J. (2022). Computing optical meteor flux using global meteor network data. Monthly Notices of the Royal Astronomical Society, 515(2), 2322-2339.]&lt;br /&gt;
&lt;br /&gt;
: [https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stab2557/6368869 Moorhead, A. V., Clements, T., &amp;amp; Vida, D. (2021). Meteor shower radiant dispersions in Global Meteor Network data. Monthly Notices of the Royal Astronomical Society, 508(1), 326-339.]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2107.12335 Vida, D., Šegon, D., Gural, P. S., Brown, P. G., McIntyre, M. J., Dijkema, T. J., Pavletić, L., Kukić, P., Mazur, M.J., Eschman, P., Roggemans, P., Merlak, A., &amp;amp; Zubović, D. (2021). The Global Meteor Network–Methodology and first results. Monthly Notices of the Royal Astronomical Society, 506(4), 5046-5074.]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2003.05458/ Moorhead, A. V., Clements, T. D., &amp;amp; Vida, D. (2020). Realistic gravitational focusing of meteoroid streams. Monthly Notices of the Royal Astronomical Society, 494(2), 2982-2994.] &lt;br /&gt;
&lt;br /&gt;
: [https://globalmeteornetwork.org/wordpress/wp-content/uploads/2018/11/Kukic-et-al-2018-Rolling-shutter.pdf  Kukić, P., Gural, P., Vida, D., Šegon, D. &amp;amp; Merlak, A. (2018) Correction for meteor centroids observed using rolling shutter cameras. WGN, Journal of the International Meteor Organization, 46:5, 154-118.]&lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/2018_WGN___RMS_sun_skirter_final.pdf  Vida, D., Mazur, M. J., Šegon, D., Kukić, P., &amp;amp; Merlak, A. (2018). Compressive strength of a skirting Daytime Arietid-first science results from low-cost Raspberry Pi-based meteor stations. WGN, Journal of the International Meteor Organization, 46, 113-118.] &lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/pdf/1911.02979.pdf Vida, D., Gural, P., Brown, P., Campbell-Brown, M., Wiegert, P. (2019) Estimating trajectories of meteors: an observational Monte Carlo approach - I. Theory. arXiv:1911.02979v4 [astro-ph.EP] 21 Apr 2020]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/pdf/1911.11734.pdf Vida, D., Gural, P., Brown, P., Campbell-Brown, M., Wiegert, P. (2019) Estimating trajectories of meteors: an observational Monte Carlo approach - II. Results. arXiv:1911.11734v1 [astro-ph.EP] 26 Novr 2019]&lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/2018_WGN___RMS_first_results-final.pdf Vida, D., Mazur, M. J., Šegon, D., Zubović, D., Kukić, P., Parag, F., &amp;amp; Macan, A. (2018). First results of a Raspberry Pi based meteor camera system. WGN, Journal of the International Meteor Organization, 46, 71-78.] &lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/Vida_IMC2016_proceedings_final.pdf Vida, D., Zubović, D., Šegon, D., Gural, P., &amp;amp; Cupec, R. (2016). Open-source meteor detection software for low-cost single-board computers. In Proceedings of the International Meteor Conference (IMC2016), Egmond, The Netherlands (pp. 2-5).] &lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/Zubovic_IMC2015_priceedings_final.pdf Zubović, D., Vida, D., Gural, P., &amp;amp; Šegon, D. (2015). Advances in the development of a low-cost video meteor station. In Proceedings of the International Meteor Conference, Mistelbach, Austria (pp. 27-30).]&lt;/div&gt;</summary>
		<author><name>MeteorsABQ</name></author>
	</entry>
	<entry>
		<id>https://globalmeteornetwork.org//wiki/index.php?title=Shopping_list_and_tools_needed&amp;diff=846</id>
		<title>Shopping list and tools needed</title>
		<link rel="alternate" type="text/html" href="https://globalmeteornetwork.org//wiki/index.php?title=Shopping_list_and_tools_needed&amp;diff=846"/>
		<updated>2025-10-01T16:29:58Z</updated>

		<summary type="html">&lt;p&gt;MeteorsABQ: /* Cooled housing for Raspberry Pi */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Ordering the correct components is the most important aspect of your camera build. Review the entire list and make sure you order the correct options. If you are not sure, posta question in the forums. You also should review the list of tools to identify what may be missing. &lt;br /&gt;
&lt;br /&gt;
= Parts and tools = &lt;br /&gt;
[[File:01_annotated.jpg|thumb|right|Annotated Parts List]]&lt;br /&gt;
&lt;br /&gt;
Click the image to the right to see a larger version of the parts and tools.&lt;br /&gt;
&lt;br /&gt;
# IMX291 sensor board (IMX307 sensor board if IMX291 sensor board is sold out)&lt;br /&gt;
# Lens with the lens holder - 4mm, 6mm are M16 mount as pictured, while other lenses might be CS which have a different holder&lt;br /&gt;
# 2x M2 screws, 6mm long - for mounting lens holder &lt;br /&gt;
# Camera housing&lt;br /&gt;
# Small cable gland (supplied with the housing)&lt;br /&gt;
# Large cable gland (supplied with the housing)&lt;br /&gt;
# Camera Power over Ethernet (PoE) cable (sometimes called a network cable by the sellers)&lt;br /&gt;
# Camera board holder (supplied with the housing)&lt;br /&gt;
# Holder metal plate (supplied with the housing)&lt;br /&gt;
# 4x M2 screws, 12 mm long for mounting camera module to bracket&lt;br /&gt;
# 1x M3-.50 screw, 6mm long for mounting camera module L-bracket to base plate&lt;br /&gt;
# Metal plate screws (supplied with the housing)&lt;br /&gt;
# Transparent weatherproof silicone &lt;br /&gt;
# Housing mounting bracket (supplied with the housing)&lt;br /&gt;
# Waterproof ethernet cable protector&lt;br /&gt;
# PoE injector to supply 48v to the camera (not shown)&lt;br /&gt;
# Raspberry Pi 5 (recommended) or Raspberry Pi 4 Model B 2GB (minimum) with official power supply (not shown)&lt;br /&gt;
# Raspberry Pi housing (not shown)&lt;br /&gt;
# 128 GB or greater microSD card (not shown)&lt;br /&gt;
# Self-amalgamating tape (not shown)&lt;br /&gt;
&lt;br /&gt;
= Purchasing parts =&lt;br /&gt;
For consistency across the network and to facilitate collaborative support, it is best to use only the camera and lens listed below, instead of assembling alternatives only because they are conveniently available. The selected camera and lenses are proven and known to work well. Feel free to source other components from any convenient seller. &lt;br /&gt;
&lt;br /&gt;
Many components, such as the Pi and microSD cards, are are available from many vendors. However, AliExpress (the Chinese equivalent of eBay) is the preferred online source for a lens, camera, and housing. AliExpress serves most of the globe and has been reliably suppling parts for a long time.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Links are to current sellers but inventory levels can vary. If a link is dead or the seller is out of stock, you should be able to find an equivalent from other sellers on AliExpress.&lt;br /&gt;
&lt;br /&gt;
== Sensor ==&lt;br /&gt;
The bare IP security camera selected for the RMS system features a Sony IMX291, available from many sellers on AliExpress. Of the options offered, choose &#039;&#039;With 48V POE cable&#039;&#039; and &#039;&#039;No lens&#039;&#039;.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002315913099.html IMX-291 Hi3516Cv300]&lt;br /&gt;
&lt;br /&gt;
If the IMX-291 camera is sold out from that vendor and you cannot find another IMX-291 vendor, you may be able to locate a suitable IMX-307 sensor.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Many vendors sell IMX-307 sensor boards that are not suited for nighttime meteor recording. It is important to buy the correct IMX-307 because only a specific hardware version combined with a specific firmware version work correctly to record meteors.  &lt;br /&gt;
&lt;br /&gt;
One RMS/GMN tester offered these thoughts:&lt;br /&gt;
 &lt;br /&gt;
* The only IMX-307 worth trying is the Hangzhou Jiefeng Technology GK7205V210, aka IVG-G3S, which is distinguishable by a white square on the board. I do not recommend a blanket ‘get-any-IMX-307’ statement for new cameras because sensor boards can be very different from each other. &lt;br /&gt;
&lt;br /&gt;
* The only acceptable IMX-307 sensor boards I&#039;ve found includes the firmware version:&lt;br /&gt;
: V5.00.R02.000739AG.10010.140400.00&#039;&#039;&#039;20000&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
* A firmware version with a similar number is NOT acceptable: &lt;br /&gt;
: V5.00.R02.000739AG.10010.140400.00&#039;&#039;&#039;20010&#039;&#039;&#039;.&lt;br /&gt;
 &lt;br /&gt;
* Here is a link to Hangzhou Jiefeng Technology: [https://www.aliexpress.us/item/3256805867050500.html Hangzhou Jiefeng Technology].&lt;br /&gt;
 &lt;br /&gt;
* When you place an order, it is best to specify the characteristics of the IMX-307. For example, your request could be something like this:&lt;br /&gt;
: &#039;&#039;GK7205V210 (IVG-G3S), with white square on circuit board, and firmware version V5.00.R02.000739AG.10010.140400.0020000&#039;&#039;.&lt;br /&gt;
 &lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; These recommendations are likely to change over time, so you should check our parts list and vendor recommendations before you place an order.&lt;br /&gt;
&lt;br /&gt;
== Lens ==&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; Buy a lens separately and select only from these options.&lt;br /&gt;
&lt;br /&gt;
Most cameras available on AliExpress are sold with a choice of lenses. The preferred lens is a 4mm f/0.95 M16 lens, which provides a ~88x45° field of view (FOV). The lens also is available separately at this link.&lt;br /&gt;
: [https://www.aliexpress.com/item/32876034491.html 4mm f/0.95 M16].&lt;br /&gt;
&lt;br /&gt;
Alternative lenses (4mm and 6 mm) are available here:&lt;br /&gt;
: [https://www.aliexpress.com/item/1005003145991079.html 4mm OR 6mm f/0.95 M16]&lt;br /&gt;
&lt;br /&gt;
If you live in an area with heavy light pollution, other options are available. We recommend using only lenses from the [[Lens Options|following list]]. Other options may not be as sensitive or may have significant distortions. See [[Lens Options|this page for more lens options]].&lt;br /&gt;
&lt;br /&gt;
== Housing ==&lt;br /&gt;
A security camera housing provides weather-tight protection without the distortion of a plastic dome. From the options offered, select &#039;&#039;Plate and Bracket&#039;&#039;. The plate holds a 38x38mm bare IP camera module on an L-shaped mounting bracket. &lt;br /&gt;
: [https://www.aliexpress.com/item/32355130687.html IP66 CCTV Camera Housing with Plate and Bracket] &lt;br /&gt;
&lt;br /&gt;
This combination also provides a pair of cable glands and some essential screws.&lt;br /&gt;
&lt;br /&gt;
== Power over Ethernet (PoE) injector, PoE switch (optional), and PoE replacement camera side cables (optional, but recommended) ==&lt;br /&gt;
&lt;br /&gt;
This combination uses network cables to connect the Raspberry Pi and the camera sensor, and injects 48V DC into the network cable to power the camera. From the list, select a plug style that is appropriate for your location. &lt;br /&gt;
&lt;br /&gt;
This is an example of plug styles available.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002704227705.html PoE Injector 48V 0.5A]&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Over short cable lengths (up to about 5m), you also can use plain PoE connectors. These connectors feed 12V from a power supply into the ethernet and extract it at the other end. Over short distances, this configuration can supply the camera with adequate power without the need for 48V injectors.&lt;br /&gt;
&lt;br /&gt;
If you operate several cameras, you can use a PoE &#039;&#039;switch&#039;&#039; instead of a PoE &#039;&#039;injector&#039;&#039;, and connect all the cameras to your network. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; You must source a PoE switch locally.&lt;br /&gt;
: [https://www.tendacn.com/product/tef1110p-8-63w.html TEF1110P-8-63W 10-Port 10/100M Desktop Switch with 8-Port PoE]&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;GOOD PRACTICE:&#039;&#039;&#039; Maintain one or more spare PoE camera side cables.&lt;br /&gt;
: [https://www.aliexpress.com/item/4001297174234.html Poe cable - Select RJ45 or RJ45DC]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Alternative cable&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The picture shows only two connectors, but you will receive all connectors needed for the IMX291 board:&lt;br /&gt;
* 1 pcs 2pin port (2.0mm)&lt;br /&gt;
* 1 pcs 4pin port (1.25mm)&lt;br /&gt;
* 1 pcs 6pin port (1.25mm)&lt;br /&gt;
* 1 pcs 8pin port (1.25mm))&lt;br /&gt;
&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002598310068.html Poe Cable]&lt;br /&gt;
&lt;br /&gt;
== Cooled housing for Raspberry Pi ==&lt;br /&gt;
&lt;br /&gt;
Please buy one of the two cases below. We have tried many others, but they are not as good.&lt;br /&gt;
&lt;br /&gt;
* [https://www.aliexpress.com/item/32959825297.html Fan-cooled case.] It has relatively quiet fans, and it&#039;s sturdy. From the options offered, ensure you select one that says &amp;quot;for Pi 4&amp;quot; if you are using a Raspberry Pi 4, or &amp;quot;for Pi 5&amp;quot; if you are using a Raspberry Pi 5. &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; There is a case variation that is fully enclosed and has no fans; do not select this option.&lt;br /&gt;
&lt;br /&gt;
* [https://www.aliexpress.com/item/1005002510605065.html Passively cooled case.] It is silent, with no fan to replace in future. Many operators have found this one satisfactory if the Pi is operated in moderate room temperatures with ample air circulation around the Pi. Some operators report diminished WiFi strength with passive fanless cases because metal heat sinks may interfere with the small antenna.&lt;br /&gt;
&lt;br /&gt;
If the Pi is in a hot environment, then choose the case with the fan. If silent operation is the priority, then go fanless but pay attention to the free circulation of air around the Pi. Case fans often use cheap sleeve bearings. If they get noisy or stop spinning later, try replacing them with a fan that uses ball bearings. Thermostatically controlled fans like the &#039;Pimaroni Fanshim&#039; can also be a good solution.&lt;br /&gt;
&lt;br /&gt;
For the Raspberry Pi 5, the OEM fan assembly should be purchased. It has a heat sink with fan speed controlled by the operating system responding to CPU temperature.&lt;br /&gt;
&lt;br /&gt;
== Real time clock (RTC) for Raspberry Pi4 ==&lt;br /&gt;
: [[File:rtc.jpg|thumb|RTC installation|200px]]&lt;br /&gt;
&lt;br /&gt;
Precise timing is essential for processing meteor data, and an RTC module assures that Raspberry Pi always has the precise time, even when power or internet is unreliable. AliExpress sells a pack of 10 but they are inexpensive, so you may want to share extras among other camera constructors in your area. &lt;br /&gt;
&lt;br /&gt;
The AliExpress store lists two RTC modules - one labelled &#039;&#039;DS3231 module&#039;&#039; and another labelled &#039;&#039;mini DS3231 module&#039;&#039;. Select the &#039;&#039;mini DS3231 module&#039;&#039; option, which is designed for the Raspberry Pi. (It has 5 pins and includes a battery.)&lt;br /&gt;
: [https://www.aliexpress.com/item/32770348851.html DS3231 RTC]&lt;br /&gt;
&lt;br /&gt;
After you plug the RTC into the Pi (see image on the right), verify that the current time is correct on the Pi, then open the terminal and run:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
sudo hwclock -w&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
This command sets the current computer time to the RTC. When the Pi boots up, it reads the correct time from the RTC.&lt;br /&gt;
&lt;br /&gt;
The Pi5 contains a built-in RTC. In most cases, the optional external battery is not needed for the Pi5&#039;s RTC.&lt;br /&gt;
&lt;br /&gt;
== Pin header ==&lt;br /&gt;
&lt;br /&gt;
This pin raises the height of the Raspberry GPIO bins so the RTC sits proud of the Raspberry Pi case. You need only 1, but the pack of 20 costs only about a dollar. &lt;br /&gt;
: [https://www.aliexpress.com/item/32549850046.html Tall header pins]&lt;br /&gt;
&lt;br /&gt;
== Network cabling ==&lt;br /&gt;
&lt;br /&gt;
You need two lengths of network cabling, one (quite short) between the Raspberry Pi and the PoE injector, and the other between the PoE injector and the camera. You should be able to easily find both of these locally, but you also can order them from AliExpress. &lt;br /&gt;
&lt;br /&gt;
Some people have found that a thin, flat network cable (shown in the figure) is useful to avoid drilling holes in walls or eaves when you want to snake a wire through a window or door. Regardless of you choice, additional sealant or insulation is required to seal the cable at the PoE connector of the camera.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002311509668.html Cat6 Flat Ethernet Cable]&lt;br /&gt;
&lt;br /&gt;
== Waterproof cable connector ==&lt;br /&gt;
&lt;br /&gt;
One end of the network cable is outdoors, connected to the PoE cable from the camera, so it must be sealed. (This connection carries data as well as 48V DC power.) &lt;br /&gt;
&lt;br /&gt;
Place the waterproof connector over the end of the network cable connector, plug the network cable into the PoE cable on the camera, then lock the connector onto the end of the PoE cable. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;GOOD PRACTICE:&#039;&#039;&#039; For extra weatherproofing, wrap the connector in self-amalgamating tape. &lt;br /&gt;
: [https://www.aliexpress.com/item/32834472563.html RJ45 Waterproof Connector Cap]&lt;br /&gt;
&lt;br /&gt;
== 128GB micro SD card or 256GB USB flash drive ==&lt;br /&gt;
&lt;br /&gt;
You can use either an SD card and a USB flash drive, but there is no need to have both. You must have at least 64GB of storage, but 128GB is recommended because 20GB of data - or more - is collected every night. The card should be fast - Class 10 UHS-1 or better. As with the cables, you can purchase a card locally or [https://www.aliexpress.com/item/32676225311.html from AliExpress]. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;WARNING:&#039;&#039;&#039; There is an &#039;&#039;&#039;[https://photographylife.com/fake-memory-cards ongoing problem with the production and sale of fraudulent memory cards that misrepresent the available storage]&#039;&#039;&#039;. Even supplies from a reputable outlet can be affected, so you should test any card you purchase. The AliExpress link has been used successfully to obtain suitable micro SD cards. If you live in North America, Costco is a reliable local source.&lt;br /&gt;
&lt;br /&gt;
If you prefer to use a USB flash drive, the [https://www.kingston.com/en/usb-flash-drives/datatraveler-kyson-high-performance-usb-flash-drive Kingston DataTraveler Kyson 256 GB] has been verified to work well. We recommend you source it locally or on [https://www.amazon.com/Kingston-DataTraveler-Kyson-256GB-DTKN/dp/B08KHZY581 amazon.com].&lt;br /&gt;
&lt;br /&gt;
== Raspberry Pi 4 or 5 ==&lt;br /&gt;
You should be able to purchase these purchased locally as well as from a domestic online source. You must have at least a 2GB RAM model, and the Raspberry Pi Model 4B is now the minimum spec. As RMS adds functionality, the 4GB or higher RAM version is suggested. Previously, a Raspberry Pi Model 3B+ was considered the minimum spec, but Pi3 does not have the performance or memory to handle busy meteor showers. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The Pi3 runs on Python 2. We are now past the July 1, 2025, cut-off point and we no longer support this version. &lt;br /&gt;
&lt;br /&gt;
: IMPORTANT:&#039;&#039;&#039; Purchase only the official 5.1V 3A 15.3W power supply for a Pi4. The Pi5 requires 5V, 5A power supply due to its increased power consumption. Most problems with Raspberry Pi units can be traced to inadequate power supplies. Please use the correct power supply for the Pi version you choose to deploy.&lt;br /&gt;
&lt;br /&gt;
== Additional items and tools ==&lt;br /&gt;
* Micro-HDMI cable: Connect a RPi 4B to a monitor.&lt;br /&gt;
* M2 and M3 screw: You may find these locally but, in some places, they may be quite difficult to locate. You may want to order hardware from the [https://www.aliexpress.com/store/4714020?spm=a2g0o.detail.1000007.1.5fc666d9tN1f8i ScrewHome Store] on AliExpress. Each [https://www.aliexpress.com/item/32981714992.html?spm=a2g0o.store_pc_groupList.8148356.10.be65539dLjPgfh packet of 50 M2x6mm, M2x12mm, and M3x6mm] machine screws costs only a few dollars.&lt;br /&gt;
* Silicone sealant: Seal the glass window and front screws in the housing.&lt;br /&gt;
* Self-amalgamating tape: Wrap and seal the cable connectors so they are weathertight.&lt;br /&gt;
* Tools:&lt;br /&gt;
: * Small wire cutters or a sharp knife&lt;br /&gt;
: * Assorted screwdrivers&lt;br /&gt;
: * Drill&lt;br /&gt;
: * RJ45 crimper to attach connectorsto the ends of the ethernet cable.&lt;br /&gt;
: * Some cameras come with a slightly different cable with a separate 12V socket for power input, as shown [https://globalmeteornetwork.org/wiki/images/d/dc/Alternatecable.jpg here]. If the power input port has a small cap, you can cover it and use the PoE on the ethernet port. If it is open, you need a pair of PoE adapters (seen in that picture in the background).&lt;br /&gt;
: * &#039;&#039;&#039;VLC&#039;&#039;&#039; software: To test and focus the camera, you must have this software. It is preinstalled on the Pi, but it also is available for Mac, Windows, or Linux from [https://www.videolan.org/vlc/ VideoLan].&lt;br /&gt;
&lt;br /&gt;
At this point, you have completed this section or you are waiting for parts. It is a good time to review the instructions for building the camera or to actually begin the process. Either way - have fun! &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_-_The_complete_how-to Back to the signpost page.]&lt;/div&gt;</summary>
		<author><name>MeteorsABQ</name></author>
	</entry>
	<entry>
		<id>https://globalmeteornetwork.org//wiki/index.php?title=Main_Page&amp;diff=845</id>
		<title>Main Page</title>
		<link rel="alternate" type="text/html" href="https://globalmeteornetwork.org//wiki/index.php?title=Main_Page&amp;diff=845"/>
		<updated>2025-10-01T15:35:18Z</updated>

		<summary type="html">&lt;p&gt;MeteorsABQ: /* GMN Plots and Images */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Welcome to the Global Meteor Network wiki page!&lt;br /&gt;
&lt;br /&gt;
The Global Meteor Network (GMN) is a world-wide organization of amateur and professional astronomers. The goal is to observe the night sky using low-light video cameras and produce meteor trajectories in a coordinated network of recording stations. Here, you can find information about the purpose and structure of the GMN, and how to assemble and operate your own meteor camera. You also will discover how to contribute to the development of RMS (the GMN software) and how your observations as a citizen scientist contribute to the ongoing understanding of our solar system&#039;s formation and evolution. &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;If you are here to find out how to build and set up a camera from scratch, jump ahead to [https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_-_The_complete_how-to this] section!&amp;lt;/span&amp;gt;&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;For German speakers, there is &amp;quot;Build camera from scratch&amp;quot; documentation written by students of [https://fsg-preetz.de/ Friedrich-Schiller-Gymnasium in Preetz] available [http://wiki.linux-astronomie.de/doku.php?id=ceres here]. This version is maintained by Friedrich-Schiller-Gymnasium in Preetz. &amp;lt;/span&amp;gt;&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Global Meteor Network overview ==&lt;br /&gt;
&lt;br /&gt;
===  [https://globalmeteornetwork.org/?page_id=141 Our mission] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=363 A brief history of the Global Meteor Network] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://www.youtube.com/watch?v=MAGq-XqD5Po Video introduction - Overview of the Global Meteor Network (IMC2020)] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://youtu.be/oM7lfQ4nmyw Video overview - Meteor tracking and the GMN from Astro Imaging Channel presentation] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/data/ Some &#039;live&#039; GMN data products] ===&lt;br /&gt;
&lt;br /&gt;
== Meteor detection station ==&lt;br /&gt;
&lt;br /&gt;
What is an RMS GMN station? An RMS-based GMN station consists of a Raspberry Pi (RPi) single board computer, a low light level security video camera, the RMS software, and a connection to the Internet via Wifi. The camera is securely mounted in a weatherproof housing, pointed at the sky, and connected to the RPi with a Power Over Ethernet (POE) cable. To be a part of the GMN network, you need a fairly powerful Raspberry Pi (Pi 4, 5, or better) and a reasonably fast Internet connection. The internet connection is required only for data upload to a central server each morning and to provide automatic updates for the RMS software. &lt;br /&gt;
&lt;br /&gt;
Nightly, the RPi records video from the camera shortly after local sunset, then continuously compressing and storing the video data on a local SSD drive. Each morning before sunrise, when capture is complete, the RPi analyzes the video and extracts  meteor observations from the previous night. These extracted video clips of detected meteors are archived and then uploaded to a server. On a &#039;busy&#039; night, the clips can total hundreds of megabytes as a result of a heavy meteor shower or a night with a lot of false detections. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Continuous progress is being made on the detection software to filter out false detections. &lt;br /&gt;
&lt;br /&gt;
The server finds meteors that were observed from more than one station, which allows the server to triangulate meteor trails in 3D and calculate the orbits of the meteors.&lt;br /&gt;
&lt;br /&gt;
=== What do I need? ===&lt;br /&gt;
&lt;br /&gt;
You need a Raspberry Pi compluter, RMS software, and a camera kit. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; We strongly recommend the Pi 4 or 5 model. &lt;br /&gt;
The software can run on a Pi3, but it is much slower and it is no longer supported. A list with everything you need is available here: [https://globalmeteornetwork.org/wiki/index.php?title=Shopping_list_and_tools_needed page].&lt;br /&gt;
&lt;br /&gt;
You can run multiple cameras on a Linux PC, and details are available &#039;&#039;&#039;[https://docs.google.com/document/d/16PSFi8RAqbenPdluhulCRaIenOkEzgs5piUhkX3yaOc/edit here]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== How do I obtain a camera? ===&lt;br /&gt;
There are two options - buy a camera or build a camera.&lt;br /&gt;
&lt;br /&gt;
==== Buy a Camera ====&lt;br /&gt;
You can buy a camera and prebuilt Pi, and ready to install. Cameras are available from several suppliers, as well as the Croatian Meteor Network, as explained here: [https://globalmeteornetwork.org/?page_id=136 this page]. &lt;br /&gt;
If you are in the UK, you can contact the UK Meteor network for advice. [https://ukmeteornetwork.org/ UK Meteor Network].&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; As of 2024, UK Meteor network can no longer sell cameras directly.&lt;br /&gt;
&lt;br /&gt;
==== Build your own from scratch ====&lt;br /&gt;
This option requires an intermediate level of DIY skills and familiarity with the Raspberry Pi, but do not be put off. The instructions are comprehensive and, if you get stuck, you can ask for advice in the forum here: &#039;&#039;&#039;[https://groups.io/g/globalmeteornetwork groups.io]&#039;&#039;&#039; forum.&lt;br /&gt;
&lt;br /&gt;
You can find out more about this option here: &#039;&#039;&#039;[[Build &amp;amp; Install &amp;amp; Setup your camera - The complete how-to]]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== Advanced RMS installations and multi-camera support ===&lt;br /&gt;
If you would like to explore advanced RMS installation options for various platforms or run multiple cameras on a single Linux computer, complete information is available on &#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Advanced_RMS_installations_and_Multi-camera_support this page]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
If you plan to run RMS software on the Raspberry Pi 4 or 5, the best supported and easiest solution is our prepared image. Complete information is available in an &#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_- Extensive how-to guide]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== Can I use a commercial all-sky camera? ===&lt;br /&gt;
&lt;br /&gt;
Generally, this is not a good idea because these cameras lack sufficient sensitivity. More information is available here: &#039;&#039;&#039;[https://globalmeteornetwork.org/?p=163 See this recent experiment]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Operate and maintain your GMN station ==&lt;br /&gt;
&lt;br /&gt;
=== Overview ===&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; GMS is a nascent operation, so you may share some of our growing pains if you choose to be involved. We are constantly solving bugs and making improvements, which is an opportunity for you to help if you have programming skills! The workload of day-to-day operation can be non-zero, and may require some of your time.&lt;br /&gt;
&lt;br /&gt;
Ideally, you should monitor your RMS Pi systems daily to identify freezes, glitches, or other problems. For example, you may see birds nesting or soiling the camera window, someone may unintentionally unplug the power cord, or animals (mice, cats, or dogs) may chew on the camera Ethernet cable. Although we make constant progress, the GMS network is not yet a &#039;power up and forget about it&#039; system. &lt;br /&gt;
&lt;br /&gt;
By its nature, the GMS network is staffed by lots of people who are willing to help newcomers get started. Here are some suggestions for daily operation of your RMS camera.&lt;br /&gt;
&lt;br /&gt;
=== What does the meteor camera do over the course of 24 hours? ===&lt;br /&gt;
&lt;br /&gt;
The RMS python-based system calculates the sundown to sunrise interval, and schedules video camera capture all night. Based on the video camera and capabilities of the Pi, the camera captures at least 25 frames per second between evening and morning twilight. During each nightly continuous image capture, the station processes captured image data and idenitfies frames that contain a minimum number of stars (usually around 20) that are worth reviewing for meteor detections. When data capture is complete, the station begins processing all frames it flagged with possible detections, then refines the astrometric accuracy of every positive detection. Using the station plate parameters (platepar) calibration file, processing iterates to find the best astrometry and photometry solution for each detected meteor. After this process analyzes each detection, summary files are created. &lt;br /&gt;
&lt;br /&gt;
The summary files include many types of information.&lt;br /&gt;
* Text file data presentation in several widely accepted formats (such as &#039;&#039;CAMS&#039;&#039; and &#039;&#039;UFOorbit&#039;&#039;).&lt;br /&gt;
* Graphic plots of detection frequencies throughout the night.&lt;br /&gt;
* Plot of all detections, showing any identified radiants.&lt;br /&gt;
* Plots of photometry, astrometry, and camera pointing drift in arc minutes throughout the course of the night as the mount or building flexes.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039;  Detailed information about plots is available here: &#039;&#039;&#039;[https://docs.google.com/document/d/132aHGn0QPzhpVN2s2n6FT6rJn39LAsPkchWJqXQb8Qk/edit?usp=sharing Explanation of GMN plots]&#039;&#039;&#039;&lt;br /&gt;
* Thumbnail images of detections.&lt;br /&gt;
* Thumbnail images of data captured throughout the night.&lt;br /&gt;
* Single image with all detections stacked together.&lt;br /&gt;
* Single image with all captured images stacked together.&lt;br /&gt;
* Flat file for correcting images.&lt;br /&gt;
* An &#039;&#039;.mp4&#039;&#039; movie time lapse of the night&#039;s captured images.&lt;br /&gt;
* Meteor shower flux charts, if specific showers are detected.&lt;br /&gt;
* Observation summary data of hardware and data recording characteristics.&lt;br /&gt;
 &lt;br /&gt;
When you click a meteor track, its data displays in the lower data window. Ultimately, all results are combined into a single compressed archive that automatically uploads each morning to the central server. &lt;br /&gt;
&lt;br /&gt;
Each morning, you can review the result files on the RPi and copy anything you want to your computer or tablet.&lt;br /&gt;
&lt;br /&gt;
===Archive data ===&lt;br /&gt;
&lt;br /&gt;
Your primary scientific data is automatically uploaded to the central server every morning after data processing is complete. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; When the night&#039;s results are uploaded, RMS purges the oldest data to free up space for the next night&#039;s run. As a result, you may want to copy some of the data to a PC, NAS, or the cloud for further analysis.&lt;br /&gt;
:       You should consider backing up the content of &#039;&#039;&#039;~/RMS_data/ArchivedFiles&#039;&#039;&#039;, which holds individual files and data that RMS determined were probably meteors. &lt;br /&gt;
&lt;br /&gt;
Details about backing up data is beyond the scope of the GMN Wiki. Tools such as Robocopy for Windows and rsync for Linux/MacOS are ideal, and they can &#039;mirror&#039; data across a network. Help to configure these tools is available in the &#039;&#039;&#039;Globalmeteornetwork&#039;&#039;&#039; group on &#039;&#039;&#039;groups.io&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
In addition, we added some automated tools that can help you back up data to a thumb drive inserted into the RPi. Assistance about these tools also is available in the &#039;&#039;&#039;Globalmeteornetwork&#039;&#039;&#039; group on &#039;&#039;&#039;groups.io&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
===Backup and restore the configuration and RSA keys===&lt;br /&gt;
&lt;br /&gt;
:&#039;&#039;&#039;NOTE:&#039;&#039;&#039; If you are on an older Buster image, you must replace username &#039;&#039;rms&#039;&#039; with username &#039;&#039;pi&#039;&#039;. For example, enter &#039;&#039;/home/pi&#039;&#039; instead of &#039;&#039;/home/rms&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
To determine which username to use, run &lt;br /&gt;
::&#039;&#039;ls /home/rms home/pi&#039;&#039;&lt;br /&gt;
to display the username that is your home directory.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Back up the configuration&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
1. Open a terminal and run the command  &#039;&#039;Scripts/RMS_Backup.sh&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
: A compressed &#039;&#039;.zip&#039;&#039; file, with all important configuration files and keys, is created in your user home directory with the prefix &#039;&#039;RMS_Backup&#039;&#039; and the &#039;&#039;.zip&#039;&#039; extension. &lt;br /&gt;
: For example, &#039;&#039;/home/rms/RMS_Backup_XX0001_2023-01-28.zip&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
2. Copy the &#039;&#039;.zip&#039;&#039; file to a safe place outside RPi. &lt;br /&gt;
&lt;br /&gt;
: Later, it will be useful to restore the system in case of failure. The &#039;&#039;.zip&#039;&#039; file contains the RSA public and private keys used to contact GMN servers, so keep it secret.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Restore the configuration&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
1. Unzip the backup file in any folder on the RPi.&lt;br /&gt;
&lt;br /&gt;
2. Copy the files &#039;&#039;.config&#039;&#039;, &#039;&#039;platepar_cmn2010.cal&#039;&#039;, and &#039;&#039;mask.bmp&#039;&#039; to the folder &#039;&#039;/home/rms/source/RMS/&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
3. Copy the files &#039;&#039;id_rsa&#039;&#039; and &#039;&#039;id_rsa.pub&#039;&#039; to the folder &#039;&#039;/home/rms/.ssh/&#039;&#039;, as shown in this example:&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;cp .config platepar_cmn2010.cal mask.bmp /home/rms/source/RMS/&#039;&#039;&lt;br /&gt;
: &#039;&#039;cp id_rsa id_rsa.pub /home/rms/.ssh/&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
4. To make sure that permission bits in the RSA key files are correct, enter:&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;chmod 400 ~/.ssh/id_rsa*&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== View the data ===&lt;br /&gt;
&lt;br /&gt;
To view data, you can use &#039;&#039;&#039;CMN_binViewer&#039;&#039;&#039; software [https://github.com/CroatianMeteorNetwork/cmn_binviewer], which is included in the RMS SD image. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; There also is a Windows version [https://github.com/CroatianMeteorNetwork/cmn_binviewer/releases] you can install.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; You can open images in astronomical FITS viewers, such as &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039; or &#039;&#039;&#039;Pixinsight&#039;&#039;&#039;, but what you see may be surprising. For example, in &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039;, the image is upside down, which is an artefact of how the software reads the image. &lt;br /&gt;
&lt;br /&gt;
In space, there is no &#039;up&#039; or &#039;down&#039;, so the FITS specification does not dictate if pixel (0,0) is at a specific corner. Some software, notably &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039;, specifies the top left corner as the origin location, which causes terrestrial images  to display vertically mirrored.&lt;br /&gt;
&lt;br /&gt;
=== Tools and utilities ===&lt;br /&gt;
&lt;br /&gt;
There are many tools available.&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;&#039;[https://www.realvnc.com/en/connect/download/viewer/ RealVNC]&#039;&#039;&#039;, &#039;&#039;&#039;[https://www.nomachine.com/ NoMachine]&#039;&#039;&#039;, &#039;&#039;&#039;[https://anydesk.com/en AnyDesk]&#039;&#039;&#039;, or &#039;&#039;&#039;[https://rustdesk.com/ RustDesk]&#039;&#039;&#039; remote connect tools provide station access from anywhere. Access to your station from outside your network is enabled by an OpenVPN connection address that is available to meteor stations.&lt;br /&gt;
: With &#039;&#039;&#039;VNC&#039;&#039;&#039; and &#039;&#039;&#039;Teamviewer&#039;&#039;&#039;, you can create an account and team on their websites, and then remotely access your station. &lt;br /&gt;
* &#039;&#039;&#039;Samba&#039;&#039;&#039; data directory access allows you to copy data results directly from your RPi to your computer or tablet.&lt;br /&gt;
* &#039;&#039;&#039;[https://github.com/CroatianMeteorNetwork/cmn_binviewer CMN_binViewer]&#039;&#039;&#039; allows you to view standard FITS image files that contain meteor detections. It runs on the RPi, and it can run under Windows.&lt;br /&gt;
* &#039;&#039;&#039;[https://sonotaco.com/soft/e_index.html UFO Orbit]&#039;&#039;&#039; allows you to process data from multiple stations, and generate unified radiants of two or more stations that see the same meteor. &#039;&#039;&#039;[https://sonotaco.com/soft/e_index.html UFO Orbit]&#039;&#039;&#039; can plot the shared object ground path and orbital characteristics, and it can output a summary file of all objects seen by more than one station.&lt;br /&gt;
* RMS software can be installed under Windows to allow much of the RMS python-based code to run on your computer. This means you can run RMS against meteor station data that was transferred to your computer from the RPi.&lt;br /&gt;
&lt;br /&gt;
You also can run RMS python jobs on the RPi to sample captured image files, and then condense them into an &#039;&#039;.mp4&#039;&#039; video. Sometimes, these videos are mesmerizing summaries that can run for more than two minutes of winter time data.&lt;br /&gt;
&lt;br /&gt;
== What can I do with my GMN station? ==&lt;br /&gt;
&lt;br /&gt;
=== Use SkyFit2 for astrometric and photometric calibration + Manually reduce observations of fireballs and compute their trajectories ===&lt;br /&gt;
* &#039;&#039;&#039;[https://www.youtube.com/watch?v=ao3J9Jf0iLQ Updated 2023 video tutorial]&#039;&#039;&#039;&lt;br /&gt;
* &#039;&#039;&#039;[https://www.youtube.com/watch?v=MOjb3qxDlX4 Old 2021 video tutorial]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/fov3d/ Generate a Google Earth KML file to show your station&#039;s field of view] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=253 Use the UFO Orbit program to estimate meteor trajectories] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=221 Urban meteor observing] ===&lt;br /&gt;
&lt;br /&gt;
== Data analysis with SkyFit2 ==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SkyFit2&#039;&#039;&#039;, a program in the RMS library, allows you to analyze optical meteor data in most of the optical formats in current use. The program supports popular video formats (&#039;&#039;.mp4&#039;&#039;, &#039;&#039;.avi&#039;&#039;, and &#039;&#039;.mkv&#039;&#039;), sequences of static images, and single images with shutter breaks.&lt;br /&gt;
&lt;br /&gt;
A &#039;&#039;&#039;[https://www.youtube.com/watch?v=ao3J9Jf0iLQ video tutorial]&#039;&#039;&#039; explains how to useg &#039;&#039;&#039;SkyFit2&#039;&#039;&#039; to run astrometric and photometric calibrations on GMN data, and it can manually reduce observations of fireballs and compute their trajectories.&lt;br /&gt;
&lt;br /&gt;
A more detailed description of &#039;&#039;&#039;SkyFit2&#039;&#039;&#039; is available on the &#039;&#039;&#039;[[SkyFit2|SkyFit2]]&#039;&#039;&#039; page.&lt;br /&gt;
&lt;br /&gt;
== FAQ ==&lt;br /&gt;
&lt;br /&gt;
=== What should I back up when I re-flash an SD card or a USB disk? ===&lt;br /&gt;
&lt;br /&gt;
You should backup the &#039;&#039;.config&#039;&#039;, platepar, and mask files that are in the RMS source directory, plus the entire content of the hidden directory &#039;&#039;/home/pi/.ssh&#039;&#039;. Refer to the section titled, &#039;&#039;&#039;Back up the configuration&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
If your SD card or USB disk fails or becomes corrupted, you can fetch the config files from the server because they are uploaded every day, together with the data.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The content of &#039;&#039;.ssh&#039;&#039; is essential for connection to the server, so you also must save these files. &lt;br /&gt;
&lt;br /&gt;
After you set up a new SD card or USB disk, return the files to their original location.&lt;br /&gt;
&lt;br /&gt;
=== What are the values in the &#039;&#039;FTPdetectinfo_*&#039;&#039;  file designated as hnr mle bin Pix/fm Rho Phi? ===&lt;br /&gt;
&lt;br /&gt;
Some of these values (hnr mle bin) are not used in RMS but they are used in CAMS, so their presence is to conform to the standard. As a result, these values are all zeros. &lt;br /&gt;
&lt;br /&gt;
There are other values:&lt;br /&gt;
* Pix/fm is the average angular speed of the meteor, in pixels, per frame.&lt;br /&gt;
* Rho, Phi are parameters that define the line of the meteor in polar coordinates, see this &#039;&#039;&#039;[https://en.wikipedia.org/wiki/Hough_transform#Theory page]&#039;&#039;&#039; for more detail. &lt;br /&gt;
: &#039;&#039;Rho&#039;&#039; is the distance of the line from the center of the image.&lt;br /&gt;
: &#039;&#039;Phi&#039;&#039; is the angle of the line, as measured from the positive direction of the Y axis. (Basically, this is a line from the center of the image to the top of the image.) The positive angles are measured clockwise, although the CAMS standard may define these parameters a bit differently, with the Y axis flipped.&lt;br /&gt;
The &#039;&#039;intensity&#039;&#039; is the sum of all pixel intensities of the meteor on a given frame. &lt;br /&gt;
&lt;br /&gt;
For example, you could represent an area around the meteor on a given frame, as shown in the figure, where the numbers are pixel intensities on an 8-bit image (so they can range from 0 to 255) and the pixel values inside the red boundary represent the meteor blob on the frame. The result? The intensity is the sum of all numbers inside the red boundary. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Later, this value is used to compute the magnitude.&lt;br /&gt;
&lt;br /&gt;
[[File:Intensity_sum.png |Intensity_sum.png ]]&lt;br /&gt;
&lt;br /&gt;
The magnitude is computed as&lt;br /&gt;
: &#039;&#039;mag = -2.5*log10(intensity sum) + photometric_offset&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
To estimate the photometric offset in &#039;&#039;&#039;SkyFit&#039;&#039;&#039;, fit the line with slope -2.5 through pairs of known magnitudes of stars and logartihms of their pixel intensity sum. Fundamentally, the photometric offset is the intercept of that line. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The constant slope of -2.5 comes from the &#039;&#039;&#039;[https://en.wikipedia.org/wiki/Apparent_magnitude#Calculations Definition of stellar magnitudes]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== GMN data policy ==&lt;br /&gt;
&lt;br /&gt;
The Global Meteor Network produces three levels of data products.&lt;br /&gt;
* Level 1 - The lowest level data (as close to &#039;raw&#039; as possible) are the FF image and FR video files saved to the RPi by the capture code and the fireball detector.&lt;br /&gt;
* Level 2 - Data is used in three ways:&lt;br /&gt;
:* The meteor detector extracts positional and brightness information of individual meteors (&#039;&#039;FTPdetectinfo&#039;&#039; file). &lt;br /&gt;
:* Images are used for astrometric and photometric calibration (platepar file). &lt;br /&gt;
:* Meteor and star detections are used to generate a range of plots, such as the single-station shower association graph and the camera drift graph. The calibrated meteor measurements are uploaded to the GMN server, together with the raw images of individual meteors.&lt;br /&gt;
* Level 3 - Software on the server correlates individual observations and computes multi-station meteor trajectories, which are published daily on the &#039;&#039;&#039;GMN [https://globalmeteornetwork.org/data/ Data website]&#039;&#039;&#039;. This data is made public under the &#039;&#039;&#039;[https://creativecommons.org/licenses/by/4.0/ CC BY 4.0 license]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
Operators of individual GMN stations exclusively own the Level 1 and Level 2 data their stations produce. In practice, this means they are free to share this data with other meteor networks if they wish. The data that is uploaded to the GMN server is not shared publicly or with other parties without the operator&#039;s consent. However, the data may be used internally by the GMN coordinators to manually produce other data products, such as the trajectory of a meteorite dropping fireball or an analysis of a meteor shower. &lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; All station operators are credited for their data in all GMN publications.&lt;br /&gt;
&lt;br /&gt;
== GMN Plots and Images Explained ==&lt;br /&gt;
&lt;br /&gt;
This document explains the data summaries produced on your system and displayed on the GMN Weblog every morning &#039;&#039;&#039;[https://docs.google.com/document/d/132aHGn0QPzhpVN2s2n6FT6rJn39LAsPkchWJqXQb8Qk/edit?pli=1&amp;amp;tab=t.0 GMN Plots and Images]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;[https://IstraStream.com IstraStream.com]&#039;&#039;&#039; was an independent hosting site primarily intended for cameras sold by IstraStream. In mid-2023, Istrastream stopped listing camera image output and the IstraStream data display was replaced with the &#039;&#039;&#039;[https://globalmeteornetwork.org/weblog/ GMN weblog]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== For more information ==&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?page_id=43 Contact the Global Meteor Network] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://groups.io/g/globalmeteornetwork Join the Global Meteor Network Forum] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://github.com/markmac99/ukmon-pitools/wiki UK Meteor Network Wiki]===&lt;br /&gt;
This wiki has numerous FAQs and tips on maintaining, monitoring and managing your system, and several explainers such as how to calibrate and create a mask, how to copy data and so forth. &lt;br /&gt;
&lt;br /&gt;
=== Important GMN resources ===&lt;br /&gt;
&lt;br /&gt;
There are two additional web pages you should know about.&lt;br /&gt;
&lt;br /&gt;
* The &#039;&#039;&#039;[https://globalmeteornetwork.org/status GMN status page]&#039;&#039;&#039; provides access to the &#039;&#039;&#039;[https://globalmeteornetwork.org/weblog/ GMN weblog]&#039;&#039;&#039;.&lt;br /&gt;
* A mapping utility website that is directly derived from GMN data: &#039;&#039;&#039;[https://tammojan.github.io/meteormap Meteor map]&#039;&#039;&#039;.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; This map takes quite a while to load. When you review the map, you must scroll down to see the full power of the data display.&lt;br /&gt;
&lt;br /&gt;
=== GMN talks ===&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/playlist?list=PLmQ5Bvz4ACYJLYfswIeAipapoeGeI6QWy GMN talk for Society for Astronomical Sciences workshop 2024 (The first 3 videos)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=IfUyCHjMATc 2023 GMN Meeting Session 1 (February 2023)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=I78KwF5-1GE 2023 GMN Meeting Session 2 (February 2023)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=wDdrG_FCyGk 2022 GMN Meeting Session 1 (February 2022)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=j_75CDPzjI4 2022 GMN Meeting Session 2 (February 2022)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=f6x9_WCVphY GMN talk at the European Space Agency&#039;s Fireball Workshop (June 2021)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=QXBTLPnPDWs 2021 GMN Meeting] - [https://www.dropbox.com/sh/ia9vagug5lxm8k9/AAB_i_1jcWThUdAHO_2gF_Ksa?dl=0 Link to slides]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=MAGq-XqD5Po Overview of the GMN - IMC2020 (September 2020)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=oM7lfQ4nmyw Overview of the GMN, Astro Imaging Channel presentation (May 2020)]&lt;br /&gt;
&lt;br /&gt;
=== GMN-related publications ===&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2206.11365 Vida, D., Blaauw Erskine, R. C., Brown, P. G., Kambulow, J., Campbell-Brown, M., &amp;amp; Mazur, M. J. (2022). Computing optical meteor flux using global meteor network data. Monthly Notices of the Royal Astronomical Society, 515(2), 2322-2339.]&lt;br /&gt;
&lt;br /&gt;
: [https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stab2557/6368869 Moorhead, A. V., Clements, T., &amp;amp; Vida, D. (2021). Meteor shower radiant dispersions in Global Meteor Network data. Monthly Notices of the Royal Astronomical Society, 508(1), 326-339.]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2107.12335 Vida, D., Šegon, D., Gural, P. S., Brown, P. G., McIntyre, M. J., Dijkema, T. J., Pavletić, L., Kukić, P., Mazur, M.J., Eschman, P., Roggemans, P., Merlak, A., &amp;amp; Zubović, D. (2021). The Global Meteor Network–Methodology and first results. Monthly Notices of the Royal Astronomical Society, 506(4), 5046-5074.]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2003.05458/ Moorhead, A. V., Clements, T. D., &amp;amp; Vida, D. (2020). Realistic gravitational focusing of meteoroid streams. Monthly Notices of the Royal Astronomical Society, 494(2), 2982-2994.] &lt;br /&gt;
&lt;br /&gt;
: [https://globalmeteornetwork.org/wordpress/wp-content/uploads/2018/11/Kukic-et-al-2018-Rolling-shutter.pdf  Kukić, P., Gural, P., Vida, D., Šegon, D. &amp;amp; Merlak, A. (2018) Correction for meteor centroids observed using rolling shutter cameras. WGN, Journal of the International Meteor Organization, 46:5, 154-118.]&lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/2018_WGN___RMS_sun_skirter_final.pdf  Vida, D., Mazur, M. J., Šegon, D., Kukić, P., &amp;amp; Merlak, A. (2018). Compressive strength of a skirting Daytime Arietid-first science results from low-cost Raspberry Pi-based meteor stations. WGN, Journal of the International Meteor Organization, 46, 113-118.] &lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/pdf/1911.02979.pdf Vida, D., Gural, P., Brown, P., Campbell-Brown, M., Wiegert, P. (2019) Estimating trajectories of meteors: an observational Monte Carlo approach - I. Theory. arXiv:1911.02979v4 [astro-ph.EP] 21 Apr 2020]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/pdf/1911.11734.pdf Vida, D., Gural, P., Brown, P., Campbell-Brown, M., Wiegert, P. (2019) Estimating trajectories of meteors: an observational Monte Carlo approach - II. Results. arXiv:1911.11734v1 [astro-ph.EP] 26 Novr 2019]&lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/2018_WGN___RMS_first_results-final.pdf Vida, D., Mazur, M. J., Šegon, D., Zubović, D., Kukić, P., Parag, F., &amp;amp; Macan, A. (2018). First results of a Raspberry Pi based meteor camera system. WGN, Journal of the International Meteor Organization, 46, 71-78.] &lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/Vida_IMC2016_proceedings_final.pdf Vida, D., Zubović, D., Šegon, D., Gural, P., &amp;amp; Cupec, R. (2016). Open-source meteor detection software for low-cost single-board computers. In Proceedings of the International Meteor Conference (IMC2016), Egmond, The Netherlands (pp. 2-5).] &lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/Zubovic_IMC2015_priceedings_final.pdf Zubović, D., Vida, D., Gural, P., &amp;amp; Šegon, D. (2015). Advances in the development of a low-cost video meteor station. In Proceedings of the International Meteor Conference, Mistelbach, Austria (pp. 27-30).]&lt;/div&gt;</summary>
		<author><name>MeteorsABQ</name></author>
	</entry>
	<entry>
		<id>https://globalmeteornetwork.org//wiki/index.php?title=Main_Page&amp;diff=844</id>
		<title>Main Page</title>
		<link rel="alternate" type="text/html" href="https://globalmeteornetwork.org//wiki/index.php?title=Main_Page&amp;diff=844"/>
		<updated>2025-09-30T21:36:45Z</updated>

		<summary type="html">&lt;p&gt;MeteorsABQ: /* IstraStream */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Welcome to the Global Meteor Network wiki page!&lt;br /&gt;
&lt;br /&gt;
The Global Meteor Network (GMN) is a world-wide organization of amateur and professional astronomers. The goal is to observe the night sky using low-light video cameras and produce meteor trajectories in a coordinated network of recording stations. Here, you can find information about the purpose and structure of the GMN, and how to assemble and operate your own meteor camera. You also will discover how to contribute to the development of RMS (the GMN software) and how your observations as a citizen scientist contribute to the ongoing understanding of our solar system&#039;s formation and evolution. &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;If you are here to find out how to build and set up a camera from scratch, jump ahead to [https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_-_The_complete_how-to this] section!&amp;lt;/span&amp;gt;&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&amp;lt;span style=&amp;quot;color:red&amp;quot;&amp;gt;For German speakers, there is &amp;quot;Build camera from scratch&amp;quot; documentation written by students of [https://fsg-preetz.de/ Friedrich-Schiller-Gymnasium in Preetz] available [http://wiki.linux-astronomie.de/doku.php?id=ceres here]. This version is maintained by Friedrich-Schiller-Gymnasium in Preetz. &amp;lt;/span&amp;gt;&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Global Meteor Network overview ==&lt;br /&gt;
&lt;br /&gt;
===  [https://globalmeteornetwork.org/?page_id=141 Our mission] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=363 A brief history of the Global Meteor Network] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://www.youtube.com/watch?v=MAGq-XqD5Po Video introduction - Overview of the Global Meteor Network (IMC2020)] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://youtu.be/oM7lfQ4nmyw Video overview - Meteor tracking and the GMN from Astro Imaging Channel presentation] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/data/ Some &#039;live&#039; GMN data products] ===&lt;br /&gt;
&lt;br /&gt;
== Meteor detection station ==&lt;br /&gt;
&lt;br /&gt;
What is an RMS GMN station? An RMS-based GMN station consists of a Raspberry Pi (RPi) single board computer, a low light level security video camera, the RMS software, and a connection to the Internet via Wifi. The camera is securely mounted in a weatherproof housing, pointed at the sky, and connected to the RPi with a Power Over Ethernet (POE) cable. To be a part of the GMN network, you need a fairly powerful Raspberry Pi (Pi 4, 5, or better) and a reasonably fast Internet connection. The internet connection is required only for data upload to a central server each morning and to provide automatic updates for the RMS software. &lt;br /&gt;
&lt;br /&gt;
Nightly, the RPi records video from the camera shortly after local sunset, then continuously compressing and storing the video data on a local SSD drive. Each morning before sunrise, when capture is complete, the RPi analyzes the video and extracts  meteor observations from the previous night. These extracted video clips of detected meteors are archived and then uploaded to a server. On a &#039;busy&#039; night, the clips can total hundreds of megabytes as a result of a heavy meteor shower or a night with a lot of false detections. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Continuous progress is being made on the detection software to filter out false detections. &lt;br /&gt;
&lt;br /&gt;
The server finds meteors that were observed from more than one station, which allows the server to triangulate meteor trails in 3D and calculate the orbits of the meteors.&lt;br /&gt;
&lt;br /&gt;
=== What do I need? ===&lt;br /&gt;
&lt;br /&gt;
You need a Raspberry Pi compluter, RMS software, and a camera kit. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; We strongly recommend the Pi 4 or 5 model. &lt;br /&gt;
The software can run on a Pi3, but it is much slower and it is no longer supported. A list with everything you need is available here: [https://globalmeteornetwork.org/wiki/index.php?title=Shopping_list_and_tools_needed page].&lt;br /&gt;
&lt;br /&gt;
You can run multiple cameras on a Linux PC, and details are available &#039;&#039;&#039;[https://docs.google.com/document/d/16PSFi8RAqbenPdluhulCRaIenOkEzgs5piUhkX3yaOc/edit here]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== How do I obtain a camera? ===&lt;br /&gt;
There are two options - buy a camera or build a camera.&lt;br /&gt;
&lt;br /&gt;
==== Buy a Camera ====&lt;br /&gt;
You can buy a camera and prebuilt Pi, and ready to install. Cameras are available from several suppliers, as well as the Croatian Meteor Network, as explained here: [https://globalmeteornetwork.org/?page_id=136 this page]. &lt;br /&gt;
If you are in the UK, you can contact the UK Meteor network for advice. [https://ukmeteornetwork.org/ UK Meteor Network].&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; As of 2024, UK Meteor network can no longer sell cameras directly.&lt;br /&gt;
&lt;br /&gt;
==== Build your own from scratch ====&lt;br /&gt;
This option requires an intermediate level of DIY skills and familiarity with the Raspberry Pi, but do not be put off. The instructions are comprehensive and, if you get stuck, you can ask for advice in the forum here: &#039;&#039;&#039;[https://groups.io/g/globalmeteornetwork groups.io]&#039;&#039;&#039; forum.&lt;br /&gt;
&lt;br /&gt;
You can find out more about this option here: &#039;&#039;&#039;[[Build &amp;amp; Install &amp;amp; Setup your camera - The complete how-to]]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== Advanced RMS installations and multi-camera support ===&lt;br /&gt;
If you would like to explore advanced RMS installation options for various platforms or run multiple cameras on a single Linux computer, complete information is available on &#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Advanced_RMS_installations_and_Multi-camera_support this page]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
If you plan to run RMS software on the Raspberry Pi 4 or 5, the best supported and easiest solution is our prepared image. Complete information is available in an &#039;&#039;&#039;[https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_- Extensive how-to guide]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
=== Can I use a commercial all-sky camera? ===&lt;br /&gt;
&lt;br /&gt;
Generally, this is not a good idea because these cameras lack sufficient sensitivity. More information is available here: &#039;&#039;&#039;[https://globalmeteornetwork.org/?p=163 See this recent experiment]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Operate and maintain your GMN station ==&lt;br /&gt;
&lt;br /&gt;
=== Overview ===&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; GMS is a nascent operation, so you may share some of our growing pains if you choose to be involved. We are constantly solving bugs and making improvements, which is an opportunity for you to help if you have programming skills! The workload of day-to-day operation can be non-zero, and may require some of your time.&lt;br /&gt;
&lt;br /&gt;
Ideally, you should monitor your RMS Pi systems daily to identify freezes, glitches, or other problems. For example, you may see birds nesting or soiling the camera window, someone may unintentionally unplug the power cord, or animals (mice, cats, or dogs) may chew on the camera Ethernet cable. Although we make constant progress, the GMS network is not yet a &#039;power up and forget about it&#039; system. &lt;br /&gt;
&lt;br /&gt;
By its nature, the GMS network is staffed by lots of people who are willing to help newcomers get started. Here are some suggestions for daily operation of your RMS camera.&lt;br /&gt;
&lt;br /&gt;
=== What does the meteor camera do over the course of 24 hours? ===&lt;br /&gt;
&lt;br /&gt;
The RMS python-based system calculates the sundown to sunrise interval, and schedules video camera capture all night. Based on the video camera and capabilities of the Pi, the camera captures at least 25 frames per second between evening and morning twilight. During each nightly continuous image capture, the station processes captured image data and idenitfies frames that contain a minimum number of stars (usually around 20) that are worth reviewing for meteor detections. When data capture is complete, the station begins processing all frames it flagged with possible detections, then refines the astrometric accuracy of every positive detection. Using the station plate parameters (platepar) calibration file, processing iterates to find the best astrometry and photometry solution for each detected meteor. After this process analyzes each detection, summary files are created. &lt;br /&gt;
&lt;br /&gt;
The summary files include many types of information.&lt;br /&gt;
* Text file data presentation in several widely accepted formats (such as &#039;&#039;CAMS&#039;&#039; and &#039;&#039;UFOorbit&#039;&#039;).&lt;br /&gt;
* Graphic plots of detection frequencies throughout the night.&lt;br /&gt;
* Plot of all detections, showing any identified radiants.&lt;br /&gt;
* Plots of photometry, astrometry, and camera pointing drift in arc minutes throughout the course of the night as the mount or building flexes.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039;  Detailed information about plots is available here: &#039;&#039;&#039;[https://docs.google.com/document/d/132aHGn0QPzhpVN2s2n6FT6rJn39LAsPkchWJqXQb8Qk/edit?usp=sharing Explanation of GMN plots]&#039;&#039;&#039;&lt;br /&gt;
* Thumbnail images of detections.&lt;br /&gt;
* Thumbnail images of data captured throughout the night.&lt;br /&gt;
* Single image with all detections stacked together.&lt;br /&gt;
* Single image with all captured images stacked together.&lt;br /&gt;
* Flat file for correcting images.&lt;br /&gt;
* An &#039;&#039;.mp4&#039;&#039; movie time lapse of the night&#039;s captured images.&lt;br /&gt;
* Meteor shower flux charts, if specific showers are detected.&lt;br /&gt;
* Observation summary data of hardware and data recording characteristics.&lt;br /&gt;
 &lt;br /&gt;
When you click a meteor track, its data displays in the lower data window. Ultimately, all results are combined into a single compressed archive that automatically uploads each morning to the central server. &lt;br /&gt;
&lt;br /&gt;
Each morning, you can review the result files on the RPi and copy anything you want to your computer or tablet.&lt;br /&gt;
&lt;br /&gt;
===Archive data ===&lt;br /&gt;
&lt;br /&gt;
Your primary scientific data is automatically uploaded to the central server every morning after data processing is complete. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; When the night&#039;s results are uploaded, RMS purges the oldest data to free up space for the next night&#039;s run. As a result, you may want to copy some of the data to a PC, NAS, or the cloud for further analysis.&lt;br /&gt;
:       You should consider backing up the content of &#039;&#039;&#039;~/RMS_data/ArchivedFiles&#039;&#039;&#039;, which holds individual files and data that RMS determined were probably meteors. &lt;br /&gt;
&lt;br /&gt;
Details about backing up data is beyond the scope of the GMN Wiki. Tools such as Robocopy for Windows and rsync for Linux/MacOS are ideal, and they can &#039;mirror&#039; data across a network. Help to configure these tools is available in the &#039;&#039;&#039;Globalmeteornetwork&#039;&#039;&#039; group on &#039;&#039;&#039;groups.io&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
In addition, we added some automated tools that can help you back up data to a thumb drive inserted into the RPi. Assistance about these tools also is available in the &#039;&#039;&#039;Globalmeteornetwork&#039;&#039;&#039; group on &#039;&#039;&#039;groups.io&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
===Backup and restore the configuration and RSA keys===&lt;br /&gt;
&lt;br /&gt;
:&#039;&#039;&#039;NOTE:&#039;&#039;&#039; If you are on an older Buster image, you must replace username &#039;&#039;rms&#039;&#039; with username &#039;&#039;pi&#039;&#039;. For example, enter &#039;&#039;/home/pi&#039;&#039; instead of &#039;&#039;/home/rms&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
To determine which username to use, run &lt;br /&gt;
::&#039;&#039;ls /home/rms home/pi&#039;&#039;&lt;br /&gt;
to display the username that is your home directory.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Back up the configuration&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
1. Open a terminal and run the command  &#039;&#039;Scripts/RMS_Backup.sh&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
: A compressed &#039;&#039;.zip&#039;&#039; file, with all important configuration files and keys, is created in your user home directory with the prefix &#039;&#039;RMS_Backup&#039;&#039; and the &#039;&#039;.zip&#039;&#039; extension. &lt;br /&gt;
: For example, &#039;&#039;/home/rms/RMS_Backup_XX0001_2023-01-28.zip&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
2. Copy the &#039;&#039;.zip&#039;&#039; file to a safe place outside RPi. &lt;br /&gt;
&lt;br /&gt;
: Later, it will be useful to restore the system in case of failure. The &#039;&#039;.zip&#039;&#039; file contains the RSA public and private keys used to contact GMN servers, so keep it secret.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Restore the configuration&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
1. Unzip the backup file in any folder on the RPi.&lt;br /&gt;
&lt;br /&gt;
2. Copy the files &#039;&#039;.config&#039;&#039;, &#039;&#039;platepar_cmn2010.cal&#039;&#039;, and &#039;&#039;mask.bmp&#039;&#039; to the folder &#039;&#039;/home/rms/source/RMS/&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
3. Copy the files &#039;&#039;id_rsa&#039;&#039; and &#039;&#039;id_rsa.pub&#039;&#039; to the folder &#039;&#039;/home/rms/.ssh/&#039;&#039;, as shown in this example:&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;cp .config platepar_cmn2010.cal mask.bmp /home/rms/source/RMS/&#039;&#039;&lt;br /&gt;
: &#039;&#039;cp id_rsa id_rsa.pub /home/rms/.ssh/&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
4. To make sure that permission bits in the RSA key files are correct, enter:&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;chmod 400 ~/.ssh/id_rsa*&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== View the data ===&lt;br /&gt;
&lt;br /&gt;
To view data, you can use &#039;&#039;&#039;CMN_binViewer&#039;&#039;&#039; software [https://github.com/CroatianMeteorNetwork/cmn_binviewer], which is included in the RMS SD image. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; There also is a Windows version [https://github.com/CroatianMeteorNetwork/cmn_binviewer/releases] you can install.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; You can open images in astronomical FITS viewers, such as &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039; or &#039;&#039;&#039;Pixinsight&#039;&#039;&#039;, but what you see may be surprising. For example, in &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039;, the image is upside down, which is an artefact of how the software reads the image. &lt;br /&gt;
&lt;br /&gt;
In space, there is no &#039;up&#039; or &#039;down&#039;, so the FITS specification does not dictate if pixel (0,0) is at a specific corner. Some software, notably &#039;&#039;&#039;FITS Liberator&#039;&#039;&#039;, specifies the top left corner as the origin location, which causes terrestrial images  to display vertically mirrored.&lt;br /&gt;
&lt;br /&gt;
=== Tools and utilities ===&lt;br /&gt;
&lt;br /&gt;
There are many tools available.&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;&#039;[https://www.realvnc.com/en/connect/download/viewer/ RealVNC]&#039;&#039;&#039;, &#039;&#039;&#039;[https://www.nomachine.com/ NoMachine]&#039;&#039;&#039;, &#039;&#039;&#039;[https://anydesk.com/en AnyDesk]&#039;&#039;&#039;, or &#039;&#039;&#039;[https://rustdesk.com/ RustDesk]&#039;&#039;&#039; remote connect tools provide station access from anywhere. Access to your station from outside your network is enabled by an OpenVPN connection address that is available to meteor stations.&lt;br /&gt;
: With &#039;&#039;&#039;VNC&#039;&#039;&#039; and &#039;&#039;&#039;Teamviewer&#039;&#039;&#039;, you can create an account and team on their websites, and then remotely access your station. &lt;br /&gt;
* &#039;&#039;&#039;Samba&#039;&#039;&#039; data directory access allows you to copy data results directly from your RPi to your computer or tablet.&lt;br /&gt;
* &#039;&#039;&#039;[https://github.com/CroatianMeteorNetwork/cmn_binviewer CMN_binViewer]&#039;&#039;&#039; allows you to view standard FITS image files that contain meteor detections. It runs on the RPi, and it can run under Windows.&lt;br /&gt;
* &#039;&#039;&#039;[https://sonotaco.com/soft/e_index.html UFO Orbit]&#039;&#039;&#039; allows you to process data from multiple stations, and generate unified radiants of two or more stations that see the same meteor. &#039;&#039;&#039;[https://sonotaco.com/soft/e_index.html UFO Orbit]&#039;&#039;&#039; can plot the shared object ground path and orbital characteristics, and it can output a summary file of all objects seen by more than one station.&lt;br /&gt;
* RMS software can be installed under Windows to allow much of the RMS python-based code to run on your computer. This means you can run RMS against meteor station data that was transferred to your computer from the RPi.&lt;br /&gt;
&lt;br /&gt;
You also can run RMS python jobs on the RPi to sample captured image files, and then condense them into an &#039;&#039;.mp4&#039;&#039; video. Sometimes, these videos are mesmerizing summaries that can run for more than two minutes of winter time data.&lt;br /&gt;
&lt;br /&gt;
== What can I do with my GMN station? ==&lt;br /&gt;
&lt;br /&gt;
=== Use SkyFit2 for astrometric and photometric calibration + Manually reduce observations of fireballs and compute their trajectories ===&lt;br /&gt;
* &#039;&#039;&#039;[https://www.youtube.com/watch?v=ao3J9Jf0iLQ Updated 2023 video tutorial]&#039;&#039;&#039;&lt;br /&gt;
* &#039;&#039;&#039;[https://www.youtube.com/watch?v=MOjb3qxDlX4 Old 2021 video tutorial]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/fov3d/ Generate a Google Earth KML file to show your station&#039;s field of view] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=253 Use the UFO Orbit program to estimate meteor trajectories] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?p=221 Urban meteor observing] ===&lt;br /&gt;
&lt;br /&gt;
== Data analysis with SkyFit2 ==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;SkyFit2&#039;&#039;&#039;, a program in the RMS library, allows you to analyze optical meteor data in most of the optical formats in current use. The program supports popular video formats (&#039;&#039;.mp4&#039;&#039;, &#039;&#039;.avi&#039;&#039;, and &#039;&#039;.mkv&#039;&#039;), sequences of static images, and single images with shutter breaks.&lt;br /&gt;
&lt;br /&gt;
A &#039;&#039;&#039;[https://www.youtube.com/watch?v=ao3J9Jf0iLQ video tutorial]&#039;&#039;&#039; explains how to useg &#039;&#039;&#039;SkyFit2&#039;&#039;&#039; to run astrometric and photometric calibrations on GMN data, and it can manually reduce observations of fireballs and compute their trajectories.&lt;br /&gt;
&lt;br /&gt;
A more detailed description of &#039;&#039;&#039;SkyFit2&#039;&#039;&#039; is available on the &#039;&#039;&#039;[[SkyFit2|SkyFit2]]&#039;&#039;&#039; page.&lt;br /&gt;
&lt;br /&gt;
== FAQ ==&lt;br /&gt;
&lt;br /&gt;
=== What should I back up when I re-flash an SD card or a USB disk? ===&lt;br /&gt;
&lt;br /&gt;
You should backup the &#039;&#039;.config&#039;&#039;, platepar, and mask files that are in the RMS source directory, plus the entire content of the hidden directory &#039;&#039;/home/pi/.ssh&#039;&#039;. Refer to the section titled, &#039;&#039;&#039;Back up the configuration&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
If your SD card or USB disk fails or becomes corrupted, you can fetch the config files from the server because they are uploaded every day, together with the data.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The content of &#039;&#039;.ssh&#039;&#039; is essential for connection to the server, so you also must save these files. &lt;br /&gt;
&lt;br /&gt;
After you set up a new SD card or USB disk, return the files to their original location.&lt;br /&gt;
&lt;br /&gt;
=== What are the values in the &#039;&#039;FTPdetectinfo_*&#039;&#039;  file designated as hnr mle bin Pix/fm Rho Phi? ===&lt;br /&gt;
&lt;br /&gt;
Some of these values (hnr mle bin) are not used in RMS but they are used in CAMS, so their presence is to conform to the standard. As a result, these values are all zeros. &lt;br /&gt;
&lt;br /&gt;
There are other values:&lt;br /&gt;
* Pix/fm is the average angular speed of the meteor, in pixels, per frame.&lt;br /&gt;
* Rho, Phi are parameters that define the line of the meteor in polar coordinates, see this &#039;&#039;&#039;[https://en.wikipedia.org/wiki/Hough_transform#Theory page]&#039;&#039;&#039; for more detail. &lt;br /&gt;
: &#039;&#039;Rho&#039;&#039; is the distance of the line from the center of the image.&lt;br /&gt;
: &#039;&#039;Phi&#039;&#039; is the angle of the line, as measured from the positive direction of the Y axis. (Basically, this is a line from the center of the image to the top of the image.) The positive angles are measured clockwise, although the CAMS standard may define these parameters a bit differently, with the Y axis flipped.&lt;br /&gt;
The &#039;&#039;intensity&#039;&#039; is the sum of all pixel intensities of the meteor on a given frame. &lt;br /&gt;
&lt;br /&gt;
For example, you could represent an area around the meteor on a given frame, as shown in the figure, where the numbers are pixel intensities on an 8-bit image (so they can range from 0 to 255) and the pixel values inside the red boundary represent the meteor blob on the frame. The result? The intensity is the sum of all numbers inside the red boundary. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Later, this value is used to compute the magnitude.&lt;br /&gt;
&lt;br /&gt;
[[File:Intensity_sum.png |Intensity_sum.png ]]&lt;br /&gt;
&lt;br /&gt;
The magnitude is computed as&lt;br /&gt;
: &#039;&#039;mag = -2.5*log10(intensity sum) + photometric_offset&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
To estimate the photometric offset in &#039;&#039;&#039;SkyFit&#039;&#039;&#039;, fit the line with slope -2.5 through pairs of known magnitudes of stars and logartihms of their pixel intensity sum. Fundamentally, the photometric offset is the intercept of that line. &lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The constant slope of -2.5 comes from the &#039;&#039;&#039;[https://en.wikipedia.org/wiki/Apparent_magnitude#Calculations Definition of stellar magnitudes]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== GMN data policy ==&lt;br /&gt;
&lt;br /&gt;
The Global Meteor Network produces three levels of data products.&lt;br /&gt;
* Level 1 - The lowest level data (as close to &#039;raw&#039; as possible) are the FF image and FR video files saved to the RPi by the capture code and the fireball detector.&lt;br /&gt;
* Level 2 - Data is used in three ways:&lt;br /&gt;
:* The meteor detector extracts positional and brightness information of individual meteors (&#039;&#039;FTPdetectinfo&#039;&#039; file). &lt;br /&gt;
:* Images are used for astrometric and photometric calibration (platepar file). &lt;br /&gt;
:* Meteor and star detections are used to generate a range of plots, such as the single-station shower association graph and the camera drift graph. The calibrated meteor measurements are uploaded to the GMN server, together with the raw images of individual meteors.&lt;br /&gt;
* Level 3 - Software on the server correlates individual observations and computes multi-station meteor trajectories, which are published daily on the &#039;&#039;&#039;GMN [https://globalmeteornetwork.org/data/ Data website]&#039;&#039;&#039;. This data is made public under the &#039;&#039;&#039;[https://creativecommons.org/licenses/by/4.0/ CC BY 4.0 license]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
Operators of individual GMN stations exclusively own the Level 1 and Level 2 data their stations produce. In practice, this means they are free to share this data with other meteor networks if they wish. The data that is uploaded to the GMN server is not shared publicly or with other parties without the operator&#039;s consent. However, the data may be used internally by the GMN coordinators to manually produce other data products, such as the trajectory of a meteorite dropping fireball or an analysis of a meteor shower. &lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; All station operators are credited for their data in all GMN publications.&lt;br /&gt;
&lt;br /&gt;
== GMN Plots and Images ==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;[https://IstraStream.com IstraStream.com]&#039;&#039;&#039; was an independent hosting site primarily intended for cameras sold by IstraStream. In mid-2023, Istrastream stopped listing camera image output and the IstraStream data display was replaced with the &#039;&#039;&#039;[https://globalmeteornetwork.org/weblog/ GMN weblog]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
This document explains plots on the Weblog &#039;&#039;&#039;[https://docs.google.com/document/d/132aHGn0QPzhpVN2s2n6FT6rJn39LAsPkchWJqXQb8Qk/edit?pli=1&amp;amp;tab=t.0 GMN Plots and Images]&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== For more information ==&lt;br /&gt;
&lt;br /&gt;
=== [https://globalmeteornetwork.org/?page_id=43 Contact the Global Meteor Network] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://groups.io/g/globalmeteornetwork Join the Global Meteor Network Forum] ===&lt;br /&gt;
&lt;br /&gt;
=== [https://github.com/markmac99/ukmon-pitools/wiki UK Meteor Network Wiki]===&lt;br /&gt;
This wiki has numerous FAQs and tips on maintaining, monitoring and managing your system, and several explainers such as how to calibrate and create a mask, how to copy data and so forth. &lt;br /&gt;
&lt;br /&gt;
=== Important GMN resources ===&lt;br /&gt;
&lt;br /&gt;
There are two additional web pages you should know about.&lt;br /&gt;
&lt;br /&gt;
* The &#039;&#039;&#039;[https://globalmeteornetwork.org/status GMN status page]&#039;&#039;&#039; provides access to the &#039;&#039;&#039;[https://globalmeteornetwork.org/weblog/ GMN weblog]&#039;&#039;&#039;.&lt;br /&gt;
* A mapping utility website that is directly derived from GMN data: &#039;&#039;&#039;[https://tammojan.github.io/meteormap Meteor map]&#039;&#039;&#039;.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; This map takes quite a while to load. When you review the map, you must scroll down to see the full power of the data display.&lt;br /&gt;
&lt;br /&gt;
=== GMN talks ===&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/playlist?list=PLmQ5Bvz4ACYJLYfswIeAipapoeGeI6QWy GMN talk for Society for Astronomical Sciences workshop 2024 (The first 3 videos)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=IfUyCHjMATc 2023 GMN Meeting Session 1 (February 2023)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=I78KwF5-1GE 2023 GMN Meeting Session 2 (February 2023)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=wDdrG_FCyGk 2022 GMN Meeting Session 1 (February 2022)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=j_75CDPzjI4 2022 GMN Meeting Session 2 (February 2022)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=f6x9_WCVphY GMN talk at the European Space Agency&#039;s Fireball Workshop (June 2021)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=QXBTLPnPDWs 2021 GMN Meeting] - [https://www.dropbox.com/sh/ia9vagug5lxm8k9/AAB_i_1jcWThUdAHO_2gF_Ksa?dl=0 Link to slides]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=MAGq-XqD5Po Overview of the GMN - IMC2020 (September 2020)]&lt;br /&gt;
&lt;br /&gt;
: [https://www.youtube.com/watch?v=oM7lfQ4nmyw Overview of the GMN, Astro Imaging Channel presentation (May 2020)]&lt;br /&gt;
&lt;br /&gt;
=== GMN-related publications ===&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2206.11365 Vida, D., Blaauw Erskine, R. C., Brown, P. G., Kambulow, J., Campbell-Brown, M., &amp;amp; Mazur, M. J. (2022). Computing optical meteor flux using global meteor network data. Monthly Notices of the Royal Astronomical Society, 515(2), 2322-2339.]&lt;br /&gt;
&lt;br /&gt;
: [https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stab2557/6368869 Moorhead, A. V., Clements, T., &amp;amp; Vida, D. (2021). Meteor shower radiant dispersions in Global Meteor Network data. Monthly Notices of the Royal Astronomical Society, 508(1), 326-339.]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2107.12335 Vida, D., Šegon, D., Gural, P. S., Brown, P. G., McIntyre, M. J., Dijkema, T. J., Pavletić, L., Kukić, P., Mazur, M.J., Eschman, P., Roggemans, P., Merlak, A., &amp;amp; Zubović, D. (2021). The Global Meteor Network–Methodology and first results. Monthly Notices of the Royal Astronomical Society, 506(4), 5046-5074.]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/abs/2003.05458/ Moorhead, A. V., Clements, T. D., &amp;amp; Vida, D. (2020). Realistic gravitational focusing of meteoroid streams. Monthly Notices of the Royal Astronomical Society, 494(2), 2982-2994.] &lt;br /&gt;
&lt;br /&gt;
: [https://globalmeteornetwork.org/wordpress/wp-content/uploads/2018/11/Kukic-et-al-2018-Rolling-shutter.pdf  Kukić, P., Gural, P., Vida, D., Šegon, D. &amp;amp; Merlak, A. (2018) Correction for meteor centroids observed using rolling shutter cameras. WGN, Journal of the International Meteor Organization, 46:5, 154-118.]&lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/2018_WGN___RMS_sun_skirter_final.pdf  Vida, D., Mazur, M. J., Šegon, D., Kukić, P., &amp;amp; Merlak, A. (2018). Compressive strength of a skirting Daytime Arietid-first science results from low-cost Raspberry Pi-based meteor stations. WGN, Journal of the International Meteor Organization, 46, 113-118.] &lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/pdf/1911.02979.pdf Vida, D., Gural, P., Brown, P., Campbell-Brown, M., Wiegert, P. (2019) Estimating trajectories of meteors: an observational Monte Carlo approach - I. Theory. arXiv:1911.02979v4 [astro-ph.EP] 21 Apr 2020]&lt;br /&gt;
&lt;br /&gt;
: [https://arxiv.org/pdf/1911.11734.pdf Vida, D., Gural, P., Brown, P., Campbell-Brown, M., Wiegert, P. (2019) Estimating trajectories of meteors: an observational Monte Carlo approach - II. Results. arXiv:1911.11734v1 [astro-ph.EP] 26 Novr 2019]&lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/2018_WGN___RMS_first_results-final.pdf Vida, D., Mazur, M. J., Šegon, D., Zubović, D., Kukić, P., Parag, F., &amp;amp; Macan, A. (2018). First results of a Raspberry Pi based meteor camera system. WGN, Journal of the International Meteor Organization, 46, 71-78.] &lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/Vida_IMC2016_proceedings_final.pdf Vida, D., Zubović, D., Šegon, D., Gural, P., &amp;amp; Cupec, R. (2016). Open-source meteor detection software for low-cost single-board computers. In Proceedings of the International Meteor Conference (IMC2016), Egmond, The Netherlands (pp. 2-5).] &lt;br /&gt;
&lt;br /&gt;
: [https://gmn.duckdns.org/wordpress/wp-content/uploads/2018/11/Zubovic_IMC2015_priceedings_final.pdf Zubović, D., Vida, D., Gural, P., &amp;amp; Šegon, D. (2015). Advances in the development of a low-cost video meteor station. In Proceedings of the International Meteor Conference, Mistelbach, Austria (pp. 27-30).]&lt;/div&gt;</summary>
		<author><name>MeteorsABQ</name></author>
	</entry>
	<entry>
		<id>https://globalmeteornetwork.org//wiki/index.php?title=Shopping_list_and_tools_needed&amp;diff=843</id>
		<title>Shopping list and tools needed</title>
		<link rel="alternate" type="text/html" href="https://globalmeteornetwork.org//wiki/index.php?title=Shopping_list_and_tools_needed&amp;diff=843"/>
		<updated>2025-09-30T18:57:07Z</updated>

		<summary type="html">&lt;p&gt;MeteorsABQ: /* Raspberry Pi 4 or 5 */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Ordering the correct components is the most important aspect of your camera build. Review the entire list and make sure you order the correct options. If you are not sure, posta question in the forums. You also should review the list of tools to identify what may be missing. &lt;br /&gt;
&lt;br /&gt;
= Parts and tools = &lt;br /&gt;
[[File:01_annotated.jpg|thumb|right|Annotated Parts List]]&lt;br /&gt;
&lt;br /&gt;
Click the image to the right to see a larger version of the parts and tools.&lt;br /&gt;
&lt;br /&gt;
# IMX291 sensor board (IMX307 sensor board if IMX291 sensor board is sold out)&lt;br /&gt;
# Lens with the lens holder - 4mm, 6mm are M16 mount as pictured, while other lenses might be CS which have a different holder&lt;br /&gt;
# 2x M2 screws, 6mm long - for mounting lens holder &lt;br /&gt;
# Camera housing&lt;br /&gt;
# Small cable gland (supplied with the housing)&lt;br /&gt;
# Large cable gland (supplied with the housing)&lt;br /&gt;
# Camera Power over Ethernet (PoE) cable (sometimes called a network cable by the sellers)&lt;br /&gt;
# Camera board holder (supplied with the housing)&lt;br /&gt;
# Holder metal plate (supplied with the housing)&lt;br /&gt;
# 4x M2 screws, 12 mm long for mounting camera module to bracket&lt;br /&gt;
# 1x M3-.50 screw, 6mm long for mounting camera module L-bracket to base plate&lt;br /&gt;
# Metal plate screws (supplied with the housing)&lt;br /&gt;
# Transparent weatherproof silicone &lt;br /&gt;
# Housing mounting bracket (supplied with the housing)&lt;br /&gt;
# Waterproof ethernet cable protector&lt;br /&gt;
# PoE injector to supply 48v to the camera (not shown)&lt;br /&gt;
# Raspberry Pi 5 (recommended) or Raspberry Pi 4 Model B 2GB (minimum) with official power supply (not shown)&lt;br /&gt;
# Raspberry Pi housing (not shown)&lt;br /&gt;
# 128 GB or greater microSD card (not shown)&lt;br /&gt;
# Self-amalgamating tape (not shown)&lt;br /&gt;
&lt;br /&gt;
= Purchasing parts =&lt;br /&gt;
For consistency across the network and to facilitate collaborative support, it is best to use only the camera and lens listed below, instead of assembling alternatives only because they are conveniently available. The selected camera and lenses are proven and known to work well. Feel free to source other components from any convenient seller. &lt;br /&gt;
&lt;br /&gt;
Many components, such as the Pi and microSD cards, are are available from many vendors. However, AliExpress (the Chinese equivalent of eBay) is the preferred online source for a lens, camera, and housing. AliExpress serves most of the globe and has been reliably suppling parts for a long time.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Links are to current sellers but inventory levels can vary. If a link is dead or the seller is out of stock, you should be able to find an equivalent from other sellers on AliExpress.&lt;br /&gt;
&lt;br /&gt;
== Sensor ==&lt;br /&gt;
The bare IP security camera selected for the RMS system features a Sony IMX291, available from many sellers on AliExpress. Of the options offered, choose &#039;&#039;With 48V POE cable&#039;&#039; and &#039;&#039;No lens&#039;&#039;.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002315913099.html IMX-291 Hi3516Cv300]&lt;br /&gt;
&lt;br /&gt;
If the IMX-291 camera is sold out from that vendor and you cannot find another IMX-291 vendor, you may be able to locate a suitable IMX-307 sensor.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Many vendors sell IMX-307 sensor boards that are not suited for nighttime meteor recording. It is important to buy the correct IMX-307 because only a specific hardware version combined with a specific firmware version work correctly to record meteors.  &lt;br /&gt;
&lt;br /&gt;
One RMS/GMN tester offered these thoughts:&lt;br /&gt;
 &lt;br /&gt;
* The only IMX-307 worth trying is the Hangzhou Jiefeng Technology GK7205V210, aka IVG-G3S, which is distinguishable by a white square on the board. I do not recommend a blanket ‘get-any-IMX-307’ statement for new cameras because sensor boards can be very different from each other. &lt;br /&gt;
&lt;br /&gt;
* The only acceptable IMX-307 sensor boards I&#039;ve found includes the firmware version:&lt;br /&gt;
: V5.00.R02.000739AG.10010.140400.00&#039;&#039;&#039;20000&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
* A firmware version with a similar number is NOT acceptable: &lt;br /&gt;
: V5.00.R02.000739AG.10010.140400.00&#039;&#039;&#039;20010&#039;&#039;&#039;.&lt;br /&gt;
 &lt;br /&gt;
* Here is a link to Hangzhou Jiefeng Technology: [https://www.aliexpress.us/item/3256805867050500.html Hangzhou Jiefeng Technology].&lt;br /&gt;
 &lt;br /&gt;
* When you place an order, it is best to specify the characteristics of the IMX-307. For example, your request could be something like this:&lt;br /&gt;
: &#039;&#039;GK7205V210 (IVG-G3S), with white square on circuit board, and firmware version V5.00.R02.000739AG.10010.140400.0020000&#039;&#039;.&lt;br /&gt;
 &lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; These recommendations are likely to change over time, so you should check our parts list and vendor recommendations before you place an order.&lt;br /&gt;
&lt;br /&gt;
== Lens ==&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; Buy a lens separately and select only from these options.&lt;br /&gt;
&lt;br /&gt;
Most cameras available on AliExpress are sold with a choice of lenses. The preferred lens is a 4mm f/0.95 M16 lens, which provides a ~88x45° field of view (FOV). The lens also is available separately at this link.&lt;br /&gt;
: [https://www.aliexpress.com/item/32876034491.html 4mm f/0.95 M16].&lt;br /&gt;
&lt;br /&gt;
Alternative lenses (4mm and 6 mm) are available here:&lt;br /&gt;
: [https://www.aliexpress.com/item/1005003145991079.html 4mm OR 6mm f/0.95 M16]&lt;br /&gt;
&lt;br /&gt;
If you live in an area with heavy light pollution, other options are available. We recommend using only lenses from the [[Lens Options|following list]]. Other options may not be as sensitive or may have significant distortions. See [[Lens Options|this page for more lens options]].&lt;br /&gt;
&lt;br /&gt;
== Housing ==&lt;br /&gt;
A security camera housing provides weather-tight protection without the distortion of a plastic dome. From the options offered, select &#039;&#039;Plate and Bracket&#039;&#039;. The plate holds a 38x38mm bare IP camera module on an L-shaped mounting bracket. &lt;br /&gt;
: [https://www.aliexpress.com/item/32355130687.html IP66 CCTV Camera Housing with Plate and Bracket] &lt;br /&gt;
&lt;br /&gt;
This combination also provides a pair of cable glands and some essential screws.&lt;br /&gt;
&lt;br /&gt;
== Power over Ethernet (PoE) injector, PoE switch (optional), and PoE replacement camera side cables (optional, but recommended) ==&lt;br /&gt;
&lt;br /&gt;
This combination uses network cables to connect the Raspberry Pi and the camera sensor, and injects 48V DC into the network cable to power the camera. From the list, select a plug style that is appropriate for your location. &lt;br /&gt;
&lt;br /&gt;
This is an example of plug styles available.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002704227705.html PoE Injector 48V 0.5A]&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Over short cable lengths (up to about 5m), you also can use plain PoE connectors. These connectors feed 12V from a power supply into the ethernet and extract it at the other end. Over short distances, this configuration can supply the camera with adequate power without the need for 48V injectors.&lt;br /&gt;
&lt;br /&gt;
If you operate several cameras, you can use a PoE &#039;&#039;switch&#039;&#039; instead of a PoE &#039;&#039;injector&#039;&#039;, and connect all the cameras to your network. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; You must source a PoE switch locally.&lt;br /&gt;
: [https://www.tendacn.com/product/tef1110p-8-63w.html TEF1110P-8-63W 10-Port 10/100M Desktop Switch with 8-Port PoE]&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;GOOD PRACTICE:&#039;&#039;&#039; Maintain one or more spare PoE camera side cables.&lt;br /&gt;
: [https://www.aliexpress.com/item/4001297174234.html Poe cable - Select RJ45 or RJ45DC]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Alternative cable&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The picture shows only two connectors, but you will receive all connectors needed for the IMX291 board:&lt;br /&gt;
* 1 pcs 2pin port (2.0mm)&lt;br /&gt;
* 1 pcs 4pin port (1.25mm)&lt;br /&gt;
* 1 pcs 6pin port (1.25mm)&lt;br /&gt;
* 1 pcs 8pin port (1.25mm))&lt;br /&gt;
&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002598310068.html Poe Cable]&lt;br /&gt;
&lt;br /&gt;
== Cooled housing for Raspberry Pi ==&lt;br /&gt;
&lt;br /&gt;
Please buy one of the two cases below. We have tried many others, but they are not as good.&lt;br /&gt;
&lt;br /&gt;
* [https://www.aliexpress.com/item/32959825297.html Fan-cooled case.] It has relatively quiet fans, and it&#039;s sturdy. From the options offered, ensure you select one that says &amp;quot;for Pi 4&amp;quot; if you are using a Raspberry Pi 4, or &amp;quot;for Pi 3B Plus&amp;quot; if you are using a Raspberry Pi 3B+. &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; There is a case variation that is fully enclosed and has no fans; do not select this option.&lt;br /&gt;
&lt;br /&gt;
* [https://www.aliexpress.com/item/1005002510605065.html Passively cooled case.] It has no fan and so is silent without the need to replace fans in future. Many operators have found this one satisfactory if the Pi is operated in an air controlled environment. Some operators reported a diminished WiFi strength when using passive fans due to the metal covering the small antenna.&lt;br /&gt;
&lt;br /&gt;
If the Pi is in a hot environment, then choose the case with the fan. If silent operation is the priority, then go fanless but pay attention to the free circulation of air around the Pi. Case fans often use cheap sleeve bearings. If they get noisy or stop spinning later, try replacing them with fans that use ball bearings.&lt;br /&gt;
&lt;br /&gt;
For the Raspberry Pi 5, the OEM fan assembly should be purchased, which has a heat sink and fan speed controlled by the operating system as it responds to CPU temperature.&lt;br /&gt;
&lt;br /&gt;
== Real time clock (RTC) for Raspberry Pi4 ==&lt;br /&gt;
: [[File:rtc.jpg|thumb|RTC installation|200px]]&lt;br /&gt;
&lt;br /&gt;
Precise timing is essential for processing meteor data, and an RTC module assures that Raspberry Pi always has the precise time, even when power or internet is unreliable. AliExpress sells a pack of 10 but they are inexpensive, so you may want to share extras among other camera constructors in your area. &lt;br /&gt;
&lt;br /&gt;
The AliExpress store lists two RTC modules - one labelled &#039;&#039;DS3231 module&#039;&#039; and another labelled &#039;&#039;mini DS3231 module&#039;&#039;. Select the &#039;&#039;mini DS3231 module&#039;&#039; option, which is designed for the Raspberry Pi. (It has 5 pins and includes a battery.)&lt;br /&gt;
: [https://www.aliexpress.com/item/32770348851.html DS3231 RTC]&lt;br /&gt;
&lt;br /&gt;
After you plug the RTC into the Pi (see image on the right), verify that the current time is correct on the Pi, then open the terminal and run:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
sudo hwclock -w&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
This command sets the current computer time to the RTC. When the Pi boots up, it reads the correct time from the RTC.&lt;br /&gt;
&lt;br /&gt;
The Pi5 contains a built-in RTC. In most cases, the optional external battery is not needed for the Pi5&#039;s RTC.&lt;br /&gt;
&lt;br /&gt;
== Pin header ==&lt;br /&gt;
&lt;br /&gt;
This pin raises the height of the Raspberry GPIO bins so the RTC sits proud of the Raspberry Pi case. You need only 1, but the pack of 20 costs only about a dollar. &lt;br /&gt;
: [https://www.aliexpress.com/item/32549850046.html Tall header pins]&lt;br /&gt;
&lt;br /&gt;
== Network cabling ==&lt;br /&gt;
&lt;br /&gt;
You need two lengths of network cabling, one (quite short) between the Raspberry Pi and the PoE injector, and the other between the PoE injector and the camera. You should be able to easily find both of these locally, but you also can order them from AliExpress. &lt;br /&gt;
&lt;br /&gt;
Some people have found that a thin, flat network cable (shown in the figure) is useful to avoid drilling holes in walls or eaves when you want to snake a wire through a window or door. Regardless of you choice, additional sealant or insulation is required to seal the cable at the PoE connector of the camera.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002311509668.html Cat6 Flat Ethernet Cable]&lt;br /&gt;
&lt;br /&gt;
== Waterproof cable connector ==&lt;br /&gt;
&lt;br /&gt;
One end of the network cable is outdoors, connected to the PoE cable from the camera, so it must be sealed. (This connection carries data as well as 48V DC power.) &lt;br /&gt;
&lt;br /&gt;
Place the waterproof connector over the end of the network cable connector, plug the network cable into the PoE cable on the camera, then lock the connector onto the end of the PoE cable. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;GOOD PRACTICE:&#039;&#039;&#039; For extra weatherproofing, wrap the connector in self-amalgamating tape. &lt;br /&gt;
: [https://www.aliexpress.com/item/32834472563.html RJ45 Waterproof Connector Cap]&lt;br /&gt;
&lt;br /&gt;
== 128GB micro SD card or 256GB USB flash drive ==&lt;br /&gt;
&lt;br /&gt;
You can use either an SD card and a USB flash drive, but there is no need to have both. You must have at least 64GB of storage, but 128GB is recommended because 20GB of data - or more - is collected every night. The card should be fast - Class 10 UHS-1 or better. As with the cables, you can purchase a card locally or [https://www.aliexpress.com/item/32676225311.html from AliExpress]. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;WARNING:&#039;&#039;&#039; There is an &#039;&#039;&#039;[https://photographylife.com/fake-memory-cards ongoing problem with the production and sale of fraudulent memory cards that misrepresent the available storage]&#039;&#039;&#039;. Even supplies from a reputable outlet can be affected, so you should test any card you purchase. The AliExpress link has been used successfully to obtain suitable micro SD cards. If you live in North America, Costco is a reliable local source.&lt;br /&gt;
&lt;br /&gt;
If you prefer to use a USB flash drive, the [https://www.kingston.com/en/usb-flash-drives/datatraveler-kyson-high-performance-usb-flash-drive Kingston DataTraveler Kyson 256 GB] has been verified to work well. We recommend you source it locally or on [https://www.amazon.com/Kingston-DataTraveler-Kyson-256GB-DTKN/dp/B08KHZY581 amazon.com].&lt;br /&gt;
&lt;br /&gt;
== Raspberry Pi 4 or 5 ==&lt;br /&gt;
You should be able to purchase these purchased locally as well as from a domestic online source. You must have at least a 2GB RAM model, and the Raspberry Pi Model 4B is now the minimum spec. As RMS adds functionality, the 4GB or higher RAM version is suggested. Previously, a Raspberry Pi Model 3B+ was considered the minimum spec, but Pi3 does not have the performance or memory to handle busy meteor showers. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The Pi3 runs on Python 2. We are now past the July 1, 2025, cut-off point and we no longer support this version. &lt;br /&gt;
&lt;br /&gt;
: IMPORTANT:&#039;&#039;&#039; Purchase only the official 5.1V 3A 15.3W power supply for a Pi4. The Pi5 requires 5V, 5A power supply due to its increased power consumption. Most problems with Raspberry Pi units can be traced to inadequate power supplies. Please use the correct power supply for the Pi version you choose to deploy.&lt;br /&gt;
&lt;br /&gt;
== Additional items and tools ==&lt;br /&gt;
* Micro-HDMI cable: Connect a RPi 4B to a monitor.&lt;br /&gt;
* M2 and M3 screw: You may find these locally but, in some places, they may be quite difficult to locate. You may want to order hardware from the [https://www.aliexpress.com/store/4714020?spm=a2g0o.detail.1000007.1.5fc666d9tN1f8i ScrewHome Store] on AliExpress. Each [https://www.aliexpress.com/item/32981714992.html?spm=a2g0o.store_pc_groupList.8148356.10.be65539dLjPgfh packet of 50 M2x6mm, M2x12mm, and M3x6mm] machine screws costs only a few dollars.&lt;br /&gt;
* Silicone sealant: Seal the glass window and front screws in the housing.&lt;br /&gt;
* Self-amalgamating tape: Wrap and seal the cable connectors so they are weathertight.&lt;br /&gt;
* Tools:&lt;br /&gt;
: * Small wire cutters or a sharp knife&lt;br /&gt;
: * Assorted screwdrivers&lt;br /&gt;
: * Drill&lt;br /&gt;
: * RJ45 crimper to attach connectorsto the ends of the ethernet cable.&lt;br /&gt;
: * Some cameras come with a slightly different cable with a separate 12V socket for power input, as shown [https://globalmeteornetwork.org/wiki/images/d/dc/Alternatecable.jpg here]. If the power input port has a small cap, you can cover it and use the PoE on the ethernet port. If it is open, you need a pair of PoE adapters (seen in that picture in the background).&lt;br /&gt;
: * &#039;&#039;&#039;VLC&#039;&#039;&#039; software: To test and focus the camera, you must have this software. It is preinstalled on the Pi, but it also is available for Mac, Windows, or Linux from [https://www.videolan.org/vlc/ VideoLan].&lt;br /&gt;
&lt;br /&gt;
At this point, you have completed this section or you are waiting for parts. It is a good time to review the instructions for building the camera or to actually begin the process. Either way - have fun! &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_-_The_complete_how-to Back to the signpost page.]&lt;/div&gt;</summary>
		<author><name>MeteorsABQ</name></author>
	</entry>
	<entry>
		<id>https://globalmeteornetwork.org//wiki/index.php?title=Shopping_list_and_tools_needed&amp;diff=842</id>
		<title>Shopping list and tools needed</title>
		<link rel="alternate" type="text/html" href="https://globalmeteornetwork.org//wiki/index.php?title=Shopping_list_and_tools_needed&amp;diff=842"/>
		<updated>2025-09-30T18:47:45Z</updated>

		<summary type="html">&lt;p&gt;MeteorsABQ: /* Real time clock (RTC) for Raspberry Pi */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Ordering the correct components is the most important aspect of your camera build. Review the entire list and make sure you order the correct options. If you are not sure, posta question in the forums. You also should review the list of tools to identify what may be missing. &lt;br /&gt;
&lt;br /&gt;
= Parts and tools = &lt;br /&gt;
[[File:01_annotated.jpg|thumb|right|Annotated Parts List]]&lt;br /&gt;
&lt;br /&gt;
Click the image to the right to see a larger version of the parts and tools.&lt;br /&gt;
&lt;br /&gt;
# IMX291 sensor board (IMX307 sensor board if IMX291 sensor board is sold out)&lt;br /&gt;
# Lens with the lens holder - 4mm, 6mm are M16 mount as pictured, while other lenses might be CS which have a different holder&lt;br /&gt;
# 2x M2 screws, 6mm long - for mounting lens holder &lt;br /&gt;
# Camera housing&lt;br /&gt;
# Small cable gland (supplied with the housing)&lt;br /&gt;
# Large cable gland (supplied with the housing)&lt;br /&gt;
# Camera Power over Ethernet (PoE) cable (sometimes called a network cable by the sellers)&lt;br /&gt;
# Camera board holder (supplied with the housing)&lt;br /&gt;
# Holder metal plate (supplied with the housing)&lt;br /&gt;
# 4x M2 screws, 12 mm long for mounting camera module to bracket&lt;br /&gt;
# 1x M3-.50 screw, 6mm long for mounting camera module L-bracket to base plate&lt;br /&gt;
# Metal plate screws (supplied with the housing)&lt;br /&gt;
# Transparent weatherproof silicone &lt;br /&gt;
# Housing mounting bracket (supplied with the housing)&lt;br /&gt;
# Waterproof ethernet cable protector&lt;br /&gt;
# PoE injector to supply 48v to the camera (not shown)&lt;br /&gt;
# Raspberry Pi 5 (recommended) or Raspberry Pi 4 Model B 2GB (minimum) with official power supply (not shown)&lt;br /&gt;
# Raspberry Pi housing (not shown)&lt;br /&gt;
# 128 GB or greater microSD card (not shown)&lt;br /&gt;
# Self-amalgamating tape (not shown)&lt;br /&gt;
&lt;br /&gt;
= Purchasing parts =&lt;br /&gt;
For consistency across the network and to facilitate collaborative support, it is best to use only the camera and lens listed below, instead of assembling alternatives only because they are conveniently available. The selected camera and lenses are proven and known to work well. Feel free to source other components from any convenient seller. &lt;br /&gt;
&lt;br /&gt;
Many components, such as the Pi and microSD cards, are are available from many vendors. However, AliExpress (the Chinese equivalent of eBay) is the preferred online source for a lens, camera, and housing. AliExpress serves most of the globe and has been reliably suppling parts for a long time.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Links are to current sellers but inventory levels can vary. If a link is dead or the seller is out of stock, you should be able to find an equivalent from other sellers on AliExpress.&lt;br /&gt;
&lt;br /&gt;
== Sensor ==&lt;br /&gt;
The bare IP security camera selected for the RMS system features a Sony IMX291, available from many sellers on AliExpress. Of the options offered, choose &#039;&#039;With 48V POE cable&#039;&#039; and &#039;&#039;No lens&#039;&#039;.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002315913099.html IMX-291 Hi3516Cv300]&lt;br /&gt;
&lt;br /&gt;
If the IMX-291 camera is sold out from that vendor and you cannot find another IMX-291 vendor, you may be able to locate a suitable IMX-307 sensor.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Many vendors sell IMX-307 sensor boards that are not suited for nighttime meteor recording. It is important to buy the correct IMX-307 because only a specific hardware version combined with a specific firmware version work correctly to record meteors.  &lt;br /&gt;
&lt;br /&gt;
One RMS/GMN tester offered these thoughts:&lt;br /&gt;
 &lt;br /&gt;
* The only IMX-307 worth trying is the Hangzhou Jiefeng Technology GK7205V210, aka IVG-G3S, which is distinguishable by a white square on the board. I do not recommend a blanket ‘get-any-IMX-307’ statement for new cameras because sensor boards can be very different from each other. &lt;br /&gt;
&lt;br /&gt;
* The only acceptable IMX-307 sensor boards I&#039;ve found includes the firmware version:&lt;br /&gt;
: V5.00.R02.000739AG.10010.140400.00&#039;&#039;&#039;20000&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
* A firmware version with a similar number is NOT acceptable: &lt;br /&gt;
: V5.00.R02.000739AG.10010.140400.00&#039;&#039;&#039;20010&#039;&#039;&#039;.&lt;br /&gt;
 &lt;br /&gt;
* Here is a link to Hangzhou Jiefeng Technology: [https://www.aliexpress.us/item/3256805867050500.html Hangzhou Jiefeng Technology].&lt;br /&gt;
 &lt;br /&gt;
* When you place an order, it is best to specify the characteristics of the IMX-307. For example, your request could be something like this:&lt;br /&gt;
: &#039;&#039;GK7205V210 (IVG-G3S), with white square on circuit board, and firmware version V5.00.R02.000739AG.10010.140400.0020000&#039;&#039;.&lt;br /&gt;
 &lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; These recommendations are likely to change over time, so you should check our parts list and vendor recommendations before you place an order.&lt;br /&gt;
&lt;br /&gt;
== Lens ==&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; Buy a lens separately and select only from these options.&lt;br /&gt;
&lt;br /&gt;
Most cameras available on AliExpress are sold with a choice of lenses. The preferred lens is a 4mm f/0.95 M16 lens, which provides a ~88x45° field of view (FOV). The lens also is available separately at this link.&lt;br /&gt;
: [https://www.aliexpress.com/item/32876034491.html 4mm f/0.95 M16].&lt;br /&gt;
&lt;br /&gt;
Alternative lenses (4mm and 6 mm) are available here:&lt;br /&gt;
: [https://www.aliexpress.com/item/1005003145991079.html 4mm OR 6mm f/0.95 M16]&lt;br /&gt;
&lt;br /&gt;
If you live in an area with heavy light pollution, other options are available. We recommend using only lenses from the [[Lens Options|following list]]. Other options may not be as sensitive or may have significant distortions. See [[Lens Options|this page for more lens options]].&lt;br /&gt;
&lt;br /&gt;
== Housing ==&lt;br /&gt;
A security camera housing provides weather-tight protection without the distortion of a plastic dome. From the options offered, select &#039;&#039;Plate and Bracket&#039;&#039;. The plate holds a 38x38mm bare IP camera module on an L-shaped mounting bracket. &lt;br /&gt;
: [https://www.aliexpress.com/item/32355130687.html IP66 CCTV Camera Housing with Plate and Bracket] &lt;br /&gt;
&lt;br /&gt;
This combination also provides a pair of cable glands and some essential screws.&lt;br /&gt;
&lt;br /&gt;
== Power over Ethernet (PoE) injector, PoE switch (optional), and PoE replacement camera side cables (optional, but recommended) ==&lt;br /&gt;
&lt;br /&gt;
This combination uses network cables to connect the Raspberry Pi and the camera sensor, and injects 48V DC into the network cable to power the camera. From the list, select a plug style that is appropriate for your location. &lt;br /&gt;
&lt;br /&gt;
This is an example of plug styles available.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002704227705.html PoE Injector 48V 0.5A]&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Over short cable lengths (up to about 5m), you also can use plain PoE connectors. These connectors feed 12V from a power supply into the ethernet and extract it at the other end. Over short distances, this configuration can supply the camera with adequate power without the need for 48V injectors.&lt;br /&gt;
&lt;br /&gt;
If you operate several cameras, you can use a PoE &#039;&#039;switch&#039;&#039; instead of a PoE &#039;&#039;injector&#039;&#039;, and connect all the cameras to your network. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; You must source a PoE switch locally.&lt;br /&gt;
: [https://www.tendacn.com/product/tef1110p-8-63w.html TEF1110P-8-63W 10-Port 10/100M Desktop Switch with 8-Port PoE]&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;GOOD PRACTICE:&#039;&#039;&#039; Maintain one or more spare PoE camera side cables.&lt;br /&gt;
: [https://www.aliexpress.com/item/4001297174234.html Poe cable - Select RJ45 or RJ45DC]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Alternative cable&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The picture shows only two connectors, but you will receive all connectors needed for the IMX291 board:&lt;br /&gt;
* 1 pcs 2pin port (2.0mm)&lt;br /&gt;
* 1 pcs 4pin port (1.25mm)&lt;br /&gt;
* 1 pcs 6pin port (1.25mm)&lt;br /&gt;
* 1 pcs 8pin port (1.25mm))&lt;br /&gt;
&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002598310068.html Poe Cable]&lt;br /&gt;
&lt;br /&gt;
== Cooled housing for Raspberry Pi ==&lt;br /&gt;
&lt;br /&gt;
Please buy one of the two cases below. We have tried many others, but they are not as good.&lt;br /&gt;
&lt;br /&gt;
* [https://www.aliexpress.com/item/32959825297.html Fan-cooled case.] It has relatively quiet fans, and it&#039;s sturdy. From the options offered, ensure you select one that says &amp;quot;for Pi 4&amp;quot; if you are using a Raspberry Pi 4, or &amp;quot;for Pi 3B Plus&amp;quot; if you are using a Raspberry Pi 3B+. &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; There is a case variation that is fully enclosed and has no fans; do not select this option.&lt;br /&gt;
&lt;br /&gt;
* [https://www.aliexpress.com/item/1005002510605065.html Passively cooled case.] It has no fan and so is silent without the need to replace fans in future. Many operators have found this one satisfactory if the Pi is operated in an air controlled environment. Some operators reported a diminished WiFi strength when using passive fans due to the metal covering the small antenna.&lt;br /&gt;
&lt;br /&gt;
If the Pi is in a hot environment, then choose the case with the fan. If silent operation is the priority, then go fanless but pay attention to the free circulation of air around the Pi. Case fans often use cheap sleeve bearings. If they get noisy or stop spinning later, try replacing them with fans that use ball bearings.&lt;br /&gt;
&lt;br /&gt;
For the Raspberry Pi 5, the OEM fan assembly should be purchased, which has a heat sink and fan speed controlled by the operating system as it responds to CPU temperature.&lt;br /&gt;
&lt;br /&gt;
== Real time clock (RTC) for Raspberry Pi4 ==&lt;br /&gt;
: [[File:rtc.jpg|thumb|RTC installation|200px]]&lt;br /&gt;
&lt;br /&gt;
Precise timing is essential for processing meteor data, and an RTC module assures that Raspberry Pi always has the precise time, even when power or internet is unreliable. AliExpress sells a pack of 10 but they are inexpensive, so you may want to share extras among other camera constructors in your area. &lt;br /&gt;
&lt;br /&gt;
The AliExpress store lists two RTC modules - one labelled &#039;&#039;DS3231 module&#039;&#039; and another labelled &#039;&#039;mini DS3231 module&#039;&#039;. Select the &#039;&#039;mini DS3231 module&#039;&#039; option, which is designed for the Raspberry Pi. (It has 5 pins and includes a battery.)&lt;br /&gt;
: [https://www.aliexpress.com/item/32770348851.html DS3231 RTC]&lt;br /&gt;
&lt;br /&gt;
After you plug the RTC into the Pi (see image on the right), verify that the current time is correct on the Pi, then open the terminal and run:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
sudo hwclock -w&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
This command sets the current computer time to the RTC. When the Pi boots up, it reads the correct time from the RTC.&lt;br /&gt;
&lt;br /&gt;
The Pi5 contains a built-in RTC. In most cases, the optional external battery is not needed for the Pi5&#039;s RTC.&lt;br /&gt;
&lt;br /&gt;
== Pin header ==&lt;br /&gt;
&lt;br /&gt;
This pin raises the height of the Raspberry GPIO bins so the RTC sits proud of the Raspberry Pi case. You need only 1, but the pack of 20 costs only about a dollar. &lt;br /&gt;
: [https://www.aliexpress.com/item/32549850046.html Tall header pins]&lt;br /&gt;
&lt;br /&gt;
== Network cabling ==&lt;br /&gt;
&lt;br /&gt;
You need two lengths of network cabling, one (quite short) between the Raspberry Pi and the PoE injector, and the other between the PoE injector and the camera. You should be able to easily find both of these locally, but you also can order them from AliExpress. &lt;br /&gt;
&lt;br /&gt;
Some people have found that a thin, flat network cable (shown in the figure) is useful to avoid drilling holes in walls or eaves when you want to snake a wire through a window or door. Regardless of you choice, additional sealant or insulation is required to seal the cable at the PoE connector of the camera.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002311509668.html Cat6 Flat Ethernet Cable]&lt;br /&gt;
&lt;br /&gt;
== Waterproof cable connector ==&lt;br /&gt;
&lt;br /&gt;
One end of the network cable is outdoors, connected to the PoE cable from the camera, so it must be sealed. (This connection carries data as well as 48V DC power.) &lt;br /&gt;
&lt;br /&gt;
Place the waterproof connector over the end of the network cable connector, plug the network cable into the PoE cable on the camera, then lock the connector onto the end of the PoE cable. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;GOOD PRACTICE:&#039;&#039;&#039; For extra weatherproofing, wrap the connector in self-amalgamating tape. &lt;br /&gt;
: [https://www.aliexpress.com/item/32834472563.html RJ45 Waterproof Connector Cap]&lt;br /&gt;
&lt;br /&gt;
== 128GB micro SD card or 256GB USB flash drive ==&lt;br /&gt;
&lt;br /&gt;
You can use either an SD card and a USB flash drive, but there is no need to have both. You must have at least 64GB of storage, but 128GB is recommended because 20GB of data - or more - is collected every night. The card should be fast - Class 10 UHS-1 or better. As with the cables, you can purchase a card locally or [https://www.aliexpress.com/item/32676225311.html from AliExpress]. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;WARNING:&#039;&#039;&#039; There is an &#039;&#039;&#039;[https://photographylife.com/fake-memory-cards ongoing problem with the production and sale of fraudulent memory cards that misrepresent the available storage]&#039;&#039;&#039;. Even supplies from a reputable outlet can be affected, so you should test any card you purchase. The AliExpress link has been used successfully to obtain suitable micro SD cards. If you live in North America, Costco is a reliable local source.&lt;br /&gt;
&lt;br /&gt;
If you prefer to use a USB flash drive, the [https://www.kingston.com/en/usb-flash-drives/datatraveler-kyson-high-performance-usb-flash-drive Kingston DataTraveler Kyson 256 GB] has been verified to work well. We recommend you source it locally or on [https://www.amazon.com/Kingston-DataTraveler-Kyson-256GB-DTKN/dp/B08KHZY581 amazon.com].&lt;br /&gt;
&lt;br /&gt;
== Raspberry Pi 4 or 5 ==&lt;br /&gt;
You should be able to purchase these purchased locally as well as from a domestic online source. You must have at least a 2GB RAM model, and the Raspberry Pi Model 4B is now the minimum spec. Previously, a Raspberry Pi Model 3B+ was considered the minimum spec, but Pi3 does not have the performance or memory to handle busy meteor showers. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The Pi3 runs on Python 2. After July 1, 2025, we will no longer support this version. &lt;br /&gt;
&lt;br /&gt;
: IMPORTANT:&#039;&#039;&#039; Purchase only the official 5.1V 3A 15.3W power supply to go with your Pi. Most problems with Raspberry Pi units can be traced to inadequate power supplies.&lt;br /&gt;
&lt;br /&gt;
== Additional items and tools ==&lt;br /&gt;
* Micro-HDMI cable: Connect a RPi 4B to a monitor.&lt;br /&gt;
* M2 and M3 screw: You may find these locally but, in some places, they may be quite difficult to locate. You may want to order hardware from the [https://www.aliexpress.com/store/4714020?spm=a2g0o.detail.1000007.1.5fc666d9tN1f8i ScrewHome Store] on AliExpress. Each [https://www.aliexpress.com/item/32981714992.html?spm=a2g0o.store_pc_groupList.8148356.10.be65539dLjPgfh packet of 50 M2x6mm, M2x12mm, and M3x6mm] machine screws costs only a few dollars.&lt;br /&gt;
* Silicone sealant: Seal the glass window and front screws in the housing.&lt;br /&gt;
* Self-amalgamating tape: Wrap and seal the cable connectors so they are weathertight.&lt;br /&gt;
* Tools:&lt;br /&gt;
: * Small wire cutters or a sharp knife&lt;br /&gt;
: * Assorted screwdrivers&lt;br /&gt;
: * Drill&lt;br /&gt;
: * RJ45 crimper to attach connectorsto the ends of the ethernet cable.&lt;br /&gt;
: * Some cameras come with a slightly different cable with a separate 12V socket for power input, as shown [https://globalmeteornetwork.org/wiki/images/d/dc/Alternatecable.jpg here]. If the power input port has a small cap, you can cover it and use the PoE on the ethernet port. If it is open, you need a pair of PoE adapters (seen in that picture in the background).&lt;br /&gt;
: * &#039;&#039;&#039;VLC&#039;&#039;&#039; software: To test and focus the camera, you must have this software. It is preinstalled on the Pi, but it also is available for Mac, Windows, or Linux from [https://www.videolan.org/vlc/ VideoLan].&lt;br /&gt;
&lt;br /&gt;
At this point, you have completed this section or you are waiting for parts. It is a good time to review the instructions for building the camera or to actually begin the process. Either way - have fun! &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_-_The_complete_how-to Back to the signpost page.]&lt;/div&gt;</summary>
		<author><name>MeteorsABQ</name></author>
	</entry>
	<entry>
		<id>https://globalmeteornetwork.org//wiki/index.php?title=Shopping_list_and_tools_needed&amp;diff=841</id>
		<title>Shopping list and tools needed</title>
		<link rel="alternate" type="text/html" href="https://globalmeteornetwork.org//wiki/index.php?title=Shopping_list_and_tools_needed&amp;diff=841"/>
		<updated>2025-09-30T18:46:27Z</updated>

		<summary type="html">&lt;p&gt;MeteorsABQ: /* Real time clock (RTC) for Raspberry Pi */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Ordering the correct components is the most important aspect of your camera build. Review the entire list and make sure you order the correct options. If you are not sure, posta question in the forums. You also should review the list of tools to identify what may be missing. &lt;br /&gt;
&lt;br /&gt;
= Parts and tools = &lt;br /&gt;
[[File:01_annotated.jpg|thumb|right|Annotated Parts List]]&lt;br /&gt;
&lt;br /&gt;
Click the image to the right to see a larger version of the parts and tools.&lt;br /&gt;
&lt;br /&gt;
# IMX291 sensor board (IMX307 sensor board if IMX291 sensor board is sold out)&lt;br /&gt;
# Lens with the lens holder - 4mm, 6mm are M16 mount as pictured, while other lenses might be CS which have a different holder&lt;br /&gt;
# 2x M2 screws, 6mm long - for mounting lens holder &lt;br /&gt;
# Camera housing&lt;br /&gt;
# Small cable gland (supplied with the housing)&lt;br /&gt;
# Large cable gland (supplied with the housing)&lt;br /&gt;
# Camera Power over Ethernet (PoE) cable (sometimes called a network cable by the sellers)&lt;br /&gt;
# Camera board holder (supplied with the housing)&lt;br /&gt;
# Holder metal plate (supplied with the housing)&lt;br /&gt;
# 4x M2 screws, 12 mm long for mounting camera module to bracket&lt;br /&gt;
# 1x M3-.50 screw, 6mm long for mounting camera module L-bracket to base plate&lt;br /&gt;
# Metal plate screws (supplied with the housing)&lt;br /&gt;
# Transparent weatherproof silicone &lt;br /&gt;
# Housing mounting bracket (supplied with the housing)&lt;br /&gt;
# Waterproof ethernet cable protector&lt;br /&gt;
# PoE injector to supply 48v to the camera (not shown)&lt;br /&gt;
# Raspberry Pi 5 (recommended) or Raspberry Pi 4 Model B 2GB (minimum) with official power supply (not shown)&lt;br /&gt;
# Raspberry Pi housing (not shown)&lt;br /&gt;
# 128 GB or greater microSD card (not shown)&lt;br /&gt;
# Self-amalgamating tape (not shown)&lt;br /&gt;
&lt;br /&gt;
= Purchasing parts =&lt;br /&gt;
For consistency across the network and to facilitate collaborative support, it is best to use only the camera and lens listed below, instead of assembling alternatives only because they are conveniently available. The selected camera and lenses are proven and known to work well. Feel free to source other components from any convenient seller. &lt;br /&gt;
&lt;br /&gt;
Many components, such as the Pi and microSD cards, are are available from many vendors. However, AliExpress (the Chinese equivalent of eBay) is the preferred online source for a lens, camera, and housing. AliExpress serves most of the globe and has been reliably suppling parts for a long time.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Links are to current sellers but inventory levels can vary. If a link is dead or the seller is out of stock, you should be able to find an equivalent from other sellers on AliExpress.&lt;br /&gt;
&lt;br /&gt;
== Sensor ==&lt;br /&gt;
The bare IP security camera selected for the RMS system features a Sony IMX291, available from many sellers on AliExpress. Of the options offered, choose &#039;&#039;With 48V POE cable&#039;&#039; and &#039;&#039;No lens&#039;&#039;.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002315913099.html IMX-291 Hi3516Cv300]&lt;br /&gt;
&lt;br /&gt;
If the IMX-291 camera is sold out from that vendor and you cannot find another IMX-291 vendor, you may be able to locate a suitable IMX-307 sensor.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Many vendors sell IMX-307 sensor boards that are not suited for nighttime meteor recording. It is important to buy the correct IMX-307 because only a specific hardware version combined with a specific firmware version work correctly to record meteors.  &lt;br /&gt;
&lt;br /&gt;
One RMS/GMN tester offered these thoughts:&lt;br /&gt;
 &lt;br /&gt;
* The only IMX-307 worth trying is the Hangzhou Jiefeng Technology GK7205V210, aka IVG-G3S, which is distinguishable by a white square on the board. I do not recommend a blanket ‘get-any-IMX-307’ statement for new cameras because sensor boards can be very different from each other. &lt;br /&gt;
&lt;br /&gt;
* The only acceptable IMX-307 sensor boards I&#039;ve found includes the firmware version:&lt;br /&gt;
: V5.00.R02.000739AG.10010.140400.00&#039;&#039;&#039;20000&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
* A firmware version with a similar number is NOT acceptable: &lt;br /&gt;
: V5.00.R02.000739AG.10010.140400.00&#039;&#039;&#039;20010&#039;&#039;&#039;.&lt;br /&gt;
 &lt;br /&gt;
* Here is a link to Hangzhou Jiefeng Technology: [https://www.aliexpress.us/item/3256805867050500.html Hangzhou Jiefeng Technology].&lt;br /&gt;
 &lt;br /&gt;
* When you place an order, it is best to specify the characteristics of the IMX-307. For example, your request could be something like this:&lt;br /&gt;
: &#039;&#039;GK7205V210 (IVG-G3S), with white square on circuit board, and firmware version V5.00.R02.000739AG.10010.140400.0020000&#039;&#039;.&lt;br /&gt;
 &lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; These recommendations are likely to change over time, so you should check our parts list and vendor recommendations before you place an order.&lt;br /&gt;
&lt;br /&gt;
== Lens ==&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; Buy a lens separately and select only from these options.&lt;br /&gt;
&lt;br /&gt;
Most cameras available on AliExpress are sold with a choice of lenses. The preferred lens is a 4mm f/0.95 M16 lens, which provides a ~88x45° field of view (FOV). The lens also is available separately at this link.&lt;br /&gt;
: [https://www.aliexpress.com/item/32876034491.html 4mm f/0.95 M16].&lt;br /&gt;
&lt;br /&gt;
Alternative lenses (4mm and 6 mm) are available here:&lt;br /&gt;
: [https://www.aliexpress.com/item/1005003145991079.html 4mm OR 6mm f/0.95 M16]&lt;br /&gt;
&lt;br /&gt;
If you live in an area with heavy light pollution, other options are available. We recommend using only lenses from the [[Lens Options|following list]]. Other options may not be as sensitive or may have significant distortions. See [[Lens Options|this page for more lens options]].&lt;br /&gt;
&lt;br /&gt;
== Housing ==&lt;br /&gt;
A security camera housing provides weather-tight protection without the distortion of a plastic dome. From the options offered, select &#039;&#039;Plate and Bracket&#039;&#039;. The plate holds a 38x38mm bare IP camera module on an L-shaped mounting bracket. &lt;br /&gt;
: [https://www.aliexpress.com/item/32355130687.html IP66 CCTV Camera Housing with Plate and Bracket] &lt;br /&gt;
&lt;br /&gt;
This combination also provides a pair of cable glands and some essential screws.&lt;br /&gt;
&lt;br /&gt;
== Power over Ethernet (PoE) injector, PoE switch (optional), and PoE replacement camera side cables (optional, but recommended) ==&lt;br /&gt;
&lt;br /&gt;
This combination uses network cables to connect the Raspberry Pi and the camera sensor, and injects 48V DC into the network cable to power the camera. From the list, select a plug style that is appropriate for your location. &lt;br /&gt;
&lt;br /&gt;
This is an example of plug styles available.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002704227705.html PoE Injector 48V 0.5A]&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Over short cable lengths (up to about 5m), you also can use plain PoE connectors. These connectors feed 12V from a power supply into the ethernet and extract it at the other end. Over short distances, this configuration can supply the camera with adequate power without the need for 48V injectors.&lt;br /&gt;
&lt;br /&gt;
If you operate several cameras, you can use a PoE &#039;&#039;switch&#039;&#039; instead of a PoE &#039;&#039;injector&#039;&#039;, and connect all the cameras to your network. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; You must source a PoE switch locally.&lt;br /&gt;
: [https://www.tendacn.com/product/tef1110p-8-63w.html TEF1110P-8-63W 10-Port 10/100M Desktop Switch with 8-Port PoE]&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;GOOD PRACTICE:&#039;&#039;&#039; Maintain one or more spare PoE camera side cables.&lt;br /&gt;
: [https://www.aliexpress.com/item/4001297174234.html Poe cable - Select RJ45 or RJ45DC]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Alternative cable&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The picture shows only two connectors, but you will receive all connectors needed for the IMX291 board:&lt;br /&gt;
* 1 pcs 2pin port (2.0mm)&lt;br /&gt;
* 1 pcs 4pin port (1.25mm)&lt;br /&gt;
* 1 pcs 6pin port (1.25mm)&lt;br /&gt;
* 1 pcs 8pin port (1.25mm))&lt;br /&gt;
&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002598310068.html Poe Cable]&lt;br /&gt;
&lt;br /&gt;
== Cooled housing for Raspberry Pi ==&lt;br /&gt;
&lt;br /&gt;
Please buy one of the two cases below. We have tried many others, but they are not as good.&lt;br /&gt;
&lt;br /&gt;
* [https://www.aliexpress.com/item/32959825297.html Fan-cooled case.] It has relatively quiet fans, and it&#039;s sturdy. From the options offered, ensure you select one that says &amp;quot;for Pi 4&amp;quot; if you are using a Raspberry Pi 4, or &amp;quot;for Pi 3B Plus&amp;quot; if you are using a Raspberry Pi 3B+. &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; There is a case variation that is fully enclosed and has no fans; do not select this option.&lt;br /&gt;
&lt;br /&gt;
* [https://www.aliexpress.com/item/1005002510605065.html Passively cooled case.] It has no fan and so is silent without the need to replace fans in future. Many operators have found this one satisfactory if the Pi is operated in an air controlled environment. Some operators reported a diminished WiFi strength when using passive fans due to the metal covering the small antenna.&lt;br /&gt;
&lt;br /&gt;
If the Pi is in a hot environment, then choose the case with the fan. If silent operation is the priority, then go fanless but pay attention to the free circulation of air around the Pi. Case fans often use cheap sleeve bearings. If they get noisy or stop spinning later, try replacing them with fans that use ball bearings.&lt;br /&gt;
&lt;br /&gt;
For the Raspberry Pi 5, the OEM fan assembly should be purchased, which has a heat sink and fan speed controlled by the operating system as it responds to CPU temperature.&lt;br /&gt;
&lt;br /&gt;
== Real time clock (RTC) for Raspberry Pi ==&lt;br /&gt;
: [[File:rtc.jpg|thumb|RTC installation|200px]]&lt;br /&gt;
&lt;br /&gt;
Precise timing is essential for processing meteor data, and an RTC module assures that Raspberry Pi always has the precise time, even when power or internet is unreliable. AliExpress sells a pack of 10 but they are inexpensive, so you may want to share extras among other camera constructors in your area. &lt;br /&gt;
&lt;br /&gt;
The AliExpress store lists two RTC modules - one labelled &#039;&#039;DS3231 module&#039;&#039; and another labelled &#039;&#039;mini DS3231 module&#039;&#039;. Select the &#039;&#039;mini DS3231 module&#039;&#039; option, which is designed for the Raspberry Pi. (It has 5 pins and includes a battery.)&lt;br /&gt;
: [https://www.aliexpress.com/item/32770348851.html DS3231 RTC]&lt;br /&gt;
&lt;br /&gt;
After you plug the RTC into the Pi (see image on the right), verify that the current time is correct on the Pi, then open the terminal and run:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
sudo hwclock -w&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
This command sets the current computer time to the RTC. When the Pi boots up, it reads the correct time from the RTC.&lt;br /&gt;
&lt;br /&gt;
The Pi5 contains a built-in RTC. In most cases, the optional exernal battery is not needed for the Pi5&#039;s RTC.&lt;br /&gt;
&lt;br /&gt;
== Pin header ==&lt;br /&gt;
&lt;br /&gt;
This pin raises the height of the Raspberry GPIO bins so the RTC sits proud of the Raspberry Pi case. You need only 1, but the pack of 20 costs only about a dollar. &lt;br /&gt;
: [https://www.aliexpress.com/item/32549850046.html Tall header pins]&lt;br /&gt;
&lt;br /&gt;
== Network cabling ==&lt;br /&gt;
&lt;br /&gt;
You need two lengths of network cabling, one (quite short) between the Raspberry Pi and the PoE injector, and the other between the PoE injector and the camera. You should be able to easily find both of these locally, but you also can order them from AliExpress. &lt;br /&gt;
&lt;br /&gt;
Some people have found that a thin, flat network cable (shown in the figure) is useful to avoid drilling holes in walls or eaves when you want to snake a wire through a window or door. Regardless of you choice, additional sealant or insulation is required to seal the cable at the PoE connector of the camera.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002311509668.html Cat6 Flat Ethernet Cable]&lt;br /&gt;
&lt;br /&gt;
== Waterproof cable connector ==&lt;br /&gt;
&lt;br /&gt;
One end of the network cable is outdoors, connected to the PoE cable from the camera, so it must be sealed. (This connection carries data as well as 48V DC power.) &lt;br /&gt;
&lt;br /&gt;
Place the waterproof connector over the end of the network cable connector, plug the network cable into the PoE cable on the camera, then lock the connector onto the end of the PoE cable. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;GOOD PRACTICE:&#039;&#039;&#039; For extra weatherproofing, wrap the connector in self-amalgamating tape. &lt;br /&gt;
: [https://www.aliexpress.com/item/32834472563.html RJ45 Waterproof Connector Cap]&lt;br /&gt;
&lt;br /&gt;
== 128GB micro SD card or 256GB USB flash drive ==&lt;br /&gt;
&lt;br /&gt;
You can use either an SD card and a USB flash drive, but there is no need to have both. You must have at least 64GB of storage, but 128GB is recommended because 20GB of data - or more - is collected every night. The card should be fast - Class 10 UHS-1 or better. As with the cables, you can purchase a card locally or [https://www.aliexpress.com/item/32676225311.html from AliExpress]. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;WARNING:&#039;&#039;&#039; There is an &#039;&#039;&#039;[https://photographylife.com/fake-memory-cards ongoing problem with the production and sale of fraudulent memory cards that misrepresent the available storage]&#039;&#039;&#039;. Even supplies from a reputable outlet can be affected, so you should test any card you purchase. The AliExpress link has been used successfully to obtain suitable micro SD cards. If you live in North America, Costco is a reliable local source.&lt;br /&gt;
&lt;br /&gt;
If you prefer to use a USB flash drive, the [https://www.kingston.com/en/usb-flash-drives/datatraveler-kyson-high-performance-usb-flash-drive Kingston DataTraveler Kyson 256 GB] has been verified to work well. We recommend you source it locally or on [https://www.amazon.com/Kingston-DataTraveler-Kyson-256GB-DTKN/dp/B08KHZY581 amazon.com].&lt;br /&gt;
&lt;br /&gt;
== Raspberry Pi 4 or 5 ==&lt;br /&gt;
You should be able to purchase these purchased locally as well as from a domestic online source. You must have at least a 2GB RAM model, and the Raspberry Pi Model 4B is now the minimum spec. Previously, a Raspberry Pi Model 3B+ was considered the minimum spec, but Pi3 does not have the performance or memory to handle busy meteor showers. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The Pi3 runs on Python 2. After July 1, 2025, we will no longer support this version. &lt;br /&gt;
&lt;br /&gt;
: IMPORTANT:&#039;&#039;&#039; Purchase only the official 5.1V 3A 15.3W power supply to go with your Pi. Most problems with Raspberry Pi units can be traced to inadequate power supplies.&lt;br /&gt;
&lt;br /&gt;
== Additional items and tools ==&lt;br /&gt;
* Micro-HDMI cable: Connect a RPi 4B to a monitor.&lt;br /&gt;
* M2 and M3 screw: You may find these locally but, in some places, they may be quite difficult to locate. You may want to order hardware from the [https://www.aliexpress.com/store/4714020?spm=a2g0o.detail.1000007.1.5fc666d9tN1f8i ScrewHome Store] on AliExpress. Each [https://www.aliexpress.com/item/32981714992.html?spm=a2g0o.store_pc_groupList.8148356.10.be65539dLjPgfh packet of 50 M2x6mm, M2x12mm, and M3x6mm] machine screws costs only a few dollars.&lt;br /&gt;
* Silicone sealant: Seal the glass window and front screws in the housing.&lt;br /&gt;
* Self-amalgamating tape: Wrap and seal the cable connectors so they are weathertight.&lt;br /&gt;
* Tools:&lt;br /&gt;
: * Small wire cutters or a sharp knife&lt;br /&gt;
: * Assorted screwdrivers&lt;br /&gt;
: * Drill&lt;br /&gt;
: * RJ45 crimper to attach connectorsto the ends of the ethernet cable.&lt;br /&gt;
: * Some cameras come with a slightly different cable with a separate 12V socket for power input, as shown [https://globalmeteornetwork.org/wiki/images/d/dc/Alternatecable.jpg here]. If the power input port has a small cap, you can cover it and use the PoE on the ethernet port. If it is open, you need a pair of PoE adapters (seen in that picture in the background).&lt;br /&gt;
: * &#039;&#039;&#039;VLC&#039;&#039;&#039; software: To test and focus the camera, you must have this software. It is preinstalled on the Pi, but it also is available for Mac, Windows, or Linux from [https://www.videolan.org/vlc/ VideoLan].&lt;br /&gt;
&lt;br /&gt;
At this point, you have completed this section or you are waiting for parts. It is a good time to review the instructions for building the camera or to actually begin the process. Either way - have fun! &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_-_The_complete_how-to Back to the signpost page.]&lt;/div&gt;</summary>
		<author><name>MeteorsABQ</name></author>
	</entry>
	<entry>
		<id>https://globalmeteornetwork.org//wiki/index.php?title=Shopping_list_and_tools_needed&amp;diff=840</id>
		<title>Shopping list and tools needed</title>
		<link rel="alternate" type="text/html" href="https://globalmeteornetwork.org//wiki/index.php?title=Shopping_list_and_tools_needed&amp;diff=840"/>
		<updated>2025-09-30T16:45:38Z</updated>

		<summary type="html">&lt;p&gt;MeteorsABQ: /* Cooled housing for Raspberry Pi */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Ordering the correct components is the most important aspect of your camera build. Review the entire list and make sure you order the correct options. If you are not sure, posta question in the forums. You also should review the list of tools to identify what may be missing. &lt;br /&gt;
&lt;br /&gt;
= Parts and tools = &lt;br /&gt;
[[File:01_annotated.jpg|thumb|right|Annotated Parts List]]&lt;br /&gt;
&lt;br /&gt;
Click the image to the right to see a larger version of the parts and tools.&lt;br /&gt;
&lt;br /&gt;
# IMX291 sensor board (IMX307 sensor board if IMX291 sensor board is sold out)&lt;br /&gt;
# Lens with the lens holder - 4mm, 6mm are M16 mount as pictured, while other lenses might be CS which have a different holder&lt;br /&gt;
# 2x M2 screws, 6mm long - for mounting lens holder &lt;br /&gt;
# Camera housing&lt;br /&gt;
# Small cable gland (supplied with the housing)&lt;br /&gt;
# Large cable gland (supplied with the housing)&lt;br /&gt;
# Camera Power over Ethernet (PoE) cable (sometimes called a network cable by the sellers)&lt;br /&gt;
# Camera board holder (supplied with the housing)&lt;br /&gt;
# Holder metal plate (supplied with the housing)&lt;br /&gt;
# 4x M2 screws, 12 mm long for mounting camera module to bracket&lt;br /&gt;
# 1x M3-.50 screw, 6mm long for mounting camera module L-bracket to base plate&lt;br /&gt;
# Metal plate screws (supplied with the housing)&lt;br /&gt;
# Transparent weatherproof silicone &lt;br /&gt;
# Housing mounting bracket (supplied with the housing)&lt;br /&gt;
# Waterproof ethernet cable protector&lt;br /&gt;
# PoE injector to supply 48v to the camera (not shown)&lt;br /&gt;
# Raspberry Pi 5 (recommended) or Raspberry Pi 4 Model B 2GB (minimum) with official power supply (not shown)&lt;br /&gt;
# Raspberry Pi housing (not shown)&lt;br /&gt;
# 128 GB or greater microSD card (not shown)&lt;br /&gt;
# Self-amalgamating tape (not shown)&lt;br /&gt;
&lt;br /&gt;
= Purchasing parts =&lt;br /&gt;
For consistency across the network and to facilitate collaborative support, it is best to use only the camera and lens listed below, instead of assembling alternatives only because they are conveniently available. The selected camera and lenses are proven and known to work well. Feel free to source other components from any convenient seller. &lt;br /&gt;
&lt;br /&gt;
Many components, such as the Pi and microSD cards, are are available from many vendors. However, AliExpress (the Chinese equivalent of eBay) is the preferred online source for a lens, camera, and housing. AliExpress serves most of the globe and has been reliably suppling parts for a long time.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Links are to current sellers but inventory levels can vary. If a link is dead or the seller is out of stock, you should be able to find an equivalent from other sellers on AliExpress.&lt;br /&gt;
&lt;br /&gt;
== Sensor ==&lt;br /&gt;
The bare IP security camera selected for the RMS system features a Sony IMX291, available from many sellers on AliExpress. Of the options offered, choose &#039;&#039;With 48V POE cable&#039;&#039; and &#039;&#039;No lens&#039;&#039;.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002315913099.html IMX-291 Hi3516Cv300]&lt;br /&gt;
&lt;br /&gt;
If the IMX-291 camera is sold out from that vendor and you cannot find another IMX-291 vendor, you may be able to locate a suitable IMX-307 sensor.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Many vendors sell IMX-307 sensor boards that are not suited for nighttime meteor recording. It is important to buy the correct IMX-307 because only a specific hardware version combined with a specific firmware version work correctly to record meteors.  &lt;br /&gt;
&lt;br /&gt;
One RMS/GMN tester offered these thoughts:&lt;br /&gt;
 &lt;br /&gt;
* The only IMX-307 worth trying is the Hangzhou Jiefeng Technology GK7205V210, aka IVG-G3S, which is distinguishable by a white square on the board. I do not recommend a blanket ‘get-any-IMX-307’ statement for new cameras because sensor boards can be very different from each other. &lt;br /&gt;
&lt;br /&gt;
* The only acceptable IMX-307 sensor boards I&#039;ve found includes the firmware version:&lt;br /&gt;
: V5.00.R02.000739AG.10010.140400.00&#039;&#039;&#039;20000&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
* A firmware version with a similar number is NOT acceptable: &lt;br /&gt;
: V5.00.R02.000739AG.10010.140400.00&#039;&#039;&#039;20010&#039;&#039;&#039;.&lt;br /&gt;
 &lt;br /&gt;
* Here is a link to Hangzhou Jiefeng Technology: [https://www.aliexpress.us/item/3256805867050500.html Hangzhou Jiefeng Technology].&lt;br /&gt;
 &lt;br /&gt;
* When you place an order, it is best to specify the characteristics of the IMX-307. For example, your request could be something like this:&lt;br /&gt;
: &#039;&#039;GK7205V210 (IVG-G3S), with white square on circuit board, and firmware version V5.00.R02.000739AG.10010.140400.0020000&#039;&#039;.&lt;br /&gt;
 &lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; These recommendations are likely to change over time, so you should check our parts list and vendor recommendations before you place an order.&lt;br /&gt;
&lt;br /&gt;
== Lens ==&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; Buy a lens separately and select only from these options.&lt;br /&gt;
&lt;br /&gt;
Most cameras available on AliExpress are sold with a choice of lenses. The preferred lens is a 4mm f/0.95 M16 lens, which provides a ~88x45° field of view (FOV). The lens also is available separately at this link.&lt;br /&gt;
: [https://www.aliexpress.com/item/32876034491.html 4mm f/0.95 M16].&lt;br /&gt;
&lt;br /&gt;
Alternative lenses (4mm and 6 mm) are available here:&lt;br /&gt;
: [https://www.aliexpress.com/item/1005003145991079.html 4mm OR 6mm f/0.95 M16]&lt;br /&gt;
&lt;br /&gt;
If you live in an area with heavy light pollution, other options are available. We recommend using only lenses from the [[Lens Options|following list]]. Other options may not be as sensitive or may have significant distortions. See [[Lens Options|this page for more lens options]].&lt;br /&gt;
&lt;br /&gt;
== Housing ==&lt;br /&gt;
A security camera housing provides weather-tight protection without the distortion of a plastic dome. From the options offered, select &#039;&#039;Plate and Bracket&#039;&#039;. The plate holds a 38x38mm bare IP camera module on an L-shaped mounting bracket. &lt;br /&gt;
: [https://www.aliexpress.com/item/32355130687.html IP66 CCTV Camera Housing with Plate and Bracket] &lt;br /&gt;
&lt;br /&gt;
This combination also provides a pair of cable glands and some essential screws.&lt;br /&gt;
&lt;br /&gt;
== Power over Ethernet (PoE) injector, PoE switch (optional), and PoE replacement camera side cables (optional, but recommended) ==&lt;br /&gt;
&lt;br /&gt;
This combination uses network cables to connect the Raspberry Pi and the camera sensor, and injects 48V DC into the network cable to power the camera. From the list, select a plug style that is appropriate for your location. &lt;br /&gt;
&lt;br /&gt;
This is an example of plug styles available.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002704227705.html PoE Injector 48V 0.5A]&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Over short cable lengths (up to about 5m), you also can use plain PoE connectors. These connectors feed 12V from a power supply into the ethernet and extract it at the other end. Over short distances, this configuration can supply the camera with adequate power without the need for 48V injectors.&lt;br /&gt;
&lt;br /&gt;
If you operate several cameras, you can use a PoE &#039;&#039;switch&#039;&#039; instead of a PoE &#039;&#039;injector&#039;&#039;, and connect all the cameras to your network. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; You must source a PoE switch locally.&lt;br /&gt;
: [https://www.tendacn.com/product/tef1110p-8-63w.html TEF1110P-8-63W 10-Port 10/100M Desktop Switch with 8-Port PoE]&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;GOOD PRACTICE:&#039;&#039;&#039; Maintain one or more spare PoE camera side cables.&lt;br /&gt;
: [https://www.aliexpress.com/item/4001297174234.html Poe cable - Select RJ45 or RJ45DC]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Alternative cable&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The picture shows only two connectors, but you will receive all connectors needed for the IMX291 board:&lt;br /&gt;
* 1 pcs 2pin port (2.0mm)&lt;br /&gt;
* 1 pcs 4pin port (1.25mm)&lt;br /&gt;
* 1 pcs 6pin port (1.25mm)&lt;br /&gt;
* 1 pcs 8pin port (1.25mm))&lt;br /&gt;
&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002598310068.html Poe Cable]&lt;br /&gt;
&lt;br /&gt;
== Cooled housing for Raspberry Pi ==&lt;br /&gt;
&lt;br /&gt;
Please buy one of the two cases below. We have tried many others, but they are not as good.&lt;br /&gt;
&lt;br /&gt;
* [https://www.aliexpress.com/item/32959825297.html Fan-cooled case.] It has relatively quiet fans, and it&#039;s sturdy. From the options offered, ensure you select one that says &amp;quot;for Pi 4&amp;quot; if you are using a Raspberry Pi 4, or &amp;quot;for Pi 3B Plus&amp;quot; if you are using a Raspberry Pi 3B+. &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; There is a case variation that is fully enclosed and has no fans; do not select this option.&lt;br /&gt;
&lt;br /&gt;
* [https://www.aliexpress.com/item/1005002510605065.html Passively cooled case.] It has no fan and so is silent without the need to replace fans in future. Many operators have found this one satisfactory if the Pi is operated in an air controlled environment. Some operators reported a diminished WiFi strength when using passive fans due to the metal covering the small antenna.&lt;br /&gt;
&lt;br /&gt;
If the Pi is in a hot environment, then choose the case with the fan. If silent operation is the priority, then go fanless but pay attention to the free circulation of air around the Pi. Case fans often use cheap sleeve bearings. If they get noisy or stop spinning later, try replacing them with fans that use ball bearings.&lt;br /&gt;
&lt;br /&gt;
For the Raspberry Pi 5, the OEM fan assembly should be purchased, which has a heat sink and fan speed controlled by the operating system as it responds to CPU temperature.&lt;br /&gt;
&lt;br /&gt;
== Real time clock (RTC) for Raspberry Pi ==&lt;br /&gt;
: [[File:rtc.jpg|thumb|RTC installation|200px]]&lt;br /&gt;
&lt;br /&gt;
Precise timing is essential for processing meteor data, and an RTC module assures that Raspberry Pi always has the precise time, even when power or internet is unreliable. AliExpress sells a pack of 10 but they are inexpensive, so you may want to share extras among other camera constructors in your area. &lt;br /&gt;
&lt;br /&gt;
The AliExpress store lists two RTC modules - one labelled &#039;&#039;DS3231 module&#039;&#039; and another labelled &#039;&#039;mini DS3231 module&#039;&#039;. Select the &#039;&#039;mini DS3231 module&#039;&#039; option, which is designed for the Raspberry Pi. (It has 5 pins and includes a battery.)&lt;br /&gt;
: [https://www.aliexpress.com/item/32770348851.html DS3231 RTC]&lt;br /&gt;
&lt;br /&gt;
After you plug the RTC into the Pi (see image on the right), verify that the current time is correct on the Pi, then open the terminal and run:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
sudo hwclock -w&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
This command sets the current computer time to the RTC. When the Pi boots up, it reads the correct time from the RTC.&lt;br /&gt;
&lt;br /&gt;
== Pin header ==&lt;br /&gt;
&lt;br /&gt;
This pin raises the height of the Raspberry GPIO bins so the RTC sits proud of the Raspberry Pi case. You need only 1, but the pack of 20 costs only about a dollar. &lt;br /&gt;
: [https://www.aliexpress.com/item/32549850046.html Tall header pins]&lt;br /&gt;
&lt;br /&gt;
== Network cabling ==&lt;br /&gt;
&lt;br /&gt;
You need two lengths of network cabling, one (quite short) between the Raspberry Pi and the PoE injector, and the other between the PoE injector and the camera. You should be able to easily find both of these locally, but you also can order them from AliExpress. &lt;br /&gt;
&lt;br /&gt;
Some people have found that a thin, flat network cable (shown in the figure) is useful to avoid drilling holes in walls or eaves when you want to snake a wire through a window or door. Regardless of you choice, additional sealant or insulation is required to seal the cable at the PoE connector of the camera.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002311509668.html Cat6 Flat Ethernet Cable]&lt;br /&gt;
&lt;br /&gt;
== Waterproof cable connector ==&lt;br /&gt;
&lt;br /&gt;
One end of the network cable is outdoors, connected to the PoE cable from the camera, so it must be sealed. (This connection carries data as well as 48V DC power.) &lt;br /&gt;
&lt;br /&gt;
Place the waterproof connector over the end of the network cable connector, plug the network cable into the PoE cable on the camera, then lock the connector onto the end of the PoE cable. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;GOOD PRACTICE:&#039;&#039;&#039; For extra weatherproofing, wrap the connector in self-amalgamating tape. &lt;br /&gt;
: [https://www.aliexpress.com/item/32834472563.html RJ45 Waterproof Connector Cap]&lt;br /&gt;
&lt;br /&gt;
== 128GB micro SD card or 256GB USB flash drive ==&lt;br /&gt;
&lt;br /&gt;
You can use either an SD card and a USB flash drive, but there is no need to have both. You must have at least 64GB of storage, but 128GB is recommended because 20GB of data - or more - is collected every night. The card should be fast - Class 10 UHS-1 or better. As with the cables, you can purchase a card locally or [https://www.aliexpress.com/item/32676225311.html from AliExpress]. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;WARNING:&#039;&#039;&#039; There is an &#039;&#039;&#039;[https://photographylife.com/fake-memory-cards ongoing problem with the production and sale of fraudulent memory cards that misrepresent the available storage]&#039;&#039;&#039;. Even supplies from a reputable outlet can be affected, so you should test any card you purchase. The AliExpress link has been used successfully to obtain suitable micro SD cards. If you live in North America, Costco is a reliable local source.&lt;br /&gt;
&lt;br /&gt;
If you prefer to use a USB flash drive, the [https://www.kingston.com/en/usb-flash-drives/datatraveler-kyson-high-performance-usb-flash-drive Kingston DataTraveler Kyson 256 GB] has been verified to work well. We recommend you source it locally or on [https://www.amazon.com/Kingston-DataTraveler-Kyson-256GB-DTKN/dp/B08KHZY581 amazon.com].&lt;br /&gt;
&lt;br /&gt;
== Raspberry Pi 4 or 5 ==&lt;br /&gt;
You should be able to purchase these purchased locally as well as from a domestic online source. You must have at least a 2GB RAM model, and the Raspberry Pi Model 4B is now the minimum spec. Previously, a Raspberry Pi Model 3B+ was considered the minimum spec, but Pi3 does not have the performance or memory to handle busy meteor showers. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The Pi3 runs on Python 2. After July 1, 2025, we will no longer support this version. &lt;br /&gt;
&lt;br /&gt;
: IMPORTANT:&#039;&#039;&#039; Purchase only the official 5.1V 3A 15.3W power supply to go with your Pi. Most problems with Raspberry Pi units can be traced to inadequate power supplies.&lt;br /&gt;
&lt;br /&gt;
== Additional items and tools ==&lt;br /&gt;
* Micro-HDMI cable: Connect a RPi 4B to a monitor.&lt;br /&gt;
* M2 and M3 screw: You may find these locally but, in some places, they may be quite difficult to locate. You may want to order hardware from the [https://www.aliexpress.com/store/4714020?spm=a2g0o.detail.1000007.1.5fc666d9tN1f8i ScrewHome Store] on AliExpress. Each [https://www.aliexpress.com/item/32981714992.html?spm=a2g0o.store_pc_groupList.8148356.10.be65539dLjPgfh packet of 50 M2x6mm, M2x12mm, and M3x6mm] machine screws costs only a few dollars.&lt;br /&gt;
* Silicone sealant: Seal the glass window and front screws in the housing.&lt;br /&gt;
* Self-amalgamating tape: Wrap and seal the cable connectors so they are weathertight.&lt;br /&gt;
* Tools:&lt;br /&gt;
: * Small wire cutters or a sharp knife&lt;br /&gt;
: * Assorted screwdrivers&lt;br /&gt;
: * Drill&lt;br /&gt;
: * RJ45 crimper to attach connectorsto the ends of the ethernet cable.&lt;br /&gt;
: * Some cameras come with a slightly different cable with a separate 12V socket for power input, as shown [https://globalmeteornetwork.org/wiki/images/d/dc/Alternatecable.jpg here]. If the power input port has a small cap, you can cover it and use the PoE on the ethernet port. If it is open, you need a pair of PoE adapters (seen in that picture in the background).&lt;br /&gt;
: * &#039;&#039;&#039;VLC&#039;&#039;&#039; software: To test and focus the camera, you must have this software. It is preinstalled on the Pi, but it also is available for Mac, Windows, or Linux from [https://www.videolan.org/vlc/ VideoLan].&lt;br /&gt;
&lt;br /&gt;
At this point, you have completed this section or you are waiting for parts. It is a good time to review the instructions for building the camera or to actually begin the process. Either way - have fun! &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_-_The_complete_how-to Back to the signpost page.]&lt;/div&gt;</summary>
		<author><name>MeteorsABQ</name></author>
	</entry>
	<entry>
		<id>https://globalmeteornetwork.org//wiki/index.php?title=Shopping_list_and_tools_needed&amp;diff=839</id>
		<title>Shopping list and tools needed</title>
		<link rel="alternate" type="text/html" href="https://globalmeteornetwork.org//wiki/index.php?title=Shopping_list_and_tools_needed&amp;diff=839"/>
		<updated>2025-09-30T16:40:39Z</updated>

		<summary type="html">&lt;p&gt;MeteorsABQ: /* Cooled housing for Raspberry Pi */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Ordering the correct components is the most important aspect of your camera build. Review the entire list and make sure you order the correct options. If you are not sure, posta question in the forums. You also should review the list of tools to identify what may be missing. &lt;br /&gt;
&lt;br /&gt;
= Parts and tools = &lt;br /&gt;
[[File:01_annotated.jpg|thumb|right|Annotated Parts List]]&lt;br /&gt;
&lt;br /&gt;
Click the image to the right to see a larger version of the parts and tools.&lt;br /&gt;
&lt;br /&gt;
# IMX291 sensor board (IMX307 sensor board if IMX291 sensor board is sold out)&lt;br /&gt;
# Lens with the lens holder - 4mm, 6mm are M16 mount as pictured, while other lenses might be CS which have a different holder&lt;br /&gt;
# 2x M2 screws, 6mm long - for mounting lens holder &lt;br /&gt;
# Camera housing&lt;br /&gt;
# Small cable gland (supplied with the housing)&lt;br /&gt;
# Large cable gland (supplied with the housing)&lt;br /&gt;
# Camera Power over Ethernet (PoE) cable (sometimes called a network cable by the sellers)&lt;br /&gt;
# Camera board holder (supplied with the housing)&lt;br /&gt;
# Holder metal plate (supplied with the housing)&lt;br /&gt;
# 4x M2 screws, 12 mm long for mounting camera module to bracket&lt;br /&gt;
# 1x M3-.50 screw, 6mm long for mounting camera module L-bracket to base plate&lt;br /&gt;
# Metal plate screws (supplied with the housing)&lt;br /&gt;
# Transparent weatherproof silicone &lt;br /&gt;
# Housing mounting bracket (supplied with the housing)&lt;br /&gt;
# Waterproof ethernet cable protector&lt;br /&gt;
# PoE injector to supply 48v to the camera (not shown)&lt;br /&gt;
# Raspberry Pi 5 (recommended) or Raspberry Pi 4 Model B 2GB (minimum) with official power supply (not shown)&lt;br /&gt;
# Raspberry Pi housing (not shown)&lt;br /&gt;
# 128 GB or greater microSD card (not shown)&lt;br /&gt;
# Self-amalgamating tape (not shown)&lt;br /&gt;
&lt;br /&gt;
= Purchasing parts =&lt;br /&gt;
For consistency across the network and to facilitate collaborative support, it is best to use only the camera and lens listed below, instead of assembling alternatives only because they are conveniently available. The selected camera and lenses are proven and known to work well. Feel free to source other components from any convenient seller. &lt;br /&gt;
&lt;br /&gt;
Many components, such as the Pi and microSD cards, are are available from many vendors. However, AliExpress (the Chinese equivalent of eBay) is the preferred online source for a lens, camera, and housing. AliExpress serves most of the globe and has been reliably suppling parts for a long time.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Links are to current sellers but inventory levels can vary. If a link is dead or the seller is out of stock, you should be able to find an equivalent from other sellers on AliExpress.&lt;br /&gt;
&lt;br /&gt;
== Sensor ==&lt;br /&gt;
The bare IP security camera selected for the RMS system features a Sony IMX291, available from many sellers on AliExpress. Of the options offered, choose &#039;&#039;With 48V POE cable&#039;&#039; and &#039;&#039;No lens&#039;&#039;.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002315913099.html IMX-291 Hi3516Cv300]&lt;br /&gt;
&lt;br /&gt;
If the IMX-291 camera is sold out from that vendor and you cannot find another IMX-291 vendor, you may be able to locate a suitable IMX-307 sensor.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Many vendors sell IMX-307 sensor boards that are not suited for nighttime meteor recording. It is important to buy the correct IMX-307 because only a specific hardware version combined with a specific firmware version work correctly to record meteors.  &lt;br /&gt;
&lt;br /&gt;
One RMS/GMN tester offered these thoughts:&lt;br /&gt;
 &lt;br /&gt;
* The only IMX-307 worth trying is the Hangzhou Jiefeng Technology GK7205V210, aka IVG-G3S, which is distinguishable by a white square on the board. I do not recommend a blanket ‘get-any-IMX-307’ statement for new cameras because sensor boards can be very different from each other. &lt;br /&gt;
&lt;br /&gt;
* The only acceptable IMX-307 sensor boards I&#039;ve found includes the firmware version:&lt;br /&gt;
: V5.00.R02.000739AG.10010.140400.00&#039;&#039;&#039;20000&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
* A firmware version with a similar number is NOT acceptable: &lt;br /&gt;
: V5.00.R02.000739AG.10010.140400.00&#039;&#039;&#039;20010&#039;&#039;&#039;.&lt;br /&gt;
 &lt;br /&gt;
* Here is a link to Hangzhou Jiefeng Technology: [https://www.aliexpress.us/item/3256805867050500.html Hangzhou Jiefeng Technology].&lt;br /&gt;
 &lt;br /&gt;
* When you place an order, it is best to specify the characteristics of the IMX-307. For example, your request could be something like this:&lt;br /&gt;
: &#039;&#039;GK7205V210 (IVG-G3S), with white square on circuit board, and firmware version V5.00.R02.000739AG.10010.140400.0020000&#039;&#039;.&lt;br /&gt;
 &lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; These recommendations are likely to change over time, so you should check our parts list and vendor recommendations before you place an order.&lt;br /&gt;
&lt;br /&gt;
== Lens ==&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; Buy a lens separately and select only from these options.&lt;br /&gt;
&lt;br /&gt;
Most cameras available on AliExpress are sold with a choice of lenses. The preferred lens is a 4mm f/0.95 M16 lens, which provides a ~88x45° field of view (FOV). The lens also is available separately at this link.&lt;br /&gt;
: [https://www.aliexpress.com/item/32876034491.html 4mm f/0.95 M16].&lt;br /&gt;
&lt;br /&gt;
Alternative lenses (4mm and 6 mm) are available here:&lt;br /&gt;
: [https://www.aliexpress.com/item/1005003145991079.html 4mm OR 6mm f/0.95 M16]&lt;br /&gt;
&lt;br /&gt;
If you live in an area with heavy light pollution, other options are available. We recommend using only lenses from the [[Lens Options|following list]]. Other options may not be as sensitive or may have significant distortions. See [[Lens Options|this page for more lens options]].&lt;br /&gt;
&lt;br /&gt;
== Housing ==&lt;br /&gt;
A security camera housing provides weather-tight protection without the distortion of a plastic dome. From the options offered, select &#039;&#039;Plate and Bracket&#039;&#039;. The plate holds a 38x38mm bare IP camera module on an L-shaped mounting bracket. &lt;br /&gt;
: [https://www.aliexpress.com/item/32355130687.html IP66 CCTV Camera Housing with Plate and Bracket] &lt;br /&gt;
&lt;br /&gt;
This combination also provides a pair of cable glands and some essential screws.&lt;br /&gt;
&lt;br /&gt;
== Power over Ethernet (PoE) injector, PoE switch (optional), and PoE replacement camera side cables (optional, but recommended) ==&lt;br /&gt;
&lt;br /&gt;
This combination uses network cables to connect the Raspberry Pi and the camera sensor, and injects 48V DC into the network cable to power the camera. From the list, select a plug style that is appropriate for your location. &lt;br /&gt;
&lt;br /&gt;
This is an example of plug styles available.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002704227705.html PoE Injector 48V 0.5A]&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Over short cable lengths (up to about 5m), you also can use plain PoE connectors. These connectors feed 12V from a power supply into the ethernet and extract it at the other end. Over short distances, this configuration can supply the camera with adequate power without the need for 48V injectors.&lt;br /&gt;
&lt;br /&gt;
If you operate several cameras, you can use a PoE &#039;&#039;switch&#039;&#039; instead of a PoE &#039;&#039;injector&#039;&#039;, and connect all the cameras to your network. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; You must source a PoE switch locally.&lt;br /&gt;
: [https://www.tendacn.com/product/tef1110p-8-63w.html TEF1110P-8-63W 10-Port 10/100M Desktop Switch with 8-Port PoE]&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;GOOD PRACTICE:&#039;&#039;&#039; Maintain one or more spare PoE camera side cables.&lt;br /&gt;
: [https://www.aliexpress.com/item/4001297174234.html Poe cable - Select RJ45 or RJ45DC]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Alternative cable&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The picture shows only two connectors, but you will receive all connectors needed for the IMX291 board:&lt;br /&gt;
* 1 pcs 2pin port (2.0mm)&lt;br /&gt;
* 1 pcs 4pin port (1.25mm)&lt;br /&gt;
* 1 pcs 6pin port (1.25mm)&lt;br /&gt;
* 1 pcs 8pin port (1.25mm))&lt;br /&gt;
&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002598310068.html Poe Cable]&lt;br /&gt;
&lt;br /&gt;
== Cooled housing for Raspberry Pi ==&lt;br /&gt;
&lt;br /&gt;
Please buy one of the two cases below. We have tried many others, but they are not as good.&lt;br /&gt;
&lt;br /&gt;
* [https://www.aliexpress.com/item/32959825297.html Fan-cooled case.] It has relatively quiet fans, and it&#039;s sturdy. From the options offered, ensure you select one that says &amp;quot;for Pi 4&amp;quot; if you are using a Raspberry Pi 4, or &amp;quot;for Pi 3B Plus&amp;quot; if you are using a Raspberry Pi 3B+. &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; There is a case variation that is fully enclosed and has no fans; do not select this option.&lt;br /&gt;
&lt;br /&gt;
* [https://www.aliexpress.com/item/1005002510605065.html Passively cooled case.] It has no fan and so is silent without the need to replace fans in future. Many operators have found this one satisfactory if the Pi is operated in an air controlled environment. Some operators reported a diminished WiFi strength when using passive fans due to the metal covering the small antenna.&lt;br /&gt;
&lt;br /&gt;
If the Pi is in a hot environment, then choose the case with the fan. If silent operation is the priority, then go fanless but pay attention to the free circulation of air around the Pi. Case fans often use cheap sleeve bearings. If they get noisy or stop spinning later, try replacing them with fans that use ball bearings.&lt;br /&gt;
 &lt;br /&gt;
&lt;br /&gt;
For the Raspberry Pi 5, the OEM fan assembly should be purchased, which has a heat sink and fan speed controlled by the operating system as it responds to CPU temperature.&lt;br /&gt;
&lt;br /&gt;
== Real time clock (RTC) for Raspberry Pi ==&lt;br /&gt;
: [[File:rtc.jpg|thumb|RTC installation|200px]]&lt;br /&gt;
&lt;br /&gt;
Precise timing is essential for processing meteor data, and an RTC module assures that Raspberry Pi always has the precise time, even when power or internet is unreliable. AliExpress sells a pack of 10 but they are inexpensive, so you may want to share extras among other camera constructors in your area. &lt;br /&gt;
&lt;br /&gt;
The AliExpress store lists two RTC modules - one labelled &#039;&#039;DS3231 module&#039;&#039; and another labelled &#039;&#039;mini DS3231 module&#039;&#039;. Select the &#039;&#039;mini DS3231 module&#039;&#039; option, which is designed for the Raspberry Pi. (It has 5 pins and includes a battery.)&lt;br /&gt;
: [https://www.aliexpress.com/item/32770348851.html DS3231 RTC]&lt;br /&gt;
&lt;br /&gt;
After you plug the RTC into the Pi (see image on the right), verify that the current time is correct on the Pi, then open the terminal and run:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
sudo hwclock -w&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
This command sets the current computer time to the RTC. When the Pi boots up, it reads the correct time from the RTC.&lt;br /&gt;
&lt;br /&gt;
== Pin header ==&lt;br /&gt;
&lt;br /&gt;
This pin raises the height of the Raspberry GPIO bins so the RTC sits proud of the Raspberry Pi case. You need only 1, but the pack of 20 costs only about a dollar. &lt;br /&gt;
: [https://www.aliexpress.com/item/32549850046.html Tall header pins]&lt;br /&gt;
&lt;br /&gt;
== Network cabling ==&lt;br /&gt;
&lt;br /&gt;
You need two lengths of network cabling, one (quite short) between the Raspberry Pi and the PoE injector, and the other between the PoE injector and the camera. You should be able to easily find both of these locally, but you also can order them from AliExpress. &lt;br /&gt;
&lt;br /&gt;
Some people have found that a thin, flat network cable (shown in the figure) is useful to avoid drilling holes in walls or eaves when you want to snake a wire through a window or door. Regardless of you choice, additional sealant or insulation is required to seal the cable at the PoE connector of the camera.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002311509668.html Cat6 Flat Ethernet Cable]&lt;br /&gt;
&lt;br /&gt;
== Waterproof cable connector ==&lt;br /&gt;
&lt;br /&gt;
One end of the network cable is outdoors, connected to the PoE cable from the camera, so it must be sealed. (This connection carries data as well as 48V DC power.) &lt;br /&gt;
&lt;br /&gt;
Place the waterproof connector over the end of the network cable connector, plug the network cable into the PoE cable on the camera, then lock the connector onto the end of the PoE cable. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;GOOD PRACTICE:&#039;&#039;&#039; For extra weatherproofing, wrap the connector in self-amalgamating tape. &lt;br /&gt;
: [https://www.aliexpress.com/item/32834472563.html RJ45 Waterproof Connector Cap]&lt;br /&gt;
&lt;br /&gt;
== 128GB micro SD card or 256GB USB flash drive ==&lt;br /&gt;
&lt;br /&gt;
You can use either an SD card and a USB flash drive, but there is no need to have both. You must have at least 64GB of storage, but 128GB is recommended because 20GB of data - or more - is collected every night. The card should be fast - Class 10 UHS-1 or better. As with the cables, you can purchase a card locally or [https://www.aliexpress.com/item/32676225311.html from AliExpress]. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;WARNING:&#039;&#039;&#039; There is an &#039;&#039;&#039;[https://photographylife.com/fake-memory-cards ongoing problem with the production and sale of fraudulent memory cards that misrepresent the available storage]&#039;&#039;&#039;. Even supplies from a reputable outlet can be affected, so you should test any card you purchase. The AliExpress link has been used successfully to obtain suitable micro SD cards. If you live in North America, Costco is a reliable local source.&lt;br /&gt;
&lt;br /&gt;
If you prefer to use a USB flash drive, the [https://www.kingston.com/en/usb-flash-drives/datatraveler-kyson-high-performance-usb-flash-drive Kingston DataTraveler Kyson 256 GB] has been verified to work well. We recommend you source it locally or on [https://www.amazon.com/Kingston-DataTraveler-Kyson-256GB-DTKN/dp/B08KHZY581 amazon.com].&lt;br /&gt;
&lt;br /&gt;
== Raspberry Pi 4 or 5 ==&lt;br /&gt;
You should be able to purchase these purchased locally as well as from a domestic online source. You must have at least a 2GB RAM model, and the Raspberry Pi Model 4B is now the minimum spec. Previously, a Raspberry Pi Model 3B+ was considered the minimum spec, but Pi3 does not have the performance or memory to handle busy meteor showers. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The Pi3 runs on Python 2. After July 1, 2025, we will no longer support this version. &lt;br /&gt;
&lt;br /&gt;
: IMPORTANT:&#039;&#039;&#039; Purchase only the official 5.1V 3A 15.3W power supply to go with your Pi. Most problems with Raspberry Pi units can be traced to inadequate power supplies.&lt;br /&gt;
&lt;br /&gt;
== Additional items and tools ==&lt;br /&gt;
* Micro-HDMI cable: Connect a RPi 4B to a monitor.&lt;br /&gt;
* M2 and M3 screw: You may find these locally but, in some places, they may be quite difficult to locate. You may want to order hardware from the [https://www.aliexpress.com/store/4714020?spm=a2g0o.detail.1000007.1.5fc666d9tN1f8i ScrewHome Store] on AliExpress. Each [https://www.aliexpress.com/item/32981714992.html?spm=a2g0o.store_pc_groupList.8148356.10.be65539dLjPgfh packet of 50 M2x6mm, M2x12mm, and M3x6mm] machine screws costs only a few dollars.&lt;br /&gt;
* Silicone sealant: Seal the glass window and front screws in the housing.&lt;br /&gt;
* Self-amalgamating tape: Wrap and seal the cable connectors so they are weathertight.&lt;br /&gt;
* Tools:&lt;br /&gt;
: * Small wire cutters or a sharp knife&lt;br /&gt;
: * Assorted screwdrivers&lt;br /&gt;
: * Drill&lt;br /&gt;
: * RJ45 crimper to attach connectorsto the ends of the ethernet cable.&lt;br /&gt;
: * Some cameras come with a slightly different cable with a separate 12V socket for power input, as shown [https://globalmeteornetwork.org/wiki/images/d/dc/Alternatecable.jpg here]. If the power input port has a small cap, you can cover it and use the PoE on the ethernet port. If it is open, you need a pair of PoE adapters (seen in that picture in the background).&lt;br /&gt;
: * &#039;&#039;&#039;VLC&#039;&#039;&#039; software: To test and focus the camera, you must have this software. It is preinstalled on the Pi, but it also is available for Mac, Windows, or Linux from [https://www.videolan.org/vlc/ VideoLan].&lt;br /&gt;
&lt;br /&gt;
At this point, you have completed this section or you are waiting for parts. It is a good time to review the instructions for building the camera or to actually begin the process. Either way - have fun! &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_-_The_complete_how-to Back to the signpost page.]&lt;/div&gt;</summary>
		<author><name>MeteorsABQ</name></author>
	</entry>
	<entry>
		<id>https://globalmeteornetwork.org//wiki/index.php?title=Shopping_list_and_tools_needed&amp;diff=838</id>
		<title>Shopping list and tools needed</title>
		<link rel="alternate" type="text/html" href="https://globalmeteornetwork.org//wiki/index.php?title=Shopping_list_and_tools_needed&amp;diff=838"/>
		<updated>2025-09-30T16:02:50Z</updated>

		<summary type="html">&lt;p&gt;MeteorsABQ: /* Cooled housing for Raspberry Pi */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Ordering the correct components is the most important aspect of your camera build. Review the entire list and make sure you order the correct options. If you are not sure, posta question in the forums. You also should review the list of tools to identify what may be missing. &lt;br /&gt;
&lt;br /&gt;
= Parts and tools = &lt;br /&gt;
[[File:01_annotated.jpg|thumb|right|Annotated Parts List]]&lt;br /&gt;
&lt;br /&gt;
Click the image to the right to see a larger version of the parts and tools.&lt;br /&gt;
&lt;br /&gt;
# IMX291 sensor board (IMX307 sensor board if IMX291 sensor board is sold out)&lt;br /&gt;
# Lens with the lens holder - 4mm, 6mm are M16 mount as pictured, while other lenses might be CS which have a different holder&lt;br /&gt;
# 2x M2 screws, 6mm long - for mounting lens holder &lt;br /&gt;
# Camera housing&lt;br /&gt;
# Small cable gland (supplied with the housing)&lt;br /&gt;
# Large cable gland (supplied with the housing)&lt;br /&gt;
# Camera Power over Ethernet (PoE) cable (sometimes called a network cable by the sellers)&lt;br /&gt;
# Camera board holder (supplied with the housing)&lt;br /&gt;
# Holder metal plate (supplied with the housing)&lt;br /&gt;
# 4x M2 screws, 12 mm long for mounting camera module to bracket&lt;br /&gt;
# 1x M3-.50 screw, 6mm long for mounting camera module L-bracket to base plate&lt;br /&gt;
# Metal plate screws (supplied with the housing)&lt;br /&gt;
# Transparent weatherproof silicone &lt;br /&gt;
# Housing mounting bracket (supplied with the housing)&lt;br /&gt;
# Waterproof ethernet cable protector&lt;br /&gt;
# PoE injector to supply 48v to the camera (not shown)&lt;br /&gt;
# Raspberry Pi 5 (recommended) or Raspberry Pi 4 Model B 2GB (minimum) with official power supply (not shown)&lt;br /&gt;
# Raspberry Pi housing (not shown)&lt;br /&gt;
# 128 GB or greater microSD card (not shown)&lt;br /&gt;
# Self-amalgamating tape (not shown)&lt;br /&gt;
&lt;br /&gt;
= Purchasing parts =&lt;br /&gt;
For consistency across the network and to facilitate collaborative support, it is best to use only the camera and lens listed below, instead of assembling alternatives only because they are conveniently available. The selected camera and lenses are proven and known to work well. Feel free to source other components from any convenient seller. &lt;br /&gt;
&lt;br /&gt;
Many components, such as the Pi and microSD cards, are are available from many vendors. However, AliExpress (the Chinese equivalent of eBay) is the preferred online source for a lens, camera, and housing. AliExpress serves most of the globe and has been reliably suppling parts for a long time.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Links are to current sellers but inventory levels can vary. If a link is dead or the seller is out of stock, you should be able to find an equivalent from other sellers on AliExpress.&lt;br /&gt;
&lt;br /&gt;
== Sensor ==&lt;br /&gt;
The bare IP security camera selected for the RMS system features a Sony IMX291, available from many sellers on AliExpress. Of the options offered, choose &#039;&#039;With 48V POE cable&#039;&#039; and &#039;&#039;No lens&#039;&#039;.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002315913099.html IMX-291 Hi3516Cv300]&lt;br /&gt;
&lt;br /&gt;
If the IMX-291 camera is sold out from that vendor and you cannot find another IMX-291 vendor, you may be able to locate a suitable IMX-307 sensor.&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Many vendors sell IMX-307 sensor boards that are not suited for nighttime meteor recording. It is important to buy the correct IMX-307 because only a specific hardware version combined with a specific firmware version work correctly to record meteors.  &lt;br /&gt;
&lt;br /&gt;
One RMS/GMN tester offered these thoughts:&lt;br /&gt;
 &lt;br /&gt;
* The only IMX-307 worth trying is the Hangzhou Jiefeng Technology GK7205V210, aka IVG-G3S, which is distinguishable by a white square on the board. I do not recommend a blanket ‘get-any-IMX-307’ statement for new cameras because sensor boards can be very different from each other. &lt;br /&gt;
&lt;br /&gt;
* The only acceptable IMX-307 sensor boards I&#039;ve found includes the firmware version:&lt;br /&gt;
: V5.00.R02.000739AG.10010.140400.00&#039;&#039;&#039;20000&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
* A firmware version with a similar number is NOT acceptable: &lt;br /&gt;
: V5.00.R02.000739AG.10010.140400.00&#039;&#039;&#039;20010&#039;&#039;&#039;.&lt;br /&gt;
 &lt;br /&gt;
* Here is a link to Hangzhou Jiefeng Technology: [https://www.aliexpress.us/item/3256805867050500.html Hangzhou Jiefeng Technology].&lt;br /&gt;
 &lt;br /&gt;
* When you place an order, it is best to specify the characteristics of the IMX-307. For example, your request could be something like this:&lt;br /&gt;
: &#039;&#039;GK7205V210 (IVG-G3S), with white square on circuit board, and firmware version V5.00.R02.000739AG.10010.140400.0020000&#039;&#039;.&lt;br /&gt;
 &lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; These recommendations are likely to change over time, so you should check our parts list and vendor recommendations before you place an order.&lt;br /&gt;
&lt;br /&gt;
== Lens ==&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; Buy a lens separately and select only from these options.&lt;br /&gt;
&lt;br /&gt;
Most cameras available on AliExpress are sold with a choice of lenses. The preferred lens is a 4mm f/0.95 M16 lens, which provides a ~88x45° field of view (FOV). The lens also is available separately at this link.&lt;br /&gt;
: [https://www.aliexpress.com/item/32876034491.html 4mm f/0.95 M16].&lt;br /&gt;
&lt;br /&gt;
Alternative lenses (4mm and 6 mm) are available here:&lt;br /&gt;
: [https://www.aliexpress.com/item/1005003145991079.html 4mm OR 6mm f/0.95 M16]&lt;br /&gt;
&lt;br /&gt;
If you live in an area with heavy light pollution, other options are available. We recommend using only lenses from the [[Lens Options|following list]]. Other options may not be as sensitive or may have significant distortions. See [[Lens Options|this page for more lens options]].&lt;br /&gt;
&lt;br /&gt;
== Housing ==&lt;br /&gt;
A security camera housing provides weather-tight protection without the distortion of a plastic dome. From the options offered, select &#039;&#039;Plate and Bracket&#039;&#039;. The plate holds a 38x38mm bare IP camera module on an L-shaped mounting bracket. &lt;br /&gt;
: [https://www.aliexpress.com/item/32355130687.html IP66 CCTV Camera Housing with Plate and Bracket] &lt;br /&gt;
&lt;br /&gt;
This combination also provides a pair of cable glands and some essential screws.&lt;br /&gt;
&lt;br /&gt;
== Power over Ethernet (PoE) injector, PoE switch (optional), and PoE replacement camera side cables (optional, but recommended) ==&lt;br /&gt;
&lt;br /&gt;
This combination uses network cables to connect the Raspberry Pi and the camera sensor, and injects 48V DC into the network cable to power the camera. From the list, select a plug style that is appropriate for your location. &lt;br /&gt;
&lt;br /&gt;
This is an example of plug styles available.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002704227705.html PoE Injector 48V 0.5A]&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; Over short cable lengths (up to about 5m), you also can use plain PoE connectors. These connectors feed 12V from a power supply into the ethernet and extract it at the other end. Over short distances, this configuration can supply the camera with adequate power without the need for 48V injectors.&lt;br /&gt;
&lt;br /&gt;
If you operate several cameras, you can use a PoE &#039;&#039;switch&#039;&#039; instead of a PoE &#039;&#039;injector&#039;&#039;, and connect all the cameras to your network. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; You must source a PoE switch locally.&lt;br /&gt;
: [https://www.tendacn.com/product/tef1110p-8-63w.html TEF1110P-8-63W 10-Port 10/100M Desktop Switch with 8-Port PoE]&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;GOOD PRACTICE:&#039;&#039;&#039; Maintain one or more spare PoE camera side cables.&lt;br /&gt;
: [https://www.aliexpress.com/item/4001297174234.html Poe cable - Select RJ45 or RJ45DC]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Alternative cable&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The picture shows only two connectors, but you will receive all connectors needed for the IMX291 board:&lt;br /&gt;
* 1 pcs 2pin port (2.0mm)&lt;br /&gt;
* 1 pcs 4pin port (1.25mm)&lt;br /&gt;
* 1 pcs 6pin port (1.25mm)&lt;br /&gt;
* 1 pcs 8pin port (1.25mm))&lt;br /&gt;
&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002598310068.html Poe Cable]&lt;br /&gt;
&lt;br /&gt;
== Cooled housing for Raspberry Pi ==&lt;br /&gt;
&lt;br /&gt;
Please buy one of the two cases below. We have tried many others, but they are not as good.&lt;br /&gt;
&lt;br /&gt;
* [https://www.aliexpress.com/item/32959825297.html Fan-cooled case.] It has relatively quiet fans, and it&#039;s sturdy. From the options offered, ensure you select one that says &amp;quot;for Pi 4&amp;quot; if you are using a Raspberry Pi 4, or &amp;quot;for Pi 3B Plus&amp;quot; if you are using a Raspberry Pi 3B+. &#039;&#039;&#039;IMPORTANT:&#039;&#039;&#039; There is a case variation that is fully enclosed and has no fans; do not select this option.&lt;br /&gt;
&lt;br /&gt;
* [https://www.aliexpress.com/item/1005002510605065.html Passively cooled case.] It has no fan and so is silent without the need to replace fans in future. Many operators have found this one satisfactory if the Pi is operated in an air controlled environment. Some operators reported a diminished WiFi strength when using passive fans due to the metal covering the small antenna.&lt;br /&gt;
&lt;br /&gt;
If the Pi is in a hot environment, then choose the case with the fan. If silent operation is the priority, then go fanless but pay attention to the free circulation of air around the Pi.&lt;br /&gt;
&lt;br /&gt;
For the Raspberry Pi 5, the OEM fan assembly should be purchased, which has a heat sink and fan speed controlled by the operating system as it responds to CPU temperature.&lt;br /&gt;
&lt;br /&gt;
== Real time clock (RTC) for Raspberry Pi ==&lt;br /&gt;
: [[File:rtc.jpg|thumb|RTC installation|200px]]&lt;br /&gt;
&lt;br /&gt;
Precise timing is essential for processing meteor data, and an RTC module assures that Raspberry Pi always has the precise time, even when power or internet is unreliable. AliExpress sells a pack of 10 but they are inexpensive, so you may want to share extras among other camera constructors in your area. &lt;br /&gt;
&lt;br /&gt;
The AliExpress store lists two RTC modules - one labelled &#039;&#039;DS3231 module&#039;&#039; and another labelled &#039;&#039;mini DS3231 module&#039;&#039;. Select the &#039;&#039;mini DS3231 module&#039;&#039; option, which is designed for the Raspberry Pi. (It has 5 pins and includes a battery.)&lt;br /&gt;
: [https://www.aliexpress.com/item/32770348851.html DS3231 RTC]&lt;br /&gt;
&lt;br /&gt;
After you plug the RTC into the Pi (see image on the right), verify that the current time is correct on the Pi, then open the terminal and run:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
sudo hwclock -w&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
This command sets the current computer time to the RTC. When the Pi boots up, it reads the correct time from the RTC.&lt;br /&gt;
&lt;br /&gt;
== Pin header ==&lt;br /&gt;
&lt;br /&gt;
This pin raises the height of the Raspberry GPIO bins so the RTC sits proud of the Raspberry Pi case. You need only 1, but the pack of 20 costs only about a dollar. &lt;br /&gt;
: [https://www.aliexpress.com/item/32549850046.html Tall header pins]&lt;br /&gt;
&lt;br /&gt;
== Network cabling ==&lt;br /&gt;
&lt;br /&gt;
You need two lengths of network cabling, one (quite short) between the Raspberry Pi and the PoE injector, and the other between the PoE injector and the camera. You should be able to easily find both of these locally, but you also can order them from AliExpress. &lt;br /&gt;
&lt;br /&gt;
Some people have found that a thin, flat network cable (shown in the figure) is useful to avoid drilling holes in walls or eaves when you want to snake a wire through a window or door. Regardless of you choice, additional sealant or insulation is required to seal the cable at the PoE connector of the camera.&lt;br /&gt;
: [https://www.aliexpress.com/item/1005002311509668.html Cat6 Flat Ethernet Cable]&lt;br /&gt;
&lt;br /&gt;
== Waterproof cable connector ==&lt;br /&gt;
&lt;br /&gt;
One end of the network cable is outdoors, connected to the PoE cable from the camera, so it must be sealed. (This connection carries data as well as 48V DC power.) &lt;br /&gt;
&lt;br /&gt;
Place the waterproof connector over the end of the network cable connector, plug the network cable into the PoE cable on the camera, then lock the connector onto the end of the PoE cable. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;GOOD PRACTICE:&#039;&#039;&#039; For extra weatherproofing, wrap the connector in self-amalgamating tape. &lt;br /&gt;
: [https://www.aliexpress.com/item/32834472563.html RJ45 Waterproof Connector Cap]&lt;br /&gt;
&lt;br /&gt;
== 128GB micro SD card or 256GB USB flash drive ==&lt;br /&gt;
&lt;br /&gt;
You can use either an SD card and a USB flash drive, but there is no need to have both. You must have at least 64GB of storage, but 128GB is recommended because 20GB of data - or more - is collected every night. The card should be fast - Class 10 UHS-1 or better. As with the cables, you can purchase a card locally or [https://www.aliexpress.com/item/32676225311.html from AliExpress]. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;WARNING:&#039;&#039;&#039; There is an &#039;&#039;&#039;[https://photographylife.com/fake-memory-cards ongoing problem with the production and sale of fraudulent memory cards that misrepresent the available storage]&#039;&#039;&#039;. Even supplies from a reputable outlet can be affected, so you should test any card you purchase. The AliExpress link has been used successfully to obtain suitable micro SD cards. If you live in North America, Costco is a reliable local source.&lt;br /&gt;
&lt;br /&gt;
If you prefer to use a USB flash drive, the [https://www.kingston.com/en/usb-flash-drives/datatraveler-kyson-high-performance-usb-flash-drive Kingston DataTraveler Kyson 256 GB] has been verified to work well. We recommend you source it locally or on [https://www.amazon.com/Kingston-DataTraveler-Kyson-256GB-DTKN/dp/B08KHZY581 amazon.com].&lt;br /&gt;
&lt;br /&gt;
== Raspberry Pi 4 or 5 ==&lt;br /&gt;
You should be able to purchase these purchased locally as well as from a domestic online source. You must have at least a 2GB RAM model, and the Raspberry Pi Model 4B is now the minimum spec. Previously, a Raspberry Pi Model 3B+ was considered the minimum spec, but Pi3 does not have the performance or memory to handle busy meteor showers. &lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;&#039;NOTE:&#039;&#039;&#039; The Pi3 runs on Python 2. After July 1, 2025, we will no longer support this version. &lt;br /&gt;
&lt;br /&gt;
: IMPORTANT:&#039;&#039;&#039; Purchase only the official 5.1V 3A 15.3W power supply to go with your Pi. Most problems with Raspberry Pi units can be traced to inadequate power supplies.&lt;br /&gt;
&lt;br /&gt;
== Additional items and tools ==&lt;br /&gt;
* Micro-HDMI cable: Connect a RPi 4B to a monitor.&lt;br /&gt;
* M2 and M3 screw: You may find these locally but, in some places, they may be quite difficult to locate. You may want to order hardware from the [https://www.aliexpress.com/store/4714020?spm=a2g0o.detail.1000007.1.5fc666d9tN1f8i ScrewHome Store] on AliExpress. Each [https://www.aliexpress.com/item/32981714992.html?spm=a2g0o.store_pc_groupList.8148356.10.be65539dLjPgfh packet of 50 M2x6mm, M2x12mm, and M3x6mm] machine screws costs only a few dollars.&lt;br /&gt;
* Silicone sealant: Seal the glass window and front screws in the housing.&lt;br /&gt;
* Self-amalgamating tape: Wrap and seal the cable connectors so they are weathertight.&lt;br /&gt;
* Tools:&lt;br /&gt;
: * Small wire cutters or a sharp knife&lt;br /&gt;
: * Assorted screwdrivers&lt;br /&gt;
: * Drill&lt;br /&gt;
: * RJ45 crimper to attach connectorsto the ends of the ethernet cable.&lt;br /&gt;
: * Some cameras come with a slightly different cable with a separate 12V socket for power input, as shown [https://globalmeteornetwork.org/wiki/images/d/dc/Alternatecable.jpg here]. If the power input port has a small cap, you can cover it and use the PoE on the ethernet port. If it is open, you need a pair of PoE adapters (seen in that picture in the background).&lt;br /&gt;
: * &#039;&#039;&#039;VLC&#039;&#039;&#039; software: To test and focus the camera, you must have this software. It is preinstalled on the Pi, but it also is available for Mac, Windows, or Linux from [https://www.videolan.org/vlc/ VideoLan].&lt;br /&gt;
&lt;br /&gt;
At this point, you have completed this section or you are waiting for parts. It is a good time to review the instructions for building the camera or to actually begin the process. Either way - have fun! &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[https://globalmeteornetwork.org/wiki/index.php?title=Build_%26_Install_%26_Setup_your_camera_-_The_complete_how-to Back to the signpost page.]&lt;/div&gt;</summary>
		<author><name>MeteorsABQ</name></author>
	</entry>
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