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@ova103, Let me know if it does NOT answer your question. |
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My Observations & troubleshooting over the years: But even with that workaround, the newer exposure algorithm makes the thresholding a challenge to dial in because most the images are fairly close to eachother in brightness regardless of stars or clouds. I've debated working with some of the AI agents out there to find different methods to select which images go into the startrails production - be it starpoint/blob-detection, local contrast, edge detection, even frequency separation. All while maintaining the stability of the RPI computers, and using the existing data/metadata to not have to reprogram/design the entire wheel. Just need to find time.. mainly time to understand/interpret/intuit C++. Can't promise fast movement on the task though. just throwing out some random ideas that have run through my brain while trying to troubleshoot his pesky issue over the years |
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@EricClaeys , here are a few examples of my night time images. In order to get any type of startrails to be successful, I've had to narrow my What I've noticed over the years: prior to the new exposure algorithm, the exposure time/gain was fairly constant at what it was manually set to - this allowed the user to tune the night time images decently. The non-startrails problem was that clouds and moon would end up blowing out the images at times, skyrocketing the brightness of the cloudy and moon filled images, hence the need for the new exposure. The skyrocketing is what made the thresholding work so well, clear images were usually always darker, so they could be pulled out easier. Cloudy usually always brighter, along with the moon. With the new exposure, the cloudy images & some of the moonlit images are pulled down decently to not be as glaringly different. But this brought the image brightness's fairly close together regardless of clear/cloudy, making the threshold value a lot harder to set to have it be reliably successful from night to night, week to week, and over the year. If the star & the cloud images are the similar brightness, they're both making it into the startrails. |
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The 7 items i the Issue list was a brain dump so in whatever order my brain decided. Possibly the only connection is they would all improve startrails.
We most likely wouldn't change the names of the files to add any information. That would break all sorts of things that look for files with names of
I'm thinking with the database you won't need to navigate anything. I understand that "seeing" the files in a "day" or "night" folder is easy to comprehend visually, though Re: --run-test (or a better name!)
Definitely in the file name - the names have to be unique, and hopefully also on the image, although maybe not in v2025.xx.xx since that will require changes to the module and overlay systems, and IMHO is a really nice thing to have, but still works without it.
It's easy to adjust the parameters and with only 50 or so images it's fairly quick to run so we could error on the side of "more" startrails to pick from rather than "fewer".
What data are you thinking about?
@Alex-developer, can you please answer this paragraph?
Just thinking out loud... Re: star count module saving data
I just added this as number 8 in the Issue. |
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Agree 100%
Clouds at a dark site are black but in a light polluted location they can be very bright. The dark clouds could easily be below the Brightness Threshold setting and hence added to the startrails. Being "newer" and maybe "less experienced" than the rest of us I view as a positive which we need, since I want to make sure Allsky is usable for folks like you. I think that's our biggest user base. Thanks - Eric |
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Pillow is an image processing library for python. After I've selected my list of files, I loop through them. Before the loop, I create a blank image that is all black and the same size and my allsky images. Inside the loop, I use My attempts at removing clouds has involved first creating a mask by making a Finally, I use the mask and the To your last question, I would not use the time and gain to correct the images themselves for display. My rpiHQ camera goes from as low as 2 microseconds exposure at noon to my maximum set of 20 seconds at night. That's 7 orders of magnitude of exposure which would require representing the brightness as a float64 to capture that dynamic range properly. However, when scanning through images to gauge brightness, you will have far more luck if you do I will take a look at the issue and see if I have any additional comments. |
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Hello,
A question on startrails: In my stratrails I see as well day and night images, although angle has been set to -6 or some other days to -12.
You can see it here: see upper left corner where DAY and NIGHT appears
However, in the documentation I read that only images of the night will be used
So why would day images be used in my strartrail?
Thanks for the feedback
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