Figuring out the source of stray light can be tricky. I have a similar halo problem with my system. Here is what I get around a bright star.
📷 Halo_Example.jpg
I run an ASA600, which is an F/7 RC with a field flattener, Chroma filters, and a Moravian camera with a IMX455 sensor. I use an ONAG guider in my system but @Mark McComiskey runs exactly the same telescope with the same filters and sensor without an ONAG and he has exactly the same halos. So, we’ve ruled out the ONAG as a possible source of this problem. (The ONAG does introduce some minor strays but they are not colored halos that look like this.) I don’t have the optical prescription for the field flattener so I can’t ray trace it to see if it’s causing this problem. To test its effect, I made a special adapter so that I could remove the reducer from optical train. The strays didn’t change at all when I removed the flattener, so it is definitely not the cause.
If I measure the size of the halos, I get 428 pixels (for the diameter of the outer red ring), which is 1.61 mm. Using the relationship shown below, that means that the reflecting surface must be 5.6 mm in front of the sensor surface, which has to be the camera window—if we assume that sensor is reflecting the light from the focused image. It certainly cannot be coming from a direct reflection from the filters.
📷 image.png
Now for the mystery. Where are the colors coming from?? At first, I thought the colors might come from diffraction from the periodic rectangular structure in the sensor; however, if that were the case, the diffraction pattern would look like two crossed rectangular “Sinc” functions, which would not have circular symmetry. We could get colors if the light were coming from a stray reflection from the color filters but they sit much further from the sensor. I looked at a double bounce within the filter but with my spacings, that produces a stray that is much smaller than what I measure. So, I’m stumped.
So, how do we get reflections from the camera window? As you know, bare glass has a reflectivity of about 4% in air. If you put a single ¼ wave layer of MgF2, you can cut the reflectivity by almost a third. If you use a higher quality, multi-layer broadband coating, you can get to about 0.5% reflectivity. The highest performance coatings can approach 0.2% - 0.25% reflectivity.
📷 image.png📷 image.png
The problem is that as the coatings become more sophisticated, making them perform well becomes increasingly more difficult. Little things like the ambient humidity can affect the performance of the coatings. Getting these coatings exactly right every single time in production is challenging. The result is that the optical performance can vary a fair amount between coating batches. So, without testing, some cameras may have windows that perform better than others.
I have a new camera on order to replace a camera on my refractor so I hope to try it on the ASA scope first to see if it works any better than the camera now on the scope. The idea is that perhaps the windows come from different coating batches and hence may have different AR properties. Mark and I currently have the same strays but @Wolfgang Promper , with the same scope and camera, doesn’t have the problem. The most likely source of the problem is the camera window but again, that doesn’t explain the colors!
Looking at the OP’s halos, my first impression is that they look too large to be coming from the camera window but of course that will vary with the focal ratio and the spacing. It would be helpful to know how far the sensor sits behind the window in that particular camera.
John