I have a question about imaging eclipses in general, and even though it's relevant to the 2024 eclipse cutting Mexico and the US, I figured this would apply to all eclipses, so I wanted to ask it in a more general subforum.
I imaged the 2017 eclipse with a 5D Mark II mounted to my C9.25, and was very happy with the images it produced. The disk of the Sun fit well onto the image sensor, as did prominences.
However, a small issue arose when trying to get the corona. I was able to fit enough of the corona in frame in the wide-dimension of the image sensor to be happy; however, I had to slew the telescope back and forth slightly along the shorter dimension of the image sensor to get shots of the corona in those directions, and then stitch them together after the fact.
For 2024, I'm considering using a focal reducer. However, I'm at the I-don't-know-what-I-don't-know stage. If I use a focal reducer, will I actually get more field of view imaged onto the sensor? I'm seeing some mentions here and there of there being vignetting issues, but I don't know how this actually will play out. I'm worried that I'm going to reduce the magnification, but also reduce the size of the imaging circle, so I end up not really gaining much.
Thoughts? What am I not considering? Like I said, I'm early in exploring this specific topic, so I'd love some input. Thanks in advance.
