Hi John
Here is a quick explanation. There are 3 images you can take as follows:
1. Your "light" or sky image which is the object you want to capture.
2. A "dark frame" which is an image with the lens cap on, at the same exposure of the sky image, so you are effectively taking an image of the thermal noise of the ccd chip.
3. A "flat field" which is essentially an image of a flat, evenly illuminated surface. A crude example would be a white wall, although I have built a “light box”. If you had a perfect optical system, the flat field would look like a white rectangle. But, due to vignetting, light gradients and dust motes, you will see variations in the white rectangle.
I have included 4 examples from the previous evening.
Original 180 sec image (includes sky image, thermal noise (exaggerated to show effects) and dust bunnies)
Dark frame (thermal noise).
Flat field (produced by my evenly illuminated light box believe it or not)
The sky image dark frame subtracted and flat fielded to just leave the image details.
Also, take a look here for a more in depth explanation.
http://www.atscope.com.au/techhelp.html
Cheers
Dennis