In practicing for the eclipse I have run into something that I do not understand.
I am using a Nikon D810 camera, a ZWO FF80 APO telescope F7.5 600mm focal length 80mm aperature, and an ND5 solar film filter from Spectrum Telescope.
When I use the Configuration Wizard to create a script, it is using an ISO of 100 and calculating an exposure of 1/1000 for the partial phases. I tested this on and the images of the full disc are VERY dark. So dark that you can barely see the image of the sun. I edited the images and I need 4 to 5 stops before the disk becomes a dark orange color (which I believe is properly exposed).
I can certainly edit the script to increase the ISO or the exposure time, or both. But my question is, how do I know that the calculations for the exposures during totality are going to be correct if the calculated exposures for the partial phases is not correct???
Any explanation of why these images seem so underexposed and what to do about totality would be GREATLY appreciated.
Tim.