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Sky Clarity
Arne and anyone else that wants to answer,
I am working on a "Sky Clarity" detector. The idea is to measure the
radiation loss to free space. So far the device looks promising.
My idea is that for tass telescopes this might be a good way to select the
best photometric nights. Big telescopes would probably also want good
"seeing", but I doubt that "seeing" makes much difference for tass
measurements. What I hope to measure is how much stuff is between the
telescope and space.
I would like to put this measure in the .fits header.
Is there some "official" fits header term to use?
Tom Droege