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ATM Airy disk frustrations
There is a question at the end of this. <g>
The term "airy disk" appeared here a little while back. I ask a
couple questions about it by email, and didn't grasp it. I
downloaded several astronomy glossaries. One said it was something
discovered by an Italian. another said it was a diffraction pattern
from a star. The ATM FAQ glossary didn't have it at all.
Yesterday I got my new copy of Texereau. I gleefully looked in the
index. Nothing. I went for the glossary. NO GLOSSARY!
I started reading. "Airy disk" didn't appear immediately, but it
said Airy described "defraction disk."
OK, diffraction disk.
Texereau's discussion starts with the diffraction disk and works back
from that to a formula. But I still haven't figured out exactly what
causes the airy disk/difraction disk.
In testing, a pinhole is used and obviously causes diffraction at the
edges of the material around the pin hole. What causes diffraction
of a "point source" star? Is it the intervening media (space dust?
Earth's atmosphere?), or is it something at the scope itself?
Jim L
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