A2

—y1

r1

^ ( "

—2y1

\n) 2

r1

Since, for the "axial" image in the Schiefspiegler, the pupil can be considered as being at the mirror for both M1 and M2, we calculate A2 in this case as though M2 were a primary, using (3.334). Then

Was this article helpful?

0 0
Telescopes Mastery

Telescopes Mastery

Through this ebook, you are going to learn what you will need to know all about the telescopes that can provide a fun and rewarding hobby for you and your family!

Get My Free Ebook


Post a comment