Baffle Design For Telescopes With Tiltable Secondary Mirrors

Paul K. Davis

doi:10.1117/12.940217

10 June 1987 Baffle Design For Telescopes With Tiltable Secondary Mirrors

Paul K. Davis

Author Affiliations +

Proceedings Volume 0766, Recent Trends in Optical Systems Design and Computer Lens Design Workshop; (1987) https://doi.org/10.1117/12.940217
Event: OE LASE'87 and EO Imaging Symposium, 1987, Los Angeles, CA, United States

Abstract

A procedure is presented for the design of primary and secondary baffles (light shields) for telescopes with tiltable secondary mirrors (typically for use in the infrared). The procedure is applied to the Space Infrared Telescope Facility (SIRTF) for which results are presented.

Citation Download Citation

Paul K. Davis "Baffle Design For Telescopes With Tiltable Secondary Mirrors", Proc. SPIE 0766, Recent Trends in Optical Systems Design and Computer Lens Design Workshop, (10 June 1987); https://doi.org/10.1117/12.940217

ACCESS THE FULL ARTICLE

INSTITUTIONAL
Select your institution to access the SPIE Digital Library.

SELECT YOUR INSTITUTION

PERSONAL
Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.

PERSONAL SIGN IN

No SPIE Account? Create one

;

PURCHASE THIS CONTENT

SUBSCRIBE TO DIGITAL LIBRARY

50 downloads per 1-year subscription

Members: $195

Non-members: $335 ADD TO CART

25 downloads per 1 - year subscription

Members: $145

Non-members: $250 ADD TO CART

PURCHASE SINGLE ARTICLE