Baffle design for telescopes with tiltable secondary mirrorsA 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.
Document ID
19880034442
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Davis, Paul K. (NASA Ames Research Center; Sterling Software Moffett Field, CA, United States)