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.
Baffle design for telescopes with tiltable secondary mirrors
Recent trends in optical systems design ; 1987 ; Los Angeles, CA, United States
01.01.1987
Aufsatz (Konferenz)
Keine Angabe
Englisch
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