Abstract
We report the design and testing of a compact system of baffles for cooled infrared telescopes. The baffle system consists of a reflecting forebaffle and a black aftbaffle and provides a high level of rejection of emission from off-axis sources. The forebaffle reflects radiation incident at angles greater than 40° off axis out of the telescope, thereby reducing the aperture heat load. The black aftbaffle absorbs radiation scattered or diffracted by the forebaffle, as well as radiation from sources within 40° off axis. We describe ground-based measurements at λ = 0.9 μm of the baffle system at ambient temperature and rocketborne measurements at far-infrared wavelengths of the baffle system at ~3 K. The effective emissivity of the cooled forebaffle was measured to be 7 × 10−3. The system has been successfully used in rocketborne measurements of the diffuse infrared background and will be used in the Infrared Telescope in Space.
© 1995 Optical Society of America
Full Article | PDF ArticleMore Like This
Massimo Gervasi, Paolo de Bernardis, Marco De Petris, Silvia Masi, and Giampaolo Pisano
Appl. Opt. 37(19) 4277-4283 (1998)
Takashi Onaka, Toyoji Yagi, Hiroshi Shibai, Hiroshi Murakami, Toshihiko Tanabè, and Tsuguo Kohno
Appl. Opt. 33(10) 1880-1888 (1994)
Christopher Morbey and J. B. Hutchings
Appl. Opt. 32(19) 3570-3584 (1993)