Thermal Analysis of a Helium II-Cooled Infrared Telescope for Spacelab
Infrared (IR) astronomical and atmospheric research is a relatively young field of scientific effort. The IR spectral range extends from 0.72 to about 1000 μm. Large amounts of energy in the universe are irradiated at infrared wavelengths from cool objects such as stars, planets, atmospheres of planets, ionized gas, and interstellar dust regions.
KeywordsMethane Dioxide Dust Enthalpy Ozone
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- 1.“Large Infrared Telescope on Spacelab-LIRTS,” ESA DP/PS (76) 18 (May 1976).Google Scholar
- 2.F. C. Witteborn and L. S. Young, “A Cooled Infrared Telescope of the SPACE SHUTTLE—the SPACELAB Infrared Telescope Facility (SIRTF)”, paper No. 76-174 presented at AIAA 14th Aerospace Sciences Meeting, Washington, D.C., January 26–28, 1976.Google Scholar
- 3.“IRAS-Report of the Joint Scientific Mission Definition Team for an Infrared Astronomical Satellite” (May 1976).Google Scholar
- 4.C. W. Keller, “Fiberglass Supports for Cryogenic Tanks,” paper presented at Cryogenic Workshop, Marshall Space Flight Center, Huntsville, Alabama, March 29–30, 1972.Google Scholar
- 5.G. Klein, Brennstoff-Wärme-Kraft 28: 223 (1976).Google Scholar
- 6.R. B. Scott, Cryogenic Engineering, D. Van Nostrand, Inc., Princeton, New Jersey (1959).Google Scholar
- 7.R. J. Frainier, in: Advances in Cryogenic Engineering, Vol. 6, Plenum Press, New York (1961), p. 20.Google Scholar