1994
DOI: 10.1117/12.190146
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<title>Contamination measurements during development and testing of the SPIRIT III cryogenic infrared telescope</title>

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Cited by 6 publications
(4 citation statements)
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“…The level of scattered radiation is an extremely sensitive function of particulate contamination levels on the cryogenic primary mirror. 15 Because signi cant particle generation was expected and observed with all mechanical cover openings on MSX, we planned to open the SPIRIT III cover after all other sys- tems had been operatedin orbit. This delay also permitted molecular outgassing to decay to lower levels.…”
Section: Spirit III Cover Ejectionmentioning
confidence: 99%
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“…The level of scattered radiation is an extremely sensitive function of particulate contamination levels on the cryogenic primary mirror. 15 Because signi cant particle generation was expected and observed with all mechanical cover openings on MSX, we planned to open the SPIRIT III cover after all other sys- tems had been operatedin orbit. This delay also permitted molecular outgassing to decay to lower levels.…”
Section: Spirit III Cover Ejectionmentioning
confidence: 99%
“…Analysis of the frequency change during the CQCM TGA warming cycle provides a measure of mass fraction removed as a function of temperature. Essentially all of the deposition evaporated between 26 and 34 K, with the peak rate at 31 K. Based on controlled laboratory experiments 14 and ground testing, 15 we identi ed the deposited material as mainly molecular oxygen, O 2 , arising from the redistribution of atmospheric oxygen condensed during prelaunch cryogenic cooling.…”
Section: Cryogenic Film Depositionmentioning
confidence: 99%
“…16 This capability proved invaluable during SPIRIT III testing, both prior to and following its integration onto the spacecraft.…”
Section: Cleaning and Inspectionsmentioning
confidence: 99%
“…A 72-A layer of material, deposited on the CQCM in was not a significant source of stray light in the SPIRIT III sensor, the 1-min interval following the cover release, was subsequently The range of BRDF values measured for the SPIRIT III primary identified as argon by thermogravimetric analysis, a procedure that mirror during the prelaunch period from 1991 to the April 1994 is monitors the depletion rate of material mass on the CQCM surface reviewed and discussed in Ref. 15. The preflight BRDF measureas its temperature is slowly increased to specify the evaporation ments of the assembled instrument were made with a portable BRDF temperature, the species, and the approximate film thickness.…”
Section: Msx Prelaunch Brdf Data Measurementsmentioning
confidence: 99%