1996
DOI: 10.1117/12.258304
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<title>Total pressure sensor results from the early operations phase of the MSX mission</title>

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Cited by 9 publications
(4 citation statements)
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“…The pressure increase produced by the venting was observed for approximately 6 h. We believe that the argon vent was stuck open because of frozen material, redundantvalve competition, or mechanical effects. 11 A result of this extended venting is cooling of the SPIRIT III cover by 6 ± C during the extended release period in response to gas expansion cooling and argon boiling-point depression. Once the venting stopped, the cover temperature stopped cooling and continued its upward trend.…”
Section: Spirit III Aperture Cover Ventingmentioning
confidence: 99%
“…The pressure increase produced by the venting was observed for approximately 6 h. We believe that the argon vent was stuck open because of frozen material, redundantvalve competition, or mechanical effects. 11 A result of this extended venting is cooling of the SPIRIT III cover by 6 ± C during the extended release period in response to gas expansion cooling and argon boiling-point depression. Once the venting stopped, the cover temperature stopped cooling and continued its upward trend.…”
Section: Spirit III Aperture Cover Ventingmentioning
confidence: 99%
“…These results have been published elsewhere. 9 The expected ionospheric and contaminant species were used to identify the types of ions to be measured in the IMS spectral calibration. 10 Ionospheric species at the MSX altitude of 900 km are predominantlyH C , He C , and O C based on the InternationalReference Ionosphere.…”
Section: Contamination Monitoring Instruments and Their Ground Calibrmentioning
confidence: 99%
“…Among these phenomena are the measurements of the early operation pressure decay, the calculation of the linear and rotational velocity of a cryogenic telescope cover as it was jettisoned from the spacecraft, detection of electrons in the auroral regions, measurement of pressure spikes during quiescent periods, the environmental effects of an intense solar bake (SECOT) of the instrument section, the effects of instrument shadowing on localized pressure, and finally the long term decay of water trapped in the spacecraft thermal blankets during ground processing. [1][2][3][4][5][6][7] Whereas most of the previous papers concentrated on several of the witnessed phenomena, this paper will focus solely on the evolution of water from the thermal blankets and discuss the depth of the water reservoir. The thermal blankets were very carefully processed prior to launch and were baked out to remove as much water as possible.…”
Section: Introductionmentioning
confidence: 99%