遥感
校准
辐射定标
摄谱仪
航天器
轨道飞行器
辐射定年
轨道力学
物理
木星(火箭家族)
紫外线
环境科学
天文
光学
地质学
卫星
量子力学
谱线
作者
Michael W. Davis,T. K. Greathouse,G. R. Gladstone,K. D. Retherford,D. C. Slater,S. A. Stern,M. H. Versteeg
摘要
Four compact planetary ultraviolet spectrographs have been built by Southwest Research Institute and successfully operated on different planetary missions. These spectrographs underwent a series of ground radiometric calibrations before delivery to their respective spacecraft. In three of the four cases, the in-flight measured sensitivity was approximately 50% lower than the ground measurement. Recent tests in the Southwest Research Institute Ultraviolet Radiometric Calibration Facility (UV-RCF) explain the discrepancy between ground and flight results. Revised ground calibration results are presented for the Rosetta-Alice, New Horizons-Alice, the Lunar Reconnaissance Orbiter Lyman- Alpha Mapping Project, and Juno-Ultraviolet Spectrograph (UVS) and are then compared to the original ground and flight calibrations. The improved understanding of the calibration system reported here will result in improved ground calibration of the upcoming Jupiter Icy Moons Explorer (JUICE)-UVS.
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