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New results from CRISTA

机译:克里斯塔的新结果

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摘要

Trace gas distributions and temperatures in the mesosphere and lower thermosphere were derived from infrared spectra measured by the two CRISTA experiments flown in November 1994 and in August 1997. CRISTA (CRyogenic Infrared Spectrometers and Telescopes for the Atmosphere) is a triple telescope cryogenically cooled infrared spectrometer which senses the Earth limb from a Shuttle orbit. The geographical coverage was -57°+68° and -74°+74° during the two missions, respectively. Each mission lasted slightly more than one week. The mesospheric set of trace gases include ozone, carbon dioxide and carbon monoxide, methane, water vapor, and atomic oxygen. In addition temperatures and pressures are obtained from the CO_2 15 μm band. The temperature/pressure results are used to derive geostrophic wind fields. Most of the data reduction required non-LTE modelling of the radiation properties of the species. Practically all data exhibit considerable large scale structures in both latitude and longitude due to planetary waves or interhemispheric transport.
机译:介绍气体分布和介质的温度和低温从1994年11月和1997年8月在1997年11月播出的二手试验测量的红外光谱来源于克里斯塔(低温红外光谱仪和大气的望远镜)是一款三重望远镜低温冷却红外光谱仪从穿梭轨道中感测地球肢体。两个任务中,地理覆盖率分别为-57°+ 68°和-74°+ 74°。每个任务持续超过一周。 Mesompheric的痕量气体套包括臭氧,二氧化碳和一氧化碳,甲烷,水蒸气和原子氧。此外,从CO_215μm波段获得温度和压力。温度/压力结果用于衍生出脱节性的风场。大多数数据减少所需的物种辐射性能的非LTE建模。实际上所有数据由于行星波或间歇式运输而在纬度和经度都表现出相当大的大规模结构。

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