Norton R H, Rinsland C P
Appl Opt. 1991 Feb 1;30(4):389-400. doi: 10.1364/AO.30.000389.
The ATMOS (atmospheric trace molecule spectroscopy) instrument, a high speed Fourier transform spectrometer operating in the middle IR (2.2-16 microm), recorded more than 1500 solar spectra at approximately 0.0105-cm(-1) resolution during its first mission onboard the shuttle Challenger in the spring of 1985. These spectra were acquired during high sun conditions for studies of the solar atmosphere and during low sun conditions for studies of the earth's upper atmosphere. This paper describes the steps by which the telemetry data were converted into spectra suitable for analysis, the analysis software and methods developed for the atmospheric and solar studies, and the ATMOS data analysis facility.
大气痕量分子光谱仪(ATMOS)是一台工作在中红外波段(2.2 - 16微米)的高速傅里叶变换光谱仪。1985年春,它在“挑战者”号航天飞机上执行首次任务期间,以约0.0105厘米⁻¹的分辨率记录了1500多个太阳光谱。这些光谱是在太阳高度较高的条件下获取的,用于研究太阳大气;以及在太阳高度较低的条件下获取的,用于研究地球高层大气。本文描述了将遥测数据转换为适合分析的光谱的步骤、为大气和太阳研究开发的分析软件及方法,以及ATMOS数据分析设施。