UARS的HALOE O3和H2O观测与地面和气球测量的比较

J. Russell, L. Gordley, P. Purcell, K. Stone
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引用次数: 0

摘要

HALOE实验于1991年9月12日美国东部时间7:11:04由发现号航天飞机在UARS卫星上发射。经过一段时间的排气后,HALOE于10月11日开始进行常规科学观测。HALOE采用太阳掩星的实验方法、气体过滤器和宽带辐射计仪器技术,测量HC、HF、CH4、NO、NO2、H2O、O3、气溶胶和温度与压力的垂直剖面。测量范围很广,从某些情况下的对流层上层到一氧化氮情况下的热层下层。掩星几何图形提供的纬度覆盖范围在一年的时间里从南纬80°到北纬80°。这个实验已经进行了三年多,基本上没有任何缺陷。根据在大气外观测太阳时的最大信号变化来判断,仪器在这段时间内的稳定性≤2%至3%。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Comparison of HALOE O3 and H2O Observations from UARS with Ground and Balloonborne Measurements
The HALOE experiment was launched on the UARS satellite by the Space Shuttle Discovery at 7:11:04 EDT on September 12, 1991. After allowing for a period of outgassing, HALOE began taking routine science observations on October 11. HALOE uses the experiment approach of solar occultation and the gas filter and broad band radiometer instrument techniques to measure vertical profiles of HCℓ, HF, CH4, NO, NO2, H2O, O3, aerosol, and temperature versus pressure. The measurements cover a broad altitude range from the upper troposphere in some cases to the lower thermosphere in the case of nitric oxide. Latitude coverage provided by the occultation geometry ranges from 80 ° S to 80 °N over the course of one year. The experiment has operated essentially without flaw for more than three years. Instrument stability over this time, as judged by the maximum signal change when viewing the sun exoatmospherically, is ≤ 2 to 3 %.
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