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The flight of SAGE III on ISS

机译:SAGE III在国际空间站上的飞行

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The Stratospheric Aerosol and Gas Experiment (SAGE)-III, an EOS instrument, will fly on three platforms beginning in 1999 with a flight aboard the Russian METEOR 3M spacecraft in a sunsynchronous orbit. SAGE III utilizes the occultatio n technique, both solar and lunar, to provide high resolution profiles of a number of species including ozone, water vapor, aerosol, and temperature. it is especially capable of measuring long term global change in these species. The METEOR 3M oribit yields polar measurements primarily and, therefore, a spaceraft in a mid-to-high inclination is needed to yield near-global coverage. The International Space Station (ISS) orbit inclination of 51.6 deg provides this additional coverage and SAGE III is scheduled to fly on ISS in 2002. The thire SAGE III instrument will be flown in a future flight of opportunity having a high inclination robit to replace and complement the METEOR 3M coverage. This paper will describe these SAGE III missions, with emphasis on the ISS flight including the coverage provided, the science this flight provides, and the mission uniques for its implementation.
机译:EOS仪器“平流层气溶胶和气体实验(SAGE)-III”将从1999年开始在三个平台上飞行,并由俄罗斯METEOR 3M航天器在太阳同步轨道上飞行。 SAGE III利用太阳和月球的掩星技术来提供包括臭氧,水蒸气,气溶胶和温度在内的许多物种的高分辨率图像。它尤其能够测量这些物种的长期全球变化。 METEOR 3M oribit主要产生极坐标测量值,因此,需要以中高倾角的太空筏产生近乎全局的覆盖范围。国际空间站(ISS)的51.6度轨道倾角提供了这一额外的覆盖范围,SAGE III计划于2002年在ISS上飞行。这架SAGE III仪器将在未来的机会中飞行,具有高倾角可替代和补充METEOR 3M的覆盖范围。本文将介绍SAGE III的这些任务,重点是ISS的飞行,包括所提供的覆盖范围,该飞行提供的科学知识以及其实施的独特任务。

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