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EARTH SCIENCE WITH THE STRATOSPHERIC AEROSOL AND GAS EXPERIMENT III (SAGE III) ON THE INTERNATIONAL SPACE STATION

机译:地球科学与平流层气溶胶和天然气实验III(Sage III)在国际空间站

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The Stratospheric Aerosol and Gas Experiment (SAGE) III is the fourth generation of solar occultation instruments operated by NASA, the first coming under a different acronym, to investigate the Earth's upper atmosphere. Three flight-ready SAGE III instruments were built by Ball Aerospace in the late 1990s, with one launched aboard the former Russian Aviation and Space Agency (now known as Roskosmos) Meteor-3M platform on 10 December 2001 (continuing until the platform lost power in 2006). Another of the original instruments was manifested for the ISS in the 2004 time frame, but was delayed because of budgetary considerations. Fortunately, that SAGE III/ISS mission was restarted in 2009 with a major focus upon filling an anticipated gap in ozone and aerosol observation in the second half of this decade. A related paper by Anderson et al. discusses the mission architecture and its implementation. Here we discuss the data that will be produced by SAGE III/ISS, including their expected accuracy and coverage.
机译:平流层气溶胶和天然气实验(SAGE)III是NASA经营的第四代太阳掩星仪器,该术语首次出现在不同的首字母缩略词,调查地球的高层大气层。三个飞行的Sage III仪器由1990年代后期由Ball Aeropace建造的仪器,其中一名推出了前俄罗斯航空和空间局(现称为Roskosmos)Meteor-3M平台(持续到平台损失势力2006)。另一个原始乐器在2004年时间框架中表现出在ISS中,但由于预算考虑因素而延迟。幸运的是,圣人III / ISS特派团于2009年重新开始,重点是填补了本十年下半年臭氧和气溶胶观测的预期差距。 Anderson等人的相关文件。讨论了使命架构及其实施。在这里,我们讨论了Sage III / ISS生产的数据,包括其预期的准确性和覆盖范围。

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