Overview of the EOS Aura Mission

被引：291

作者：

Schoeberl, MR ^{[1
]}

Douglass, AR

Hilsenrath, E

Bhartia, PK

Beer, R

Waters, JW

Gunson, MR

Froidevaux, L

Gille, JC

Barnett, JJ

Levelt, PE

DeCola, P

机构：

[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[2] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA

[3] Univ Colorado, Boulder, CO 80309 USA

[4] Univ Oxford, Oxford OX1 2JD, England

[5] Royal Dutch Meteorol Inst, KNMI, KSAS, NL-3730 AE De Bilt, Netherlands

[6] NASA, Washington, DC 20546 USA

来源：

IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING | 2006年 / 44卷 / 05期

关键词：

atmospheric composition; Aura; Earth Observing Sytem (EOS); remote sensing; satellites;

D O I：

10.1109/TGRS.2005.861950

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

Aura, the last of the large Earth Observing System observatories, was launched on July 15, 2004. Aura is designed to make comprehensive stratospheric and tropospheric composition measurements from its four instruments, the High Resolution Dynamics Limb Sounder (HIRDLS), the Microwave Limb Sounder (MLS), the Ozone Monitoring Instrument (OMI), and the Tropospheric Emission Spectrometer (TES). With the exception of HIRDLS, all of the instruments are performing as expected, and HIRDLS will likely be able to deliver most of their planned data products. We summarize the mission, instruments, and synergies in this paper.

引用

页码：1066 / 1074

页数：9

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