In-flight performance of the Ozone Monitoring Instrument

被引：4
|
作者：
Schenkeveld, V. M. Erik [1 ]
Jaross, Glen [2 ]
Marchenko, Sergey [3 ]
Haffner, David [3 ]
Kleipool, Quintus L. [1 ]
Rozemeijer, Nico C. [4 ]
Veefkind, J. Pepijn [1 ,5 ]
Levelt, Pieternel F. [1 ,5 ]
机构：
[1] Royal Netherlands Meteorol Inst KNMI, De Bilt, Netherlands
[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA
[3] Sci Syst & Applicat Inc, Lanham, MD USA
[4] TriOpSys BV, Utrecht, Netherlands
[5] Delft Univ Technol, Fac Civil Engn & Geosci, Delft, Netherlands
来源：
ATMOSPHERIC MEASUREMENT TECHNIQUES | 2017年 / 10卷 / 05期
关键词：
GOMOS; NM;
D O I：
10.5194/amt-10-1957-2017
中图分类号：
P4 [大气科学（气象学）];
学科分类号：
0706 ; 070601 ;
摘要：
The Dutch-Finnish Ozone Monitoring Instrument (OMI) is an imaging spectrograph flying on NASA's EOS Aura satellite since 15 July 2004. OMI is primarily used to map trace-gas concentrations in the Earth's atmosphere, obtaining mid-resolution (0.4-0.6 nm) ultraviolet-visible (UVVIS; 264-504 nm) spectra at multiple (30-60) simultaneous fields of view. Assessed via various approaches that include monitoring of radiances from selected ocean, land ice and cloud areas, as well as measurements of line profiles in the solar spectra, the instrument shows low optical degradation and high wavelength stability over the mission lifetime. In the regions relatively free from the slowly unraveling "row anomaly" (RA) the OMI irradiances have degraded by 38 %, while radiances have changed by 1-2 %. The long-term wavelength calibration of the instrument remains stable to 0.005-0.020 nm.
引用
收藏
页码：1957 / 1986
页数：30
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