Validation of the Aura Ozone Monitoring Instrument total column ozone product

被引:173
作者
McPeters, R. [1 ]
Kroon, M. [3 ]
Labow, G. [4 ]
Brinksma, E. [3 ]
Balis, D. [2 ]
Petropavlovskikh, I. [5 ]
Veefkind, J. P. [3 ]
Bhartia, P. K. [1 ]
Levelt, P. F. [3 ]
机构
[1] NASA, Goddard Space Flight Ctr, Atmospheres Lab, Greenbelt, MD 20771 USA
[2] Aristotle Univ Thessaloniki, GR-54124 Thessaloniki, Greece
[3] Royal Netherlands Meteorol Inst, NL-3730 AE De Bilt, Netherlands
[4] Sci Syst & Applicat Inc, Lanham, MD 20706 USA
[5] NOAA, ESRL, Boulder, CO 80305 USA
关键词
D O I
10.1029/2007JD008802
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
This paper is an overview of the validation of the total column ozone data products from the Ozone Monitoring Instrument (OMI) on board the NASA EOS- Aura satellite. OMI is an imaging UV/visible spectrometer that maps global ozone on a daily basis. There are two ozone products from OMI, one derived using the traditional TOMS retrieval algorithm and another derived using a Differential Optical Absorption Spectroscopy algorithm that is being developed to take advantage of the hyperspectral capabilities of OMI. Validation is primarily performed through comparison with a network of Dobson and Brewer ground stations and secondarily through campaigns conducted specifically to validate Aura. Comparison with an ensemble of 76 Northern Hemisphere ground stations shows that OMI-TOMS total column ozone averages 0.4% higher than the station average, with station-to-station standard deviation of +/- 0.6%. The comparison shows that the OMI-TOMS ozone was stable over the 2-year period with no evidence of drift relative to the ground network. The OMI-DOAS product is also stable but with a 1.1% offset and a seasonal variation of +/- 2%. During four aircraft validation campaigns using the NASA DC-8 and WB-57 aircraft, ozone above the aircraft was measured using an actinic flux instrument and compared with OMI ozone. These comparisons showed agreement within 2% over a broad range of latitude and viewing conditions. Only during the high-latitude flights did the OMI-DOAS ozone show the effects of a solar zenith angle dependent error.
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页数:9
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