Upper Mesospheric Ozone Density Profile Retrievals from the OSIRIS Instrument

Details Upper Mesospheric Ozone Density Profile Retrievals from the OSIRIS Instrument Upper Mesospheric Ozone Density Profile Retrievals from the OSIRIS Instrument

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agusmsa31a..04s&link_type=abstract

American Geophysical Union, Spring Meeting 2009, abstract #SA31A-04

Astronomy and Astrophysics

Astrophysics

7500 Solar Physics, Astrophysics, And Astronomy

Scientific paper

Since 2001 the Canadian built instrument OSIRIS aboard the Odin satellite has been observing the middle atmosphere at wavelengths spanning from near UV to IR. In the upper mesosphere oxygen A-band dayglow observations, at 762 nm, are used to retrieve global ozone density profiles. The retrieval method, results, seasonal variations, and errors are discussed along with cross-validation of OSIRIS ozone profiles with those of the SABER instrument aboard TIMED.

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