An intercomparison of mesospheric ozone profiles determined by the UVSP and SAGE II solar occultation experiments

Details An intercomparison of mesospheric ozone profiles determined by the UVSP and SAGE II solar occultation experiments An intercomparison of mesospheric ozone profiles determined by the UVSP and SAGE II solar occultation experiments

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989p%26ss...37...97a&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 37, Jan. 1989, p. 97-104.

Computer Science

6

Atmospheric Composition, Mesosphere, Ozonometry, Polarimetry, Sage Satellite, Ultraviolet Spectrometers, Error Analysis, Optical Thickness

Scientific paper

A comparison is made of individual UVSP and SAGE II mesospheric ozone profiles between 50 and 70 km altitude as determined by the solar occultation technique. The generally good agreement between the two data sets below about 57 km leads to the conclusion that they may be considered as complementary, thus extending the effective altitude range of both. Comparison of the long-term ozone trend at 55.5 km shows a systematic difference of a few percent between the two measurements.

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