Equatorial ozone profiles from the Solar Maximum Mission - A comparison with theory

Details Equatorial ozone profiles from the Solar Maximum Mission - A comparison with theory Equatorial ozone profiles from the Solar Maximum Mission - A comparison with theory

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984p%26ss...32..503a&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 32, April 1984, p. 503-513.

Computer Science

9

Altitude, Equatorial Atmosphere, Mesosphere, Ozonometry, Solar Maximum Mission, Ultraviolet Spectrometers, Absorption Cross Sections, Atmospheric Composition, Equinoxes, Photochemical Reactions, Solar Flux, Stellar Occultation, Sunset, Water Vapor

Scientific paper

The UV spectrometer polarimeter on the Solar Maximum Mission has been utilized to measure mesospheric O3 altitude profiles by the technique of solar occultation. Sunset data are presented for 1980, during the fall equinoctal period within + or - 20 deg of the geographic equator. Mean O3 concentrations are (40, 16, 5.5, and 1.5) x 10 to the 9th/cu cm at 50, 55, 60, and 65 km, respectively. Some profiles exhibit altitude structure which is wavelike. The mean O3 profile is fit best with the results of a time-dependent model if the assumed water-vapor mixing ratio employed varies from 6 ppm at 65 km.

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