Mesospheric O3, H and H2O at high latitudes - A theoretical model

Details Mesospheric O3, H and H2O at high latitudes - A theoretical model Mesospheric O3, H and H2O at high latitudes - A theoretical model

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981p%26ss...29..819b&link_type=abstract

Planetary and Space Science, vol. 29, Aug. 1981, p. 819-823.

Other

5

Atmospheric Composition, Atmospheric Moisture, Hydrogen Atoms, Mesosphere, Ozone, Polar Regions, Atmospheric Chemistry, Atmospheric Heating, Atmospheric Models, Solar Terrestrial Interactions

Scientific paper

The high latitude thermosphere is characterized by a large heat input which produces a strong wind field. In a previous work (Rodrigo et al., 1981), the modification of the vertical transport mechanisms produced by high latitude horizontal winds was studied. The resulting concentration profiles are used here to study the influence at mesospheric levels. An improved agreement with experimental measurements is obtained. High solar zenithal angles could explain other differences between the high and middle latitude mesospheres, especially below approximately 80 km.

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