Physics
Scientific paper
Jun 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984p%26ss...32..667r&link_type=abstract
Planetary and Space Science (ISSN 0032-0633), vol. 32, June 1984, p. 667-684. Research supported by the Science and Engineering
Physics
76
Auroral Zones, Gravity Waves, Thermosphere, Vertical Motion, Winds Aloft, Arctic Regions, Fabry-Perot Interferometers, Time Response
Scientific paper
Vertical winds of tens of meters/sec or more are a ubiquitous feature of the upper thermosphere's wind field in those polar regions that are under the direct influence of magnetospheric energy and momentum sources. In periods of moderate geomagnetic activity, there are regions of systematic vertical winds which exhibit a diurnal variation. Such winds, and large systematic downward winds at times of large disturbances on the poleward boundary of the afternoon auroral oval, appear to be associated with downward divergences or upward convergences of the ion drag-induced horizontal winds acting in addition to the variety of high latitudinal heat sources. Much stronger upward winds which are observed in association with the expansion phase of geomagnetic disturbances are strongly timeand space-dependent and have to be placed in the context of very large disturbances of the horizontal wind field.
Charleton P. J.
Lloyd Nicole
McCormac F. G.
Rees David
Smith Reginald W.
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