Empirical model for general circulation of the atmosphere at ionospheric levels above 100 km

Details Empirical model for general circulation of the atmosphere at ionospheric levels above 100 km Empirical model for general circulation of the atmosphere at ionospheric levels above 100 km

May 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978p%26ss...26..387v&link_type=abstract

Planetary and Space Science, Volume 26, Issue 5, p. 387-398.

Physics

Scientific paper

This paper presents an empirical model for space-time distribution of the basic parameters of the general circulation of the atmosphere at ionospheric levels (E-and F-regions). The model is based on the results of a physico-statistical analysis of experimental data on the measurement of horizontal ionospheric drifts by close spaced receivers, carried out by the world network of stations in 1958-1970. This model allows an evaluation of the motion parameters at a given latitude, local time, season and the level of solar activity to be made. The limitations and shortcomings of the model are discussed, the results are compared with theoretical and semi-empirical schemes of the atmospheric general circulation, as well as with data of both rocket measurements of wind and drift measurements of plasma by the method of incoherent scatter of radio waves. The physics of the results obtained are stressed. The characteristics of the model are tested and defined using the materials af the coordinated program of drift measurements in the E-region from 8 stations of the northern hemisphere in 1971-1974. The characteristics of motions at higher latitudes and the longitudinal effect are discussed.

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