Empirical model of plasma convection at latitudes of the main ionization trough

Details Empirical model of plasma convection at latitudes of the main ionization trough Empirical model of plasma convection at latitudes of the main ionization trough

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ge%26ae..24..515f&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 24, May-June 1984, p. 515-517. In Russian.

Computer Science

Sound

Convective Flow, Ionospheric Drift, Ionospheric Ion Density, Polar Regions, Reception Diversity, Space Plasmas, Atmospheric Models, Drift Rate, F Region, Ionospheric Sounding

Scientific paper

The proposed empirical model is based on measurements of plasma drift velocity using the short-baseline diversity reception technique at Zhigansk (L = 4) and Iakutsk (L = 3). Results obtained with the model indicate that the principal mechanism for the formation of the main trough is weak plasma convection at subauroral latitudes in conditions of the absence of ionization sources and the 'impoverishment' of F-region plasma due to the usual recombination processes.

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