F-region dynamo in the evening - Interpretation of equatorial Delta D anomaly found by MAGSAT

Details F-region dynamo in the evening - Interpretation of equatorial Delta D anomaly found by MAGSAT F-region dynamo in the evening - Interpretation of equatorial Delta D anomaly found by MAGSAT

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983jatp...45..401t&link_type=abstract

Journal of Atmospheric and Terrestrial Physics (ISSN 0021-9169), vol. 45, June 1983, p. 401-408. Research supported by the Unive

Physics

29

Dynamo Theory, F Region, Ionospheric Currents, Magnetic Variations, Magsat Satellites, Evening, Ionospheric Conductivity, Solar Activity Effects

Scientific paper

The F-region dynamo is examined to explain anomalous variations of the magnetic D-component observed by MAGSAT. Meridional currents caused by neutral pressure gradients can well reproduce this event, including the dependence on solar activity. Eastward winds are also consistent with these observations. The role of the F-region dynamo is discussed in relation to electric fields and currents in the whole ionosphere.

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