Dynamo currents representing geomagnetic L variation demonstrated by a multi-layer ionospheric model

Details Dynamo currents representing geomagnetic L variation demonstrated by a multi-layer ionospheric model Dynamo currents representing geomagnetic L variation demonstrated by a multi-layer ionospheric model

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984p%26ss...32..629x&link_type=abstract

Planetary and Space Science (ISSN 0032-0632), vol. 32, May 1984, p. 629-633.

Physics

Atmospheric Models, Dynamo Theory, Geomagnetism, Ionospheric Currents, Magnetic Variations, Atmospheric Stratification, Auroral Zones, Lunar Tides, Midlatitude Atmosphere, Polar Caps

Scientific paper

A multi-layer ionospheric model and lunar (2,2) tidal mode have been used to calculate dynamo current systems representing lunar geomagnetic semidiurnal variations. Since both the height variation of the ionospheric conductivities and latitudinal dependence of the height of the conductivity peaks have been taken into account, the dynamo current systems agree with equivalent ones (estimated from geomagnetic data) better than those for a thin shell model of the ionospheric conductivity, especially in the polar region.

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