The effect of solar-wind parameters on geomagnetic activity

Details The effect of solar-wind parameters on geomagnetic activity The effect of solar-wind parameters on geomagnetic activity

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ge%26ae..22..257v&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 22, Mar.-Apr. 1982, p. 257-262. In Russian.

Computer Science

1

Auroral Zones, Geomagnetism, Interplanetary Magnetic Fields, Magnetic Storms, Solar Terrestrial Interactions, Solar Wind Velocity, Annual Variations, Magnetic Poles, Summer, Winter

Scientific paper

The paper examines the effect of solar wind velocity and the polarity of the By component of the interplanetary magnetic field on geomagnetic activity in the auroral zone. It is shown that, at arbitrary orientation of the By component, an increase of the solar wind velocity is accompanied by an increase of geomagnetic activity. For both Bz greater than zero and Bz less than zero, the substorm intensity during the summer is greater in the case of negative polarity of the By component, while the substorm intensity is greater during the winter in the case of positive polarity of the By component.

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