Geomagnetic effects of high-velocity fluxes in the solar wind

Details Geomagnetic effects of high-velocity fluxes in the solar wind Geomagnetic effects of high-velocity fluxes in the solar wind

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ge%26ae..21..497d&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 21, May-June 1981, p. 497-500. In Russian.

Computer Science

Geomagnetism, Magnetic Storms, Solar Terrestrial Interactions, Solar Wind Velocity, Error Analysis, Magnetic Variations

Scientific paper

The geomagnetic effects of high-velocity fluxes in the solar wind on a sub p, AE, and Dst indices are investigated. It is shown that the degree of disturbance of the solar wind in the high-velocity fluxes determines the intensity of the corresponding geomagnetic variations. For most of the high-velocity fluxes, the A sub p, AE, and Dst indices reach their maximum values when the first phase of the flux (i.e., the region of compressed solar wind) passes by the earth.

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