Manifestation of configurations of magnetic clouds of the solar wind in geomagnetic activity

Details Manifestation of configurations of magnetic clouds of the solar wind in geomagnetic activity Manifestation of configurations of magnetic clouds of the solar wind in geomagnetic activity

Aug 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cosre..47..268b&link_type=abstract

Cosmic Research, Volume 47, Issue 4, pp.268-278

Computer Science

1

96.50.Uv

Scientific paper

On the basis of an analysis of the data of multi-satellite observations of magnetic clouds at the path Venus-Earth, the dependence of their geoeffectiveness on the orientation in the ecliptic plane and position relative to the Sun-Earth line is determined in the paper. The cloud parameters were determined on the basis of the model of a force-free cylindrical flux rope. The search for magnetic clouds in the flow of data from the monitoring space vehicle was performed using a special-purpose computer program.

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