The solar wind streams from flares - Magnetic field configuration at 1 a.u.

Details The solar wind streams from flares - Magnetic field configuration at 1 a.u. The solar wind streams from flares - Magnetic field configuration at 1 a.u.

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987p%26ss...35..793b&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 35, June 1987, p. 793-798.

Computer Science

1

Interplanetary Magnetic Fields, Solar Flares, Solar Wind, Hodographs, Magnetic Disturbances, Magnetic Field Configurations

Scientific paper

The hodographs of the IMF vector B near the Earth during flare-induced geomagnetic disturbances are considered. It is found that B either rotates in one direction, or oscillates, or moves chaotically. The chaotic component is also present in the cases of regular rotation or oscillation. These features are interpreted as evidence of the closed, or nearly closed, magnetic field configuration in flare streams. The chaotic component may be due to external forces which cause local deformations of some parts of magnetic loops.

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