Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..811b&link_type=abstract
Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, Sept. 1987, p. 811-819. In Russian. In Russian.
Astronomy and Astrophysics
Astronomy
Interplanetary Magnetic Fields, Magnetic Field Configurations, Solar Flares, Solar Terrestrial Interactions, Space Plasmas, Chaos, Geomagnetism, Magnetic Disturbances
Scientific paper
Hodographs of the interplanetary magnetic field vector B near the earth during 29 flare-induced geomagnetic disturbances are considered. It is found that B either rotates in one direction, oscillates, or moves chaotically. The chaotic component is also present in cases of regular rotation or oscillation. These features are taken as evidence for a closed or nearly closed magnetic-field geometry in the plasma ejected by flares. The chaotic component may be due to external forces causing local deformations of certain parts of the magnetic field line loops.
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