Terrestrial geomagnetic effects of interplanetary shock fronts from near-zone high-intensity isolated flares

Details Terrestrial geomagnetic effects of interplanetary shock fronts from near-zone high-intensity isolated flares Terrestrial geomagnetic effects of interplanetary shock fronts from near-zone high-intensity isolated flares

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ge%26ae..20..508i&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 20, May-June 1980, p. 508-514. In Russian.

Physics

1

Geomagnetism, Interplanetary Medium, Magnetic Effects, Shock Fronts, Solar Flares, Axes (Reference Lines)

Scientific paper

A unique relationship is established between the presence (or absence) of geomagnetic effects (SSI and SI) after an isolated high-intensity flare in the near zone on the solar disk and the orientation of the magnetic axis of a bipolar group on the sun. The relationship is interpreted in terms of a pronounced flattening of flare-induced shock fronts with respect to the vertical plane running through the flare and parallel to the bipolar group axis.

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