Flare induced geomagnetic activity and orientation of the photospheric magnetic field

Details Flare induced geomagnetic activity and orientation of the photospheric magnetic field Flare induced geomagnetic activity and orientation of the photospheric magnetic field

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982natur.299...42w&link_type=abstract

Nature, vol. 299, Sept. 2, 1982, p. 42-44.

Physics

4

Geomagnetism, Magnetic Storms, Photosphere, Solar Flares, Solar Terrestrial Interactions, Energy Transfer, Errors, Magnetoactivity, Solar Magnetic Field, Type 4 Bursts

Scientific paper

An investigation of the relationships between geomagnetic disturbances, flare energies and flare-site magnetic field directions for all large flares in the 1968-1979 period has uncovered no significant differences between the average energies of flares with northward, southward, or east-west magnetic fields. Although the inferred direction of the field at the site of a flare appears to control the geoefficiency of the flare to some degree, the relationship between geoefficiency and field direction is found to be unclear.

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