Variations of the equatorial boundary of polar aurorae as a function of solar sources.

Details Variations of the equatorial boundary of polar aurorae as a function of solar sources. Variations of the equatorial boundary of polar aurorae as a function of solar sources.

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ge%26ae..30..421e&link_type=abstract

Geomagn. Aeron., Vol. 30, No. 3, p. 421 - 423

Physics

Aurorae: Solar-Terrestrial Relations

Scientific paper

The equatorial boundary of the auroral oval is considered as a function of the type and parameters of solar sources such as flares, coronal holes and winking filaments. It is established that the increase in intensity and the position of a solar source relative to the central meridian leads to an increase in auroral activity, expansion of the auroral oval and a decrease in the geomagnetic latitude of the equatorial boundary of polar aurorae.

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