Distribution of Solar Flares around the Sun and Their Association with Forbush Decreases

Details Distribution of Solar Flares around the Sun and Their Association with Forbush Decreases Distribution of Solar Flares around the Sun and Their Association with Forbush Decreases

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3593s&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

1

Scientific paper

Solar flare is a gignatic discharge of lighting and solar mass due to abrupt release of the energy stored in the magnetic fields in the zone around the sunspots. In this work we have studied the relation of occurrence of solar flares in different hemispheric zones and cosmic ray Forbush decreases for the period of 1986 to 2000. It is investigated that the flares having the optical importance ≥ 2B might be the reason for Fobush decreases. Northern zone between 15° to 30° and southern zone between 0° to 30° are found most effective to produce Forbush decreases.

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