Dependence of GMS with Ap>_50 on solar features' locations

Details Dependence of GMS with Ap>_50 on solar features' locations Dependence of GMS with Ap>_50 on solar features' locations

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....9.3568k&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

An attempt has been made to locate the solar features and their effective locations on the solar disk causing the geomagnetic storms (GMSs) with Ap≥50 on Earth. Eighty four GMSs have been investigated using solar geophysical data (SGD) and interplanetary data during the period 1978-93. It is observed statistically that Hα, X-ray solar flares and active prominences and disappearing filaments (APDFs) which have occurred within lower heliographic latitudinal/longitudinal zones are associated with larger number of GMSs at Earth.

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