Computer Science
Scientific paper
Aug 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....4..227y&link_type=abstract
IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Conference Papers. Volume 4 (A85-2
Computer Science
Solar Cycles, Solar Flares, Annual Variations, Statistical Distributions
Scientific paper
Utilizing the major solar flare data for the period 1955-79, a comprehensive analysis of these flares is presented. Based on this analysis it is found that the major solar flare activity was highest in the latitude interval 10-20 deg N. The longitudinal distribution is found to be approximately the same in both the east and west hemispheres and this distribution can be approximated by a Gaussian curve. The flare frequency is linearly proportional to sun-spot number. Moreover with increasing Comprehensive Flare Index (CFI), the flare frequency first increases, and then after a certain value it decreases almost exponentially to small value for highest CFI.
Agrawal S. P.
Badruddin
Yadav N. R.
Yadav Ravi Shankar
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