Studies on some aspects of solar X-ray flares.

Details Studies on some aspects of solar X-ray flares. Studies on some aspects of solar X-ray flares.

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999injpb..73..695d&link_type=abstract

Indian J. Phys., Part B, Vol. 73B, No. 5, p. 695 - 699

Physics

Solar X-Ray Flares

Scientific paper

Studies have been made on the solar X-ray flares observed by GOES during the period July 1993 - June 1994, which encompasses the post-maximum phase of 22nd solar cycle. It has been examined that N-S asymmetry remains positive in respect of both latitudinal position and intensity of X-ray flares and increases with the increase of intensity. The E-W asymmetry is found to be zero, when longitudinal distribution is considered; but it remains positive up to a certain intensity value above which it becomes negative. The duration and rise time lie respectively in the ranges of values 5 - 15 min and 0 - 5 min. The distribution of impulsiveness of X-ray flares follows an almost binomial distribution pattern peaking around 0.45.

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