Fast intensity variations of hard X-rays from solar flares

Details Fast intensity variations of hard X-rays from solar flares Fast intensity variations of hard X-rays from solar flares

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988kosis..26..578b&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 26, July-Aug. 1988, p. 578-583. In Russian.

Statistics

Radiant Flux Density, Solar Flares, Solar X-Rays, Monte Carlo Method, Statistical Analysis, Venera Satellites

Scientific paper

A method for analyzing the variability of solar-flare X-rays is proposed. A statistical analysis of the time profiles of the X-ray emission from 147 flares has identified only two flares in which the shortest statistically significant characteristic variation time amounted to 0.08 sec. Monte Carlo simulation showed that the fastest variations, given the existing count statistics in the detectors, can be explained by statistical fluctuations.

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