A statistical analysis of H-alpha emission from solar flares

Details A statistical analysis of H-alpha emission from solar flares A statistical analysis of H-alpha emission from solar flares

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26as...82..543y&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 82, no. 3, March 1990, p. 543-552. Research supported by Rut

Astronomy and Astrophysics

Astrophysics

3

Emission Spectra, H Alpha Line, Solar Flares, Statistical Analysis, Frequency Distribution, Solar Cycles, Solar X-Rays

Scientific paper

The durations, maximum intensities, and corrected areas of 16,342 H-alpha flare events during the years 1980, 1983, 1986 and 1987 are examined. The distributions of these parameters reveal some important properties of solar flare activity. In common with past studies, notably at X-ray and H-alpha wavelengths, it is found that there is no evidence to suggest that there is more than one class of event. It is concluded that there is no correlation between flare area and flare duration for the H-alpha events studied.

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