The calculation and analysis of the radiation energy of optical solar flares observed in 1978

Details The calculation and analysis of the radiation energy of optical solar flares observed in 1978 The calculation and analysis of the radiation energy of optical solar flares observed in 1978

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kfnt....3...46k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 3, Nov.-Dec. 1987, p. 46-49, 67. In Russian.

Physics

1

Line Spectra, Radiant Flux Density, Solar Flares, Solar Spectra, H Alpha Line, Lyman Spectra, Solar Radiation

Scientific paper

The radiation energies of the low-temperature regions of 5508 flares observed in 1978 are calculated. The radiation in all of the lines and continua of the hydrogen series (beginning with Lyman) with typical parameters of flares with different intensities is taken into account. Data on the H-alpha intensity, and area and lifetime of each flare are taken from observations. The total energy radiated by the flares increases with an increase in importance. With a decrease in flare energy to 5 x 10 to the 20th J, the number of flares increases and then rapidly decreases.

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