Soft X-ray emission from active regions shortly before solar flares

Details Soft X-ray emission from active regions shortly before solar flares Soft X-ray emission from active regions shortly before solar flares

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...76..377w&link_type=abstract

Solar Physics, vol. 76, Mar. 1982, p. 377-386. Research supported by the Lockheed Independent Research Program;

Physics

7

Solar Activity Effects, Solar Corona, Solar Flares, Solar X-Rays, Astronomical Models, Emission Spectra, H Alpha Line, Particle Intensity, Plasma Heating

Scientific paper

Detailed examination of the variations in the intensity of soft X-ray emission prior to many solar flares are presented. In addition, these preflare intensity variations are contrasted with the variations typically observed for the same active regions in the absence of a flare. It is shown that a 5-20 min preflare brightening phase is not typically observed. These observations are discussed in context with other complementary investigations and theoretical models.

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