Study of solar-type-II radio bursts and H-alpha flares

Details Study of solar-type-II radio bursts and H-alpha flares Study of solar-type-II radio bursts and H-alpha flares

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ijrsp..21...97v&link_type=abstract

Indian Journal of Radio & Space Physics (ISSN 0367-8393), vol. 21, no. 2, p. 97-100.

Physics

Space Physics

H Alpha Line, Solar Flares, Solar Radio Bursts, Emission Spectra, Shock Waves

Scientific paper

An analysis of the relationship of solar type-II radio bursts with H-alpha flares has been presented. The study shows that 75 percent of type-II bursts is associated with bright H-alpha flares of importance equal to or less than 1. The two-ribbon H-alpha flares are 15 times more strongly associated with type-II bursts than the compact flares. Type-II bursts start 1-15 min after the onset of H-alpha flares. The time interval between start of type-II bursts and peak of H-alpha flares is +/- 5 min. This differs from the results found by earlier investigators. The 66 percent of type-II bursts is associated with flares' bright points in H-alpha emissions.

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