Some peculiarities of the X-ray bursts and their relation with emission in the Hα-line, on the example of flare of 16 May, 1981.

Details Some peculiarities of the X-ray bursts and their relation with emission in the Hα-line, on the example of flare of 16 May, 1981. Some peculiarities of the X-ray bursts and their relation with emission in the Hα-line, on the example of flare of 16 May, 1981.

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994kosis..32..165l&link_type=abstract

Kosmicheskie Issledovaniia, Tom 32, Vyp. 6, p. 165 - 171

Physics

Solar Flares: Hard X Rays, Solar Flares: Soft X Rays, Solar X-Ray Bursts

Scientific paper

The effect of quasi-periodicity of the soft X-ray bursts in active regions during the preflare phase was investigated. It was examined the space-time connection of the hard X-ray bursts with localization of the flare emission knots, which have been seen on the Hα-filtergrams received at the centre of the Hα-line and its wings. The analysis of the fine structure of the two-ribbon flare, revealed by the equidensity method was given.

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