Evaporation causes flare-related radio burst continuum depressions

Details Evaporation causes flare-related radio burst continuum depressions Evaporation causes flare-related radio burst continuum depressions

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..145..151a&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 145, no. 1, p. 151-168.

Physics

11

H Alpha Line, Noise Storms, Solar Activity, Solar Flares, Solar Magnetic Field, Solar Radio Bursts, Chromosphere, Magnetic Signatures, Solar Corona, Solar Flux

Scientific paper

We study the active region NOAA 6718 and the development of a (2N, M3.6) flare in radio and H-alpha. Due to our knowledge of the magnetic field structure in the active region, we are able to associate the different radio flare burst components with the stages in the H-alpha flare evolution. A discussion of the data in terms of chromospheric flare kernel heating reveals that in the present case the observed flare-related radio burst continuum switch-off is caused by the penetration of hot, ablated gas into the coronal radio source.

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