An unusual behaviour of the white-light flare on 11 October, 1974

Details An unusual behaviour of the white-light flare on 11 October, 1974 An unusual behaviour of the white-light flare on 11 October, 1974

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995soph..158..387f&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 158, no. 2, p. 387-390

Physics

4

Continuous Radiation, Line Spectra, Solar Flares, Solar Physics, Solar Spectra, Sun, Continuous Spectra, Mathematical Models, Solar Corona, Spectral Emission

Scientific paper

It was found that in the spectrum of the white-light flare on 11 Oct. 1974, at the time of continuum maximum, the intensity of K1 in the Ca II K line increased very significantly an reached nearly half of the continuum intensity. The duration of this unusual increase is less than 4 min. It seems that existing semi-empirical models can reproduce neither this characteristic nor the chromospheric condensation.

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