Continuum of white-light flares and model atmosphere

Details Continuum of white-light flares and model atmosphere Continuum of white-light flares and model atmosphere

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988acaps...8...61g&link_type=abstract

(Acta Astrophysica Sinica, vol. 8, 1988, p. 61-67) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 12, June 1988, p. 1

Astronomy and Astrophysics

Astrophysics

Atmospheric Models, Continuous Spectra, Solar Atmosphere, Solar Flares, Chromosphere, Nonequilibrium Thermodynamics, Photosphere, Visible Spectrum

Scientific paper

Based on general observed facts of the continuum emission of white-light solar flares, the relation between the continuum spectrum and model atmospheres is investigated semiempirically through a series of non-LTE model calculations. The results show that either a temperature increase in deep layers of the photosphere or the existence of a plateau structure in the trasition region can explain the observed white-light enhancement.

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