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=1988cha%26a..12..146g&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 12, Issue 2, p. 146-151.

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

Based on general observed facts of the continuum emission of white-light flares, we investigated semi-empirically the relation between the continuum spectrum and model atmospheres 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 transition region can explain the observed white-light enhancement. As to theoretical explanations of such structures, we also put forward certain views.

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