Origin of the low-temperature emission of solar and stellar flares

Details Origin of the low-temperature emission of solar and stellar flares Origin of the low-temperature emission of solar and stellar flares

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983azh....60..964l&link_type=abstract

Astronomicheskii Zhurnal, Vol. 60, p.964

Astronomy and Astrophysics

Astronomy

2

Scientific paper

An enhancement of the gas density, only 1 to 10 km thick, is formed due
to the gas-dynamic response to the flare heating. It is considered to be
the source of the low-temperature emission. The energy balance of the
enhancement is considered.

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