Comments on hydrodynamic models for the influence of flares upon the chromosphere

Details Comments on hydrodynamic models for the influence of flares upon the chromosphere Comments on hydrodynamic models for the influence of flares upon the chromosphere

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pazh....6..597s&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Sept.-Oct. 1980, p. 597-601.) Soviet Astronomy Letters, vol. 6, Sept.-Oct. 1980, p.

Astronomy and Astrophysics

Astronomy

1

Chromosphere, Hydrodynamic Equations, Solar Flares, Continuous Spectra, High Energy Electrons, High Temperature Plasmas, Light Emission, Radiant Cooling, Shock Wave Interaction, Solar Prominences, Spontaneous Emission, Temperature Distribution, Thermal Plasmas, Thermal Stability, Velocity Distribution

Scientific paper

Some comments are given on the present status of the theory of nonsteady
hydrodynamic phenomena triggered by the release of energy in a solar
flare. In particular, the impulsive optical continuum emission known as
a white flare could result from thermal instability in the heated
chromospheric plasma.

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