State of the chromospheric and photospheric material of the subflare. II. Semiempirical photospheric models

Details State of the chromospheric and photospheric material of the subflare. II. Semiempirical photospheric models State of the chromospheric and photospheric material of the subflare. II. Semiempirical photospheric models

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001kfnt...17..113c&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 17, no. 2, p. 113-120

Physics

1

Scientific paper

The study of physical conditions in the flare loop on 2 August 1990 is continued. From the semiempirical simulations, the thermodynamic and magnetic properties and the line-of-sight velocities at the photospheric part of the flare loop were investigated. The models reveal the presence of some inhomogeneous layers in the distributions of temperature, total hydrogen number density, electron number density, and LOS velocities with depth in the flare atmosphere. In the impulsive phase these inhomogeneities penetrated to the photosphere down to its base and dissipated with time.

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