Self-consistent models of flare heated solar chromospheres

Details Self-consistent models of flare heated solar chromospheres Self-consistent models of flare heated solar chromospheres

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...118..139f&link_type=abstract

Astronomy and Astrophysics, vol. 118, no. 1, Feb. 1983, p. 139-146. Research supported by Nanjing University.

Astronomy and Astrophysics

Astrophysics

14

Chromosphere, Solar Flares, Stellar Models, X Ray Irradiation, Electron Beams, Electron Density (Concentration), Emission Spectra, Plasma Heating

Scientific paper

For the first time self consistent models of an X-ray irradiated flaring chromosphere have been derived, together with a model of an electron heated chromosphere. The atmospheric radiation losses have been computed by including Lα, Lβ, LyC, Hα, Mg II and Ca II and H- emission. The hydrogen radiation losses were computed using complete linearization of the transfer, energy balance and hydrostatic equilibrium equations coupled with the statistical equilibrium equations. This method permits a substantial increase in the accuracy of the radiation loss estimate without requiring excessive computing time.

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