Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...263..982a&link_type=abstract
Astrophysical Journal, Part 1, vol. 263, Dec. 15, 1982, p. 982-986.
Astronomy and Astrophysics
Astrophysics
39
Chromosphere, Energy Budgets, Magnetic Field Configurations, Solar Atmosphere, Solar Corona, Solar Magnetic Field, Conductive Heat Transfer, Energy Transfer, Flow Velocity, Magnetohydrodynamic Flow, Plasma Temperature, Radiative Transfer, Solar Spectra, Stellar Models, Temperature Dependence
Scientific paper
Models of the chromosphere-corona transition region in which energy is supplied by thermal conduction and downflow of hot material and lost by radiation are investigated for different magnetic field geometries and for different dependences of downflow velocity on the local temperature. It is shown that neither the field geometry nor the dependence of velocity on temperature are important factors in the comparison of empirical and theoretical emission measures. Each of the models works well for T higher than 250,000 K but fails badly for temperatures lower than that.
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