Energy balance in the chromosphere - Corona transition region

Details Energy balance in the chromosphere - Corona transition region Energy balance in the chromosphere - Corona transition region

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974sva....18..396d&link_type=abstract

(Astronomicheskii Zhurnal, vol. 51, May-June 1974, p. 671, 672.) Soviet Astronomy, vol. 18, Nov.-Dec. 1974, p. 396. Translation.

Astronomy and Astrophysics

Astronomy

Chromosphere, Far Ultraviolet Radiation, Heat Budget, Solar Corona, Transition Layers, Conductive Heat Transfer, Convective Heat Transfer, Line Spectra, Radiative Heat Transfer, Solar Granulation, Solar Spectra

Scientific paper

The height dependence found by Kopp (1972) for the fraction of the solar surface emitting extreme-ultraviolet lines indicates that the radiation of the transition layer (log T ranging from 5.3 to 6.3) originates above the middle of supergranular cells. Hence the downward conductive energy flux from the corona determined from the radiative flux in these lines, contrary to Kopp's claim, agrees with previous findings. The conductive flux plays the chief role in establishing the temperature-height profile in the transition layer.

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