Modeling the solar photosphere and chromosphere

Details Modeling the solar photosphere and chromosphere Modeling the solar photosphere and chromosphere

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mmsai..48..401a&link_type=abstract

(Advanced School of Astronomy, Course on the Sun, a Tool for Stellar Physics, 6th, Erice, Italy, Aug. 8-21, 1976.) Società Astro

Physics

1

Atmospheric Models, Chromosphere, Photosphere, Solar Atmosphere, Stellar Models, Brightness Temperature, Lyman Spectra, Radiative Transfer, Solar Physics, Solar Temperature

Scientific paper

Some aspects of modeling the solar photosphere and chromosphere with allowance for the characteristics produced by hydrodynamic and magnetic processes, on the basis of modern solar data are examined. The problem of asigning heights, geometrical or optical, to specific features of the solar atmosphere is discussed, along with the establishment of reference points and height scales.

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