Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985sao..rept.....a&link_type=abstract
Semiannual Report, 1 Jan. - 31 Dec. 1984 Smithsonian Astrophysical Observatory, Cambridge, MA.
Astronomy and Astrophysics
Astrophysics
Chromosphere, Mathematical Models, Solar Atmosphere, Spectroheliographs, Brightness Temperature, Equilibrium Equations, Hydrostatics, Line Spectra, Radiative Transfer, Thermodynamics
Scientific paper
Solar chromospheric models are described. The models included are based on the observed spectrum, and on the assumption of hydrostatic equilibrium. The calculations depend on realistic solutions of the radiative transfer and statistical equilibrium equations for optically thick lines and continua, and on including the effects of large numbers of lines throughout the spectrum. Although spectroheliograms show that the structure of the chromosphere is highly complex, one-dimensional models of particular features are reasonably successful in matching observed spectra. Such models were applied to the interpretation of chromospheric observations.
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