Formation of the H-Beta line in solar chromosphere magnetic field

Details Formation of the H-Beta line in solar chromosphere magnetic field Formation of the H-Beta line in solar chromosphere magnetic field

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986acasn..27..217z&link_type=abstract

(Acta Astronomica Sinica, vol. 27, no. 3, 1986, p. 217-226) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 11, March

Astronomy and Astrophysics

Astrophysics

13

Absorption Spectra, Chromosphere, H Beta Line, Solar Magnetic Field, Spectral Line Width, Doppler Effect, Electric Field Strength, Perturbation Theory, Quantum Mechanics, Radiative Transfer, Stokes Law Of Radiation

Scientific paper

The paper considers the effects of the microscopic electric field, Doppler broadening and radiation damping in the solar atmosphere magnetic field as well as the use of the perturbation theory of quantum mechanics to determine the broadening mechanisms and the absorption coefficient of the H beta line. The VAL quiet chromosphere model is used to solve the Unno-Beckers equations of radiative transfer for the H beta line and to obtain a numerical solution of the Stokes parameters of this line.

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