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 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987cha%26a..11...42z&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 11, Issue 1, p. 42-48.

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

We consider the effects of microscopic electric field, Doppler broadening and radiation damping in the solar atmosphere magnetic field and use the perturbation theory of quantum mechanics to determine the broadening mechanisms and the absorption coefficient of the Hβ line. We then use the VAL quiet chromosphere model to solve the Unno-Beckers equations of radiative transfer for the Hβ line and obtain a numerical solution of the Stokes parameters of this line.

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