Non-LTE line formation in the presence of magnetic fields

Details Non-LTE line formation in the presence of magnetic fields Non-LTE line formation in the presence of magnetic fields

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...216..531a&link_type=abstract

Astrophysical Journal, Part 1, vol. 216, Sept. 1, 1977, p. 531-539.

Other

43

Difference Equations, Radiative Transfer, Stellar Atmospheres, Stellar Magnetic Fields, Thermodynamic Equilibrium, Line Spectra, Polarization Characteristics, Statistical Analysis, Stellar Models, Stokes Law Of Radiation

Scientific paper

The equations of radiative transfer and statistical equilibrium in the presence of a magnetic field are presented. A general difference equation scheme for solving the vector transfer equation in Stokes parameters, allowing for arbitrary variations of the magnetic field and other quantities, is described. The solution of the Stokes non-LTE problem for Ca II by the complete linearization method is described, and numerical examples of the procedure are presented.

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