Response functions for magnetic lines

Details Response functions for magnetic lines Response functions for magnetic lines

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....56..111l&link_type=abstract

Astronomy and Astrophysics, vol. 56, no. 1-2, Apr. 1977, p. 111-115.

Mathematics

31

Atmospheric Models, Magnetic Effects, Polarized Light, Radiative Transfer, Solar Magnetic Field, Solar Spectra, Circular Polarization, Doppler Effect, Eigenvalues, Fraunhofer Lines, Lines Of Force, Magnetoactivity, Matrices (Mathematics), Perturbation Theory, Stokes Law Of Radiation, Velocity Distribution

Scientific paper

A perturbative solution to the equations of radiative transfer for polarized light is presented. This solution permits the evaluation of the influence of velocity fields and magnetic inhomogeneities on the Stokes-parameter profiles of magnetoactive Fraunhofer lines. The concept of a response function for polarized light is introduced. The frequency dependence of the response functions and their related symmetry properties are examined in some detail.

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