Integrated circular polarization of spectral lines due to inhomogeneous magnetic and velocity fields

Details Integrated circular polarization of spectral lines due to inhomogeneous magnetic and velocity fields Integrated circular polarization of spectral lines due to inhomogeneous magnetic and velocity fields

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978sva....22...43p&link_type=abstract

(Astronomicheskii Zhurnal, vol. 55, no. 1, 1978, p. 79-83.) Soviet Astronomy, vol. 22, Jan.-Feb. 1978, p. 43-46. Translation.

Astronomy and Astrophysics

Astronomy

2

Circular Polarization, Line Spectra, Stellar Atmospheres, Stellar Magnetic Fields, Velocity Distribution, Absorption Spectra, Flow Velocity, Magnetohydrodynamic Flow, Nonuniform Magnetic Fields, Spectral Line Width, Sunspots

Scientific paper

Analytical expressions are derived for the integral circular polarization of spectral lines that is produced under the influence of a nonuniform magnetic field and nonuniform macroscopic velocity field. The integral circular polarization is obtained as a function of the gradients of these fields and as a function of the line strength for different profiles of the absorption coefficient.

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