Non-LTE resonance line polarization with partial redistribution - The solar CA II K line

Details Non-LTE resonance line polarization with partial redistribution - The solar CA II K line Non-LTE resonance line polarization with partial redistribution - The solar CA II K line

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...98....1s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 98, July 1985, p. 1-22.

Physics

18

K Lines, Nonequilibrium Thermodynamics, Polarization Characteristics, Resonance Lines, Solar Atmosphere, Solar Spectra, Abundance, Atmospheric Models, Calcium, Coherent Scattering, Line Spectra, Radiative Transfer, Solar Physics

Scientific paper

The non-LTE equations for the transfer of polarized radiation are solved for a two-level model of the Ca II K ion in the atmospheric models of Gingerich et al. (1971) and Vernazza et al. (1981). The line formation model treats partial redistribution effects, including collisions. The effects of magnetic fields and of quantum mechanical interference are neglected. The response of the intensity, percentage polarization and Q Stokes parameter to changes in the calcium abundance, van der Waals damping parameter and atmospheric models is discussed.

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