Nonequilibrium polarized radiation transfer in the solar spots: Fe I

Details Nonequilibrium polarized radiation transfer in the solar spots: Fe I Nonequilibrium polarized radiation transfer in the solar spots: Fe I

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001kfnt...17..331s&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 17, no. 4, p. 331-339

Physics

Scientific paper

Using accelerated Lambda-iteration method we solved unequilibrium polarized radiation transfer problem for Fe I lines in the cool and hot spot models. In low layers of the cool model the conditions of line formation are close to equilibrium, where as in the hot model slight neutral iron overionization by UV-radiation occurs. We investigated NLTE-effects and magnetic field influense on Fe I lines formation in the solar spots. It is shown that polarization of the radiation sufficiently decreases formation depths of magnetically sensitive lines.

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