New contribution functions for Zeeman split spectral lines

Details New contribution functions for Zeeman split spectral lines New contribution functions for Zeeman split spectral lines

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...286..269s&link_type=abstract

Astronomy and Astrophysics 286, 269-274 (1994)

Astronomy and Astrophysics

Astrophysics

9

Line: Formation, Line: Profile, Polarization, Sun: Magnetic Fields

Scientific paper

The recently introduced emergent line radiation contribution function (Achmad + de Jager + Nieuwenhuijzen 1991; Gurtovenko + Sheminova + Sarychev 1991) is extended to the Stokes vector of Zeeman split spectral lines. This contribution function is compared to the line depresssion contribution function on the basis of an analytical relation and of numerical NLTE computations of a set of spectral lines. In general the two contribution functions give very similar results, although in some cases the one or the other of them is more suitable.

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