Physics
Scientific paper
Feb 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..143..229l&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 143, no. 2, p. 229-234.
Physics
8
Line Spectra, Polarization (Waves), Solar Atmosphere, Solar Spectra, Zeeman Effect, Iron, Radiative Transfer, Solar Magnetic Field
Scientific paper
The anomalous Zeeman splitting of the Fe II line at 614.9 nm results in four unusual properties of the polarization signature of this line in the presence of magnetic fields: the absence of linear polarization, no magnetooptical effect, the independence of intensity at line center from the inclination of the field, and a depolarizing self-absorption. The origin of these properties is illustrated in terms of the transfer of line radiation in an idealized solar atmosphere.
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