
doi: 10.1007/bf00650356
The polarization structure in several spectral lines in solar type stars is computed using the method described by McKenna (1981, 1984a). The frequency redistribution function used for these calculations is a linear combination ofRII andRIII. The line profiles and polarization structures have been computed for several weak solar resonance lines includingKi λ 7664 A, Sri λ4607 A, Baii λ4554 A, for various polar angles along the stellar disk. Both the line profiles and polarization structures as well as the center to limb behavior of the line center polarization agree well with observations.
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