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Line formation in a magnetic field and the interpretation of magnetographic measurements
Authors:J Staude
Institution:(1) Zentralinstitut für Solar-Terrestrische Physik (HHI), Sonnenobservatorium Einsteinturm, Potsdam, D.D.R.
Abstract:The strong temperature dependence of the line Fei lambda 5250.2 Amacr has been studied by calculating line contours and magnetographic calibration curves for different spot models and the BCA. Line contours calculated for arbitrary depth dependence of the magnetic field vector show depolarization effects within the Zeeman components for transversal fields with variable direction and changes of the observed plane of polarization if anomalous dispersion is taken into account.The observed anomalous splitting of the pgr-component may be interpreted best by suggesting discrete inhomogeneities of the magnetic field within sunspots.
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