ABOUT INFLUENCE OF INHOMOGENEITIES OF MAGNETIC FIELDS ON LINE CONTOURS AND MAGNETOGRAPHIC MEASUREMENTS

被引:18
作者
STAUDE, J
机构
[1] Heinrich-Hertz-Institut für solar-terrestrische Physik, Sonnenobservatorium Einsteinturm, Potsdam
关键词
D O I
10.1007/BF00155373
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The discrepancies between theoretical and experimental calibration curves for solar magnetographs (Severny, 1967) may be explained by horizontal inhomogeneities of the observed but not resolved magnetic field region. Using the Unno solution of the equations of transfer simple two-stream models have been constructed. For the more complicated case of a depth dependence of the magnetic field vector it is shown assuming pure absorption and permitting arbitrary variations of the magnetic field vector and the atmosphere model with depth that a solution of the equations of transfer may be found by iteration. © 1969 D. Reidel Publishing Company.
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页码:264 / &
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