PROFILES OF FRAUNHOFER LINES IN PRESENCE OF ZEEMAN SPLITTING .I. ZEEMAN TRIPLET

被引：97
作者：
BECKERS, JM
机构：
[1] Sacramento Peak Observatory, Air Force Cambridge Research Laboratories, Sunspot, N.M.
来源：
SOLAR PHYSICS | 1969年 / 9卷 / 02期
关键词：
D O I：
10.1007/BF02391659
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
For the case of pure absorption lines (LTE) a method is described which enables the general computation of Zeeman-split line profiles. The magnetic field vector, the Doppler shift and the line absorption coefficient is permitted to vary arbitrarily with optical depth. Elliptical birefringence (e.g., Faraday rotation) of the solar atmosphere is taken into account. Some numerical examples are given and some interesting behaviors of the line profiles are discussed. © 1969 D. Reidel Publishing Company.
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页码：372 / &
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