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.

引用

页码：372 / &

共 19 条

[1] ABRAMOWITZ M, 1964, HANDBOOK MATHEMATICA
[2] Aller, 1963, ATMOSPHERES SUN STAR
[3] Beckers J. M., 1968, Solar Physics, V5, P15, DOI 10.1007/BF00147116
[4] Beckers J. M., 1968, SOL PHYS, V4, P303
[5] INTENSITY VELOCITY AND MAGNETIC STRUCTURE OF A SUNSPOT REGION .3. ON ORIGIN OF APPARENT PI COMPONENT IN SUNSPOT UMBRAE
BECKERS, JM
SCHROTER, EH
[J]. SOLAR PHYSICS, 1969, 7 (01) : 22 - &
[6] BORN M, 1965, OPTIK
[7] EVANS JW, 1964, ROME M SOLAR MAGNE 4, P123
[8] GINGERICH O, 1967, SOL PHYS, V3, P5
[9] GOLDBERG L, 1960, ASTROPHYS J S, V45, P1
[10] ON THE LINE-ABSORPTION COEFFICIENT DUE TO DOPPLER EFFECT AND DAMPING
HARRIS, DL
[J]. ASTROPHYSICAL JOURNAL, 1948, 108 (01) : 112 - 115

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