LINE FORMATION IN A MAGNETIC FIELD

被引：42

作者：

REES, DE

机构：

[1] Dept. of Applied Mathematics, University of Sydney

来源：

SOLAR PHYSICS | 1969年 / 10卷 / 02期

关键词：

D O I：

10.1007/BF00145514

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The effect of noncoherent scattering is examined for an absorption line formed in a uniform magnetic field. It is shown that the Stokes parameters of the line radiation may be computed by using the line source function in the absence of a magnetic field as a first approximation for that in the presence of a magnetic field. © 1969 D. Reidel Publishing Company.

引用

页码：268 / &

共 12 条

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HUMMER, DG
[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1968, 138 (01) : 73 - &
[4] KATZ IM, 1968, ASTRON ZH, V45, P1066
[5] KRYLOV VI, 1962, APPROXIMATE CALCULAT, P114
[6] MATTIG W, 1966, 1966 P M SUNSP FIR, P194
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[9] STEPANOV VE, 1958, IZV KRYMSK ASTROFIZ, V18, P136
[10] APPROXIMATE INTEGRATION OF THE EQUATION OF TRANSFER
SYKES, JB
[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1951, 111 (04) : 377 - 386

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