ON PSEUDO-PI-COMPONENT IN SUNSPOT SPECTRA

被引：3

作者：

GOHRING, R

机构：

[1] Fraunhofer Institut, Freiburg i.Br.

来源：

SOLAR PHYSICS | 1969年 / 8卷 / 02期

关键词：

D O I：

10.1007/BF00155374

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The visibility, contrast and displacement of the pseudo-π-component of a Zeeman triplet, explained as due to saturation, is computed for the triplet at 5250 {superset beside subset}A (Fe i). Examples of the computational results are given (Figures 1-3). © 1969 D. Reidel Publishing Company.

引用

页码：271 / &

共 8 条

[1] INTENSITY VELOCITY AND MAGNETIC STRUCTURE OF A SUNSPOT REGION .3. ON ORIGIN OF APPARENT PI COMPONENT IN SUNSPOT UMBRAE [J].

BECKERS, JM ;

SCHROTER, EH .

SOLAR PHYSICS, 1969, 7 (01) :22-&

[2]

HENOUX JC, 1968, SOL PHYS, V4, P515

[3]

HOLWEGER H, 1967, Z ASTROPHYS, V65, P365

[4]

KJELDSETH MO, 1968, SOL PHYS, V4, P267

[5]

MALTBY P, 1968, ASTROPHYS LETT, V1, P189

[6]

MATTIG W, 1966, 1966 P M SUNSP FIR, P194

[7]

Severny A.B., 1959, ASTRON ZH, V36, P208

[8]

Unno W., 1956, PASJ, V8, P108

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