CENTER LIMB OBSERVATIONS OF INHOMOGENEITIES IN SOLAR ATMOSPHERE .3. TIME DEPENDENT FINE STRUCTURE OF CA II EMISSION

被引：18

作者：

WILSON, PR

EVANS, CD

机构：

来源：

SOLAR PHYSICS | 1971年 / 18卷 / 01期

关键词：

D O I：

10.1007/BF00146029

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：29 / &

共 11 条

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[3]

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[6] SOLAR H-LINES K-LINES [J].

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[7]

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[8]

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[9]

WHITE OR, 1968, SOL PHYS, V3, P523

[10] 3-COMPONENT MODEL FOR FORMATION OF CHROMOSPHERIC CAII K LINE [J].

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