CORONAL HOLE AT 7 MARCH 1970 SOLAR ECLIPSE

被引：27

作者：

WALDMEIER, M ^{[1
]}

机构：

[1] SWISS FED OBSERV,ZURICH,SWITZERLAND

来源：

SOLAR PHYSICS | 1975年 / 40卷 / 02期

关键词：

D O I：

10.1007/BF00162382

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：351 / 358

页数：8

共 15 条

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[2]

[Anonymous], 1956, Z ASTROPHYS

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WITHBROE, GL ;

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SOLAR PHYSICS, 1974, 34 (01) :105-111

[4] CORONAL HOLE AND ITS IDENTIFICATION AS SOURCE OF A HIGH-VELOCITY SOLAR-WIND STREAM [J].

KRIEGER, AS ;

TIMOTHY, AF ;

ROELOF, EC .

SOLAR PHYSICS, 1973, 29 (02) :505-525

[5] PROPERTIES OF A CORONAL HOLE DERIVED FROM EXTREME-ULTRAVIOLET OBSERVATIONS [J].

MUNRO, RH ;

WITHBROE, GL .

ASTROPHYSICAL JOURNAL, 1972, 176 (02) :511-&

[6] ENERGY BUDGET IN CORONAL HOLES [J].

NOCI, G .

SOLAR PHYSICS, 1973, 28 (02) :403-407

[7] IDENTIFICATION AND ANALYSIS OF STRUCTURES IN CORONA FROM X-RAY PHOTOGRAPHY [J].

VAIANA, GS ;

KRIEGER, AS ;

TIMOTHY, AF .

SOLAR PHYSICS, 1973, 32 (01) :81-116

[8]

Waldmeier M., 1971, Physics of the solar corona, P130

[9]

WALDMEIER M, 1950, Z ASTROPHYS, V27, P24

[10]

WALDMEIER M, 1971, ASTRON MITT EIDGEN S, V13

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