CORONAL MAGNETIC-FIELDS INFERRED FROM SOURCE DISTRIBUTION OF CORRELATED BURSTS AND CONCURRENT TYPE-I STORM

被引：0

作者：

KAI, K ^{[1
]}

NAKAJIMA, H ^{[1
]}

机构：

[1] TOKYO ASTRON OBSERV,MITAKA,TOKYO,JAPAN

来源：

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：379 / 386

页数：8

共 21 条

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[2]

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[3]

DAIGNE G, 1971, SOLAR MAGNETIC FIELD, P609

[4]

Dulk G. A., 1973, Proceedings of the Astronomical Society of Australia, V2, P211

[5]

DULK GA, 1971, ASTROPHYS LETT COMM, V8, P235

KAI, K .

[7]

kai K., 1969, Proceedings of the Astronomical Society of Australia, V1, P186

[8]

KAI K, IN PRESS

[9]

KUNDU MR, 1965, SOLAR RADIO ASTRONOM, P452

[10] CORONAL MAGNETIC FIELD PATTERNS INFERRED FROM RADIO OBSERVATIONS [J].

LANTOSJARRY, MF .