KILOMETER-WAVE TYPE-III BURST - HARMONIC EMISSION REVEALED BY DIRECTION AND TIME OF ARRIVAL

被引：13

作者：

ALVAREZ, H ^{[1
]}

HADDOCK, FT ^{[1
]}

POTTER, WH ^{[1
]}

机构：

[1] RADIO ASTRON OBSERV,ANN ARBOR,MI 48104

来源：

SOLAR PHYSICS | 1974年 / 34卷 / 02期

关键词：

D O I：

10.1007/BF00153676

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：413 / 420

页数：8

共 9 条

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[3] PREVALENCE OF SECOND-HARMONIC RADIATION IN TYPE-III BURSTS OBSERVED AT KILOMETRIC WAVELENGTHS [J].

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ALVAREZ, H .

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[4]

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[5] SPECTRAL OBSERVATIONS OF SOLAR RADIO BURSTS .4. EXCITERS OF FAST-DRIFT BURSTS [J].

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[6]

Smith D. F., 1970, Advances in astronomy and astrophysics vol.7, P147

[7]

SMITH DF, 1973, HIGH ENERGY PHENOMEN, P558

[8]

STONE RG, 1973, HIGH ENERGY PHENOMEN, P519

[9] DYNAMIC THEORY OF TYPE-III SOLAR RADIO BURSTS [J].

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SOLAR PHYSICS, 1972, 24 (02) :444-+

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