NECESSITY OF FUNDAMENTAL EMISSION IN TYPE 3 BURSTS

被引：5

作者：

SMITH, DF ^{[1
]}

DAVIS, WD ^{[1
]}

机构：

[1] NATL CTR ATMOSPH RES,HIGH ALTITUDE OBSERV,BOULDER,CO 80303

来源：

SOLAR PHYSICS | 1975年 / 41卷 / 02期

关键词：

D O I：

10.1007/BF00154080

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：439 / 447

页数：9

共 16 条

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[3] TYPE-III SOLAR RADIO BURST STORMS OBSERVED AT LOW FREQUENCIES .3. STREAMER DENSITY, INHOMOGENEITIES, AND SOLAR WIND SPEED [J].

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[4]

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[5]

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

HADDOCK, FT ;

ALVAREZ, H .

SOLAR PHYSICS, 1973, 29 (01) :183-196

[7]

HEYVAERTS J, 1974, ASTRON ASTROPHYS, V30, P211

[8] LONG-LIVED SECTORS OF ENHANCED DENSITY IRREGULARITIES IN SOLAR-WIND [J].

HOUMINER, Z ;

HEWISH, A .

PLANETARY AND SPACE SCIENCE, 1972, 20 (10) :1703-&

[9]

HUNDHAUSEN AJ, 1970, SOLAR TERRESTRIAL 2, P1

[10]

LIN RP, 1973, ASTROPHYS LETT COMM, V14, P191

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