PREVALENCE OF SECOND-HARMONIC RADIATION IN TYPE-III BURSTS OBSERVED AT KILOMETRIC WAVELENGTHS

被引：37

作者：

HADDOCK, FT ^{[1
]}

ALVAREZ, H ^{[1
]}

机构：

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

来源：

关键词：

D O I：

10.1007/BF00153448

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：183 / 196

页数：14

共 20 条

[1] TYPE 3 RADIO BURSTS IN OUTER CORONA
ALEXANDER, JK
MALITSON, HH
STONE, RG
[J]. SOLAR PHYSICS, 1969, 8 (02) : 388 - +
[2] SOLAR-WIND DENSITY MODEL FROM KM-WAVE TYPE-III BURSTS
ALVAREZ, H
HADDOCK, FT
[J]. SOLAR PHYSICS, 1973, 29 (01) : 197 - 209
[3] BOISCHOT A, 1967, ANN ASTROPHYS, V30, P85
[4] Fainberg J., 1970, Solar Physics, V15, P433, DOI 10.1007/BF00151850
[5] HADDOCK FT, 1971, URSI M LOS ANG
[6] HADDOCK FT, 1970, B AM ASTRON SOC, V2, P291
[7] HADDOCK FT, 1971, APR URSI M WASH
[8] HADDOCK FT, 1970, B AM ASTRON SOC, V3, P6
[9] CHARACTERISTICS OF TYPE III RADIO BURSTS
MALVILLE, JM
[J]. ASTROPHYSICAL JOURNAL, 1962, 136 (01) : 266 - &
[10] THEORY OF TYPE-II AND TYPE-III SOLAR RADIO BURSTS .1. IMPOSSIBILITY OF NONTHERMAL EMISSION DUE TO COMBINATION SCATTERING OFF THERMAL FLUCTUATIONS
MELROSE, DB
[J]. AUSTRALIAN JOURNAL OF PHYSICS, 1970, 23 (06): : 871 - &