ENERGETIC ELECTRONS, TYPE-III RADIO-BURSTS, AND IMPULSIVE SOLAR-FLARE X-RAYS

被引:81
作者
KANE, SR
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D O I
10.1086/159121
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P1 [天文学];
学科分类号
0704 ;
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页码:1113 / 1121
页数:9
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[1]   ENERGETIC SOLAR FLARE X-RAYS OBSERVED BY SATELLITE AND THEIR CORRELATION WITH SOLAR RADIO AND ENERGETIC PARTICLE EMISSION [J].
ARNOLDY, RL ;
KANE, SR ;
WINCKLER, JR .
ASTROPHYSICAL JOURNAL, 1968, 151 (2P1) :711-&
[3]  
BROWN JC, SOLAR GAMMA X AND EU, P246
[4]   INDIRECT ESTIMATION OF ENERGY DISPOSITION BY NONTHERMAL ELECTRONS IN SOLAR-FLARES [J].
HUDSON, HS ;
CANFIELD, RC ;
KANE, SR .
SOLAR PHYSICS, 1978, 60 (01) :137-142
[5]  
Kane S. R., 1974, Coronal Disturbances, P105
[6]  
Kane S. R., 1980, SOLAR FLARES, P187
[7]   CORRELATED OBSERVATIONS OF A SPATIALLY RESOLVED TYPE-III SOLAR RADIO-BURST GROUP AND THE ASSOCIATED HARD X-RAY-EMISSION [J].
KANE, SR ;
PICK, M ;
RAOULT, A .
ASTROPHYSICAL JOURNAL, 1980, 241 (02) :L113-L116
[8]   LOCATION OF ELECTRON ACCELERATION REGION IN SOLAR-FLARES [J].
KANE, SR ;
LIN, RP .
SOLAR PHYSICS, 1972, 23 (02) :457-&
[9]   EVIDENCE FOR A COMMON ORIGIN OF ELECTRONS RESPONSIBLE FOR IMPULSIVE X-RAY AND TYPE-III RADIO BURSTS [J].
KANE, SR .
SOLAR PHYSICS, 1972, 27 (01) :174-181
[10]   SPECTRAL CHARACTERISTICS OF IMPULSIVE SOLAR-FLARE X-RAYS GREATER THAN OR APPROXIMATELY EQUAL TO 10 KEV [J].
KANE, SR ;
ANDERSON, KA .
ASTROPHYSICAL JOURNAL, 1970, 162 (03) :1003-&