INTERPRETATION OF DISTINCT TYPE-IV-MA-BURSTS AND TYPE-IV-MU-BURSTS ON BASIS OF MICRO-INSTABILITIES AND OF RESONANT NONLINEAR-INTERACTION OF WAVES

被引:6
作者
MOLLWO, L [1 ]
机构
[1] DAWB,ZENT INST SOLAR TERR PHYS,BERLIN,EAST GERMANY
关键词
D O I
10.1007/BF00152679
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:497 / 511
页数:15
相关论文
共 77 条
[1]   TYPE 3 RADIO BURSTS IN OUTER CORONA [J].
ALEXANDER, JK ;
MALITSON, HH ;
STONE, RG .
SOLAR PHYSICS, 1969, 8 (02) :388-+
[3]  
[Anonymous], 1964, NASA SPECIAL PUBLICA
[4]  
BAUMGARTEL K, 1967, ERGEBNISSE PLASMAPHY, V1
[5]  
BAUMGARTEL K, 1969, THESIS HUMBOLDT U
[6]  
BAUMGARTEL K, TO BE PUBLISHED
[7]   CONVECTIVE AND ABSOLUTE ION CYCLOTRON INSTABILITIES IN HOMOGENEOUS PLASMAS [J].
BEASLEY, CO ;
CORDEY, JG .
PLASMA PHYSICS, 1968, 10 (04) :411-&
[8]  
Bers A., 1963, WAVES ANISOTROPIC PL
[9]   SOLAR CORONAL STREAMERS .2. EVOLUTION OF DISCRETE FEATURES FROM SUN TO 1 AU [J].
BOHLIN, JD .
SOLAR PHYSICS, 1970, 13 (01) :153-&
[10]   ROCKET-CORONAGRAPH PHOTOMETRY OF 7 MARCH, 1970 CORONA FROM 3 TO 8.5 RS [J].
BOHLIN, JD ;
KOOMEN, MJ ;
TOUSEY, R .
SOLAR PHYSICS, 1971, 21 (02) :408-&