MODEL FOR DEVELOPMENT OF A SOLAR OUTBURST BASED ON OBSERVATIONS WITH CULGOORA RADIO SPECTROGRAPH AND HELIOGRAPH

被引:10
作者
KAI, K [1 ]
机构
[1] CSIRO,DIV RADIOPHYS,SYDNEY,AUSTRALIA
关键词
D O I
10.1007/BF00152233
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:217 / 226
页数:10
相关论文
共 18 条
[1]   MOVING TYPE-IV RADIO BURST AND ITS RELATION TO CORONAL MAGNETIC-FIELD [J].
DULK, GA ;
ALTSCHULER, MD .
SOLAR PHYSICS, 1971, 20 (02) :438-+
[2]  
DULK GA, 1971, AUST J PHYS, V24, P239
[3]   CORONAL MAGNETIC-FIELD STRUCTURE DERIVED FROM 2-FREQUENCY RADIOHELIOGRAPH OBSERVATIONS [J].
KAI, K ;
SHERIDAN, KV .
SOLAR PHYSICS, 1974, 35 (01) :181-192
[4]  
KAI K, IN PRESS
[5]  
McLean D. J., 1973, Proceedings of the Astronomical Society of Australia, V2, P222
[6]  
Robinson R. D., 1974, Proceedings of the Astronomical Society of Australia, V2, P258
[7]  
Schmahl EJ, 1972, P ASTRON SOC AUSTRAL, V2, P95
[8]  
SCHMAHL EJ, 1973, AUSTRALIAN J PHY S29
[9]  
Sheridan K. V., 1967, Proceedings of the Astronomical Society of Australia, V1, P58
[10]  
SHERIDAN KV, 1973, P I ELEC ELECTRON EN, V61, P1321