SPATIAL STRUCTURE AND TEMPORAL DEVELOPMENT OF A SOLAR X-RAY FLARE OBSERVED FROM SKYLAB ON JUNE 15, 1973

被引:57
作者
PALLAVICINI, R
VAIANA, GS
KAHLER, SW
KRIEGER, AS
机构
[1] SMITHSONIAN ASTROPHYS OBSERV,CAMBRIDGE,MA 02138
[2] AMER SCI & ENGN INC,CAMBRIDGE,MA 02138
关键词
D O I
10.1007/BF00158459
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:411 / 433
页数:23
相关论文
共 25 条
[1]   ON ASSOCIATION BETWEEN LOOP PROMINENCES + FLARES [J].
BRUZEK, A .
ASTROPHYSICAL JOURNAL, 1964, 140 (02) :746-&
[2]  
BRUZEK A, 1969, SOLAR FLARES SPACE R, P61
[3]  
Culhane J. L., 1970, Solar Physics, V15, P394, DOI 10.1007/BF00151847
[5]   OSO-7 OBSERVATIONS OF SOLAR X-RAYS IN ENERGY-RANGE 10-100 KEV [J].
DATLOWE, DW ;
ELCAN, MJ ;
HUDSON, HS .
SOLAR PHYSICS, 1974, 39 (01) :155-174
[6]  
Godoli G., 1975, Osservazioni e Memorie dell'Osservatorio Astrofisico di Arcetri, P169
[7]  
HORAN DM, 1973, COMMUNICATION
[8]   SOFT-X-RAY AND MICROWAVE OBSERVATIONS OF HOT REGIONS IN SOLAR-FLARES [J].
HUDSON, HS ;
OHKI, K .
SOLAR PHYSICS, 1972, 23 (01) :155-&
[9]  
Kahler S. W., 1975, Astrophysical Journal. Letters to the Editor, V199, pL57, DOI 10.1086/181848
[10]  
Krieger A. S., 1971, SOLAR MAGNETIC FIELD, V43, P397