COMPARISON OF 3 SOLAR ACTIVE REGIONS BASED ON THEIR SOFT-X-RAY LINE SPECTRA

被引:10
作者
BRABBAN, DH [1 ]
机构
[1] MULLARD SPACE SCI LAB,DORKING,SURREY,ENGLAND
关键词
D O I
10.1007/BF00155081
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:449 / 464
页数:16
相关论文
共 21 条
[1]   CORONAL SURVEY IN X-RAYS OF O VII AND NE IX [J].
ACTON, LW ;
CATURA, RC ;
WOLFSON, CJ ;
CULHANE, JL ;
MEYEROTT, AJ .
SOLAR PHYSICS, 1972, 26 (01) :183-&
[2]   FURTHER X-RAY SPECTRA OF SOLAR ACTIVE REGIONS [J].
BATSTONE, RM ;
EVANS, K ;
PARKINSON, JH ;
POUNDS, KA .
SOLAR PHYSICS, 1970, 13 (02) :389-+
[3]  
BEIGMAN IL, 1967, SOV ASTRON, V11, P531
[4]   CRYSTAL SPECTROMETRY OF ACTIVE REGIONS ON SUN [J].
BRABBAN, DH ;
GLENCROSS, WM .
PROCEEDINGS OF THE ROYAL SOCIETY OF LONDON SERIES A-MATHEMATICAL AND PHYSICAL SCIENCES, 1973, 334 (1597) :231-+
[5]  
CHAMBE G, 1971, ASTRON ASTROPHYS, V12, P210
[6]  
CHARLES MW, 1968, THESIS U LEICESTER
[7]   INTERPRETATION OF SOLAR HELIUM-LIKE ION LINE INTENSITIES [J].
GABRIEL, AH ;
JORDAN, C .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1969, 145 (02) :241-&
[8]  
HENKE BL, 1967, NORELCO REP, V14, P112