MODEL FOR X-RAY-EMISSION FROM LOOP PROMINENCES

被引:3
作者
PHILLIPS, KJH [1 ]
ZIRKER, JB [1 ]
机构
[1] UNIV HAWAII,INST ASTRON,HONOLULU,HI 96822
关键词
D O I
10.1007/BF02260208
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:41 / 58
页数:18
相关论文
共 33 条
[1]  
Alfven H., 1963, COSMICAL ELECTRODYNA
[2]  
Allen C. W., 1973, ASTROPHYSICAL QUANTI
[3]  
Athay R. G., 1971, Physics of the solar corona, P36
[4]   ON ASSOCIATION BETWEEN LOOP PROMINENCES + FLARES [J].
BRUZEK, A .
ASTROPHYSICAL JOURNAL, 1964, 140 (02) :746-&
[5]  
Carnahan B., 1969, APPL NUMERICAL METHO
[6]   IONIZATION EQUILIBRIUM AND RADIATIVE COOLING OF A LOW-DENSITY PLASMA [J].
COX, DP ;
TUCKER, WH .
ASTROPHYSICAL JOURNAL, 1969, 157 (3P1) :1157-&
[7]  
Culhane J. L., 1970, Solar Physics, V15, P394, DOI 10.1007/BF00151847
[8]   TRANSPORT COEFFICIENTS IN CHROMOSPHERE AND CORONAL GAS .2. THERMAL CONDUCTIVITY [J].
DELCROIX, A ;
LEMAIRE, A .
ASTROPHYSICAL JOURNAL, 1969, 156 (2P1) :787-&
[9]  
FISHER RR, 1974, SOL PHYS, V35, P401, DOI 10.1007/BF00151963
[10]   RAPID FINE STRUCTURE IN A BURST OF HARD SOLAR X-RAY OBSERVED BY OSO-5 [J].
FROST, KJ .
ASTROPHYSICAL JOURNAL, 1969, 158 (3P2) :L159-+