CORONAL HOLES - MASS-LOSS DRIVEN BY MAGNETIC RECONNECTION

被引:23
作者
MULLAN, DJ [1 ]
AHMAD, IA [1 ]
机构
[1] ANDRULIS RES CORP,BETHESDA,MD 20014
关键词
D O I
10.1007/BF00153482
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:347 / 350
页数:4
相关论文
共 18 条
[1]   X-RAY ANALYSIS OF A POLAR PLUME [J].
AHMAD, IA ;
WEBB, DF .
SOLAR PHYSICS, 1978, 58 (02) :323-336
[2]  
BRUECKNER GE, 1980, 17 P GEN ASS IAU
[3]  
Davis JM, 1980, B AM ASTRON SOC, V12, P518
[4]   MAGNETIC-PROPERTIES OF X-RAY BRIGHT POINTS [J].
GOLUB, L ;
KRIEGER, AS ;
HARVEY, JW ;
VAIANA, GS .
SOLAR PHYSICS, 1977, 53 (01) :111-121
[5]   SPATIAL AND TEMPORAL VARIATIONS OF EUV CORONAL BRIGHT POINTS [J].
HABBAL, SR ;
WITHBROE, GL .
SOLAR PHYSICS, 1981, 69 (01) :77-97
[6]   THEORETICAL MODEL OF FLARES AND PROMINENCES .1. EVAPORATING FLARE MODEL [J].
HIRAYAMA, T .
SOLAR PHYSICS, 1974, 34 (02) :323-338
[7]  
KOHL JL, 1980, ASTROPHYS J LETT, V241, pL121
[8]  
KOPP RA, 1976, SOL PHYS, V49, P43, DOI 10.1007/BF00221484
[9]   ENERGY ADDITION IN THE SOLAR-WIND [J].
LEER, E ;
HOLZER, TE .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1980, 85 (NA9) :4681-4688
[10]  
LOW BC, 1980, B AM ASTRON SOC, V12, P902