HYDRAULIC CONCENTRATION OF MAGNETIC-FIELDS IN SOLAR PHOTOSPHERE .1. TURBULENT PUMPING

被引:41
作者
PARKER, EN
机构
[1] UNIV CHICAGO,DEPT PHYS,CHICAGO,IL 60637
[2] UNIV CHICAGO,DEPT ASTRON & ASTROPHYS,CHICAGO,IL 60637
关键词
D O I
10.1086/152835
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:563 / 568
页数:6
相关论文
共 39 条
[1]  
ALFVEN H, 1961, ARK FYS, V19, P375
[2]  
ALFVEN H, 1963, SOLAR CORONA
[3]  
[Anonymous], 1941, VIERTELJAHRESSCHRIFT
[4]  
Beckers J. M., 1968, SOL PHYS, V4, P142
[6]  
BECKERS JM, 1968, SOL PHYS, V3, P258
[7]  
Bohm-Vitense E., 1958, Z ASTROPHYS, V46, P108
[8]  
Chandrasekhar S., 1961, HYDRODYNAMIC HYDROMA
[9]   SOME KINEMATICAL MODELS FOR SMALL-SCALE SOLAR MAGNETIC FIELDS [J].
CLARK, A .
PHYSICS OF FLUIDS, 1966, 9 (03) :485-&
[10]  
Clark A. Jr., 1968, Solar Physics, V4, P386, DOI 10.1007/BF00147904