AMPLIFICATION OF MAGNETIC-FIELDS DURING RADIATION ERA

被引:10
作者
BAIERLEIN, R
机构
[1] Department of Physics, Wesleyan University, Middletown,CT,06457, United States
关键词
Compendex;
D O I
10.1093/mnras/184.4.843
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Magnetic fields
引用
收藏
页码:843 / 870
页数:28
相关论文
共 13 条
[2]   EVOLUTION OF COSMIC-RADIATION SPECTRUM UNDER INFLUENCE OF TURBULENT HEATING .1. THEORY [J].
CHAN, KL ;
JONES, BJT .
ASTROPHYSICAL JOURNAL, 1975, 200 (02) :454-460
[3]   COSMIC TURBULENCE [J].
DRURY, LOC ;
STEWART, JM .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1976, 177 (02) :377-383
[4]   MAGNETIC-FIELDS IN EARLY UNIVERSE [J].
HARRISON, ER .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1973, 165 (02) :185-200
[5]   STANDARD MODEL OF EARLY UNIVERSE [J].
HARRISON, ER .
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1973, 11 :155-186
[6]   GENERATION OF MAGNETIC FIELDS IN RADIATION ERA [J].
HARRISON, ER .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1970, 147 (03) :279-&
[7]  
REES MJ, 1972, ASTRON ASTROPHYS, V19, P189
[9]   ON THE FINE-SCALE STRUCTURE OF VECTOR FIELDS CONVECTED BY A TURBULENT FLUID [J].
SAFFMAN, PG .
JOURNAL OF FLUID MECHANICS, 1963, 16 (04) :545-572
[10]  
SPITZER L, 1956, PHYSICS FULLY IONIZE