HEATING OF SOLAR ACTIVE REGIONS BY MAGNETIC ENERGY DISSIPATION - STEADY-STATE CASE

被引:85
作者
TUCKER, WH
机构
关键词
D O I
10.1086/152498
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:285 / 289
页数:5
相关论文
共 16 条
[1]  
Alfven H., 1963, COSMICAL ELECTRODYNA
[2]   FORCE-FREE MAGNETIC-FIELD STRUCTURES AND THEIR ROLE IN SOLAR-ACTIVITY [J].
BARNES, CW ;
STURROCK, PA .
ASTROPHYSICAL JOURNAL, 1972, 174 (03) :659-&
[3]   FURTHER X-RAY SPECTRA OF SOLAR ACTIVE REGIONS [J].
BATSTONE, RM ;
EVANS, K ;
PARKINSON, JH ;
POUNDS, KA .
SOLAR PHYSICS, 1970, 13 (02) :389-+
[4]  
Beigman I. L., 1970, Astronomicheskii Zhurnal, V47, P1030
[5]   PROCESSES OF MAGNETIC-ENERGY CONVERSION AND SOLAR FLARES [J].
COPPI, B ;
FRIEDLAND, AB .
ASTROPHYSICAL JOURNAL, 1971, 169 (02) :379-+
[6]   ANOMALOUS PLASMA RESISTIVITY AT LOW ELECTRIC FIELDS [J].
COPPI, B ;
MAZZUCAT.E .
PHYSICS OF FLUIDS, 1971, 14 (01) :134-+
[7]  
GOLD T, 1964, PHYSICS SOLAR FLARES, P389
[8]   ELECTRICAL CONDUCTIVITY OF A HIGHLY TURBULENT PLASMA [J].
HAMBERGER, SM ;
FRIEDMAN, M .
PHYSICAL REVIEW LETTERS, 1968, 21 (10) :674-+
[9]  
KAUFMAN AN, 1966, PLASMA PHYSICS THEOR
[10]  
KRIEGER AS, 1971, SOLAR MAGNETIC FIELD, P397