GENERATION OF MAGNETIC FIELDS IN ASTROPHYSICAL BODIES .3. TURBULENT DIFFUSION OF FIELDS AND EFFICIENT DYNAMOS

被引：111

作者：

PARKER, EN

机构：

来源：

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D O I：

10.1086/150766

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：279 / &

共 18 条

[1] THE EFFECT OF HOMOGENEOUS TURBULENCE ON MATERIAL LINES AND SURFACES
BATCHELOR, GK
[J]. PROCEEDINGS OF THE ROYAL SOCIETY OF LONDON SERIES A-MATHEMATICAL AND PHYSICAL SCIENCES, 1952, 213 (1114): : 349 - &
[2] BATCHELOR GK, 1956, SURVEYS MECHANICS
[3] ELSASSER WM, 1956, REV MOD PHYS, V29, P135
[4] GROWTH OF TURBULENT MAGNETIC FIELDS
KRAICHNAN, RH
[J]. PHYSICS OF FLUIDS, 1967, 10 (04) : 859 - +
[5] KRAICHNAN RH, UNPUBLISHED COMMUNIC
[6] KRAUSE F, 1969, ACTA U WRAT, P157
[7] A MAGNETO-KINEMATIC MODEL OF SOLAR CYCLE
LEIGHTON, RB
[J]. ASTROPHYSICAL JOURNAL, 1969, 156 (1P1) : 1 - &
[8] LUNDQUIST S, 1952, ARK FYS, V5, P297
[9] GENERATION OF MAGNETIC FIELDS IN ASTROPHYSICAL BODIES .2. GALACTIC FIELD
PARKER, EN
[J]. ASTROPHYSICAL JOURNAL, 1971, 163 (02) : 255 - &
[10] ORIGIN OF MAGNETIC FIELDS
PARKER, EN
[J]. ASTROPHYSICAL JOURNAL, 1970, 160 (02) : 383 - &