NON-LINEAR EVOLUTION OF THE MAGNETO-HYDRODYNAMIC KELVIN-HELMHOLTZ INSTABILITY

被引：97

作者：

MIURA, A

机构：

来源：

关键词：

D O I：

10.1103/PhysRevLett.49.779

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

引用

页码：779 / 782

页数：4

共 10 条

AXFORD, WI ;

HINES, CO .

[2] KELVIN-HELMHOLTZ INSTABILITY IN A HIGH-BETA COLLISIONLESS PLASMA [J].

DOBROWOLNY, M .

[3]

DUNGEY JW, 1955, P IONOSPHERE C, P225

[4] MAGNETIC VISCOSITY IN RELATIVISTIC ACCRETION DISKS [J].

EARDLEY, DM ;

LIGHTMAN, AP .

[5] LONG-WAVELENGTH TURBULENCE AND HEATING OF SOLAR WIND [J].

JOKIPII, JR ;

DAVIS, L .

[6]

MIURA A, UNPUB

[7]

Parker E. N., 1963, Interplanetary dynamical processes

[8]

PARKER EN, 1958, ASTROPHYS J, V128, P6640

[9]

RUSSELL CT, 1978, SPACE SCI REV, V22, P68

[10] 2-FLUID MODEL OF SOLAR WIND [J].

STURROCK, PA ;

HARTLE, RE .