Published March 1987 | Version v1
Report Open

Instability due to magnetic viscosity in perpendicular MHD

Creators

  • 1. Royal Inst. of Techn., Stockholm (Sweden). Dep. of Plasma Physics and Fusion Research
  • 2. Max Planck Inst. fuer Plasmaphysik, Garching (Germany,F.R.)

Description

The Perpendicular MHD model predicts exponentially growing Alfven waves in a static, homogeneous plasma equilibrium with isotropic pressure when gyroviscosity is included. (authors)

Availability note (English)

Also available from:Royal Inst. of Techn.,Library,S-10044 Stockholm (Sweden).

Files

19038130.pdf

Files (104.6 kB)

Name Size Download all
md5:69e51b4d6cacb0f61c9c839d5bd2d835
104.6 kB Preview Download

Additional details

Publishing Information

Imprint Pagination
9 p.
Report number
TRITA-PFU--86-12

INIS

Country of Publication
Sweden
Country of Input or Organization
Sweden
INIS RN
19038130
Subject category
S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
Descriptors DEI
EQUILIBRIUM PLASMA; INSTABILITY; LARMOR RADIUS; MAGNETOHYDRODYNAMICS; PLASMA; PLASMA SIMULATION; VISCOSITY
Descriptors DEC
FLUID MECHANICS; HYDRODYNAMICS; MECHANICS; SIMULATION