Published June 1997 | Version v1
Journal article

Shear wave dissipation in planar magnetic X-points

  • 1. University of Waikato, Private Bag 3105, Hamilton (New Zealand)
  • 2. Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, Hawaiian Island 96822 (United States)

Description

The resistive dissipation of nonlinear shear wave disturbances is discussed. We consider an incompressible, open-quotes openclose quotes X-point geometry, in which mass and energy are free to enter and leave the reconnection region. An analytic treatment is possible which unifies many of the dynamic and steady-state X-point solutions obtained previously. We show that while field disturbances in the plane of the X-point have the potential for rapid energy release when suitably driven, perpendicular shear disturbances dissipate slowly, at a rate ∼η1/2, where η is the plasma resistivity. This behavior can be understood in terms of the absence of flux pileup in nonplanar shear wave disturbances. We conclude that only planar shear waves have the potential for fast magnetic energy release. copyright 1997 The American Astronomical Society

Additional details

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
481
Journal Issue
2
Journal Page Range
p. 996-1003.
ISSN
0004-637X
CODEN
ASJOAB

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
29007991
Subject category
S30: DIRECT ENERGY CONVERSION; S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
Descriptors DEI
DISSIPATION FACTOR; HYDROMAGNETIC WAVES; INCOMPRESSIBLE FLOW; MAGNETIC RECONNECTION; MAGNETOHYDRODYNAMICS; NONLINEAR PROBLEMS; PLASMA; SHEAR
Descriptors DEC
FLUID FLOW; FLUID MECHANICS; HYDRODYNAMICS; MECHANICS