Shear Wave Dissipation in Planar MagneticX‐Points
Author(s) -
I. J. D. Craig,
A. N. McClymont
Publication year - 1997
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/304082
Subject(s) - physics , dissipation , shear (geology) , mechanics , planar , classical mechanics , magnetic field , resistive touchscreen , energy flux , nonlinear system , perpendicular , magnetohydrodynamics , alfvén wave , condensed matter physics , geometry , quantum mechanics , petrology , computer graphics (images) , computer science , geology , mathematics , engineering , electrical engineering
The resistive dissipation of nonlinear shear wave disturbances is discussed. We consider an incompressible, “open” 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
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