Singularity formation in a class of stretched solutions of the equations for ideal magneto-hydrodynamics

被引:9
|
作者
Gibbon, JD [1 ]
Ohkitani, K
机构
[1] Kyoto Univ, Math Sci Res Inst, Kyoto 6068502, Japan
[2] Univ London Imperial Coll Sci Technol & Med, Dept Math, London SW7 2BZ, England
关键词
D O I
10.1088/0951-7715/14/5/316
中图分类号
O29 [应用数学];
学科分类号
070104 ;
摘要
A class of stretched solutions of the equations for three-dimensional, incompressible, ideal magneto-hydrodynamics (MM) is studied. In Elsasser variables, V+/- = U +/- B, these solutions have the form V+/- = (upsilon (+/-), upsilon (+/-)(3)) where upsilon (+/-) = upsilon (+/-)(x, y, t) and upsilon (+/-)(3)(x, y, z, t) = zy(+/-)(x, y, t) + beta (+/-)(x, y, t). Two-dimensional partial differential equations for gamma (+/-), upsilon (+/-) and beta (+/-) are obtained that are valid in a tubular domain which is infinite in the z-direction with periodic cross section. Pseudo-spectral computations of these equations provide evidence for a blow-up in finite time in the above variables. This apparent blow-up is an infinite energy process that gives rise to certain subtleties; while all the variables appear to blow-up simultaneously, the two-dimensional part of the magnetic field b = 1/2(upsilon (+) - upsilon (-)) blows up at a very late stage. This 2 singularity in b is hard to detect numerically but supporting analytical evidence of a Lagrangian nature is provided for its existence. In three dimensions these solutions correspond to magnetic vortices developing along the axis of the tube prior to breakdown.
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页码:1239 / 1264
页数:26
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