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Existence and stability of compressible current-vortex sheets in three-dimensional magnetohydrodynamics

机译:三维磁流体动力学中可压缩电流涡旋片的存在与稳定性

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Compressible vortex sheets are fundamental waves, along with shocks and rarefaction waves, in entropy solutions to multidimensional hyperbolic systems of conservation laws. Understanding the behavior of compressible vortex sheets is an important step towards our full understanding of fluid motions and the behavior of entropy solutions. For the Euler equations in two-dimensional gas dynamics, the classical linearized stability analysis on compressible vortex sheets predicts stability when the Mach number M > root 2 and instability when M > root 2; and Artola and Majda's analysis reveals that the nonlinear instability may occur if planar vortex sheets are perturbed by highly oscillatory waves even when M > root 2. For the Euler equations in three dimensions, every compressible vortex sheet is violently unstable and this instability is the analogue of the Kelvin-Helmholtz instability for incompressible fluids. The purpose of this paper is to understand whether compressible vortex sheets in three dimensions, which are unstable in the regime of pure gas dynamics, become stable under the magnetic effect in three-dimensional magnetohydrodynamics (MHD). One of the main features is that the stability problem is equivalent to a free-boundary problem whose free boundary is a characteristic surface, which is more delicate than noncharacteristic free-boundary problems. Another feature is that the linearized problem for current-vortex sheets in MHD does not meet the uniform Kreiss-Lopatinskii condition. These features cause additional analytical difficulties and especially prevent a direct use of the standard Picard iteration to the nonlinear problem. In this paper, we develop a nonlinear approach to deal with these difficulties in three-dimensional MHD. We first carefully formulate the linearized problem for the current-vortex sheets to show rigorously that the magnetic effect makes the problem weakly stable and establish energy estimates, especially high-order energy estimates, in terms of the nonhomogeneous terms and variable coefficients. Then we exploit these results to develop a suitable iteration scheme of the Nash-Moser-Hormander type to deal with the loss of the order of derivative in the nonlinear level and establish its convergence, which leads to the existence and stability of compressible current-vortex sheets, locally in time, in three-dimensional MHD.
机译:可压缩的涡旋片是基波,以及冲击波和稀疏波,是对守恒律的多维双曲系统的熵解。理解可压缩涡流片的行为是迈向我们全面理解流体运动和熵解行为的重要一步。对于二维气体动力学中的欧拉方程,在可压缩涡旋片上进行的经典线性稳定性分析预测了当马赫数M>根2时的稳定性和当M>根2时的不稳定性。 Artola和Majda的分析表明,即使当M>根2时,如果平面涡旋片受到高振荡波的扰动,非线性不稳定也可能发生。对于三维的Euler方程,每个可压缩涡旋片都是剧烈不稳定的,并且这种不稳定性是类似的不可压缩流体的Kelvin-Helmholtz不稳定性本文的目的是了解在纯磁动力学范围内不稳定的三维可压缩涡流片在三维磁流体动力学(MHD)的磁性作用下是否稳定。主要特征之一是稳定性问题等效于自由边界是特征表面的自由边界问题,它比非特征性自由边界问题更为微妙。另一个特征是MHD中的电流涡旋片的线性化问题不满足统一的Kreiss-Lopatinskii条件。这些特征引起额外的分析困难,尤其是阻止标准Picard迭代直接用于非线性问题。在本文中,我们开发了一种非线性方法来解决三维MHD中的这些困难。我们首先仔细地为电流涡旋片精心制定线性化问题,以严格表明磁效应使问题变得微弱稳定,并根据非齐次项和可变系数建立了能量估计,尤其是高阶能量估计。然后,我们利用这些结果开发出一个合适的Nash-Moser-Hormander型迭代方案,以处理非线性水平上导数阶的损失并建立其收敛性,从而导致可压缩电流涡旋的存在和稳定性。三维MHD,在当地及时显示。

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