Stability and inviscid limit of the 3D anisotropic MHD system near a background magnetic field with mixed fractional partial dissipation

Abstract

A main result of this paper establishes the global stability of the three-dimensional MHD equations near a background magnetic field with mixed fractional partial dissipation with α,β∈(12,1]\alpha, \beta\in(\frac{1}{2}, 1]. Namely, the velocity equations involve dissipation (Λ12α+Λ22α+σΛ32α)u(\Lambda_1^{2\alpha} + \Lambda_2^{2\alpha}+\sigma \Lambda_3^{2\alpha})u with the case σ=1\sigma=1 and σ=0\sigma=0. The magnetic equations without partial magnetic diffusion Λi2βbi\Lambda_i^{2\beta} b_i but with the diffusion (−Δ)βb(-\Delta)^\beta b, where Λis(s>0)\Lambda_i^{s} (s>0) with i=1,2,3i=1, 2, 3 are the directional fractional operators. Then we focus on the vanishing vertical kinematic viscosity coefficient limit of the MHD system with the case σ=1\sigma=1 to the case σ=0\sigma=0. The convergent result is obtained in the sense of H1H^1-norm

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