WebMHD can be described by a set of equations consisting of a continuity equation, an equation of motion, an equation of state, Ampère's Law, Faraday's law, and Ohm's law. As with any fluid description to a kinetic system, a closure approximation must be applied to highest moment of the particle distribution equation. WebMar 5, 2024 · In this paper, we consider the following thr ee-dimensional (3D) generalized MHD-Boussinesq equations: ∇· u = 0 , ∇· b = 0 , u ( x , 0 )= u 0 ( x ) , b ( x , 0 )= b 0 ( x ) …
On smoothness of 3D generalized MHD equations
WebDec 1, 2003 · To the best of our knowledge, Corollary 1.3 provides the first non-uniqueness result for the weak solutions to generalized MHD equations (1.1) with α i ∈ (0, 5/4), i = … WebMay 2, 2024 · This paper considers the problem of the local existence for the generalized MHD equations with fractional dissipative terms $$\\Lambda ^{2\\alpha } u$$ Λ 2 α u for the velocity field and $$\\Lambda ^{2\\beta } b$$ Λ 2 β b for the magnetic field, respectively. Based on some new commutator estimates, local existence for the generalized MHD … black auctioneers drogheda
Global well-posedness of the generalized magnetohydrodynamic equations ...
WebJun 21, 2014 · In this paper we prove the global-in-time existence of smooth solutions of the 2D generalized MHD system with fractional diffusion (-\Delta )^\alpha u, 0<\alpha <\frac {1} {2}. 1 Introduction In this paper, we consider the following 2D generalized MHD system [ 4 ]: \begin {aligned}&\mathrm {div}\,u=\mathrm {div}\,b=0,\end {aligned} (1.1) WebOct 22, 2015 · In this paper, we consider regularity criteria for the 3D generalized MHD and Hall-MHD systems with fractional dissipative terms. Some scaling invariant regularity criteria are established for the two systems. Global regularity for the Hall-MHD equation is also proved for the case $$\\alpha \\ge \\frac{5}{4}, \\beta \\ge \\frac{7}{4}$$ α ≥ 5 4 , β ≥ 7 4 . WebSep 24, 2024 · We proved analytically that for \varepsilon small enough, in the case of prepared initial velocity, we can solve the 3D rotating MHD system by solving only its linear part and the 2D Navier–Stokes equation. Since prepared data are something that can be easily managed in industry and laboratories, our method will make things easier in practice. black auburn hair color