MHD surface type quasi-modes of a current sheet model
نویسندگان
چکیده
Resonantly damped surface type quasi-modes are computed as eigenmodes of the linear dissipative MHD equations for a simple equilibrium model of a current sheet. The current sheet is modeled by a nonuniform plasma layer embedded in a uniform plasma environment. The physical equilibrium variables change in a continuous way in the nonuniform plasma layer. In particular, this is the case with both the strength and the orientation of the equilibrium magnetic field resulting from an electric current in the nonuniform plasma layer. The equilibrium layer can be viewed as a model for a reconnection site in the solar atmosphere or for current sheets in the Earth’s magnetosphere. Two surface type eigenmodes (kink and sausage) are numerically found that can propagate along the nonuniform plasma layer. The phase speeds of these eigenmodes are smaller than the Alfvén speed in the uniform environment. For oblique propagation to the equilibrium magnetic field, the eigenmodes resonantly couple to localized Alfvén waves leading to damped quasi-modes. It is shown that the wave damping is strongly anisotropic and that the dependence of the relative damping rate on the angle of propagation is different for the sausage and the kink type eigenmodes
منابع مشابه
Spectral Quasi-linearization for MHD Nanofluid Stagnation Boundary Layer Flow due to a Stretching/Shrinking Surface
This article concentrates on the effect of MHD heat mass transfer on the stagnation point nanofluid flow over a stretching or shrinking sheet with homogeneous-heterogeneous reactions. The flow analysis is disclosed in the neighborhood of stagnation point. Features of heat transport are characterized with Newtonian heating. The homogeneous-heterogeneous chemical reaction between the fluid and di...
متن کاملUnsteady convective flow for MHD powell-eyring fluid over inclined permeable surface
The current article has investigated unsteady convective flow for MHD non-Newtonian Powell-Eyring fluid embedded porous medium over inclined permeable stretching sheet. We have pondered the thermophoresis parameter, chemical reaction, variable thermal conductivity, Brownian motion, variable heat source and variable thermal radiation in temperature and concentration profiles. Using similar trans...
متن کاملPrepared for the U.s. Department of Energy, under Contract De-ac02-76ch03073 Princeton Plasma Physics Laboratory Princeton University, Princeton, New Jersey
Based on the ideal MHD model the stability of ballooning modes is investigated by employing realistic 3D magnetospheric equilibria, in particular for the substorm growth phase. Previous MHD ballooning stability calculations making use of approximations on the plasma compressibility can give rise to erroneous conclusions. Our results show that without making approximations on the plasma compress...
متن کاملA Coronal Magnetic Field Model with Horizontal Volume and Sheet Currents
When globally mapping the observed photospheric magnetic field into the corona, the interaction of the solar wind and magnetic field has been treated either by imposing source surface boundary conditions that tacitly require volume currents outside the source surface (Schatten, Wilcox, and Ness, 1969) or by limiting the interaction to thin current sheets between oppositely directed field region...
متن کاملResonant absorption in dissipative flux tubes
We study the resonant absorption of MHD waves in magnetized flux tubes with a radial density inhomogeneity. Within the approximation that resistive and viscous processes are operative in thin layers surrounding the singularities of the MHD equations, we give the full spectrum of the eigenfrequencies and damping rates of the MHD quasi modes of the tube. Both surface and body modes are analyzed.
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 1997