Exact magnetohydrodynamic equilibria with flow and effects on the Shafranov shift

Abstract

Exact solutions of the equation governing the equilibrium magetohydrodynamic states of an axisymmetric plasma with incompressible flows of arbitrary direction [H. Tasso and G.N.Throumoulopoulos, Phys. Pasmas {\bf 5}, 2378 (1998)] are constructed for toroidal current density profiles peaked on the magnetic axis in connection with the ansatz $S=-ku$, where $S=d/du[\varrho (d\Phi /du{)}^2]$ ($k$ is a parameter, $u$ labels the magnetic surfaces; $\varrho (u)$ and $\Phi (u)$ are the density and the electrostatic potential, respectively). They pertain to either unbounded plasmas of astrophysical concern or bounded plasmas of arbitrary aspect ratio. For $k=0$, a case which includes flows parallel to the magnetic field, the solutions are expressed in terms of Kummer functions while for $k\ne 0$ in terms of Airy functions. On the basis of a tokamak solution with $k\ne 0$ describing a plasma surrounded by a perfectly conducted boundary of rectangular cross-section it turns out that the Shafranov shift is a decreasing function which can vanish for a positive value of $k$. This value is larger the smaller the aspect ratio of the configuration.

13 pages, 2 figures. v2:Eq (3) has been corrected. A new figure (Fig. 2) has been added in order to illustrate u-contours in connection with solution (24) and the Shafranov shift. Also, a sentence referring to Fig. 2 has been added after Eq. (25)

References in corpus (1)

• Axisymmetric equilibria of a gravitating plasma with incompressible flows

Cited by in corpus (2)

• On non existence of tokamak equilibria with purely poloidal flow
• On the steady axisymmetric vortex rings for 3-D incompressible Euler flows