Intrinsic Ambipolarity and Rotation in Stellarators

P. Helander and A. N. Simakov
Phys. Rev. Lett. 101, 145003 – Published 29 September 2008

Abstract

It is shown that collisional plasma transport is intrinsically ambipolar only in quasiaxisymmetric or quasihelically symmetric magnetic configurations. Only in such fields can the plasma rotate freely, and then only in the direction of quasisymmetry. In a non-quasi-symmetric magnetic field, the average radial electric field is determined by parallel viscosity, which in turn is usually governed by collisional processes. Locally, the radial electric field may be affected by turbulent Reynolds stress producing zonal flows, but on a radial average taken over several ion gyroradii, it is determined by parallel viscosity, at least if the turbulence is electrostatic and obeys the conventional gyrokinetic orderings. This differs from the situation in a tokamak, where there is no flow damping by parallel viscosity in the symmetry direction and the turbulent Reynolds stress may affect the global radial electric field.

  • Received 17 March 2008

DOI:https://doi.org/10.1103/PhysRevLett.101.145003

©2008 American Physical Society

Authors & Affiliations

P. Helander1 and A. N. Simakov2

  • 1Max-Planck-Institut für Plasmaphysik, 17491 Greifswald, Germany
  • 2Los Alamos National Laboratory, Los Alamos, New Mexico 87544, USA

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 101, Iss. 14 — 3 October 2008

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review Letters

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×