Hostname: page-component-cd9895bd7-gbm5v Total loading time: 0 Render date: 2024-12-25T04:23:13.352Z Has data issue: false hasContentIssue false
  • English
  • Français

SPECTOR3D: a resistive magnetohydrodynamic stability code for stellarators

Published online by Cambridge University Press:  20 December 2006

B.F. McMILLAN  and
R.G. STORER
B.F. McMILLAN
Affiliation:
Department of Theoretical Physics, Research School of Physical Sciences and Engineering, The Australian National University, Australia and School of Physics, Sydney University, Australia
R.G. STORER
Affiliation:
School of Chemistry, Physics and Earth Sciences, Flinders University, SA 5052, Australia ([email protected])
Get access Rights & Permissions [Opens in a new window]

Abstract

SPECTOR3D is a magnetohydrodynamic (MHD) code designed to study the resistive stability and mode spectrum of stellarators. It finds the spectrum of the linearized, compressible, resistive MHD equations. Some typical results are given for a tokamak model with toroidal field ripple and a 17-period Heliotron.

Type
Papers
Information
Journal of Plasma Physics , Volume 72 , Issue 6 , December 2006 , pp. 829 - 832
Copyright
2006 Cambridge University Press

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)