Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-26T00:57:41.988Z Has data issue: false hasContentIssue false

Helicity resonant influence on the local Alfvén resonance structure in straight stellarators

Published online by Cambridge University Press:  10 March 2003

I. O. GIRKA
Affiliation:
Kharkiv National University, Svobody Sq. 4, Kharkiv, 61077, Ukraine ([email protected])
V. I. LAPSHIN
Affiliation:
Kharkiv National University, Svobody Sq. 4, Kharkiv, 61077, Ukraine ([email protected])

Abstract

Distribution of antenna-driven electromagnetic wave fields within the local Alfvén resonance is studied under resonant conditions such that the axial period of the fundamental harmonic of the magnetohydrodynamic oscillations in the axial direction is twice as large as the pitch length, and the poloidal number of the fundamental harmonic is twice as small as the polarity of the helical coils. It is shown that taking account of the helical inhomogeneity of the steady magnetic field can remove the infinite discontinuity of the wave fields that takes place in a straight magnetic field rather than with electron inertia or a finite ion Larmor radius.

Type
Research Article
Copyright
2002 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.)