skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Efficient magnetic fields for supporting toroidal plasmas

Journal Article · · Physics of Plasmas
DOI:https://doi.org/10.1063/1.4943201· OSTI ID:22599045
 [1];  [2]
  1. Institute for Research in Electronics and Applied Physics, University of Maryland, College Park, Maryland 20742 (United States)
  2. Department of Applied Physics and Applied Mathematics, Columbia University, New York, New York 10027 (United States)

The magnetic field that supports tokamak and stellarator plasmas must be produced by coils well separated from the plasma. However, the larger the separation, the more difficult it is to produce a given magnetic field in the plasma region, so plasma configurations should be chosen that can be supported as efficiently as possible by distant coils. The efficiency of an externally generated magnetic field is a measure of the field's shaping component magnitude at the plasma compared to the magnitude near the coils; the efficiency of a plasma equilibrium can be measured using the efficiency of the required external shaping field. Counterintuitively, plasma shapes with low curvature and spectral width may have low efficiency, whereas plasma shapes with sharp edges may have high efficiency. Two precise measures of magnetic field efficiency, which correctly identify such differences in difficulty, will be examined. These measures, which can be expressed as matrices, relate the externally produced normal magnetic field on the plasma surface to the either the normal field or current on a distant control surface. A singular value decomposition (SVD) of either matrix yields an efficiency ordered basis for the magnetic field distributions. Calculations are carried out for both tokamak and stellarator cases. For axisymmetric surfaces with circular cross-section, the SVD is calculated analytically, and the range of poloidal and toroidal mode numbers that can be controlled to a given desired level is determined. If formulated properly, these efficiency measures are independent of the coordinates used to parameterize the surfaces.

OSTI ID:
22599045
Journal Information:
Physics of Plasmas, Vol. 23, Issue 3; Other Information: (c) 2016 AIP Publishing LLC; Country of input: International Atomic Energy Agency (IAEA); ISSN 1070-664X
Country of Publication:
United States
Language:
English

Cited By (8)

Stellarator Research Opportunities: A Report of the National Stellarator Coordinating Committee journal February 2018
Curl-free magnetic fields for stellarator optimization journal October 2019
Designing stellarator coils by a modified Newton method using FOCUS journal April 2018
An improved current potential method for fast computation of stellarator coil shapes journal February 2017
Recent advances in stellarator optimization journal October 2017
An adjoint method for gradient-based optimization of stellarator coil shapes journal May 2018
Curl-free magnetic fields for stellarator optimization text January 2019
Combined plasma-coil optimization algorithms text January 2020