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Title: Simulating gyrokinetic microinstabilities in stellarator geometry with GS2

Journal Article · · Physics of Plasmas
DOI:https://doi.org/10.1063/1.3662064· OSTI ID:22047122
; ; ; ; ;  [1];  [2];  [3];  [4]
  1. Princeton Plasma Physics Laboratory, Princeton, New Jersey 08543 (United States)
  2. General Atomics, San Diego, California 92186 (United States)
  3. Department of Physics, University of Maryland, College Park, Maryland 20742 (United States)
  4. Max-Planck-Institut fuer Plasmaphysik, D-17491 Greifswald (Germany)

The nonlinear gyrokinetic code GS2 has been extended to treat non-axisymmetric stellarator geometry. Electromagnetic perturbations and multiple trapped particle regions are allowed. Here, linear, collisionless, electrostatic simulations of the quasi-axisymmetric, three-field period national compact stellarator experiment (NCSX) design QAS3-C82 have been successfully benchmarked against the eigenvalue code FULL. Quantitatively, the linear stability calculations of GS2 and FULL agree to within {approx}10%.

OSTI ID:
22047122
Journal Information:
Physics of Plasmas, Vol. 18, Issue 12; Other Information: (c) 2011 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 1070-664X
Country of Publication:
United States
Language:
English