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Title: Drift-Alfven kinetic stability theory in the ballooning mode approximation

Journal Article · · Phys Fluids B; (United States)
DOI:https://doi.org/10.1063/1.858937· OSTI ID:5971327

The coupled drift-shear Alfven mode including the complete Bessel function gyroradius effect and the /del//sub /perpendicular///ital B/ -curvature guiding center drift resonance of kinetic theory is solved for the toroidal ballooning mode eigenvalues and eigenfunctions. Comparisons between nonlocal (ballooning) and local kinetic theory and between nonlocal fluid and kinetic theory are made. The critical plasma pressure for kinetic ballooning mode instability is only the same as the magnetohydrodynamic (MHD) theory critical pressure /beta//sub MHD/ for /eta//sub /ital i//=0. The critical kinetic theory plasma pressure /beta//sub /ital K//(/eta//sub /ital i//) is well below /beta//sub MHD/ and the kinetic theory growth rate is unstable for all /ital k/. The MHD second stability region is also unstable in the kinetic theory. The kinetic theory growth rate is a maximum around /ital k//le/0.3--0.5 for finite aspect ratio /epsilon//sub /ital n//=/ital r//sub /ital n////ital R/. The effects of trapped electrons are found to be weakly stabilizing both analytically and numerically, and the instability is still significant outside the ideal MHD stable window from the ion magnetic drift resonances when /eta//sub /ital i///approx gt/1. The kinetic growth rate is a function of the six dimensionless parameters /ital k/, /ital q//sup 2//beta/, /epsilon//sub /ital n//, /ital s/, /eta//sub /ital i//, and /tau/=/ital T//sub /ital e////ital T//sub /ital i//.

Research Organization:
Department of Physics and Institute for Fusion Studies, The University of Texas at Austin, Austin, Texas 78712(US); Department of Physics, Korea Advanced Institute of Science and Technology, Post Office Box 150, Cheongryangni, Seoul, Korea
OSTI ID:
5971327
Journal Information:
Phys Fluids B; (United States), Vol. 1:8
Country of Publication:
United States
Language:
English