Here, we find that the kinetic and fluid linear drift resonances have several similarities. The reason for our interest in this is that our fluid model has recently been shown to be exact for drift waves and other modes in that frequency range. Thus, transport is driven by the fluid linear growth rate and our drift wave system behaves like a cold beam-plasma system although it has a finite temperature. A main similarity is that neither fluid nor kinetic responses should be expanded in the curvature in the bulk interior of tokamaks. That we can use the fluid response close to the magnetic drift resonance is a consequence of the fact that the closure is exact. A systematic orbit integration technique is introduced for deriving the fluid model and evaluating the effects of nonlinearities. Published by AIP Publishing.
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Univ Calif San Diego, Ctr Astrophys & Space Sci, La Jolla, CA 92093 USA
Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USAUniv Calif San Diego, Ctr Astrophys & Space Sci, La Jolla, CA 92093 USA
McDevitt, C. J.
Diamond, P. H.
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Univ Calif San Diego, Ctr Astrophys & Space Sci, La Jolla, CA 92093 USA
Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USAUniv Calif San Diego, Ctr Astrophys & Space Sci, La Jolla, CA 92093 USA
Diamond, P. H.
Gurcan, O. D.
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Univ Calif San Diego, Ctr Astrophys & Space Sci, La Jolla, CA 92093 USA
Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USAUniv Calif San Diego, Ctr Astrophys & Space Sci, La Jolla, CA 92093 USA
Gurcan, O. D.
Hahm, T. S.
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Princeton Univ, Princeton Plasma Phys Lab, Princeton, NJ 08543 USAUniv Calif San Diego, Ctr Astrophys & Space Sci, La Jolla, CA 92093 USA