2012
DOI: 10.1063/1.4739291
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Magnetic island evolution in hot ion plasmas

Abstract: Effects of finite ion temperature on magnetic island evolution are studied by means of numerical simulations of a reduced set of two-fluid equations which include ion as well as electron diamagnetism in slab geometry. The polarization current is found to be almost an order of magnitude larger in hot than in cold ion plasmas, due to the strong shear of ion velocity around the separatrix of the magnetic islands. As a function of the island width, the propagation speed decreases from the electron drift velocity (… Show more

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Cited by 17 publications
(19 citation statements)
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References 37 publications
(66 reference statements)
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“…The resulting expression of the tearing instability index in the subsonic regime ω < k // C s , appropriate to the experiments of this paper, is presented in [46] and has been extensively studied numerically in [47] validating, for small as well as large islands the generic expression:…”
Section: Further Discussion Of the Instability Conditions For Ntms In...mentioning
confidence: 99%
“…The resulting expression of the tearing instability index in the subsonic regime ω < k // C s , appropriate to the experiments of this paper, is presented in [46] and has been extensively studied numerically in [47] validating, for small as well as large islands the generic expression:…”
Section: Further Discussion Of the Instability Conditions For Ntms In...mentioning
confidence: 99%
“…16 This technique of imposing a magnetic island has been used to determine the electrostatic potential in rotating islands and analyse the adiabatic response of ions, 17 to determine the impact of small rotating islands on the bootstrap current, 18 to study the impact of a static island on ITG turbulence, 12,13,16 to prove the existence of a vortex mode related to the presence of the island, 15 and to analyse the stability of magnetic islands in reduced two-fluid models. 19 This approach, where the magnetic island is externally imposed, is based on the time scale separation between ITG and tearing modes. Essentially, the total magnetic field (including island) is imposed as B ¼ B 0 þ dB, where B 0 is the background magnetic field and dB is the perturbation.…”
Section: Description Of the Model Normalizations Used In This Pamentioning
confidence: 99%
“…In order to investigate the self-consistent couplings of ITG turbulence and tearing modes in a simple, tractable form, we employ a simple five-field two-fluid model [21,40,41] in a Cartesian slab geometry [21,[41][42][43][44] similar to that used in previous studies, considered together only in Ishizawa et al [21,41]. The simulation radial and poloidal domains span the range −a ≤ x ≤ a and −b/2 ≤ y < b/2 respectively, with Dirichlet boundary conditions on all fluctuating fields at x = ±a and periodic boundary conditions at y = ±b/2.…”
Section: A Model Overviewmentioning
confidence: 99%