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1 Magnetic components existing in geodesic acoustic modes Deng Zhou Institute of Plasma Physics, Chinese Academy of Sciences
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2 Introduction Zonal flows : m/n=0/0 electrostatic modes, with Geodesic Acoustic modes : dominant m/n=0/0 modes with GAMs are characterized by a m=1 poloidal density perturbation; Interaction between poloidal variational magnetic drift and the m=1 poloidal density perturbation results in a m=2 radial drift and a symmetric drift component. => The polarized radial drift is balanced by poloidal symmetric magnetic drift => while the m=2 radial current requires a m=2 parallel current to make total current divergent free, i. e., a m=2 magnetic perturbation.
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3 Recent experiment and numerical support Recent experiments have observed magnetic perturbations coexisting with GAMs[1,2]. Numerical simulations based on MHD also reveals that a perpendicular magnetic perturbation with dominant mode number m=2 coexists with GAMs, almost proportional to the electrostatic potential in magnitude[2]. [1]A. V. Melnikov, V. A. Vershkov, L. G. Eliseev, et al., Plasma Phys. Control. Fusion 87, S41 (2006). [2]H. L. Berk, C. J. Boswell, D. Borba, et al., Nucl. Fusion 46, S888 (2006).
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4 Physics Model large aspect ratio tokamak with a circular cross section, and the equilibrium magnetic field, The perturbed scalar and vector potentials
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5 Expanding the drift kinetic equation order by order Introduce a small parameter
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6 Solution to the lowest order Eq. Written as
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7 Quasi-neutral condition(1) Quasi-neutral condition Yields
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8 Parallel Ampere’s law(1) The parallel current * No m=1 magnetic perturbation presents. Using quasi-neutrality(1) results ===
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9 The equation of 2 nd order The same procedure to solve the 2 nd order equation to obtain
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10 Quasi-neutrality(2) ===
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11 Parallel Ampere’s law(2) The m=2 parallel current ==
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12 Simplified forms of current The current expression is written using quasi-neutrality condition(2) Further simplified using quasi-neutrality condition(1)
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13 An alternative approach for the current The interaction between magnetic drift and m=1 perturbation causes a m=2 radial current which requires a m=2 parallel current to make total current divergent free. The explicit expression
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14 GAM dispersion Balancing the poloidal invariant radial drift current and the polarization current results in the dispersion relation of GAMs Its asymptotic solution for large q is
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15 Divergent free of current The relation yields Generally Then this current is equal to that obtained from solving 2th drift kinetic equations The corresponding magnetic perturbation is
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16 Conclusion There always exists a m=2 magnetic perturbation components accompanying the GAMS while the m=1 components is 0. The perturbation is caused by the coupling between the m=1 plasma response and the m=1 poloidal variation of magnetic drift, which leads to a m=2 parallel current.
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