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Radial properties of the geodesic acoustic mode
Author(s) -
Zhenqian Li,
Jiaqi Dong,
Zheng-Mao Sheng,
M. Y. Yu,
Weixing Wang
Publication year - 2017
Publication title -
physics of plasmas
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.75
H-Index - 160
eISSN - 1089-7674
pISSN - 1070-664X
DOI - 10.1063/1.5004427
Subject(s) - physics , geodesic , tokamak , toroid , phase velocity , plasma , computational physics , kinetic energy , thermal , turbulence , radial velocity , mechanics , classical mechanics , astrophysics , optics , nuclear physics , mathematical analysis , mathematics , meteorology , stars
In magnetized toroidal plasmas, neoclassical effects and turbulent drift waves can induce the geodesic acoustic mode (GAM). We simulate the GAM using the gyro-kinetic code GTS for typical tokamak parameters and investigate its properties, especially its frequency continuum, evolution of its radial wave number, and propagation characteristics. The simulation results are compared with those of the relevant theory and experiment. It is found that the radial phase velocity of the GAM is roughly proportional to the ion thermal speed.

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