Gyrokinetic modelling of the Alfven mode activity in ASDEX Upgrade with an isotropic slowing-down fast-particle distribution

被引:5
|
作者
Vannini, F. [1 ]
Biancalani, A. [2 ]
Bottino, A. [1 ]
Hayward-Schneider, T. [1 ]
Lauber, P. [1 ]
Mishchenko, A. [3 ]
Poli, E. [1 ]
Rettino, B. [1 ]
Vlad, G. [4 ]
Wang, X. [1 ]
机构
[1] Max Planck Inst Plasma Phys, Boltzmann Str 2, D-85748 Garching, Germany
[2] Leonard Vinci Pole Univ, Res Ctr, F-92916 Paris, France
[3] Max Planck Inst Plasma Phys, Wendelstein Str 1, D-17491 Greifswald, Germany
[4] ENEA, FSN, CR Frascati, Via E Fermi 45, I-00044 Frascati, Italy
关键词
Alfven instabilities; ASDEX Upgrade; isotropic slowing-down; equivalent Maxwellian; TAE; EPM; NEUTRAL BEAM INJECTION; ELECTROSTATIC OSCILLATIONS; ENERGETIC PARTICLES; INSTABILITIES; DRIVEN; WAVES; EIGENMODES; EXCITATION; STABILITY; LOSSES;
D O I
10.1088/1741-4326/ac8b1e
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
In the present paper, the evolution of the Alfven modes (AMs) is studied in a realistic ASDEX Upgrade equilibrium by analyzing the results of simulations with the global, electromagnetic, gyrokinetic particle-in-cell code ORB5. The energetic particles (EPs) are modelled both via the newly implemented isotropic slowing-down and with Maxwellian distribution functions. The comparison of the numerical results shows that modelling the EPs with the equivalent Maxwellian rather than with the slowing-down, does not significantly affect the frequency of the driven AM, while its growth rate appears to be underestimated with a quantitative difference as large as almost 30%. Additionally the choice of the isotropic slowing-down allows a better description of the nonlinear modification of the dominant AM frequency, while an equivalent Maxwellian underestimates it. A good comparison with the experimental spectrogram is found.
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页数:19
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