Reduced fluid-kinetic equations for low-frequency dynamics, magnetic reconnection, and electron heating in low-beta plasmas

被引:103
作者
Zocco, Alessandro [1 ,2 ]
Schekochihin, Alexander A. [2 ]
机构
[1] Culham Sci Ctr, Euratom CCFE Fus Assoc, Abingdon OX14 3DB, Oxon, England
[2] Univ Oxford, Rudolf Peierls Ctr Theoret Phys, Oxford OX1 3NP, England
关键词
free energy; magnetic reconnection; plasma collision processes; plasma flow; plasma heating; plasma kinetic theory; plasma simulation; tearing instability; COLLISIONLESS RECONNECTION; ASTROPHYSICAL GYROKINETICS; MODES; INSTABILITIES; TURBULENCE; OSCILLATIONS; MECHANISM; FIELD;
D O I
10.1063/1.3628639
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
A minimal model for magnetic reconnection and, generally, low-frequency dynamics in low-beta plasmas is proposed. The model combines analytical and computational simplicity with physical realizability: it is a rigorous limit of gyrokinetics for plasma beta of order the electron-ion mass ratio. The model contains collisions and can be used both in the collisional and collisionless reconnection regimes. It includes gyrokinetic ions (not assumed cold) and allows for the topological rearrangement of the magnetic field lines by either resistivity or electron inertia, whichever predominates. The two-fluid dynamics are coupled to electron kinetics-electrons are not assumed isothermal and are described by a reduced drift-kinetic equation. The model, therefore allows for irreversibility and conversion of magnetic energy into electron heat via parallel phase mixing in velocity space. An analysis of the exchanges between various forms of free energy and its conversion into electron heat is provided. It is shown how all relevant linear waves and regimes of the tearing instability (collisionless, semicollisional, and fully resistive) are recovered in various limits of our model. An efficient way to simulate our equations numerically is proposed, via the Hermite representation of the velocity space. It is shown that small scales in velocity space will form, giving rise to a shallow Hermite-space spectrum, whence it is inferred that, for steady-state or sufficiently slow dynamics, the electron heating rate will remain finite in the limit of vanishing collisionality. (C) 2011 American Institute of Physics. [doi:10.1063/1.3628639]
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页数:24
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