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Concept
Gyrokinetics
Summary
Gyrokinetics is a theoretical framework to study plasma behavior on perpendicular spatial scales comparable to the gyroradius and frequencies much lower than the particle cyclotron frequencies.
These particular scales have been experimentally shown to be appropriate for modeling plasma turbulence. The trajectory of charged particles in a magnetic field is a helix that winds around the field line. This trajectory can be decomposed into a relatively slow motion of the guiding center along the field line and a fast circular motion, called gyromotion. For most plasma behavior, this gyromotion is irrelevant. Averaging over this gyromotion reduces the equations to six dimensions (3 spatial, 2 velocity, and time) rather than the seven (3 spatial, 3 velocity, and time). Because of this simplification, gyrokinetics governs the evolution of charged rings with a guiding center position, instead of gyrating charged particles.
Fundamentally, the gyrokinetic model assumes the plasma is strongly magnetized ( ), the perpendicular spatial scales are comparable to the gyroradius ( ), and the behavior of interest has low frequencies ( ). We must also expand the distribution function, , and assume the perturbation is small compared to the background (). The starting point is the Fokker–Planck equation and Maxwell's equations. The first step is to change spatial variables from the particle position to the guiding center position . Then, we change velocity coordinates from to the velocity parallel , the magnetic moment , and the gyrophase angle . Here parallel and perpendicular are relative to , the direction of the magnetic field, and is the mass of the particle. Now, we can average over the gyrophase angle at constant guiding center position, denoted by , yielding the gyrokinetic equation.
The electrostatic gyrokinetic equation, in the absence of large plasma flow, is given by
Here the first term represents the change in the perturbed distribution function, , with time. The second term represents particle streaming along the magnetic field line.
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