Journal
FRONTIERS IN ASTRONOMY AND SPACE SCIENCES
Volume 9, Issue -, Pages -Publisher
FRONTIERS MEDIA SA
DOI: 10.3389/fspas.2022.1010133
Keywords
quasilinear theory; guiding-center approximation; wave-particle resonance; Hamiltonian formulation; action-angle coordinates
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Funding
- NSF-PHY [2206302]
- NASA [NNX17AI15G, 80NSSC21K1323]
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The Hamiltonian formulations of quasilinear theory for uniform and nonuniform magnetized plasmas are presented. The transition from two-dimensional to three-dimensional quasilinear diffusion is discussed, and the diffusion tensor for nonuniform magnetized plasmas is derived, incorporating both radial diffusion and its connection to diffusion in two-dimensional velocity space.
Hamiltonian formulations of quasilinear theory are presented for the cases of uniform and nonuniform magnetized plasmas. First, the standard quasilinear theory of Kennel and Engelmann (Kennel, Phys. Fluids, 1966, 9, 2377) is reviewed and reinterpreted in terms of a general Hamiltonian formulation. Within this Hamiltonian representation, we present the transition from two-dimensional quasilinear diffusion in a spatially uniform magnetized background plasma to three-dimensional quasilinear diffusion in a spatially nonuniform magnetized background plasma based on our previous work (Brizard and Chan, Phys. Plasmas, 2001, 8, 4762-4771; Brizard and Chan, Phys. Plasmas, 2004, 11, 4220-4229). The resulting quasilinear theory for nonuniform magnetized plasmas yields a 3 x 3 diffusion tensor that naturally incorporates quasilinear radial diffusion as well as its synergistic connections to diffusion in two-dimensional invariant velocity space (e.g., energy and pitch angle).
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