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The Velocity-Space Signature of Transit-Time Damping

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arxiv 2401.16697 v2 pith:5I7HD7QV submitted 2024-01-30 physics.plasm-ph

classification physics.plasm-ph
keywords dampingplasmaturbulencebetaenergyfieldmagneticparticles
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abstract

Transit-time damping (TTD) is a process in which the magnetic mirror force -- induced by the parallel gradient of magnetic field strength -- interacts with resonant plasma particles in a time-varying magnetic field, leading to the collisionless damping of electromagnetic waves and the resulting energization of those particles through the perpendicular component of the electric field, $E_\perp$. In this study, we utilize the recently developed field-particle correlation technique to analyze gyrokinetic simulation data. This method enables the identification of the velocity-space structure of the TTD energy transfer rate between waves and particles during the damping of plasma turbulence. Our analysis reveals a unique bipolar pattern of energy transfer in velocity space characteristic of TTD. By identifying this pattern, we provide clear evidence of TTD's significant role in the damping of strong plasma turbulence. Additionally, we compare the TTD signature with that of Landau damping (LD). Although they both produce a bipolar pattern of phase-space energy density loss and gain about the parallel resonant velocity of the Alfv\'enic waves, they are mediated by different forces and exhibit different behaviors as $v_\perp \to 0$. We also explore how the dominant damping mechanism varies with ion plasma beta $\beta_i$, showing that TTD dominates over LD for $\beta_i > 1$. This work deepens our understanding of the role of TTD in the damping of weakly collisional plasma turbulence and paves the way to seek the signature of TTD using \emph{in situ} spacecraft observations of turbulence in space plasmas.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. The Dielectric Response of Plasmas with Arbitrary Gyrotropic Velocity Distributions

    physics.plasm-ph 2025-06 conditional novelty 6.0 of 10

    ALPS now uses high-order Chebyshev fits to improve the analytic continuation needed to compute damped plasma wave modes for arbitrary gyrotropic velocity distributions.

  2. Impact of Two-Population $\alpha$-particle Distributions on Plasma Stability

    astro-ph.SR 2024-12 conditional novelty 6.0 of 10

    Solar wind stability predictions match observed ion-scale wave signatures only when alpha particles are modeled as two populations (core and beam) rather than one.

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