CURRENT SHEETS AND COLLISIONLESS DAMPING IN KINETIC PLASMA TURBULENCE

We present the first study of the formation and dissipation of current sheets at electron scales in a wave-driven, weakly collisional, three-dimensional kinetic turbulence simulation. We investigate the relative importance of dissipation associated with collisionless damping via resonant wave-partic...

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Bibliographic Details
Published in:Astrophysical journal. Letters 2013-07, Vol.771 (2), p.1-6
Main Authors: TENBARGE, J M, Howes, G G
Format: Article
Language:English
Subjects:
astronomy & astrophysics
ASTRONOMY AND ASTROPHYSICS
Current sheets
Damping
Dissipation
Fluid dynamics
Fluid flow
Heating
plasmas
Simulation
solar wind
Turbulence
Turbulent flow
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Summary:We present the first study of the formation and dissipation of current sheets at electron scales in a wave-driven, weakly collisional, three-dimensional kinetic turbulence simulation. We investigate the relative importance of dissipation associated with collisionless damping via resonant wave-particle interactions versus dissipation in small-scale current sheets in weakly collisional plasma turbulence. Current sheets form self-consistently from the wave-driven turbulence, and their filling fraction is well correlated to the electron heating rate. However, the weakly collisional nature of the simulation necessarily implies that the current sheets are not significantly dissipated via Ohmic dissipation. Rather, collisionless damping via the Landau resonance with the electrons is sufficient to account for the measured heating as a function of scale in the simulation, without the need for significant Ohmic dissipation. This finding suggests the possibility that the dissipation of the current sheets is governed by resonant wave-particle interactions and that the locations of current sheets correspond spatially to regions of enhanced heating.
ISSN:2041-8205
2041-8213
DOI:10.1088/2041-8205/771/2/L27