Effective viscosity, resistivity, and Reynolds number in weakly collisional plasma turbulence

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Abstract

We examine dissipation and energy conversion in weakly collisional plasma turbulence, employing in situ observations from the Magnetospheric Multiscale mission and kinetic particle-in-cell simulations of proton-electron plasma. A previous result indicated the presence of viscous-like and resistive-like scaling of average energy conversion rates -analogous to scalings characteristic of collisional systems. This allows for extraction of collisional-like coefficients of effective viscosity and resistivity, and thus also determination of ef fecti v e Re ynolds numbers based on these coef ficients. The ef fecti v e Re ynolds number, as a measure of the available bandwidth for turbulence to populate various scales, links turbulence macroscale properties with kinetic plasma properties in a no v el way.

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Yang, Y., Matthaeus, W. H., Oughton, S., Bandyopadhyay, R., Pecora, F., Parashar, T. N., … Shay, M. A. (2024). Effective viscosity, resistivity, and Reynolds number in weakly collisional plasma turbulence. Monthly Notices of the Royal Astronomical Society, 528(4), 6119–6128. https://doi.org/10.1093/mnras/stae355

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