Sub-grid-scale effects in magnetised plasma turbulence

Bogdan Teaca, Evgeny Gorbunov, Daniel Told, Alejandro Bañón Navarro, Frank Jenko

Research output: Contribution to journalArticlepeer-review

6 Citations (Scopus)
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Abstract

In the present paper, we use a coarse-graining approach to investigate the nonlinear redistribution of free energy in both position and scale space for weakly collisional magnetised plasma turbulence. For this purpose, we use high-resolution numerical simulations of gyrokinetic (GK) turbulence that span the proton-electron range of scales, in a straight magnetic guide field geometry. Accounting for the averaged effect of the particles' fast gyro-motion on the slow plasma fluctuations, the GK approximation captures the dominant energy redistribution mechanisms in strongly magnetised plasma turbulence. Here, the GK system is coarse grained with respect to a cut-off scale, separating in real space the contributions to the nonlinear interactions from the coarse-grid scales and the sub-grid scales (SGS). We concentrate on the analysis of nonlinear SGS effects. Not only does this allow us to investigate the flux of free energy across the scales, but also to now analyse its spatial density. We find that the net value of scale flux is an order of magnitude smaller than both the positive and negative flux density contributions. The dependence of the results on the filter type is also analysed. Moreover, we investigate the advection of energy in position space. This rather novel approach for GK turbulence can help in the development of SGS models that account for advective unstable structures for space and fusion plasmas, and with the analysis of the turbulent transport saturation.

Original languageEnglish
Article number905870209
Number of pages287
JournalJournal of Plasma Physics
Volume87
Issue number2
Early online date19 Mar 2021
DOIs
Publication statusPublished - Apr 2021

Bibliographical note

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This document is the author’s post-print version, incorporating any revisions agreed during the peer-review process. Some differences between the published version and this version may remain and you are advised to consult the published version if you wish to cite from it.

Funder

B.T. would like to thank G. Plunk, D. Hatch and T. Görler for discussions on the theoretical and numerical of aspects of GK turbulence. This work was partially supported by B. Teaca's EPSRC grant no. EP/P02064X/1. We acknowledge the Max-Planck Princeton Center for Plasma Physics for facilitating the discussions that lead to this paper. We thank the anonymous referees for their constructive criticism, which lead to an improved form for the article. Publisher Copyright: © 2021 The Author(s).

Keywords

  • astrophysical plasmas
  • plasma nonlinear phenomena

ASJC Scopus subject areas

  • Condensed Matter Physics

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