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Local fluxes in magnetohydrodynamic turbulence

Published online by Cambridge University Press:  02 November 2022

Alexandros Alexakis Open the ORCID record for Alexandros Alexakis [Opens in a new window]  and
Sergio Chibbaro
Alexandros Alexakis*
Affiliation:
Laboratoire de Physique de l'Ecole Normale Supérieure, ENS, Université PSL, CNRS, Sorbonne Université, Université Paris-Diderot, Sorbonne Paris Cité, Paris, France
Sergio Chibbaro
Affiliation:
Université Paris-Saclay, CNRS, LISN, 91400 Orsay, France
*
†Email address for correspondence: [email protected]
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Abstract

Using highly resolved direct numerical simulations we examine the statistical properties of the local energy flux rate $\varPi _\ell (x)$ towards small scales for three isotropic turbulent magnetohydrodynamic flows, which differ in strength and structure of the magnetic field. We analyse the cascade process in both kinetic and magnetic energy, disentangling the different flux contributions to the overall energy dynamics. The results show that the probability distribution of the local energy flux develops long tails related to extreme events, similar to the hydrodynamic case. The different terms of the energy flux display different properties and show sensitivity to the type of the flow examined. We further examine the joint probability density function between the local energy flux and the gradients of the involved fields. The results point out a correlation with the magnetic field gradients, showing, however, a dispersion much stronger than what is observed in hydrodynamic flows. Finally, it is also shown that the local energy flux shows some dependence on the local amplitude of the magnetic field. The present results have implications for subgrid-scale models, which we discuss.

Keywords

plasma flowsplasma simulation
Type
Research Article
Information
Journal of Plasma Physics , Volume 88 , Issue 5 , October 2022 , 905880515
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Copyright
Copyright © The Author(s), 2022. Published by Cambridge University Press

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References

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