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Local and global properties of energy transfer in models of plasma turbulence

Published online by Cambridge University Press:  26 January 2021

Christian L. Vásconez*
Affiliation:
Departamento de Física, Escuela Politécnica Nacional, Ladrón de Guevara E11-253, 170525Quito, Ecuador
D. Perrone
Affiliation:
ASI – Italian Space Agency, Via del Politecnico snc, 00133Rome, Italy
R. Marino
Affiliation:
Laboratoire de Mécanique des Fluides et d'Acoustique, CNRS, École Centrale de Lyon, Université Claude Bernard Lyon 1, INSA de Lyon, ÉcullyF-69134, France
D. Laveder
Affiliation:
Université Côte d'Azur, CNRS, Observatoire de la Côte d'Azur, Laboratoire J. L. Lagrange, Boulevard de l'Observatoire, CS 34229, 06304Nice CEDEX 4, France
F. Valentini
Affiliation:
Dipartimento di Fisica, Università della Calabria, I-87036Rende (CS), Italy
S. Servidio
Affiliation:
Dipartimento di Fisica, Università della Calabria, I-87036Rende (CS), Italy
P. Mininni
Affiliation:
Departamento de Física, Universidad de Buenos Aires and IFIBA, CONICET, 1428Buenos Aires, Argentina
L. Sorriso-Valvo
Affiliation:
Istituto per la Scienza e Tecnologia dei Plasmi (ISTP), Consiglio Nazionale delle Ricerche, Via Amendola 122/D, 70126Bari, Italy Swedish Institute of Space Physics, Ångström Laboratory, Lägerhyddsvägen 1, SE-751 21Uppsala, Sweden
*
Email address for correspondence: christian.vasconez@epn.edu.ec

Abstract

The nature of the turbulent energy transfer rate is studied using direct numerical simulations of weakly collisional space plasmas. This is done comparing results obtained from hybrid Vlasov–Maxwell simulations of collisionless plasmas, Hall magnetohydrodynamics and Landau fluid models reproducing low-frequency kinetic effects, such as the Landau damping. In this turbulent scenario, estimates of the local and global scaling properties of different energy channels are obtained using a proxy of the local energy transfer. This approach provides information on the structure of energy fluxes, under the assumption that the turbulent cascade transfers most of the energy that is then dissipated at small scales by various kinetic processes in these kinds of plasmas.

Type
Research Article
Copyright
Copyright © The Author(s), 2021. Published by Cambridge University Press

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References

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