Local energy transfer rate and kinetic processes: the fate of turbulent energy in two-dimensional Hybrid Vlasov-Maxwell numerical simulations
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Accepted version
Author(s)
Type
Journal Article
Abstract
The nature of the cross-scale connections between the inertial range turbulent energy
cascade and the small-scale kinetic processes in collisionless plasmas is explored through
the analysis of two-dimensional Hybrid Vlasov-Maxwell numerical simulation (HVM),
with
α
particles, and through a proxy of the turbulent energy transfer rate, namely the
Local Energy Transfer rate (LET). Correlations between pairs of variables, including
those related to kinetic processes and to deviation from Maxwellian distributions, are
first evidenced. Then, the general properties and the statistical scaling laws of the LET
are described, confirming its reliability for the description of the turbulent cascade and
revealing its textured topology. Finally, the connection between such proxy and the diag-
nostic variables is explored using conditional averaging, showing that several quantities
are enhanced in the presence of large positive energy flux, and reduced near sites of neg-
ative flux. These observations can help determining which processes are involved in the
dissipation of energy at small scales, as for example ion-cyclotron or mirror instabilities
typically associated with perpendicular anisotropy of temperature.
cascade and the small-scale kinetic processes in collisionless plasmas is explored through
the analysis of two-dimensional Hybrid Vlasov-Maxwell numerical simulation (HVM),
with
α
particles, and through a proxy of the turbulent energy transfer rate, namely the
Local Energy Transfer rate (LET). Correlations between pairs of variables, including
those related to kinetic processes and to deviation from Maxwellian distributions, are
first evidenced. Then, the general properties and the statistical scaling laws of the LET
are described, confirming its reliability for the description of the turbulent cascade and
revealing its textured topology. Finally, the connection between such proxy and the diag-
nostic variables is explored using conditional averaging, showing that several quantities
are enhanced in the presence of large positive energy flux, and reduced near sites of neg-
ative flux. These observations can help determining which processes are involved in the
dissipation of energy at small scales, as for example ion-cyclotron or mirror instabilities
typically associated with perpendicular anisotropy of temperature.
Date Issued
2018-04-15
Date Acceptance
2018-03-22
Citation
Journal of Plasma Physics, 2018, 84 (2)
ISSN
1469-7807
Publisher
Cambridge University Press (CUP)
Journal / Book Title
Journal of Plasma Physics
Volume
84
Issue
2
Copyright Statement
© Cambridge University Press 2018. This paper has been accepted for publication and will appear in a revised form, subsequent to peer-review and/or editorial input by Cambridge University Press.
Subjects
Science & Technology
Physical Sciences
Physics, Fluids & Plasmas
Physics
plasma nonlinear phenomena
plasma simulation
space plasma physics
SOLAR-WIND TURBULENCE
TEMPERATURE ANISOTROPY
MAGNETIC RECONNECTION
1 AU
FLUCTUATIONS
CASCADE
PLASMA
MHD
INTERMITTENCY
VELOCITY
0202 Atomic, Molecular, Nuclear, Particle And Plasma Physics
Fluids & Plasmas
Publication Status
Published
Article Number
725840201
Date Publish Online
2018-04-15