Abstract

Turbulent space and astrophysical plasmas exhibit a complex dynamics, which involves nonlinear coupling across different temporal and spatial scales. There is growing evidence that impulsive events, such as magnetic reconnection instabilities, lead to a spatially localized enhancement of energy dissipation, thus speeding up the energy transfer at small scales. Capturing such a diverse dynamics is challenging. Here, we employ the Multidimensional Iterative Filtering (MIF) method, a novel technique for the analysis of non-stationary multidimensional signals. Unlike other traditional methods (e.g. based on Fourier or wavelet decomposition), MIF does not require any previous assumption on the functional form of the signal to be identified. Using MIF, we carry out a multiscale analysis of Hall-magnetohydrodynamic (HMHD) and hybrid particle-in-cell (HPIC) numerical simulations of decaying plasma turbulence. The results assess the ability of MIF to spatially identify and separate the different scales (the MHD inertial range, the sub-ion kinetic and the dissipation scales) of the plasma dynamics. Furthermore, MIF decomposition allows localized current structures to be detected and their contribution to the statistical and spectral properties of turbulence to be characterized. Overall, MIF arises as a very promising technique for the study of turbulent plasma environments.

Highlights

  • Turbulent space and astrophysical plasmas exhibit a complex dynamics, which involves nonlinear coupling across different temporal and spatial scales

  • Using Multidimensional Iterative Filtering (MIF), we carry out a multiscale analysis of Hall-magnetohydrodynamic (HMHD) and hybrid particle-in-cell (HPIC) numerical simulations of decaying plasma turbulence

  • At large scales, where the plasma can be described as a fluid within the framework of magnetohydrodynamics (MHD), magnetic spectra follow a Kolmogorov-like power-law, which denotes the existence of an inertial range where the scale-to-scale energy transfer takes place, without losses, via interactions between the turbulent eddies (Iroshnikov 1963; Kraichnan 1965)

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Summary

Numerical simulations of plasma turbulence

The datasets used in this work were produced by two high-resolution numerical simulations of plasma turbulence, employing a fluid HMHD and a HPIC model, respectively. Their evolution into fully developed turbulence, as well as their statistical properties, have been thoroughly characterized in Papini et al (2019b)

The HMHD model
The HPIC model
Numerical setup
Datasets of fully developed turbulence
Multidimensional Iterative Filtering
Multiscale analysis of fully developed turbulence
Current structures and intermittency
Discussion
Reconnection and enhanced turbulent dissipation
Full Text
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