Power Anisotropy, Dispersion Signature and Turbulence Diffusion Region in the 3D Wavenumber Domain of Space Plasma Turbulence
Rong Lin, Jiansen He, Xingyu Zhu, Lei Zhang, Die Duan, Fouad Sahraoui,, and Daniel Verscharen

TL;DR
This paper uses the k-filtering technique on MMS spacecraft data to analyze 3D turbulence features in space plasma, revealing anisotropy, dispersion signatures, and the turbulence diffusion region in wavenumber space.
Contribution
It provides the first 3D visualization of electric and magnetic spectral bifurcation and characterizes the turbulence diffusion region with anisotropic wavevector distribution.
Findings
Magnetic and electric fluctuations show spectral anisotropy in the sub-ion range.
First 3D image of electric-magnetic power spectrum bifurcation.
Identification of turbulence diffusion region with anisotropic wavevector distribution.
Abstract
We explore the multi-faceted important features of turbulence (e.g., anisotropy, dispersion, diffusion) in the three-dimensional (3D) wavenumber domain (, , ), by employing the k-filtering technique to the high-quality measurements of fields and particles from the MMS multi-spacecraft constellation. We compute the 3D power spectral densities (PSDs) of magnetic and electric fluctuations (marked as and ), both of which show a prominent spectral anisotropy in the sub-ion range. We give the first 3D image of the bifurcation between power spectra of the electric and magnetic fluctuations, by calculating the ratio between and $\rm{PSD}(\delta…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Tropical and Extratropical Cyclones Research
