130 citations · 1.1k across the 28 of their papers we have counts for
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The incompressible energy cascade rate in anisotropic solar wind turbulence
N. Andrés, F. Sahraoui, Huang +2
Context. The presence of a magnetic guide field induces several types of anisotropy in solar wind turbulence. The energy cascade rate between scales in the inertial range depends s…
Exact law for compressible pressure-anisotropic magnetohydrodynamic turbulence: toward linking energy cascade and instabilities
P. Simon, F. Sahraoui
We derive a first exact law for compressible pressure-anisotropic magnetohydrodynamic turbulence. For a gyrotropic pressure tensor, we study the double-adiabatic case and show the…
Fluid energy cascade rate and kinetic damping: new insight from 3D Landau-fluid simulations
R. Ferrand, F. Sahraoui, D. Laveder +3
Using an exact law for incompressible Hall magnetohydrodynamics (HMHD) turbulence, the energy cascade rate is computed from three-dimensional HMHD-CGL (bi-adiabatic ions and isothe…
Power Anisotropy, Dispersion Signature and Turbulence Diffusion Region in the 3D Wavenumber Domain of Space Plasma Turbulence
Rong Lin, Jiansen He, Xingyu Zhu +4
We explore the multi-faceted important features of turbulence (e.g., anisotropy, dispersion, diffusion) in the three-dimensional (3D) wavenumber domain (, $k_{\perp,1}…
General exact law of compressible isentropic magnetohydrodynamic flows: theory and spacecraft observations in the solar wind
Pauline Simon, Fouad Sahraoui
Various forms of exact laws governing magnetohydrodynamic (MHD) turbulence have been derived either in the incompressibility limit, or for isothermal compressible flows. Here we pr…
The evolution of compressible solar wind turbulence in the inner heliosphere: PSP, THEMIS and MAVEN observations
N. Andrés, F. Sahraoui, L. Z. Hadid +5
The first computation of the compressible energy transfer rate from 0.2 AU up to 1.7 AU is obtained using PSP, THEMIS and MAVEN observations. The compressible energy…