Scaling laws for the energy transfer in space plasma turbulence
R Marino, L Sorriso-Valvo - Physics Reports, 2023 - Elsevier
One characteristic trait of space plasmas is the multi-scale dynamics resulting from non-
linear transfers and conversions of various forms of energy. Routinely evidenced in a range …
linear transfers and conversions of various forms of energy. Routinely evidenced in a range …
Magnetohydrodynamic and kinetic scale turbulence in the near-Earth space plasmas: a (short) biased review
The near-Earth space is a unique laboratory to explore turbulence and energy dissipation
processes in magnetized plasmas thanks to the availability of high-quality data from various …
processes in magnetized plasmas thanks to the availability of high-quality data from various …
Pressure–strain interaction as the energy dissipation estimate in collisionless plasma
The dissipative mechanism in weakly collisional plasma is a topic that pervades decades of
studies without a consensus solution. We compare several energy dissipation estimates …
studies without a consensus solution. We compare several energy dissipation estimates …
Dissipation measures in weakly collisional plasmas
The physical foundations of the dissipation of energy and the associated heating in weakly
collisional plasmas are poorly understood. Here, we compare and contrast several …
collisional plasmas are poorly understood. Here, we compare and contrast several …
Energy transfer in reconnection and turbulence
Reconnection and turbulence are two of the most commonly observed dynamical processes
in plasmas, but their relationship is still not fully understood. Using 2.5 D kinetic particle-in …
in plasmas, but their relationship is still not fully understood. Using 2.5 D kinetic particle-in …
Energy cascade rate measured in a collisionless space plasma with mms data and compressible hall magnetohydrodynamic turbulence theory
The first complete estimation of the compressible energy cascade rate| ϵ C| at
magnetohydrodynamic (MHD) and subion scales is obtained in Earth's magnetosheath …
magnetohydrodynamic (MHD) and subion scales is obtained in Earth's magnetosheath …
In Situ Observation of Hall Magnetohydrodynamic Cascade in Space Plasma
We present estimates of the turbulent energy-cascade rate derived from a Hall-
magnetohydrodynamic (MHD) third-order law. We compute the contribution from the Hall …
magnetohydrodynamic (MHD) third-order law. We compute the contribution from the Hall …
Linking Small-scale Solar Wind Properties with Large-scale Coronal Source Regions through Joint Parker Solar Probe–Metis/Solar Orbiter Observations
D Telloni, GP Zank, L Sorriso-Valvo… - The Astrophysical …, 2022 - iopscience.iop.org
The solar wind measured in situ by Parker Solar Probe in the very inner heliosphere is
studied in combination with the remote-sensing observation of the coronal source region …
studied in combination with the remote-sensing observation of the coronal source region …
The incompressible energy cascade rate in anisotropic solar wind turbulence
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 …
wind turbulence. The energy cascade rate between scales in the inertial range depends …
Compressible turbulence in the interstellar medium: New insights from a high-resolution supersonic turbulence simulation
R Ferrand, S Galtier, F Sahraoui… - The Astrophysical …, 2020 - iopscience.iop.org
The role of supersonic turbulence in structuring the interstellar medium (ISM) remains an
unsettled question. Here, this problem is investigated using a new exact law of compressible …
unsettled question. Here, this problem is investigated using a new exact law of compressible …