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 …
Turbulence in space plasmas: Who needs it?
WH Matthaeus - Physics of Plasmas, 2021 - pubs.aip.org
The complex nonlinear dynamical phenomenon described as turbulence, is known to have
a great impact on fluids, magnetohydrodynamic systems, and on plasmas. This paper …
a great impact on fluids, magnetohydrodynamic systems, and on plasmas. This paper …
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 …
Three-dimensional modelling of the shock–turbulence interaction
The complex interaction between shocks and plasma turbulence is extremely important to
address crucial features of energy conversion in a broad range of astrophysical systems. We …
address crucial features of energy conversion in a broad range of astrophysical systems. We …
Quantifying energy conversion in higher-order phase space density moments in plasmas
Weakly collisional and collisionless plasmas are typically far from local thermodynamic
equilibrium (LTE), and understanding energy conversion in such systems is a forefront …
equilibrium (LTE), and understanding energy conversion in such systems is a forefront …
MHD turbulence: a biased review
AA Schekochihin - Journal of Plasma Physics, 2022 - cambridge.org
This review of scaling theories of magnetohydrodynamic (MHD) turbulence aims to put the
developments of the last few years in the context of the canonical time line (from Kolmogorov …
developments of the last few years in the context of the canonical time line (from Kolmogorov …
Turbulence in the outer heliosphere
The solar wind (SW) and local interstellar medium (LISM) are turbulent media. Their
interaction is governed by complex physical processes and creates heliospheric regions …
interaction is governed by complex physical processes and creates heliospheric regions …
Subproton-scale intermittency in near-sun solar wind turbulence observed by the parker solar probe
High time-resolution solar wind magnetic field data are employed to study statistics
describing intermittency near the first perihelion (∼ 35.6 R⊙) of the Parker Solar Probe …
describing intermittency near the first perihelion (∼ 35.6 R⊙) of the Parker Solar Probe …
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 …
Turbulent energy transfer and proton–electron heating in collisionless plasmas
Despite decades of study of high-temperature weakly collisional plasmas, a complete
understanding of how energy is transferred between particles and fields in turbulent …
understanding of how energy is transferred between particles and fields in turbulent …