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 waves in open coronal structures
D Banerjee, S Krishna Prasad, V Pant… - Space Science …, 2021 - Springer
Modern observatories have revealed the ubiquitous presence of magnetohydrodynamic
waves in the solar corona. The propagating waves (in contrast to the standing waves) are …
waves in the solar corona. The propagating waves (in contrast to the standing waves) are …
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 …
Pathways to dissipation in weakly collisional plasmas
Observed turbulence in space and astrophysics is expected to involve cascade and
subsequent dissipation and heating. Contrary to standard collisional fluid turbulence, the …
subsequent dissipation and heating. Contrary to standard collisional fluid turbulence, the …
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 …
Coherent events at ion scales in the inner heliosphere: Parker solar probe observations during the first encounter
Abstract The Parker Solar Probe mission has shown the ubiquitous presence of strong
magnetic field deflections, namely switchbacks, during its first perihelion where it was …
magnetic field deflections, namely switchbacks, during its first perihelion where it was …
Energy dissipation and entropy in collisionless plasma
It is well known that collisionless systems are dissipation free from the perspective of particle
collision and thus conserve entropy. However, processes such as magnetic reconnection …
collision and thus conserve entropy. However, processes such as magnetic reconnection …
Energy conversion in turbulent weakly collisional plasmas: Eulerian hybrid Vlasov-Maxwell simulations
Kinetic simulations based on the Eulerian Hybrid Vlasov-Maxwell (HVM) formalism permit
the examination of plasma turbulence with a useful resolution of the proton velocity …
the examination of plasma turbulence with a useful resolution of the proton velocity …
A case for electron-astrophysics
The smallest characteristic scales, at which electron dynamics determines the plasma
behaviour, are the next frontier in space and astrophysical plasma research. The analysis of …
behaviour, are the next frontier in space and astrophysical plasma research. The analysis of …
Current sheets, plasmoids and flux ropes in the heliosphere: Part ii: Theoretical aspects
Our understanding of processes occurring in the heliosphere historically began with
reduced dimensionality-one-dimensional (1D) and two-dimensional (2D) sketches and …
reduced dimensionality-one-dimensional (1D) and two-dimensional (2D) sketches and …