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 …
The multi-scale nature of the solar wind
D Verscharen, KG Klein, BA Maruca - Living Reviews in Solar Physics, 2019 - Springer
The solar wind is a magnetized plasma and as such exhibits collective plasma behavior
associated with its characteristic spatial and temporal scales. The characteristic length …
associated with its characteristic spatial and temporal scales. The characteristic length …
Turbulence theories and statistical closure approaches
Y Zhou - Physics Reports, 2021 - Elsevier
When discussing research in physics and in science more generally, it is common to ascribe
equal importance to the three components of the scientific trinity: theoretical, experimental …
equal importance to the three components of the scientific trinity: theoretical, experimental …
[HTML][HTML] 3D turbulent reconnection: Theory, tests, and astrophysical implications
Magnetic reconnection, topological changes in magnetic fields, is a fundamental process in
magnetized plasmas. It is associated with energy release in regions of magnetic field …
magnetized plasmas. It is associated with energy release in regions of magnetic field …
Solar wind electrons alphas and protons (SWEAP) investigation: Design of the solar wind and coronal plasma instrument suite for solar probe plus
JC Kasper, R Abiad, G Austin, M Balat-Pichelin… - Space Science …, 2016 - Springer
Abstract The Solar Wind Electrons Alphas and Protons (SWEAP) Investigation on Solar
Probe Plus is a four sensor instrument suite that provides complete measurements of the …
Probe Plus is a four sensor instrument suite that provides complete measurements of the …
The solar wind as a turbulence laboratory
In this review we will focus on a topic of fundamental importance for both astrophysics and
plasma physics, namely the occurrence of large-amplitude low-frequency fluctuations of the …
plasma physics, namely the occurrence of large-amplitude low-frequency fluctuations of the …
Reconnection in a weakly stochastic field
A Lazarian, ET Vishniac - The Astrophysical Journal, 1999 - iopscience.iop.org
We examine the effect of weak, small-scale magnetic field structure on the rate of
reconnection in a strongly magnetized plasma. This affects the rate of reconnection by …
reconnection in a strongly magnetized plasma. This affects the rate of reconnection by …
High-frequency heating of the solar wind triggered by low-frequency turbulence
J Squire, R Meyrand, MW Kunz, L Arzamasskiy… - Nature …, 2022 - nature.com
The fast solar wind's high speeds and non-thermal features require that considerable
heating occurs well above the Sun's surface. Two leading theories seem incompatible: low …
heating occurs well above the Sun's surface. Two leading theories seem incompatible: low …
[كتاب][B] Magnetohydrodynamic turbulence
D Biskamp - 2003 - books.google.com
This book presents an introduction to, and modern account of, magnetohydrodynamic
(MHD) turbulence, an active field both in general turbulence theory and in various areas of …
(MHD) turbulence, an active field both in general turbulence theory and in various areas of …
Astrophysical gyrokinetics: kinetic and fluid turbulent cascades in magnetized weakly collisional plasmas
AA Schekochihin, SC Cowley, W Dorland… - The Astrophysical …, 2009 - iopscience.iop.org
This paper presents a theoretical framework for understanding plasma turbulence in
astrophysical plasmas. It is motivated by observations of electromagnetic and density …
astrophysical plasmas. It is motivated by observations of electromagnetic and density …