Results 151 to 160 of about 16,475 (273)
Frontiers in Astronomy and Space SciencesThe energy dissipation in collisionless plasmas as the solar wind is not yet fully understood. The intermittent nature of magnetic structures appears to be a fundamental part of the energy cascade.
Andres F. Guerrero Guio +2 more
doaj +1 more source
Open-Source Software Analysis Tool to Investigate Space Plasma Turbulence and Nonlinear DYNamics (ODYN). [PDF]
Earth Space Sci, 2020 Teodorescu E, Echim MM.
europepmc +1 more source
Electrochemical Science Advances, Volume 6, Issue 4, August 2026.ABSTRACT Flow capacitive deionisation is an advanced electrochemical technology for water purification and energy‐related applications. It represents a viable alternative to conventional desalination methods due to its low operating voltage, continuous electrode regeneration, and stable performance under moderate‐to‐high salinity conditions. The use of
Nayan Chandra Roy +3 more
wiley +1 more source
First Kinetic 3‐D Simulations of the High‐Latitude Electrojet Spanning an Entire Turbulent Flux Tube
Geophysical Research Letters, Volume 53, Issue 13, 16 July 2026.Abstract Radar and rocket observations of the terrestrial ionosphere frequently measure turbulent plasma waves, especially during geospace storms. The non‐linear behavior of these waves remains poorly characterized. This paper presents the first fully kinetic 3‐D particle‐in‐cell simulations of Farley–Buneman (FB) turbulence spanning an entire high ...
Meers Oppenheim +4 more
wiley +1 more source
Nuclear FusionThis study focuses on understanding how turbulence is suppressed in particularly heated JET plasma discharges showing enhanced confinement, namely $99896$ , which uses a nearly 50–50 deuterium–tritium mixture, showing signs of enhanced plasma confinement.
A. Di Siena +12 more
doaj +1 more source
Interplanetary Electric Fields for Extreme Magnetic Storms
Geophysical Research Letters, Volume 53, Issue 13, 16 July 2026.Abstract Using a list of sudden‐commencement storms, the ring‐current index, and 1‐h near‐Earth solar‐wind measurements from solar cycles 20–25, we develop extreme‐value statistical models relating storm intensity D=max{−Dst} $D=\max \left\{-Dst\right\}$ to the storm main‐phase maximum duskward interplanetary electric field E $E$.
Jeffrey J. Love +3 more
wiley +1 more source
Beta-dependent Properties of Solar Wind Current Sheets at 1 au
The Astrophysical Journal LettersWe utilize plasma turbulence in interplanetary coronal mass ejections as a natural laboratory to analyze more than 4600 current sheets observed over a broad range of electron and proton beta values, 10 ^−2 ≲ β _e ≲ 10 and 10 ^−3 ≲ β _p ≲ 10.
Zubair I. Shaikh +3 more
doaj +1 more source
Unraveling the Fine‐Scale Tapestry of Solar Wind at 1AU
Geophysical Research Letters, Volume 53, Issue 13, 16 July 2026.Abstract Solar wind is a complex network of distinct magnetic flux tubes, each contained and separated by a current sheet. In this study, more than 50,000 current sheets in the solar wind are identified and characterized for the first time, using multi‐point Cluster observations during solar minimum and maximum intervals.
M. Akhavan‐Tafti +3 more
wiley +1 more source
Turbulence Theories and Modelling of Fluids and Plasmas [PDF]
, 2001 Theoretical and heuristic modelling methods are reviewed for studying turbulence phenomena of fluids and plasmas. Emphasis is put on understanding of effects on turbulent characteristics due to inhomogeneities of field and plasma parameters.
Itoh, S.-I. +3 more
core
Energy Cascade and Damping in Fast-mode Compressible Turbulence
The Astrophysical Journal LettersCompressible turbulence governs energy transfer across scales in space and astrophysical systems. Capturing both the turbulence cascade and damping is therefore crucial for models of energy conversion, plasma heating, and particle transport in diverse ...
Chuanpeng Hou +3 more
doaj +1 more source