Emergence and Detection of Electron-Scale Current Sheets in Turbulence with MMS Observations and fully kinetic 3D simulations
Zachary Davis, Alexandros Chasepis, Colby Haggerty, Luca Comisso, Derek Sikorski
physics.plasm-ph, astro-ph.SR
Submitted: 2026-07-27
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Particle Injection and Nonthermal Particle Acceleration in Relativistic Magnetic Reconnection
- Particle Acceleration in Relativistic Plasma Turbulence
- Radiative turbulent flares in magnetically-dominated plasmas
- Statistical Analysis of Current Sheets in Three-Dimensional Magnetohydrodynamic Turbulence
- Scalings of intermittent structures in magnetohydrodynamic turbulence
- Intermittency and Dissipative Structures Arising from Relativistic Magnetized Turbulence
- The Complex Structure of Magnetic Field Discontinuities in the Turbulent Solar Wind
- Clustering of Intermittent Magnetic and Flow Structures near Parker Solar Probe's First Perihelion -- A Partial-Variance-of-Increments Analysis
- Ion and Electron Acceleration in Fully Kinetic Plasma Turbulence
- Simulations of relativistic collisionless shocks: shock structure and particle acceleration
- Statistics of Current and Vorticity Structures in Relativistic Turbulence
- Machine-Learning Characterization of Intermittency in Relativistic Pair Plasma Turbulence: Single and Double Sheet Structures
- Transition from ion-coupled to electron-only reconnection: Basic physics and implications for plasma turbulence
- Role of reconnection in inertial kinetic-Alfven turbulence
- Electron-only reconnection in kinetic Alfv'en turbulence
- Electron-Scale Current Sheets and Energy Dissipation in 3D Kinetic-Scale Plasma Turbulence with Low Electron Beta
- Why does steady-state magnetic reconnection have a maximum local rate of order 0.1?
- Relativistic Asymmetric Reconnection
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