Effects of Alfv'enicity on the Compressible Energy Cascade in Magnetohydrodynamic Solar Wind Turbulence: Evidence from Parker Solar Probe, Solar Orbiter, and WIND observations

arXiv:2609.37856 · physics.plasm-ph, astro-ph.SR, physics.space-ph · Submitted 2026-09-29 · Read on arXiv

physics.plasm-ph, astro-ph.SR, physics.space-ph

Submitted: 2026-09-29

Updated: 2026-09-29

Terminology

• Parker Solar Probe — 6× in this paper
• Anisotropy — 3× in this paper · explained in 3 episodes
• Alignment — 2× in this paper · explained in 1 episode
• Analyzer — 2× in this paper · explained in 1 episode
• Clustering — 1× in this paper · explained in 2 episodes
• Magnetohydrodynamics (MHD) — 1× in this paper · explained in 3 episodes
• alpha — 1× in this paper · explained in 1 episode

Sources

• The Energy Cascade Rate in Supersonic Magnetohydrodynamic Turbulence

Related papers

• Is Your AI Fast Enough to Run a Fusion Reactor?
• GyroSwin: 5D Surrogates for Gyrokinetic Plasma Turbulence Simulations
• Electromagnetic ghosts in pair plasmas
• Collisionless whistler heat-flux instability in ultra-high- beta plasmas
• Rugged magneto-hydrodynamic invariants in weakly collisional plasma turbulence: Two-dimensional hybrid simulation results
• Hybrid Fourier Neural Operator-Plasma Fluid Model for Fast and Accurate Multiscale Simulations of High Power Microwave Breakdown