collaborators

9 papers

physics.plasm-ph2026

A Neural Operator Closure for Landau Damping in Electrostatic Plasma

Samuel Burles, Enrico Camporeale, Oreste Pezzi

We present a data-driven plasma fluid closure for both linear and nonlinear electrostatic Landau damping in one dimension. A Fourier Neural Operator (FNO) is trained online within…

physics.space-ph2026

Energetic particle-mediated interplanetary shocks observed by Solar Orbiter

D. Trotta, D. Lario, B. Reville +10

Context: In collisionless shocks, energetic particles can carry sufficient pressure to modify the upstream plasma and the shock structure itself, a regime often invoked in theories…

physics.space-ph2026

Transport of electrons in tangled magnetic fields

Daniel Verscharen, Natasha Jeffrey, Anton Artemyev +6

Cosmic magnetic fields are typically inhomogeneous and often highly tangled due to large-scale plasma flows, turbulence, and instabilities. If the variations in the magnetic field…

physics.plasm-ph2026

Numerical simulations of waves and turbulence in coronal loops: observables and spectra

Fabio Feraco, Francesco Pucci, Claudio Meringolo +11

We investigate numerically the time evolution of velocity and magnetic field fluctuations in a coronal loop, focusing on the dynamics due to both phase mixing and turbulent cascade…

astro-ph.SR2026

Evidence of energy conversion in weakly collisional plasma during an interplanetary coronal mass ejection

Omkar Dhamane, Anil Raghav, Simone Benella +14

Intervals of enhanced turbulent fluctuations are typically less frequent within the magnetic cloud region of an interplanetary coronal mass ejection (ICME). We investigate two such…

astro-ph.SR2025

Stochastic Heating in the Sub-Alfvénic Solar Wind

Trevor A. Bowen, Tamar Ervin, Alfred Mallet +7

Collisionless dissipation of turbulence is important for heating plasmas in astrophysical, space physics, and laboratory environments, controlling energy, momentum and particle tra…