collaborators

6 papers

physics.plasm-ph2026

Turbulent Magnetogenesis and Large-scale Magnetic Dynamo Amplification in Ion--electron Plasmas

Fabio Bacchini, Francesco Pucci, Sergio Servidio +2

Using fully kinetic simulations that capture unprecedentedly large (from electron to ion) scales, we study magnetogenesis driven by continuous large-scale forcing until nonlinear d…

physics.plasm-ph2026

Reconnection-induced electron energization in magnetospheric Kelvin-Helmholtz dynamics

Silvia Ferro, Fabio Bacchini, Giuseppe Arrò +2

The Kelvin-Helmholtz instability (KHI) is a major driver of multiscale plasma dynamics at velocity shear layers, where it can promote the formation of current sheets and the onset…

physics.plasm-ph2026

Plasma Mixing Driven by the Collisionless Kelvin-Helmholtz Instability: Insights from fully kinetic simulation and density-based diagnostics

Silvia Ferro, Fabio Bacchini, Giuseppe Arrò +2

Simulations and observations of the low-latitude magnetosphere-magnetosheath boundary layer indicate that the Kelvin-Helmholtz instability (KHI) drives vortex structures that enhan…

physics.ins-det2026

Characterization of the Low Energy Excess using a NUCLEUS detector

H. Abele, G. Angloher, B. Arnold +62

The NUCLEUS experiment aims to detect coherent elastic neutrino-nucleus scattering of reactor antineutrinos using low-threshold, gram-scale cryogenic calorimeters. Similar to other…

physics.space-ph2024

Evaluation of scale-dependent kurtosis with HelioSwarm

Francesco Pecora, Francesco Pucci, Francesco Malara +4

Plasma turbulence involves complex, nonlinear interactions of electromagnetic fields and charged particles across multiple scales. Studying these phenomena in space plasmas, like t…

astro-ph.SR2024

Large Scale Linear Magnetic Holes with Magnetic Mirror Properties in Hybrid Simulations of Solar Wind Turbulence

Giuseppe Arrò, Francesco Califano, Francesco Pucci +2

Magnetic holes (MHs) are coherent magnetic field dips whose size ranges from fluid to kinetic scale, ubiquitously observed in the heliosphere and in planetary environments. Despite…