activity
20242026
collaborators

11 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

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

Assessing VBz variations during CME propagation: a preparatory study for the HENON mission using EUHFORIA

G. Prete, A. Niemela, S. Poedts +21

Coronal mass ejections (CMEs) are among the main drivers of space weather hazards. In this context, HENON is a new space mission designed to carry out observations in the solar win…

gr-qc2026

The Role of Inhomogeneities in the Turbulent Accretion of Black Holes

Giuseppe Ficarra, Michele Arcuri, Rita Megale +1

Observations of supermassive black holes by the Event Horizon Telescope reveal significant inhomogeneities, most likely related to density and magnetic field perturbations. To mode…

physics.plasm-ph2025

Numerical investigation of kinetic instabilities in BGK equilibria under collisional effects

Sofia Zanelli, Gabriele Celebre, Sergio Servidio +1

An unstable one-dimensional Bernstein-Greene-Kruskal (BGK) mode has been studied through high-precision numerical simulations. The initial turbulent, periodic equilibrium state is…

physics.plasm-ph2025

Long-living Equilibria in Kinetic Astrophysical Plasma Turbulence

Mario Imbrogno, Claudio Meringolo, Sergio Servidio +3

Turbulence in classical fluids is characterized by persistent structures that emerge from the chaotic landscape. We investigate the analogous process in fully kinetic plasma turbul…