papers

Publications (8)

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…

astro-ph.SR2021

Magnetic reconnection as a mechanism to produce multiple protonpopulations and beams locally in the solar wind

B. Lavraud, R. Kieokaew, N. Fargette +37

Context. Spacecraft observations early revealed frequent multiple proton populations in the solar wind. Decades of research on their origin have focused on processes such as magnet…

physics.space-ph2019

Particle transport in hybrid PIC shock simulations: A comparison of diagnostics

D. Trotta, D. Burgess, G. Prete +2

Recent in-situ and remote observations suggest that the transport regime associated with shock accelerated particles may be anomalous {i.e., the Mean Square Displacement (MSD) of s…

astro-ph.SR2023

Energetic particle dynamics in a simplified model of a solar wind magnetic switchback

F. Malara, S. Perri, J. Giacalone +1

Context. Recent spacecraft observations in the inner heliosphere have revealed the presence of local Alfvenic reversals of the magnetic field, while the field magnitude remains alm…

astro-ph.SR2013

Yaglom law in the expanding solar wind

G. Gogoberidze, S. Perri, V. Carbone

We study the Yaglom law, which relates the mixed third order structure function to the average dissipation rate of turbulence, in a uniformly expanding solar wind by using the two…

physics.plasm-ph2017

Charge proportional and weakly mass-dependent acceleration of different ion species in the Earth's magnetotail

F. Catapano, G. Zimbardo, S. Perri +4

Energetic particles with energies from tens of keV to a few hundreds keV are frequently observed in the Earth's magnetotail. Here we study, by means of a test particle numerical si…