activity
20072023
most citedObservation of inertial energy cascade in interplanetary space plasma

316 citations · 1.2k across the 28 of their papers we have counts for

collaborators

28 papers

cond-mat.stat-mech2023★ 14 cited

Ergodic observables in non-ergodic systems: the example of the harmonic chain

Marco Baldovin, Raffaele Marino, Angelo Vulpiani

In the framework of statistical mechanics the properties of macroscopic systems are deduced starting from the laws of their microscopic dynamics. One of the key assumptions in this…

astro-ph.SR2023★ 3 cited

Does Turbulence along the Coronal Current Sheet Drive Ion Cyclotron Waves?

Daniele Telloni, Gary P. Zank, Laxman Adhikari +32

Evidence for the presence of ion cyclotron waves, driven by turbulence, at the boundaries of the current sheet is reported in this paper. By exploiting the full potential of the jo…

physics.space-ph2023★ 23 cited

Helios 2 observations of solar wind turbulence decay in the inner heliosphere

Luca Sorriso-Valvo, Raffaele Marino, Foldes Raffaello +5

The linear scaling of the mixed third-order moment of the magnetohydrodynamic fluctuations is used to estimate the energy transfer rate of the turbulent cascade in the expanding so…

physics.plasm-ph2022★ 10 cited

Efficient kinetic Lattice Boltzmann simulation of three-dimensional Hall-MHD Turbulence

Raffaello Foldes, Emmanuel Lévêque, Raffaele Marino +4

Simulating plasmas in the Hall-MagnetoHydroDynamics (Hall-MHD) regime represents a valuable {approach for the investigation of} complex non-linear dynamics developing in astrophysi…

astro-ph.SR2022★ 56 cited

Observation of Magnetic Switchback in the Solar Corona

Daniele Telloni, Gary P. Zank, Marco Stangalini +49

Switchbacks are sudden, large radial deflections of the solar wind magnetic field, widely revealed in interplanetary space by the Parker Solar Probe. The switchbacks' formation mec…

physics.space-ph2021

Sudden depletion of Alfvénic turbulence in the rarefaction region of corotating solar wind high speed streams at 1 AU: possible solar origin?

Giuseppina Carnevale, Roberto Bruno, Raffaele Marino +2

A canonical description of a corotating solar wind high speed stream, in terms of velocity profile, would indicate three main regions:a stream interface or corotating interaction r…