activity
20182026
most citedOn the Scaling Properties of Magnetic Field Fluctuations Through the Inner Heliosphere

41 citations · 92 across the 10 of their papers we have counts for

collaborators

11 papers

physics.space-ph2026

Electric Potential Patterns Forecasting in the Southern Hemisphere with Deep Learning Techniques

Francesco Pio Ramunno, Simone Mestici, Igino Coco +5

Space weather disturbances driven by the solar wind can degrade satellite navigation, disrupt radio communications, and threaten power infrastructure, making accurate forecasting o…

physics.space-ph2026

Self-organization of local streamline structures and energy transfer rate in compressible plasma turbulence

Simone Benella, Virgilio Quattrociocchi, Emanuele Papini +4

We examine how local streamline topology and energy cascade rate self-organize in plasma turbulence for both compressible and incompressible regimes. Using a fully-compressible Hal…

astro-ph.EP2025

Mission Analysis for the HENON CubeSat Mission to a Large Sun-Earth Distant Retrograde Orbit

S. Cicalò, E. M. Alessi, L. Provinciali +9

The HEliospheric pioNeer for sOlar and interplanetary threats defeNce (HENON) mission is a CubeSat Space Weather mission, designed to operate in a Sun-Earth Distant Retrograde Orbi…

physics.space-ph2024★ 2 cited

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★ 1 cited

Predicting the energetic proton flux with a machine learning regression algorithm

Mirko Stumpo, Monica Laurenza, Simone Benella +1

The need of real-time of monitoring and alerting systems for Space Weather hazards has grown significantly in the last two decades. One of the most important challenge for space mi…

astro-ph.SR2024

Comparative study of the kinetic properties of proton and alpha beams in the Alfvénic wind observed by SWA-PAS onboard Solar Orbiter

Roberto Bruno, Rossana DeMarco, Raffaella D Amicis +12

The problems of heating and acceleration of solar wind particles are of significant and enduring interest in astrophysics. The interactions between waves and particles are crucial…

physics.space-ph2023

Unveiling plasma energization and energy transport in the Earth Magnetospheric System: the need for future coordinated multiscale observations

A. Retino, L. Kepko, H. Kucharek +31

Energetic plasma is everywhere in the Universe. The terrestrial Magnetospheric System is a key case where direct measures of plasma energization and energy transport can be made in…

astro-ph.IM2023

Multi-point Assessment of the Kinematics of Shocks (MAKOS): A Heliophysics Mission Concept Study

Katherine A. Goodrich, Lynn B. Wilson, Steven Schwartz +6

Collisionless shocks are fundamental processes that are ubiquitous in space plasma physics throughout the Heliosphere and most astrophysical environments. Earth's bow shock and int…

physics.space-ph2023★ 36 cited

Three-dimensional modelling of the shock-turbulence interaction

Domenico Trotta, Oreste Pezzi, David Burgess +12

The complex interaction between shocks and plasma turbulence is extremely important to address crucial features of energy conversion in a broad range of astrophysical systems. We s…

physics.space-ph2020★ 41 cited

On the Scaling Properties of Magnetic Field Fluctuations Through the Inner Heliosphere

Tommaso Alberti, Monica Laurenza, Giuseppe Consolini +4

Although the interplanetary magnetic field variability has been extensively investigated in situ by means of data coming from several space missions, the newly launched missions pr…

physics.geo-ph2018★ 12 cited

Global diagnostics of ionospheric absorption during X-ray solar flares based on 8-20MHz noise measured by over-the-horizon radars

O. I. Berngardt, J. M. Ruohoniemi, J. -P. St-Maurice +9

An analysis of noise attenuation during eighty solar flares between 2013 and 2017 was carried out at frequencies 8-20 MHz using thirty-four SuperDARN radars and the EKB ISTP SB RAS…