activity
20222026
most citedMarkovian Features of the Solar Wind at Sub-Proton Scales

22 citations · 47 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2026★ 1 cited

Review of Machine Learning Models for Solar Energetic Particle Prediction

Spiridon Kasapis, Pouya Hosseinzadeh, Kathryn Whitman +73

Solar energetic particle (SEP) events have attracted increasing attention due to their significant radiation hazards for aviation, spacecraft electronics, and human missions beyond…

astro-ph.SR2026

Evidence of energy conversion in weakly collisional plasma during an interplanetary coronal mass ejection

Omkar Dhamane, Anil Raghav, Simone Benella +14

Intervals of enhanced turbulent fluctuations are typically less frequent within the magnetic cloud region of an interplanetary coronal mass ejection (ICME). We investigate two such…

physics.space-ph2024

Derivation of generalized Kappa distribution from scaling properties of solar wind magnetic field fluctuations at kinetic scales

Daniele Belardinelli, Simone Benella, Mirko Stumpo +1

Kinetic scale dynamics in weakly-collisional space plasmas usually exhibits a self-similar statistics of magnetic field fluctuations which implies the existence of an invariant pro…

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.SR2023★ 6 cited

Disentangling the solar activity-solar wind predictive causality at Space Climate scales

Raffaele Reda, Mirko Stumpo, Luca Giovannelli +2

The variability in the magnetic activity of the Sun is the main source of the observed changes in the plasma and electromagnetic environments within the heliosphere. The primary wa…

physics.plasm-ph2023

Linking Langevin equation to scaling properties of space plasma turbulence at sub-ion scales

Simone Benella, Mirko Stumpo, Tommaso Alberti +5

Current understanding of the kinetic-scale turbulence in weakly-collisional plasmas still remains elusive. We employ a general framework in which the turbulent energy transfer is e…

physics.space-ph2022

Dynamical information flow within the magnetosphere-ionosphere system during magnetic storms

Mirko Stumpo, Simone Benella, Giuseppe Consolini +1

The direct role of successive intense magnetospheric substorms in injecting/energizing particles into the storm-time ring current is still debated and controversial. Whereas in the…

astro-ph.SR2022★ 14 cited

Reconciling Parker Solar Probe observations and magnetohydrodynamic theory

Tommaso Alberti, Simone Benella, Giuseppe Consolini +2

The Parker Solar Probe mission provides a unique opportunity to characterize several features of the solar wind at different heliocentric distances. Recent findings have shown a tr…

physics.space-ph2022

Kramers-Moyal analysis of interplanetary magnetic field fluctuations at sub-ion scales

Simone Benella, Mirko Stumpo, Giuseppe Consolini +3

In the framework of statistical time series analysis of complex dynamics we present a multiscale characterization of solar wind turbulence in the near-Earth environment. The data a…

physics.data-an2022★ 3 cited

Markov property of the Super-MAG Auroral Electrojet Indices

Simone Benella, Giuseppe Consolini, Mirko Stumpo +2

The dynamics of the Earth's magnetosphere exhibits strongly fluctuating patterns as well as non-stationary and non-linear interactions, more pronounced during magnetospheric substo…

physics.space-ph2022★ 22 cited

Markovian Features of the Solar Wind at Sub-Proton Scales

Simone Benella, Mirko Stumpo, Giuseppe Consolini +3

The interplanetary magnetic field carried out from the Sun by the solar wind displays fluctuations on a wide range of scales. While at large scales, say at frequencies lower than 0…