22 citations · 55 across the 12 of their papers we have counts for
12 papers
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…
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…
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…
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…
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…
Turbulence and particle energization in twisted flux ropes in solar-wind conditions
Oreste Pezzi, Domenico Trotta, Simone Benella +6
Context. The mechanisms regulating the transport and energization of charged particles in space and astrophysical plasmas are still debated. Plasma turbulence is known to be a powe…
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…
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…
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…
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…
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…
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…