98 citations · 531 across the 19 of their papers we have counts for
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Evolution of the Shock Properties of the 2023 March 13 Event from In-Situ and Remote-Sensing Data
Federica Chiappetta, Giuseppe Nisticò, Massimo Chimenti +6
Shocks driven by coronal mass ejections (CMEs) are the most powerful accelerators of gradual solar energetic particles (SEPs) in the inner heliosphere. On 2023 March 13, a halo CME…
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…
Interpretation of flat energy spectra upstream of fast interplanetary shocks
Silvia Perri, Giuseppe Prete, Gaetano Zimbardo +6
Interplanetary shocks are large-scale heliospheric structures often caused by eruptive phenomena at the Sun, and represent one of the main sources of energetic particles. Several i…
Probing the Density Fine Structuring of the Solar Corona with Comet Lovejoy
Giuseppe Nisticò, Gaetano Zimbardo, Silvia Perri +3
The passage of sungrazing comets in the solar corona can be a powerful tool to probe the local plasma properties. Here, we carry out a study of the striae pattern appearing in the…
Coherent events at ion scales in the inner Heliosphere: \textit{Parker Solar Probe} observations during the first Encounter
Denise Perrone, Roberto Bruno, Raffaella D'Amicis +7
\textit{Parker Solar Probe} has shown the ubiquitous presence of strong magnetic field deflections, namely switchbacks, during its first perihelion where it was embedded in a highl…
The Complex Structure of Magnetic Field Discontinuities in the Turbulent Solar Wind
A. Greco, S. Perri, S. Servidio +2
Using high resolution Cluster satellite observations, we show that the turbulent solar wind is populated by magnetic discontinuities at different scales, going from proton down to…