2 papers
astro-ph.SR2026
A wavelet-based model of magnetic turbulence over a Parker spiral field
Andrea Larosa, Francesco Pucci, Francesco Malara +7
The propagation of Solar Energetic Particles (SEPs) through the heliosphere is strongly influenced by solar-wind magnetic turbulence, which governs particle scattering, field-line…
astro-ph.SR2025
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…