Modelling large solar proton events with the shock-and-particle model

Modelling large solar proton events with the shock-and-particle model

We have developed a new version of a model that combines a two-dimensional Sun-to-Earth magnetohydrodynamic (MHD) simulation of the propagation of a CME-driven shock and a simulation of the transport of particles along the interplanetary magnetic field (IMF) line connecting the shock front and the o...

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Bibliographic Details
Main Authors: Pomoell Jens, Aran Angels, Jacobs Carla, Rodríguez-Gasén Rosa, Poedts Stefaan, Sanahuja Blai
Format: Article
Language:English
Published: EDP Sciences 2015-01-01
Series:Journal of Space Weather and Space Climate
Subjects:
Space weather
Shocks
Interplanetary medium
Energetic particle
SEP
Online Access:http://dx.doi.org/10.1051/swsc/2015015

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