Advancing interplanetary magnetohydrodynamic models through solar energetic particle modelling: Insights from the 2013 March 15 SEP event
[Aims] This study utilises a modelling approach to investigate the impact of perturbed solar wind conditions caused by multiple interplanetary coronal mass ejections (ICMEs) on the evolution of solar energetic particle (SEP) distributions. Furthermore, we demonstrate the utility of SEP models in eva...
| Autores: | , , , , , |
|---|---|
| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2023 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/347344 |
| Acceso en línea: | http://hdl.handle.net/10261/347344 |
| Access Level: | acceso abierto |
| Palabra clave: | Sun: coronal mass ejections (CMEs) Sun: heliosphere Solar wind Sun: particle emission |
| Sumario: | [Aims] This study utilises a modelling approach to investigate the impact of perturbed solar wind conditions caused by multiple interplanetary coronal mass ejections (ICMEs) on the evolution of solar energetic particle (SEP) distributions. Furthermore, we demonstrate the utility of SEP models in evaluating the performance of solar wind and coronal mass ejection (CME) models. To illustrate these concepts, we focussed on modelling the gradual SEP event that occurred on 2023 March 15. |
|---|