Challenges in Forecasting the Evolution of a Distorted CME Observed During the First Close Solar Orbiter Perihelion

Coronal Mass Ejections (CMEs), drivers of the most severe Space Weather disturbances, are often assumed to evolve self-similarly during their propagation. However, open magnetic field structures in the corona, leading to higher-speed streams in the ambient solar wind, can be source of strong distort...

ver descrição completa

Detalhes bibliográficos

Principais autores:	Alessandro Liberatore, Carlos R. Braga, Manuela Temmer, Greta M. Cappello, Daniele Telloni, Paulett C. Liewer, Angelos Vourlidas, Marco Velli, Daniel Heyner, Hans-Ulrich Auster, Ingo Richter, Daniel Schmid, David Fischer, Christian Möstl
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2024-01-01
Colecção:	The Astrophysical Journal
Assuntos:	Solar corona Active solar corona Solar coronal mass ejections Solar wind Space weather
Acesso em linha:	https://doi.org/10.3847/1538-4357/ad5003
Tags:	Adicionar Tag Sem tags, seja o primeiro a adicionar uma tag!