Understanding the Complex Morphology of a Coronal Mass Ejection: Multiview Analysis and Numerical Modeling

Understanding the Complex Morphology of a Coronal Mass Ejection: Multiview Analysis and Numerical Modeling

Although all coronal mass ejections (CMEs) that propagate into the heliosphere should contain a magnetic flux rope (MFR) component, the majority do not exhibit the expected white-light MFR morphology of a leading edge plus a cavity. This different appearance could be the result of distortion of the...

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Bibliographic Details
Main Authors: Cecilia Mac Cormack, Abril Sahade, Angelos Vourlidas, Phillip Hess, Robin Colaninno, Teresa Nieves-Chinchilla
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Solar coronal mass ejections
Solar magnetic fields
Heliosphere
Magnetohydrodynamical simulations
Online Access:https://doi.org/10.3847/1538-4357/ade311
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https://doi.org/10.3847/1538-4357/ade311

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