Magnetic Structure and Propagation of Two Interacting CMEs From the Sun to Saturn

One of the grand challenges in heliophysics is the characterization of coronal mass ejection (CME) magnetic structure and evolution from eruption at the Sun through heliospheric propagation. At present, the main difficulties are related to the lack of direct measurements of the coronal magnetic fiel...

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Detalles Bibliográficos
Autores principales: Palmerio, Erika, Nieves‐Chinchilla, Teresa, Kilpua, Emilia K. J., Barnes, David, Zhukov, Andrei N., Jian, Lan K., Witasse, Olivier, Provan, Gabrielle, Tao, Chihiro, Lamy, Laurent, Bradley, Thomas J., Mays, M. Leila, Möstl, Christian, Roussos, Elias, Futaana, Yoshifumi, Masters, Adam, Sánchez‐Cano, Beatriz
Formato: Online Artículo Texto
Lenguaje:English
Publicado: John Wiley and Sons Inc. 2021
Materias:
Research Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9286593/
https://www.ncbi.nlm.nih.gov/pubmed/35864948
http://dx.doi.org/10.1029/2021JA029770

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9286593/
https://www.ncbi.nlm.nih.gov/pubmed/35864948
http://dx.doi.org/10.1029/2021JA029770

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