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How coronal mass ejections are influenced by the morphology and toroidal flux of their source magnetic flux ropes?

Fuente: arXiv

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Bibliographic Details
Main Authors:	Guo, J. H., Linan, L., Poedts, S., Guo, Y., Schmieder, B., Lani, A., Ni, Y. W., Brchnelova, M., Perri, B., Baratashvili, T., Li, S. T., Chen, P. F.
Format:	Preprint
Published:	2024
Subjects:	Solar and Stellar Astrophysics Astrophysics of Galaxies Space Physics
Online Access:	Acceder al recurso
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