Spatial Relationship between CMEs and Prominence Eruptions during SC 24 and SC 25

Spatial Relationship between CMEs and Prominence Eruptions during SC 24 and SC 25

During their propagation, coronal mass ejections (CMEs) and prominences sometimes display a nonradial motion. During the years after the solar minimum, the CME central position angle tended to be offset closer to the equator compared to that of the associated prominence eruptions (PE). No such effec...

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Bibliographic Details
Main Authors: Kostadinka Koleva, Nat Gopalswamy, Pooja Devi, Seiji Yashiro, Grzegorz Michalek
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Solar coronal mass ejections
Solar prominences
Online Access:https://doi.org/10.3847/1538-4357/ad2df3

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