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Imaging and Radio Signatures of Shock–Plasmoid Interaction

Understanding how shocks interact with coronal structures is crucial for understanding the mechanisms of particle acceleration in the solar corona and inner heliosphere. Using simultaneous radio and white-light observations, we investigate the interaction between a coronal mass ejection (CME)-driven...

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Bibliografische Detailangaben
Hauptverfasser: Pankaj Kumar, Judith T. Karpen, P. K. Manoharan, N. Gopalswamy
Format: Artigo
Sprache:Inglês
Veröffentlicht: IOP Publishing 2025-01-01
Schriftenreihe:The Astrophysical Journal Letters
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Online-Zugang:https://doi.org/10.3847/2041-8213/ae0009
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