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Simulations of Structured Upflows from Plumes and Their Connection to the Solar Wind

Small-scale transient jetlet activity and associated upflows from coronal hole plumes are potential sources of the solar wind. To elucidate the magnetic origins and driving mechanisms of such upflows, we perform three-dimensional (3D) radiative magnetohydrodynamic simulations using the MURaM code, s...

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Bibliografiske detaljer
Principais autores: K. Bora, L. P. Chitta, Yajie Chen, D. Przybylski, David I. Pontin, N. Panyam
Format: Artigo
Sprog:Inglês
Udgivet: IOP Publishing 2025-01-01
Serier:The Astrophysical Journal Letters
Fag:
Online adgang:https://doi.org/10.3847/2041-8213/ae2027
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