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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Autori principali:	K. Bora, L. P. Chitta, Yajie Chen, D. Przybylski, David I. Pontin, N. Panyam
Natura:	Artigo
Lingua:	Inglês
Pubblicazione:	IOP Publishing 2025-01-01
Serie:	The Astrophysical Journal Letters
Soggetti:	Solar coronal holes Solar coronal plumes Radiative magnetohydrodynamics Magnetohydrodynamical simulations
Accesso online:	https://doi.org/10.3847/2041-8213/ae2027
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