Comparison of Plasma Dynamics in Coronal Holes and Quiet Sun Using Flux Emergence Simulations

This paper presents a comparison of plasma dynamics in coronal holes (CHs) and quiet Sun (QS) through 2.5D MHD flux emergence simulations. The magnetic reconnection between the emerging and the preexisting flux leads to the formation of cool, dense plasmoids with hot boundaries, and hot and cool jet...

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Detalhes bibliográficos

Principais autores:	Vishal Upendran, Durgesh Tripathi, Bhargav Vaidya, Mark C. M. Cheung, Takaaki Yokoyama
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2025-01-01
Colecção:	The Astrophysical Journal
Assuntos:	Solar wind Solar coronal heating Magnetohydrodynamics Solar magnetic flux emergence Solar magnetic reconnection Solar magnetic fields
Acesso em linha:	https://doi.org/10.3847/1538-4357/adc5fd
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