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...

Descripció completa

Dades bibliogràfiques

Autors principals:	Vishal Upendran, Durgesh Tripathi, Bhargav Vaidya, Mark C. M. Cheung, Takaaki Yokoyama
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2025-01-01
Col·lecció:	The Astrophysical Journal
Matèries:	Solar wind Solar coronal heating Magnetohydrodynamics Solar magnetic flux emergence Solar magnetic reconnection Solar magnetic fields
Accés en línia:	https://doi.org/10.3847/1538-4357/adc5fd
Etiquetes:	Afegir etiqueta Sense etiquetes, Sigues el primer a etiquetar aquest registre!