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What Determines the Brightness of the Magnetically Open Solar Corona?: Insights from Three-dimensional Radiative Magnetohydrodynamic Simulations and Observations

Fuente: arXiv

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Détails bibliographiques
Auteur principal:	Iijima, Haruhisa
Format:	Preprint
Publié:	2025
Sujets:	Solar and Stellar Astrophysics Space Physics
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

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