The Chromosphere Underneath a Coronal Bright Point

Coronal bright points (CBPs) are sets of small-scale coronal loops, connecting opposite magnetic polarities, primarily characterized by their enhanced extreme-ultraviolet (EUV) and X-ray emission. Being ubiquitous, they are thought to play an important role in heating the solar corona. We aim at cha...

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Bibliographic Details
Published in:	The Astrophysical Journal
Main Authors:	Souvik Bose, Daniel Nóbrega-Siverio, Bart De Pontieu, Luc Rouppe van der Voort
Format:	Article
Language:	English
Published:	IOP Publishing 2023-01-01
Subjects:	Solar coronal heating Solar spicules Solar chromosphere Solar corona Solar magnetic flux emergence Computational methods
Online Access:	https://doi.org/10.3847/1538-4357/acb544

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