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A Community Data Set for Comparing Automated Coronal Hole Detection Schemes

Automated detection schemes are nowadays the standard approach for locating coronal holes in extreme-UV images from the Solar Dynamics Observatory (SDO). However, factors such as the noisy nature of solar imagery, instrumental effects, and others make it challenging to identify coronal holes using t...

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Autori principali: Martin A. Reiss, Karin Muglach, Emily Mason, Emma E. Davies, Shibaji Chakraborty, Veronique Delouille, Cooper Downs, Tadhg M. Garton, Jeremy A. Grajeda, Amr Hamada, Stephan G. Heinemann, Stefan Hofmeister, Egor Illarionov, Robert Jarolim, Larisza Krista, Chris Lowder, Erwin Verwichte, Charles N. Arge, Laura E. Boucheron, Claire Foullon, Michael S. Kirk, Alexander Kosovichev, Andrew Leisner, Christian Möstl, James Turtle, Astrid Veronig
Natura: Artigo
Lingua:Inglês
Pubblicazione: IOP Publishing 2024-01-01
Serie:The Astrophysical Journal Supplement Series
Soggetti:
Solar coronal holes
Solar corona
Solar wind
Accesso online:https://doi.org/10.3847/1538-4365/ad1408
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