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Implications of the abundance of halo coronal mass ejections for the strength of solar cycle 25

Fuente: arXiv

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Dettagli Bibliografici
Autori principali:	Gopalswamy, Nat, Michalek, Grzegorz, Yashiro, Seiji, Makela, Pertti, Akiyama, Sachiko, Xie, Hong
Natura:	Preprint
Pubblicazione:	2024
Soggetti:	Solar and Stellar Astrophysics
Accesso online:	Acceder al recurso
Tags:	Aggiungi Tag Nessun Tag, puoi essere il primo ad aggiungerne!!

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