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Role of Magnetic Arcades in Explaining the Puzzle of the Gamma-Ray Emission from the Solar Disk

The interpretation of gamma-ray emission originating from the solar disk (0.5° in angular size) as due to the interaction of Galactic Cosmic Rays (GCRs) with the solar atmosphere has remained a central challenge in solar physics. After the seminal work by Seckel, Stanev, and Gaisser based on GCRs’ m...

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Bibliografski detalji
Glavni autori: Eleonora Puzzoni, Federico Fraschetti, József Kóta, Joe Giacalone
Format: Artigo
Jezik:Inglês
Izdano: IOP Publishing 2024-01-01
Serija:The Astrophysical Journal
Teme:
Online pristup:https://doi.org/10.3847/1538-4357/ad65ea
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