Small-scale Magnetic Fields Are Critical to Shaping Solar Gamma-Ray Emission
The Sun is a bright gamma-ray source due to hadronic cosmic-ray interactions with solar gas. While it is known that incoming cosmic rays must generally first be reflected by solar magnetic fields to produce outgoing gamma rays, theoretical models have yet to reproduce the observed spectra. We introd...
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| Principais autores: | , , , |
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| פורמט: | Artigo |
| שפה: | Inglês |
| יצא לאור: |
IOP Publishing
2024-01-01
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| סדרה: | The Astrophysical Journal |
| נושאים: | |
| גישה מקוונת: | https://doi.org/10.3847/1538-4357/ad158f |
| תגים: |
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