The TeV Sun Rises: Discovery of Gamma rays from the Quiescent Sun with HAWC
arXiv:2212.00815 · doi:10.1103/PhysRevLett.131.051201
Abstract
We report the first detection of a TeV gamma-ray flux from the solar disk (6.3), based on 6.1 years of data from the High Altitude Water Cherenkov (HAWC) observatory. The 0.5--2.6 TeV spectrum is well fit by a power law, dN/dE = , with TeV cm s and . The flux shows a strong indication of anticorrelation with solar activity. These results extend the bright, hard GeV emission from the disk observed with Fermi-LAT, seemingly due to hadronic Galactic cosmic rays showering on nuclei in the solar atmosphere. However, current theoretical models are unable to explain the details of how solar magnetic fields shape these interactions. HAWC's TeV detection thus deepens the mysteries of the solar-disk emission.
15 pages, 8 figures including supplementary material. Accepted for publication in Physical Review Letters
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Cited by in corpus (10)
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- Role of magnetic arcades in explaining the puzzle of the gamma-ray emission from the solar disk
- Super-Kamiokande Strongly Constrains Leptophilic Dark Matter Capture in the Sun
- Revisiting the propagation of highly-energetic gamma rays in the Galaxy
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