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. 2023 Aug 4;131(5):051201.
doi: 10.1103/PhysRevLett.131.051201.

Discovery of Gamma Rays from the Quiescent Sun with HAWC

A Albert  1 R Alfaro  2 C Alvarez  3 J C Arteaga-Velázquez  4 D Avila Rojas  2 H A Ayala Solares  5 R Babu  6 E Belmont-Moreno  2 C Brisbois  7 K S Caballero-Mora  3 T Capistrán  8 A Carramiñana  9 S Casanova  10 O Chaparro-Amaro  11 U Cotti  4 J Cotzomi  12 S Coutiño de León  13 E De la Fuente  14 R Diaz Hernandez  9 B L Dingus  1   7 M A DuVernois  13 M Durocher  1 J C Díaz-Vélez  14 R W Ellsworth  7 K Engel  7 C Espinoza  2 K L Fan  7 K Fang  13 M Fernández Alonso  5 H Fleischhack  15   16   17 N Fraija  8 J A García-González  18 F Garfias  8 M M González  8 J A Goodman  7 J P Harding  1 S Hernandez  2 J Hinton  19 D Huang  6 F Hueyotl-Zahuantitla  3 P Hüntemeyer  6 A Iriarte  8 V Joshi  20 S Kaufmann  21 J Lee  22 J T Linnemann  23 A L Longinotti  8 G Luis-Raya  21 K Malone  24 O Martinez  12 J Martínez-Castro  11 J A Matthews  25 P Miranda-Romagnoli  26 J A Morales-Soto  4 E Moreno  12 M Mostafá  5 A Nayerhoda  10 L Nellen  27 M U Nisa  23 R Noriega-Papaqui  26 L Olivera-Nieto  19 N Omodei  28 Y Pérez Araujo  8 E G Pérez-Pérez  21 C D Rho  29 D Rosa-González  9 E Ruiz-Velasco  19 H Salazar  12 D Salazar-Gallegos  23 A Sandoval  2 M Schneider  7 J Serna-Franco  2 A J Smith  7 Y Son  22 R W Springer  30 O Tibolla  21 K Tollefson  23 I Torres  9 R Torres-Escobedo  31 R Turner  6 F Ureña-Mena  9 E Varela  12 L Villaseñor  12 X Wang  6 I J Watson  22 E Willox  7 S Yun-Cárcamo  7 H Zhou  31 C de León  4 J F Beacom  32   33   34 T Linden  35 K C Y Ng  36 A H G Peter  32   33   34   37 B Zhou  38 HAWC Collaboration
Affiliations

Discovery of Gamma Rays from the Quiescent Sun with HAWC

A Albert et al. Phys Rev Lett. .

Abstract

We report the first detection of a TeV γ-ray flux from the solar disk (6.3σ), 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=A(E/1 TeV)^{-γ}, with A=(1.6±0.3)×10^{-12} TeV^{-1} cm^{-2} s^{-1} and γ=3.62±0.14. 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.

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