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Discovery of Gamma Rays from the Quiescent Sun with HAWC

Authors
Albert, A.[Albert, A.]Alfaro, R.[Alfaro, R.]Alvarez, C.[Alvarez, C.]Arteaga-Velázquez, J.C.[Arteaga-Velázquez, J.C.]Avila, Rojas D.[Avila Rojas, D.]Ayala, Solares H.A.[Ayala Solares, H.A.]Babu, R.[Babu, R.]Belmont-Moreno, E.[Belmont-Moreno, E.]Brisbois, C.[Brisbois, C.]Caballero-Mora, K.S.[Caballero-Mora, K.S.]Capistrán, T.[Capistrán, T.]Carramiñana, A.[Carramiñana, A.]Casanova, S.[Casanova, S.]Chaparro-Amaro, O.[Chaparro-Amaro, O.]Cotti, U.[Cotti, U.]Cotzomi, J.[Cotzomi, J.]Coutiño, De León S.[Coutiño De León, S.]De, La Fuente E.[De La Fuente, E.]Diaz, Hernandez R.[Diaz Hernandez, R.]Dingus, B.L.[Dingus, B.L.]Duvernois, M.A.[Duvernois, M.A.]Durocher, M.[Durocher, M.]Díaz-Vélez, J.C.[Díaz-Vélez, J.C.]Ellsworth, R.W.[Ellsworth, R.W.]Engel, K.[Engel, K.]Espinoza, C.[Espinoza, C.]Fan, K.L.[Fan, K.L.]Fang, K.[Fang, K.]Fernández, Alonso M.[Fernández Alonso, M.]Fleischhack, H.[Fleischhack, H.]Fraija, N.[Fraija, N.]García-González, J.A.[García-González, J.A.]Garfias, F.[Garfias, F.]González, M.M.[González, M.M.]Goodman, J.A.[Goodman, J.A.]Harding, J.P.[Harding, J.P.]Hernandez, S.[Hernandez, S.]Hinton, J.[Hinton, J.]Huang, D.[Huang, D.]Hueyotl-Zahuantitla, F.[Hueyotl-Zahuantitla, F.]Hüntemeyer, P.[Hüntemeyer, P.]Iriarte, A.[Iriarte, A.]Joshi, V.[Joshi, V.]Kaufmann, S.[Kaufmann, S.]Lee, J.[Lee, J.]Linnemann, J.T.[Linnemann, J.T.]Longinotti, A.L.[Longinotti, A.L.]Luis-Raya, G.[Luis-Raya, G.]Malone, K.[Malone, K.]Martinez, O.[Martinez, O.]Martínez-Castro, J.[Martínez-Castro, J.]Matthews, J.A.[Matthews, J.A.]Miranda-Romagnoli, P.[Miranda-Romagnoli, P.]Morales-Soto, J.A.[Morales-Soto, J.A.]Moreno, E.[Moreno, E.]Mostafá, M.[Mostafá, M.]Nayerhoda, A.[Nayerhoda, A.]Nellen, L.[Nellen, L.]Nisa, M.U.[Nisa, M.U.]Noriega-Papaqui, R.[Noriega-Papaqui, R.]Olivera-Nieto, L.[Olivera-Nieto, L.]Omodei, N.[Omodei, N.]Pérez, Araujo Y.[Pérez Araujo, Y.]Pérez-Pérez, E.G.[Pérez-Pérez, E.G.]Rho, C.D.[Rho, C.D.]Rosa-González, D.[Rosa-González, D.]Ruiz-Velasco, E.[Ruiz-Velasco, E.]Salazar, H.[Salazar, H.]Salazar-Gallegos, D.[Salazar-Gallegos, D.]Sandoval, A.[Sandoval, A.]Schneider, M.[Schneider, M.]Serna-Franco, J.[Serna-Franco, J.]Smith, A.J.[Smith, A.J.]Son, Y.[Son, Y.]Springer, R.W.[Springer, R.W.]Tibolla, O.[Tibolla, O.]Tollefson, K.[Tollefson, K.]Torres, I.[Torres, I.]Torres-Escobedo, R.[Torres-Escobedo, R.]Turner, R.[Turner, R.]Ureña-Mena, F.[Ureña-Mena, F.]Varela, E.[Varela, E.]Villaseñor, L.[Villaseñor, L.]Wang, X.[Wang, X.]Watson, I.J.[Watson, I.J.]Willox, E.[Willox, E.]Yun-Cárcamo, S.[Yun-Cárcamo, S.]Zhou, H.[Zhou, H.]De, León C.[De León, C.]Beacom, J.F.[Beacom, J.F.]Linden, T.[Linden, T.]Ng, K.C.Y.[Ng, K.C.Y.]Peter, A.H.G.[Peter, A.H.G.]Zhou, B.[Zhou, B.]
Issue Date
3-Aug-2023
Publisher
American Physical Society
Citation
Physical Review Letters, v.131, no.5
Indexed
SCIE
SCOPUS
Journal Title
Physical Review Letters
Volume
131
Number
5
URI
https://scholarworks.bwise.kr/skku/handle/2021.sw.skku/107896
DOI
10.1103/PhysRevLett.131.051201
ISSN
0031-9007
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. © 2023 American Physical Society.
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