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Cosmic rays can interact with the solar atmosphere and produce a slew of secondary messengers, making the Sun a bright gamma-ray source in the sky.
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Igor V. Moskalenko, Troy A. Porter, and Seth W. Digel, “Inverse Compton scattering on solar photons, heliospheric modulation, and neutrino astrophysics,” Astrophys. J. 652
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J. Allison et al. , “Recent developments in Geant4,” Nucl. Instrum. Meth. A835
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Baosheng Gao, Songzhan Chen, Zhe Li, Chunxu Yu, Kuiyong Liu, and Huihai He, “Study of Solar Gamma Rays basing on Geant4 code,” The Fluorescence detector Array of Single-pixel Telescopes: Contributions to the 35th International Cosmic Ray Conference (ICRC 2017) , PoS ICRC2017
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Zhe Li, Songzhan Chen, Yuncheng Nan, Huihai He, and Cong Li, “Estimation of solar disk gamma-ray emission based on Geant4,” PoS ICRC2019
2019
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2019
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Zihao Yang, Christian Bethge, Hui Tian, Steven Tomczyk, Richard Morton, Giulio Del Zanna, Scott W. McIntosh, Bidya Binay Karak, Sarah Gibson, Tanmoy Samanta, Jiansen He, Yajie Chen, and Linghua Wang, “Global maps of the magnetic field in the solar corona,” Science 369
2020
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Elena Orlando and Andrew Strong, “Stellarics: inverse compton emission from the quiet sun and stars from kev to tev,” Journal of Cosmology and Astroparticle Physics 2021
2021
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