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- W4385304818 abstract "In this contribution we study the possibility of the formation of cosmic ray ensembles (CRE) created by the interaction of ultra-high energy (UHE) photons with the magnetic field of the Sun. The lack of observation of those UHE and the difficulties for their identification given the current methodologies motivates this study. We performed simulations using the PRESHOWER program in order to simulate the expected extensive air showers which might be spatially correlated generated upon entering the Earth's atmosphere. We found characteristic features like very thing and extremely elongates cascades of secondary photons with their corresponding energies spanning the entire cosmic range spectrum. Shower footprints are as large as hundreds of kilometers." @default.
- W4385304818 created "2023-07-28" @default.
- W4385304818 creator A5006392977 @default.
- W4385304818 date "2023-08-28" @default.
- W4385304818 modified "2023-10-14" @default.
- W4385304818 title "Simulation of the isotropic ultra-high energy photons flux in the solar magnetic field and a comparison with observations made by the HAWC and Fermi-LAT observatories" @default.
- W4385304818 doi "https://doi.org/10.22323/1.444.0446" @default.
- W4385304818 hasPublicationYear "2023" @default.
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