@misc{10481/79034,
year = {2022},
month = {12},
url = {https://hdl.handle.net/10481/79034},
abstract = {High energy cosmic rays illuminate the Sun and produce an image that could be observed in up to five different
channels: a cosmic-ray shadow (whose energy dependence has been studied by HAWC); a gamma-ray flux
(observed at E   200 GeV by Fermi-LAT); a muon shadow (detected by ANTARES and IceCube); a neutron flux
(undetected, as there are no hadronic calorimeters in space); a flux of high energy neutrinos. Since these signals are
correlated, the ones already observed can be used to reduce the uncertainty in the still undetected ones. Here we
define a simple setup that uses the Fermi-LAT and HAWC observations to imply very definite fluxes of neutrons
and neutrinos from the solar disk. In particular, we provide a fit of the neutrino flux at 10 GeV–10 TeV that
includes its dependence on the zenith angle and on the period of the solar cycle. This flux represents a neutrino
floor in indirect dark matter searches. We show that in some benchmark models the current bounds on the dark
matter–nucleon cross section push the solar signal below this neutrino floor.},
organization = {Spanish Government},
organization = {Junta de Andalucia		
PID2019-107844GB-C21/AEI/10.13039/501100011033	
FQM 101	
P18-FR-5057},
publisher = {American Astronomical Society},
title = {The Solar Disk at High Energies},
doi = {10.3847/1538-4357/aca020},
author = {Gutiérrez González, Miguel and Masip Mellado, Manuel and Muñoz, Sergio},
}