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- W2945802597 abstract "The IceCube Neutrino Observatory at the geographic South Pole, with its surface array IceTop, detects three different components of extensive air showers: the total signal at the surface, low energy muons on the periphery of the showers, and high energy muons in the deep In Ice array of IceCube. These measurements enable determination of the energy spectrum and composition of cosmic rays from PeV to EeV energies, the anisotropy in the distribution of cosmic ray arrival directions, the muon density of cosmic ray air showers, and the PeV gamma-ray flux. Furthermore, IceTop can be used as a veto for the neutrino measurements. The latest results from these IceTop analyses will be presented along with future plans." @default.
- W2945802597 created "2019-05-29" @default.
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- W2945802597 date "2019-01-01" @default.
- W2945802597 modified "2023-09-23" @default.
- W2945802597 title "Latest Cosmic Ray Results from IceTop and IceCube" @default.
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- W2945802597 doi "https://doi.org/10.1051/epjconf/201921003005" @default.
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