Elemental cosmic ray spectra are described by low-energy Galactic, high-energy Galactic, and extragalactic components with no additional Galactic component needed between 10 PeV and 1 EeV.
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Elemental cosmic ray spectra reveal two populations of Galactic sources and an immediate transition to an extragalactic component after the knee
Elemental cosmic ray spectra are described by low-energy Galactic, high-energy Galactic, and extragalactic components with no additional Galactic component needed between 10 PeV and 1 EeV.