A four-component model of two Galactic and two extragalactic source populations reproduces the correlated spectral, composition, and anisotropy structures of cosmic rays from tens of GeV to 100 EeV.
Cosmic Ray Spectrum from 250 TeV to 10 PeV using IceTop
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abstract
We report here an extension of the measurement of the all-particle cosmic-ray spectrum with IceTop to lower energy. The new measurement gives full coverage of the knee region of the spectrum and reduces the gap in energy between previous IceTop and direct measurements. With a new trigger that selects events in closely spaced detectors in the center of the array, the IceTop energy threshold is lowered by almost an order of magnitude below its previous threshold of 2 PeV. In this paper, we explain how the new trigger is implemented, and we describe the new machine-learning method developed to deal with events with very few detectors hit. We compare the results with previous measurements by IceTop and others that overlap at higher energy and with HAWC and Tibet in the 100 TeV range.
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Co-evolution of cosmic ray energy spectra, composition, and anisotropies
A four-component model of two Galactic and two extragalactic source populations reproduces the correlated spectral, composition, and anisotropy structures of cosmic rays from tens of GeV to 100 EeV.