Enhancing the cosmic-ray mass sensitivity of air-shower arrays by combining radio and muon detectors
Author:
Funder
Helmholtz-Gemeinschaft
Publisher
Springer Science and Business Media LLC
Subject
Physics and Astronomy (miscellaneous),Engineering (miscellaneous)
Link
http://link.springer.com/content/pdf/10.1140/epjc/s10052-019-6859-4.pdf
Reference40 articles.
1. A. Aab et al. (Pierre Auger Collaboration), Observation of a large-scale anisotropy in the arrival directions of cosmic rays above $$8 \times 10^{18}$$ 8 × 10 18 eV. Science 357, 1266–1270 (2017). https://doi.org/10.1126/science.aan4338
2. K.-H. Kampert, M. Unger, Measurements of the cosmic ray composition with air shower experiments. Astropart. Phys. 35, 660 (2012). https://doi.org/10.1016/j.astropartphys.2012.02.004
3. F.G. Schröder, Radio detection of cosmic-ray air showers and high-energy neutrinos. Prog. Part. Nucl. Phys. 93, 1 (2017). https://doi.org/10.1016/j.ppnp.2016.12.002
4. T. Huege, Radio detection of cosmic ray air showers in the digital era. Phys. Rep. 620, 1 (2016). https://doi.org/10.1016/j.physrep.2016.02.001
5. A. Aab et al. (Pierre Auger Collaboration), Combined fit of spectrum and composition data as measured by the Pierre Auger Observatory. JCAP 04, 038 (2017). https://doi.org/10.1088/1475-7516/2017/04/038
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