Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/111958
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Type: Journal article
Title: Neutrinos and Cosmic Rays Observed by IceCube
Author: Collaboration, I.
Aartsen, M.G.
Ackermann, M.
Adams, J.
Aguilar, J.A.
Ahlers, M.
Ahrens, M.
Samarai, I.A.
Altmann, D.
Andeen, K.
Anderson, T.
Ansseau, I.
Anton, G.
Archinger, M.
Argüelles, C.
Auffenberg, J.
Axani, S.
Bai, X.
Barwick, S.W.
Baum, V.
et al.
Citation: Advances in Space Research; 62:2902-2930
Publisher: Elsevier
Issue Date: 2018
ISSN: 0273-1177
1879-1948
Statement of
Responsibility: 
M.G. Aartsen ... G.C. Hill ... S. Robertson ... A. Wallace ... B. J. Whelan ... et al. (IceCube Collaboration)
Abstract: The core mission of the IceCube Neutrino observatory is to study the origin and propagation of cosmic rays. IceCube, with its surface component IceTop, observes multiple signatures to accomplish this mission. Most important are the astrophysical neutrinos that are produced in interactions of cosmic rays, close to their sources and in interstellar space. IceCube is the first instrument that measures the properties of this astrophysical neutrino flux, and constrains its origin. In addition, the spectrum, composition and anisotropy of the local cosmic-ray flux are obtained from measurements of atmospheric muons and showers. Here we provide an overview of recent findings from the analysis of IceCube data, and their implications on our understanding of cosmic rays.
Keywords: IceCube; neutrinos; cosmic rays
Rights: © 2017 COSPAR. Published by Elsevier Ltd. All rights reserved.
DOI: 10.1016/j.asr.2017.05.030
Published version: http://dx.doi.org/10.1016/j.asr.2017.05.030
Appears in Collections:Aurora harvest 8
Physics publications

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