Astrophysical neutrinos and cosmic rays observed by IceCube

M.G. Aartsen; Mark Ackerman; J. Adams; J.A. Aguilar; Markus Tobias Ahlers; M. Ahrens; D. Altman; K. Andeen; T. Anderson; I Ansseau; G. Anton; M. Archinger; C. Arguelles; J. Auffenberg; S. Axani; X. Bai; S.W. Barwick; V. Baum; R. Bay; J.J. Beatty; J. Becker Tjus; D. Jason Koskinen; Michael James Larson; M Rameez; Morten Ankersen Medici; Subir Sarkar; E. Hansen; G. Yodh; M. Zoll

doi:10.1016/j.asr.2017.05.030

Astrophysical neutrinos and cosmic rays observed by IceCube

M.G. Aartsen, Mark Ackerman, J. Adams, J.A. Aguilar, Markus Tobias Ahlers, M. Ahrens, D. Altman, K. Andeen, T. Anderson, I Ansseau, G. Anton, M. Archinger, C. Arguelles, J. Auffenberg, S. Axani, X. Bai, S.W. Barwick, V. Baum, R. Bay, J.J. BeattyJ. Becker Tjus, D. Jason Koskinen, Michael James Larson, M Rameez, Morten Ankersen Medici, Subir Sarkar, E. Hansen, G. Yodh, M. Zoll

16 Citations (Scopus)

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 to our understanding of cosmic rays.

Original language	English
Journal	Advances in Space Research
Volume	62
Issue number	10
Pages (from-to)	2902-2930
Number of pages	29
ISSN	0273-1177
DOIs	https://doi.org/10.1016/j.asr.2017.05.030
Publication status	Published - 15 Nov 2018

Access to Document

10.1016/j.asr.2017.05.030

Cite this

Aartsen, M. G., Ackerman, M., Adams, J., Aguilar, J. A., Ahlers, M. T., Ahrens, M., Altman, D., Andeen, K., Anderson, T., Ansseau, I., Anton, G., Archinger, M., Arguelles, C., Auffenberg, J., Axani, S., Bai, X., Barwick, S. W., Baum, V., Bay, R., ... Zoll, M. (2018). Astrophysical neutrinos and cosmic rays observed by IceCube. Advances in Space Research, 62(10), 2902-2930. https://doi.org/10.1016/j.asr.2017.05.030

Aartsen, MG, Ackerman, M, Adams, J, Aguilar, JA, Ahlers, MT, Ahrens, M, Altman, D, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Archinger, M, Arguelles, C, Auffenberg, J, Axani, S, Bai, X, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Becker Tjus, J, Koskinen, DJ, Larson, MJ, Rameez, M, Medici, MA, Sarkar, S, Hansen, E, Yodh, G & Zoll, M 2018, 'Astrophysical neutrinos and cosmic rays observed by IceCube', Advances in Space Research, vol. 62, no. 10, pp. 2902-2930. https://doi.org/10.1016/j.asr.2017.05.030

@article{f24eb832ee694095981a73f4687fb7b0,

title = "Astrophysical neutrinos and cosmic rays observed by IceCube",

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 to our understanding of cosmic rays.",

author = "M.G. Aartsen and Mark Ackerman and J. Adams and J.A. Aguilar and Ahlers, {Markus Tobias} and M. Ahrens and D. Altman and K. Andeen and T. Anderson and I Ansseau and G. Anton and M. Archinger and C. Arguelles and J. Auffenberg and S. Axani and X. Bai and S.W. Barwick and V. Baum and R. Bay and J.J. Beatty and {Becker Tjus}, J. and Koskinen, {D. Jason} and Larson, {Michael James} and M Rameez and Medici, {Morten Ankersen} and Subir Sarkar and E. Hansen and G. Yodh and M. Zoll",

year = "2018",

month = nov,

day = "15",

doi = "10.1016/j.asr.2017.05.030",

language = "English",

volume = "62",

pages = "2902--2930",

journal = "Advances in Space Research",

issn = "0273-1177",

publisher = "Pergamon Press",

number = "10",

}

TY - JOUR

T1 - Astrophysical neutrinos and cosmic rays observed by IceCube

AU - Aartsen, M.G.

AU - Ackerman, Mark

AU - Adams, J.

AU - Aguilar, J.A.

AU - Ahlers, Markus Tobias

AU - Ahrens, M.

AU - Altman, D.

AU - Andeen, K.

AU - Anderson, T.

AU - Ansseau, I

AU - Anton, G.

AU - Archinger, M.

AU - Arguelles, C.

AU - Auffenberg, J.

AU - Axani, S.

AU - Bai, X.

AU - Barwick, S.W.

AU - Baum, V.

AU - Bay, R.

AU - Beatty, J.J.

AU - Becker Tjus, J.

AU - Koskinen, D. Jason

AU - Larson, Michael James

AU - Rameez, M

AU - Medici, Morten Ankersen

AU - Sarkar, Subir

AU - Hansen, E.

AU - Yodh, G.

AU - Zoll, M.

PY - 2018/11/15

Y1 - 2018/11/15

N2 - 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 to our understanding of cosmic rays.

AB - 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 to our understanding of cosmic rays.

U2 - 10.1016/j.asr.2017.05.030

DO - 10.1016/j.asr.2017.05.030

M3 - Journal article

SN - 0273-1177

VL - 62

SP - 2902

EP - 2930

JO - Advances in Space Research

JF - Advances in Space Research

IS - 10

ER -

Astrophysical neutrinos and cosmic rays observed by IceCube

Abstract

Access to Document

Fingerprint

Cite this