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    Cosmic ray composition and energy spectrum from 1-30 PeV using the 40-string configuration of IceTop and IceCube

    Access Status
    Fulltext not available
    Authors
    Abbasi, R.
    Abdou, Y.
    Ackermann, M.
    Adams, J.
    Aguilar, J.
    Ahlers, M.
    Altmann, D.
    Andeen, K.
    Auffenberg, J.
    Bai, X.
    Baker, M.
    Barwick, S.
    Baum, V.
    Bay, R.
    Beattie, K.
    Beatty, J.
    Bechet, S.
    Becker, J.
    Becker, K.
    Bell, M.
    Benabderrahmane, M.
    Benzvi, S.
    Berdermann, J.
    Berghaus, P.
    Berley, D.
    Bernardini, E.
    Bertrand, D.
    Besson, D.
    Bindig, D.
    Bissok, M.
    Blaufuss, E.
    Blumenthal, J.
    Boersma, D.
    Bohm, C.
    Bose, D.
    Böser, S.
    Botner, O.
    Brayeur, L.
    Brown, A.
    Bruijn, R.
    Brunner, J.
    Buitink, S.
    Caballero-Mora, K.
    Carson, Michael
    Casey, J.
    Casier, M.
    Chirkin, D.
    Christy, B.
    Clevermann, F.
    Cohen, S.
    Cowen, D.
    Silva, A.
    Danninger, M.
    Daughhetee, J.
    Davis, J.
    De Clercq, C.
    Descamps, F.
    Desiati, P.
    De Vries-Uiterweerd, G.
    Deyoung, T.
    Díaz-Vélez, J.
    Dreyer, J.
    Dumm, J.
    Dunkman, M.
    Eagan, R.
    Eisch, J.
    Ellsworth, R.
    Engdegård, O.
    Euler, S.
    Evenson, P.
    Fadiran, O.
    Fazely, A.
    Fedynitch, A.
    Feintzeig, J.
    Feusels, T.
    Filimonov, K.
    Finley, C.
    Fischer-Wasels, T.
    Flis, S.
    Franckowiak, A.
    Franke, R.
    Frantzen, K.
    Fuchs, T.
    Gaisser, T.
    Gallagher, J.
    Gerhardt, L.
    Gladstone, L.
    Glüsenkamp, T.
    Goldschmidt, A.
    Goodman, J.
    Góra, D.
    Grant, D.
    Groß, A.
    Grullon, S.
    Gurtner, M.
    Date
    2013
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Abbasi, R. and Abdou, Y. and Ackermann, M. and Adams, J. and Aguilar, J. and Ahlers, M. and Altmann, D. et al. 2013. Cosmic ray composition and energy spectrum from 1-30 PeV using the 40-string configuration of IceTop and IceCube. Astroparticle Physics. 42: pp. 15-32.
    Source Title
    Astroparticle Physics
    DOI
    10.1016/j.astropartphys.2012.11.003
    ISSN
    0927-6505
    School
    Department of Exploration Geophysics
    URI
    http://hdl.handle.net/20.500.11937/27719
    Collection
    • Curtin Research Publications
    Abstract

    The mass composition of high energy cosmic rays depends on their production, acceleration, and propagation. The study of cosmic ray composition can therefore reveal hints of the origin of these particles. At the South Pole, the IceCube Neutrino Observatory is capable of measuring two components of cosmic ray air showers in coincidence: the electromagnetic component at high altitude (2835 m) using the IceTop surface array, and the muonic component above ~1 TeV using the IceCube array. This unique detector arrangement provides an opportunity for precision measurements of the cosmic ray energy spectrum and composition in the region of the knee and beyond. We present the results of a neural network analysis technique to study the cosmic ray composition and the energy spectrum from 1 PeV to 30 PeV using data recorded using the 40-string/40-station configuration of the IceCube Neutrino Observatory.

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