All-particle cosmic ray energy spectrum measured with 26 IceTop stations
Abstract
We report on a measurement of the cosmic ray energy spectrum with the IceTop air shower array, the surface component of the IceCube Neutrino Observatory at the South Pole. The data used in this analysis were taken between June and October, 2007, with 26 surface stations operational at that time, corresponding to about one third of the final array. The fiducial area used in this analysis was 0.122 km^2. The analysis investigated the energy spectrum from 1 to 100 PeV measured for three different zenith angle ranges between 0{\deg} and 46{\deg}. Because of the isotropy of cosmic rays in this energy range the spectra from all zenith angle intervals have to agree. The cosmic-ray energy spectrum was determined under different assumptions on the primary mass composition. Good agreement of spectra in the three zenith angle ranges was found for the assumption of pure proton and a simple two-component model. For zenith angles {\theta} < 30{\deg}, where the mass dependence is smallest, the knee in the cosmic ray energy spectrum was observed between 3.5 and 4.32 PeV, depending on composition assumption. Spectral indices above the knee range from -3.08 to -3.11 depending on primary mass composition assumption. Moreover, an indication of a flattening of the spectrum above 22 PeV were observed.
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Cite
@article{arxiv.1202.3039,
title = {All-particle cosmic ray energy spectrum measured with 26 IceTop stations},
author = {IceCube Collaboration and R. Abbasi and Y. Abdou and T. Abu-Zayyad and M. Ackermann and J. Adams and J. A. Aguilar and M. Ahlers and D. Altmann and K. Andeen and J. Auffenberg and X. Bai and M. Baker and S. W. Barwick and V. Baum and R. Bay and J. L. Bazo Alba and K. Beattie and J. J. Beatty and S. Bechet and J. K. Becker and K. -H. Becker and M. Bell and M. L. Benabderrahmane and S. BenZvi and J. Berdermann and P. Berghaus and D. Berley and E. Bernardini and D. Bertrand and D. Z. Besson and D. Bindig and M. Bissok and E. Blaufuss and J. Blumenthal and D. J. Boersma and C. Bohm and D. Bose and S. Böser and O. Botner and L. Brayeur and A. M. Brown and S. Buitink and K. S. Caballero-Mora and M. Carson and M. Casier and D. Chirkin and B. Christy and F. Clevermann and S. Cohen and D. F. Cowen and A. H. Cruz Silva and M. V. D'Agostino and M. Danninger and J. Daughhetee and J. C. Davis and C. De Clercq and T. Degner and F. Descamps and P. Desiati and G. de Vries-Uiterweerd and T. DeYoung and J. C. Díaz-Vélez and J. Dreyer and J. P. Dumm and M. Dunkman and J. Eisch and R. W. Ellsworth and O. Engdegård and S. Euler and P. A. Evenson and O. Fadiran and A. R. Fazely and A. Fedynitch and J. Feintzeig and T. Feusels and K. Filimonov and C. Finley and T. Fischer-Wasels and S. Flis and A. Franckowiak and R. Franke and T. K. Gaisser and J. Gallagher and L. Gerhardt and L. Gladstone and T. Glüsenkamp and A. Goldschmidt and J. A. Goodman and D. Góra and D. Grant and A. Groß and S. Grullon and M. Gurtner and C. Ha and A. Haj Ismail and A. Hallgren and F. Halzen and K. Han and K. Hanson and P. Heimann and D. Heinen and K. Helbing and R. Hellauer and S. Hickford and G. C. Hill and K. D. Hoffman and B. Hoffmann and A. Homeier and K. Hoshina and W. Huelsnitz and P. O. Hulth and K. Hultqvist and S. Hussain and A. Ishihara and E. Jacobi and J. Jacobsen and G. S. Japaridze and H. Johansson and A. Kappes and T. Karg and A. Karle and J. Kiryluk and F. Kislat and S. R. Klein and S. Klepser and J. -H. Köhne and G. Kohnen and H. Kolanoski and L. Köpke and S. Kopper and D. J. Koskinen and M. Kowalski and M. Krasberg and G. Kroll and J. Kunnen and N. Kurahashi and T. Kuwabara and M. Labare and K. Laihem and H. Landsman and M. J. Larson and R. Lauer and J. Lünemann and J. Madsen and R. Maruyama and K. Mase and H. S. Matis and K. Meagher and M. Merck and P. Mészáros and T. Meures and S. Miarecki and E. Middell and N. Milke and J. Miller and T. Montaruli and R. Morse and S. M. Movit and R. Nahnhauer and J. W. Nam and U. Naumann and S. C. Nowicki and D. R. Nygren and S. Odrowski and A. Olivas and M. Olivo and A. O'Murchadha and S. Panknin and L. Paul and C. Pérez de los Heros and D. Pieloth and J. Posselt and P. B. Price and G. T. Przybylski and K. Rawlins and P. Redl and E. Resconi and W. Rhode and M. Ribordy and M. Richman and B. Riedel and J. P. Rodrigues and F. Rothmaier and C. Rott and T. Ruhe and D. Rutledge and B. Ruzybayev and D. Ryckbosch and H. -G. Sander and M. Santander and S. Sarkar and K. Schatto and M. Scheel and T. Schmidt and S. Schöneberg and A. Schönwald and A. Schukraft and L. Schulte and A. Schultes and O. Schulz and M. Schunck and D. Seckel and B. Semburg and S. H. Seo and Y. Sestayo and S. Seunarine and A. Silvestri and M. W. E. Smith and G. M. Spiczak and C. Spiering and M. Stamatikos and T. Stanev and T. Stezelberger and R. G. Stokstad and A. Stößl and E. A. Strahler and R. Ström and M. Stüer and G. W. Sullivan and H. Taavola and I. Taboada and A. Tamburro and S. Ter-Antonyan and S. Tilav and P. A. Toale and S. Toscano and D. Tosi and N. van Eijndhoven and A. Van Overloop and J. van Santen and M. Vehring and M. Voge and C. Walck and T. Waldenmaier and M. Wallraff and M. Walter and R. Wasserman and Ch. Weaver and C. Wendt and S. Westerhoff and N. Whitehorn and K. Wiebe and C. H. Wiebusch and D. R. Williams and R. Wischnewski and H. Wissing and M. Wolf and T. R. Wood and K. Woschnagg and C. Xu and D. L. Xu and X. W. Xu and J. P. Yanez and G. Yodh and S. Yoshida and P. Zarzhitsky and M. Zoll},
journal= {arXiv preprint arXiv:1202.3039},
year = {2012}
}
Comments
38 pages, 17 figures