| タイトル | All-Particle Cosmic Ray Energy Spectrum Measured with 26 Icetop Stations |
| 本文（外部サイト） | http://hdl.handle.net/2060/20140011440 |
| 著者（英） | Abbasi, R.; Auffenberg, J.; BenZvi, S.; Aguilar, J. A.; Andeen, K.; Altmann, D.; Ahlers, M.; Beatty, J. J.; Bell, M.; Baum, V.; Bechet, S.; Ackermann, M.; Adams, J.; Abdou, Y.; Bazo Alba, J. L.; Becker, K.-H; Benabderrahmane, M. L.; Abu-Zayyad, T.; Baker, M.; Bay, R.; Bai, X.; Stamatikos, M.; Barwick, S. W.; Becker, J. K.; Beattie, K. |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 2013-04-01 |
| 言語 | eng |
| 内容記述 | We report on a measurement of the cosmic ray energy spectrum with the IceTop air shower array, thesurface component of the IceCube Neutrino Observatory at the South Pole. The data used in this analysiswere 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 square kilometers.The analysis investigated the energy spectrum from 1 to 100 PeV measured for three different zenithangle ranges between 0 and 46. Because of the isotropy of cosmic rays in this energy range the spectrafrom all zenith angle intervals have to agree. The cosmic-ray energy spectrum was determined under differentassumptions on the primary mass composition. Good agreement of spectra in the three zenithangle ranges was found for the assumption of pure proton and a simple two-component model. Forzenith angles theta less than 30 deg., where the mass dependence is smallest, the knee in the cosmic ray energy spectrumwas observed at about 4 PeV, with a spectral index above the knee of about -3.1. Moreover, an indicationof a flattening of the spectrum above 22 PeV was observed. |
| NASA分類 | Physics of Elementary Particles and Fields; Astrophysics |
| レポートNO | GSFC-E-DAA-TN10580 |
| 権利 | Copyright, Distribution under U.S. Government purpose rights |
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