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Description
  • We describe the method devised to reconstruct inclined cosmic-ray air showers with zenith angles greater than 60 degrees detected with the surface array of the Pierre Auger Observatory. The measured signals at the ground level are fitted to muon density distributions predicted with atmospheric cascade models to obtain the relative shower size as an overall normalization parameter. The method is evaluated using simulated showers to test its performance. The energy of the cosmic rays is calibrated using a sub-sample of events reconstructed with both the fluorescence and surface array techniques. The reconstruction method described here provides the basis of complementary analyses including an independent measurement of the energy spectrum of ultra-high energy cosmic rays using very inclined events collected by the Pierre Auger Observatory.
  • We describe the method devised to reconstruct inclined cosmic-ray air showers with zenith angles greater than 60 degrees detected with the surface array of the Pierre Auger Observatory. The measured signals at the ground level are fitted to muon density distributions predicted with atmospheric cascade models to obtain the relative shower size as an overall normalization parameter. The method is evaluated using simulated showers to test its performance. The energy of the cosmic rays is calibrated using a sub-sample of events reconstructed with both the fluorescence and surface array techniques. The reconstruction method described here provides the basis of complementary analyses including an independent measurement of the energy spectrum of ultra-high energy cosmic rays using very inclined events collected by the Pierre Auger Observatory. (en)
Title
  • Reconstruction of inclined air showers detected with the pierre Auger Observatory
  • Reconstruction of inclined air showers detected with the pierre Auger Observatory (en)
skos:prefLabel
  • Reconstruction of inclined air showers detected with the pierre Auger Observatory
  • Reconstruction of inclined air showers detected with the pierre Auger Observatory (en)
skos:notation
  • RIV/00216208:11320/14:10283730!RIV15-MSM-11320___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • I, P(7AMB14AR005), P(ED2.1.00/03.0058), P(GA14-17501S), P(LG13007)
http://linked.open...iv/cisloPeriodika
  • 8
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
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http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 41637
http://linked.open...ai/riv/idVysledku
  • RIV/00216208:11320/14:10283730
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • cosmic ray experiments; ultra high energy cosmic rays (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • GB - Spojené království Velké Británie a Severního Irska
http://linked.open...ontrolniKodProRIV
  • [A74DFD3295A0]
http://linked.open...i/riv/nazevZdroje
  • Journal of Cosmology and Astroparticle Physics
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
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http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...v/svazekPeriodika
  • 8
http://linked.open...iv/tvurceVysledku
  • Abreu, P.
  • Aglietta, M.
  • Ahn, E. J.
  • Novotný, Vladimír
  • Ave, M.
  • Ahlers, M.
  • Nosek, Dalibor
  • Allekotte, I.
  • Aublin, J.
  • Aab, A.
  • Al Samarai, I.
  • Albuquerque, I. F. M.
  • Allen, J.
  • Allison, P.
  • Almela, A.
  • Alvarez-Muniz, J.
  • Ambrosio, M.
  • Aminaei, A.
  • Anchordoqui, L.
  • Andringa, S.
  • Aramo, C.
  • Arqueros, F.
  • Asorey, H.
  • Assis, P.
  • Avenier, M.
  • Avila, G.
  • Badescu, A. M.
  • Barber, K. B.
  • Batista, R. Alves
  • Baus, C.
  • Baeuml, J.
  • Alvarez Castillo, J.
http://linked.open...ain/vavai/riv/wos
  • 000341848800019
issn
  • 1475-7516
number of pages
http://bibframe.org/vocab/doi
  • 10.1088/1475-7516/2014/08/019
http://localhost/t...ganizacniJednotka
  • 11320
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