Cosmic Ray Detection with IceTop / IceCube - Villa Olmo

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Air Shower Observables Primary energy: 1 – 100 PeV Electromagnetic particles O(10) – O(100) MeV IceTop Low energy muons O(1) – O(10) GeV High energy muons (> 500 GeV) # Muons: O(10) - (1000) Data IceCube Muon Estimator Iron Protons IceTop Energy 18
IceTop Energy Reconstruction Protons Differential Flux Spectra in S 125 Energy conversion function: Depend on zenith band and primary composition → Reconstruction of primary energy spectra depends on a priori composition assumption 19
Page 1 and 2: Cosmic Ray Detection with IceTop /
Page 3 and 4: IceCube Site Amundsen-Scott Station
Page 5 and 6: Digital Optical Module Design Requi
Page 7 and 8: IceTop Station 7
Page 9 and 10: Local Coincidence and Trigger Tank
Page 11 and 12: Tank Signal Distribution HG-LG tran
Page 13 and 14: Lateral Distribution Energy: ~ 10 P
Page 15 and 16: Fit Procedure and Resolutions Nega
Page 17: Cosmic Ray Physics with IceCube 17
Page 21 and 22: Response Matrix One matrix for ea
Page 23 and 24: Muon Identification with IceTop On
Page 25 and 26: IceTop−IceCube Coincident Events
Page 27 and 28: Cosmic Ray Composition Proton fract
Page 29: Summary 90% of IceCube are install

Cosmic Ray Detection with IceTop / IceCube - Villa Olmo

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