Cosmic Ray Detection with IceTop / IceCube - Villa Olmo

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Energy Range & Physics Goals Energy Threshold (# Stations ≥ 5) 90% 3.2 PeV (Iron) 1.8 PeV (Proton) IceTop Threshold < 1 PeV for # Stations ≥ 3 (less accurate) Main Physics Motivations: Cosmic ray energy spectrum between 1 PeV and 1 EeV Cosmic ray composition (Search for transition between galactic and extra-galactic cosmic rays) Test of hadronic interaction models 16
Cosmic Ray Physics with IceCube 17
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: Fit Procedure and Resolutions Nega
Page 19 and 20: IceTop Energy Reconstruction Proton
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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