Cosmic Ray Detection with IceTop / IceCube - Villa Olmo

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Cosmic Ray Detection with IceTop / IceCube - Villa Olmo

Cosmic Ray Detection with IceTop / IceCube - Villa Olmo

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Tank Signal Distribution<br />

HG-LG transition<br />

Few DOMs (2-3) <strong>with</strong><br />

low cross-over values<br />

Dynamic range: 4,5 orders of magnitude<br />

~ 20 VEM (~2500 PE)<br />

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Muon Calibration Calibrating the tank signals in Vertical Equivalent Muons HG-LG crossover 10

Tank Signal Distribution HG-LG transition Few DOMs (2-3) <strong>with</strong> low cross-over values Dynamic range: 4,5 orders of magnitude ~ 20 VEM (~2500 PE) 11

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: Local Coincidence and Trigger Tank
Page 13 and 14: Lateral Distribution Energy: ~ 10 P
Page 15 and 16: Fit Procedure and Resolutions Nega
Page 17 and 18: Cosmic Ray Physics with IceCube 17
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