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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<strong>IceTop</strong> Layout<br />

String 43<br />

String 35<br />

125 m<br />

Tank 35A<br />

~ 25 m<br />

10 m<br />

Tank 35B<br />

6

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<strong>IceTop</strong> Layout String 43 String 35 125 m Tank 35A ~ 25 m 10 m Tank 35B 6

<strong>IceTop</strong> Station 7

Page 1 and 2: Cosmic Ray Detection with IceTop /
Page 3 and 4: IceCube Site Amundsen-Scott Station
Page 5: Digital Optical Module Design Requi
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 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