Cosmic Ray Detection with IceTop / IceCube - Villa Olmo

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<strong>IceTop</strong> Station LG DOM HG DOM Perlite 0.9 m 0.57 m ICE diffuse reflective coating 1.86 m 8
Local Coincidence and Trigger Tank A Tank B High Gain: ► High Voltage: ~ 1250 V ► Gain: 5E6 61 notifies 63 ► Disc. Thr.: ~ 20 PE ► Disc. Rate: ~ 1600 Hz ► LC-Rate: ~ 20 Hz Low Gain: 62 64 ► High Voltage: ~ 750 V ► Gain: 1E5 ► Disc. Thr.: ~ 200 PE ► Disc. Rate: 30-100 Hz LC-Window: ±1µs ► LC-Rate: ~ 7 Hz Simple Majority Trigger condition: 6 LC-hits (at least 2 stations) <strong>with</strong>in 5 µs (readout window: ±10 µs, IC59-Rate: 22 Hz) 9
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: IceTop Station 7
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

Cosmic Ray Detection with IceTop / IceCube - Villa Olmo

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