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Setup of a Drift Tube Muon Trackera
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AbstractIn this work the setup and
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3.5.5 Pattern Recognition . . . . .
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viii
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essential for vetoing these events.
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Chapter 2NeutrinosThe standard mode
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However, it did not yet deliver an
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Table 2.1: Neutrino oscillation par
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this assumption, the Standard Solar
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Figure 2.1: Neutrino flux at Earth
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asymmetry between neutrino and anti
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Figure 2.3: Expected ¯ν e energy
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Nb neutrino/fission-11010-2Neutrino
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108−dE/dx (MeV g −1 cm 2 )65432
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Figure 3.3: Setup of the muon track
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zyxModule b.0Module a.0Module b.1Mo
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Figure 3.6: Display of the slow con
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plastic scintillators. To avoid all
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N hitsHitmap Plane 06000h_hitmap0En
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Table 3.4: Data structure for calib
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TDC SpectrumN/[2 Channels]1000800H_
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Table 3.5: List of variables calcul
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with ∆⃗q = ⃗q n − ⃗q n−
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N [a.u.]∆ α (x)2200020000da0Entr
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d[mm]Reco Drift Distances201816H_RE
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N [a.u.]Real DataReal data0.06MCh1E
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χ 2N [a.u.]Probability103×10hc2p0
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N [a.u]Residuals20001800h0Entries 3
- Page 60 and 61: Counts/(10 keV × day × 100 tons)1
- Page 62 and 63: 4.1.3 Čerenkov LightČerenkov dete
- Page 64 and 65: 4.2 The Borexino DetectorThe Borexi
- Page 66 and 67: muons, is reduced by going deep und
- Page 68 and 69: (typically below 50 cm), the locati
- Page 70 and 71: 510Counts/(10 keV x day x 100 tons)
- Page 72 and 73: counts/days*4 hitsDay (Red) and Nig
- Page 74 and 75: eeSurvival probability for ν e, P0
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- Page 78 and 79: P C P DSCINT C SCINT DySCINT BSCINT
- Page 80 and 81: Figure 5.2: The CMT setup on top of
- Page 82 and 83: Angular AcceptanceAngular Acceptanc
- Page 84 and 85: Comparison nhits=3 vs nhits=4N [a.u
- Page 86 and 87: Table 5.3: Overview of all muon run
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- Page 90 and 91: Reco Hits in Scintillatory [mm]1000
- Page 92 and 93: PMTPMTScintillatorPMTPMTFigure 5.16
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- Page 96 and 97: Zenith Angle CMT and BX-GL Tracks h
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- Page 100 and 101: Distance d between CMT and BX-GL Tr
- Page 102 and 103: Angular difference αN [arbitrary u
- Page 104 and 105: [m]z bxTrack Position in BX x=0 Pla
- Page 106 and 107: N [arbitrary units]∆y all data200
- Page 108 and 109: To determine the Borexino tracking
- Page 112 and 113: espectively. The channel numbers ar
- Page 114 and 115: xyϕϕ ′βx ′µFigure C.2: Rela
- Page 116 and 117: the z-coordinate z op,0 of the firs
- Page 118 and 119: xyEvent: 470, Entry: 470, Time Tue
- Page 120 and 121: [14] Ch. Kraus et al. Final Results
- Page 122 and 123: [49] T. Araki et al. Experimental i
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- Page 126: Jan Lenkeit und Björn Wonsak sowie