- Page 1 and 2: Setup of a Drift Tube Muon Trackera
- Page 3: AbstractIn this work the setup and
- Page 6 and 7: 3.5.5 Pattern Recognition . . . . .
- Page 10 and 11: essential for vetoing these events.
- Page 13 and 14: Chapter 2NeutrinosThe standard mode
- Page 15 and 16: However, it did not yet deliver an
- Page 17 and 18: Table 2.1: Neutrino oscillation par
- Page 19 and 20: this assumption, the Standard Solar
- Page 21 and 22: Figure 2.1: Neutrino flux at Earth
- Page 23 and 24: asymmetry between neutrino and anti
- Page 25 and 26: Figure 2.3: Expected ¯ν e energy
- Page 27: Nb neutrino/fission-11010-2Neutrino
- Page 30 and 31: 108−dE/dx (MeV g −1 cm 2 )65432
- Page 32 and 33: Figure 3.3: Setup of the muon track
- Page 34 and 35: zyxModule b.0Module a.0Module b.1Mo
- Page 36 and 37: Figure 3.6: Display of the slow con
- Page 38 and 39: plastic scintillators. To avoid all
- Page 40 and 41: N hitsHitmap Plane 06000h_hitmap0En
- Page 42 and 43: Table 3.4: Data structure for calib
- Page 44 and 45: TDC SpectrumN/[2 Channels]1000800H_
- Page 46 and 47: Table 3.5: List of variables calcul
- Page 48 and 49: with ∆⃗q = ⃗q n − ⃗q n−
- Page 50 and 51: N [a.u.]∆ α (x)2200020000da0Entr
- Page 52 and 53: d[mm]Reco Drift Distances201816H_RE
- Page 54 and 55: N [a.u.]Real DataReal data0.06MCh1E
- Page 56 and 57: χ 2N [a.u.]Probability103×10hc2p0
- Page 58 and 59:
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
- Page 76 and 77:
the CMT to the Borexino tracking, t
- 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
- Page 88 and 89:
N/dayAll Triggers vs Time12000h_tim
- Page 90 and 91:
Reco Hits in Scintillatory [mm]1000
- Page 92 and 93:
PMTPMTScintillatorPMTPMTFigure 5.16
- Page 94 and 95:
the CMT data file and the Borexino
- Page 96 and 97:
Zenith Angle CMT and BX-GL Tracks h
- Page 98 and 99:
Lateral x Resolution CMT - IDhlatx_
- 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 110 and 111:
Table A.1: Variables that can be se
- 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
- Page 124 and 125:
116
- Page 126:
Jan Lenkeit und Björn Wonsak sowie