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024 7 _ |a 10.3204/DESY-THESIS-2015-048
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037 _ _ |a PUBDB-2015-05197
041 _ _ |a English
088 1 _ |a DESY-THESIS-2015-048
088 _ _ |a DESY-THESIS-2015-048
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100 1 _ |a Lenkeit, Jan
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245 _ _ |a Timing Calibration of the Trigger System for the Drift Tube Detector of the OPERA Neutrino Oscillation Experiment
|f 2007-10-04 - 2015-11-11
260 _ _ |a Hamburg
|c 2015
|b Verlag Deutsches Elektronen-Synchrotron
300 _ _ |a 160
336 7 _ |a Output Types/Dissertation
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336 7 _ |a DISSERTATION
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336 7 _ |a PHDTHESIS
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336 7 _ |a Thesis
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336 7 _ |a Report
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336 7 _ |a doctoralThesis
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502 _ _ |a Universität Hamburg, Diss., 2015
|c Universität Hamburg
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520 _ _ |a The OPERA experiment searches for muon neutrino to tau neutrino oscillations in an almost pure muon neutrino beam. The goal is to observe the oscillations in appearance mode by using a large-scale lead/emulsion target to resolve individual tau neutrino interactions. Magnetic spectrometers measure the charge and momentum of beam induced muons leaving the target sections. The Precision Tracker, a drift tube detector consisting of almost 10000 drift tubes, provides the tracking information inside the spectrometers. The coordinate measurement in the drift tubes is derived from a time measurement relative to an external trigger signal. In order to reach the required momentum resolution of less than 25 % for particle momenta up to 25 GeV, the uncertainty on the trigger timing must not exceed a value of 5 ns. In this thesis, a procedure for the timing calibration of the trigger system is presented. A step-by-step calibration of the corresponding signal paths is described. Applying all calibration results, a spatial resolution of 255 µm is achieved for the Precision Tracker, meeting the specified requirements. Furthermore, a method using the calibrated trigger system for performing time of flight measurements with atmospheric muons is developed. The average error on the measured flight times is +-4.5 ns.
536 _ _ |a 613 - Matter and Radiation from the Universe (POF3-613)
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650 _ 7 |x Diss.
693 _ _ |a CNGS
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