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Setup of a Drift Tube Muon Tracker and Calibration of Muon ...

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Appendix DComparison <strong>of</strong> CNGS Tracks inBorexino <strong>and</strong> OPERAAs described in Section 5.5, a comparison <strong>of</strong> muons originating from the CNGSbeam that have crossed both the Borexino <strong>and</strong> the OPERA detector has been done.This section summarizes the necessary coordinate transformations for this task.BorexinoOPERAz bxy opx opx bxy bxCNGSz opFigure D.1: Relative coordinate systems <strong>of</strong> Borexino <strong>and</strong> OPERABoth the Borexino <strong>and</strong> OPERA coordinate systems are shown in Fig. D.1. Sincethe muon tracks are to be compared within Borexino, the Borexino coordinate systemis taken as the reference system. Assume, the <strong>of</strong>fset between both detectors is∆x, ∆y <strong>and</strong> ∆z in the Borexino system, the transformation is trivial:x = x bx = ∆x − z op ,y = y bx = ∆y − x op ,z = z bx = ∆z + y op .For each muon track, OPERA provides five parameters: one slope <strong>and</strong> the accordingz-intercept for each the x −z <strong>and</strong> the y −z plane: s x , x op,0 , s y <strong>and</strong> y op,0 respectivelyas well as the inverse momentum 1 p . The z-intercept is not given for z op = 0, instead107

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