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Test and calibration of large drift tube chambers with cosmic rays

机译:用宇宙射线测试和校准大型漂移管腔

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A cosmic ray measurement facility has been set up at Ludwig-Maximilians-University Munich (LMU) and is used at present to commission and calibrate Monitored Drift Tube (MDT) chambers for the muon spectrometer of the ATLAS experiment. Each of these chambers-produced in collaboration with the Max-Planck-Institut fu/spl uml/r Physik and the Joint Institute for Nuclear Research in Dubna-consists of 432 drift tubes with a diameter of 3 cm, which are arranged in 2/spl times/3 layers, and measures 3.8 m/spl times/2.2 m/spl times/0.5 m. At the LMU site, the MDT chambers are completed, equipped with their final front-end electronics and taken into operation for the first time. The gas leak rate of the chamber is determined and its high voltage stability is tested. The response of all drift tubes and its homogeneity across the chamber is measured in the Cosmic Ray Facility. Two MDT chambers which were precisely mapped with an X-Ray tomograph provide reference tracking for the enclosed third chamber which is to be calibrated. The sense wire positions are determined from a comparison of the drift time measurements with the reference tracks. The geometry of the tested chamber-the grid constants of the drift tubes in a layer, the distances and tilt angles of the layers-can then be derived from these positions. Alignment systems are used to monitor chamber movements at the micrometer level. In the ongoing series commissioning, a rate of one chamber per week has been achieved. The parameters describing the geometry of the MDT chambers are determined with a precision in the 10 /spl mu/m range. The measurements with cosmic muons complement the chamber surveys performed during construction and will provide an important input for the calibration of the entire ATLAS muon spectrometer.
机译:慕尼黑路德维希-马克西米利安斯大学(LMU)已建立了宇宙射线测量设备,目前用于调试和校准ATLAS实验的μ子光谱仪的监测漂移管(MDT)室。这些小室中的每一个都是与Max-Planck-Institut fu / spl uml / r Physik和杜布纳联合核科学研究所合作生产的,由432根直径3 cm的漂移管组成,这些漂移管以2 / spl次/ 3层,尺寸为3.8 m / spl次/2.2 m / spl次/0.5 m。在LMU现场,MDT腔室已经完成,配备了它们的最终前端电子设备,并且首次投入使用。确定腔室的气体泄漏率,并测试其高压稳定性。所有漂移管的响应及其在整个腔室中的均匀性均在Cosmic Ray Facility中测量。用X射线断层扫描仪精确绘制的两个MDT腔室为要校准的封闭第三腔室提供了参考跟踪。根据漂移时间测量值与参考轨迹的比较来确定传感线的位置。然后,可以从这些位置得出被测腔室的几何形状-一层中的漂移管的栅格常数,层的距离和倾斜角。对准系统用于监视千分尺级别的腔室运动。在正在进行的系列调试中,每周达到一个腔室的速度。确定MDT腔室几何形状的参数的精度在10 / spl mu / m范围内确定。宇宙μ子的测量补充了在施工过程中进行的室内测量,将为整个ATLASμ子光谱仪的校准提供重要的输入。

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