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Absolute energy calibration of the Telescope Array fluorescence detector with an electron linear accelerator

机译:带有电子线性加速器的望远镜阵列荧光探测器的绝对能量校准

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The Electron Light Source(ELS) is a new light source for the absolute energy calibration of cosmic ray Fluorescence Detector(FD) telescopes. The ELS is a compact electron linear accelerator with a typical output of 109 electrons per pulse at 40 MeV. We fire the electron beam vertically into the air 100 m in front of the telescope. The electron beam excites the gases of the atmosphere in the same way as the charged particles of the cosmic ray induced extensive air shower. The gases give off the same light with the same wavelength dependence. The light passes through a small amount of atmosphere and is collected by the same mirror and camera with their wavelength dependence. In this way we can use the electron beam from ELS to make an end-to-end calibration of the telescope. In September 2010, we began operation of the ELS and the FD telescopes observed the fluorescence photons from the air shower which was generated by the electron beam. In this article, we will reort the status of analysis of the absolute energy calibration with data which was taken in September 2010, and beam monitor study in November 2011.b For the full authorlist see Appendix “Collaborations” in this volume
机译:电子光源(ELS)是用于宇宙射线荧光检测器(FD)望远镜的绝对能量校准的新光源。 ELS是一种紧凑的电子线性加速器,在40 MeV的电压下,每个脉冲的典型输出为109个电子。我们将电子束垂直发射到望远镜前方100 m的空气中。电子束以与宇宙射线引起的大范围空气喷淋的带电粒子相同的方式激发大气中的气体。气体以相同的波长依赖性发出相同的光。光穿过少量的大气,并由相同的镜子和照相机以其波长依赖性收集。这样,我们可以使用ELS的电子束对望远镜进行端到端校准。在2010年9月,我们开始运行ELS,而FD望远镜观察到了由电子束产生的空气喷淋中的荧光光子。在本文中,我们将使用2010年9月进行的数据和2011年11月进行的光束监控器研究重新定义绝对能量校准的分析状态。b有关完整的作者列表,请参阅本卷的附录“合作”。

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