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Refined Lateral Energy Correction Functions for the KASCADE-Grande Experiment Based on Geant4 Simulations

机译:基于GEANT4模拟的KASCADE-GRANDE实验精细横向能量校正功能

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In previous studies of KASCADE-Grande data, a Monte Carlo simulation code based on the GEANT3 program has been developed to describe the energy deposited by EAS particles in the detector stations. In an attempt to decrease the simulation time and ensure compatibility with the geometry description in standard KASCADE-Grande analysis software, several structural elements have been neglected in the implementation of the Grande station geometry. To improve the agreement between experimental and simulated data, a more accurate simulation of the response of the KASCADE-Grande detector is necessary. A new simulation code has been developed based on the GEANT4 program, including a realistic geometry of the detector station with structural elements that have not been considered in previous studies. The new code is used to study the influence of a realistic detector geometry on the energy deposited in the Grande detector stations by particles from EAS events simulated by CORSIKA. Lateral Energy Correction Functions are determined and compared with previous results based on GEANT3.
机译:在先前的Kascade-Grande数据的研究中,已经开发了一种基于Geant3程序的蒙特卡罗模拟代码来描述探测器站中的EAS粒子沉积的能量。为了试图减少模拟时间并确保与标准KASCADE-GRANDE分析软件中的几何描述兼容,在德国几何形状的实施中已经忽略了几种结构元素。为了改善实验和模拟数据之间的协议,需要更准确地模拟KASCADE-GRANDE探测器的响应。基于GEANT4程序开发了一种新的仿真代码,包括具有在先前研究中未考虑的结构元素的探测器站的现实几何形状。新代码用于研究现实检测器几何形状对由Corsika模拟的EAS事件的粒子在Grande探测器站中沉积的能量的影响。确定并将横向能量校正功能与基于GEANT3的先前结果进行了比较。

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