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首页> 外文期刊>Physics of atomic nuclei >Employing cherenkov radiation and fluorescence light in calibrating the energy of giant air showers
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Employing cherenkov radiation and fluorescence light in calibrating the energy of giant air showers

机译:利用切伦科夫辐射和荧光来校准巨型淋浴器的能量

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摘要

A classic procedure for estimating the energy of giant air showers in terms of the parameter s(600) (density of energy deposition in a scintillator at a distance of 600 m from the shower axis) is analyzed on the basis of the model of quark-gluon strings. A simulation of the signal s(600) by means of the CORSIKA code leads to estimates of energy that are approximately 1.6 times lower than those adopted at the Yakutsk array. Estimates of energy on the basis of Cherenkov radiation agree with experimental data within the errors. Calculations of the distributions of energy deposited in the atmosphere indicate that more than 20% of this energy can be deposited at distances in excess of 100 m from the shower axis.
机译:在夸克模型的基础上,分析了根据参数s(600)(闪烁体在距淋浴轴600 m的距离内的能量沉积密度)估算巨型风淋能量的经典程序。胶子弦。通过CORSIKA代码对信号s(600)进行仿真,得出的能量估算值比雅库茨克阵列采用的能量估算值低约1.6倍。在契伦科夫辐射的基础上估算的能量与误差范围内的实验数据吻合。对沉积在大气中的能量分布的计算表明,该能量的20%以上可以在距淋浴轴100 m以上的距离处沉积。

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