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Cosmic ray elemental composition study by using an artificial neural network based on the measurement of the lateral particle density distribution in showers induced by primaries in the 30-10000 TeV energy region

机译:宇宙射线元素组成研究通过使用人工神经网络在30-10000 Tev能量区域中初探的淋迹横向粒子密度分布的测量

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The mass composition plays an important role for understanding the origin of the UHE cosmic rays. Thecomposition in the energy region at and beyond the knee is important because it is related to the sites of cosmic rayproductions and accelerations. In order to perform the composition measurement, an artificial neural network (ANN)has been implemented, it is based on a set of composition estimators obtained by a detailed study of the lateral particledensity distribution. Showers induced by protons, He nuclei, CNO group and iron nuclei have been generated in theenergy region (30-10000) TeV, the lateral particle density distribution was estimated. In this paper the estimators arepresented, the performance of the mass discrimination is discussed.
机译:群众成分对理解UHE宇宙射线的起源起着重要作用。在膝盖和超出膝盖的能量区域中的分解是重要的,因为它与宇宙射线产品和加速度的网站有关。为了执行组合测量,已经实现了人工神经网络(ANN),它基于通过详细研究横向分布而获得的一组组合估计。由质子诱导的淋浴,HE核,CNO组和铁核在TEAENERGY地区(30-10000)TEV中产生,估计横向粒子密度分布。在本文中,估计人士讨论了,讨论了大规模歧视的性能。

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