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    • Developments and Results in the Context of the JEM-EUSO Program Obtained with the ESAF Simulation and Analysis Framework

    The European Physical Journal C（2023）

    Nihon University | University of Alabama in Huntsville | Université de Paris | City University of New York (CUNY) | INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo | Istituto Nazionale di Fisica Nucleare-Sezione di Torino | University of Tübingen | Istituto Nazionale di Fisica Nucleare-Sezione di Bari | Lomonosov Moscow State University | NASA Marshall Space Flight Center | Karlsruhe Institute of Technology (KIT) | RIKEN | Institute of Experimental Physics | KTH Royal Institute of Technology | University of Chicago | Istituto Nazionale di Fisica Nucleare-Sezione di Roma Tor Vergata | Istituto Nazionale di Fisica Nucleare-Sezione di Napoli | Max Planck Institute for Physics | Istituto Nazionale di Fisica Nucleare-Sezione di Catania | Palacký University | University of California | Università degli Studi di Torino | Pennsylvania State University | Omega | Universidad de Alcalá (UAH) | Università di Napoli Federico II | Colorado School of Mines | University of Tokyo | Konan University | ECAP | NASA Goddard Space Flight Center | Institute of Physics of the Czech Academy of Sciences | Università di Roma Tor Vergata | National Centre for Nuclear Research | University of Utah | Univ. Constantine I | National Astronomical Observatory | University of Iowa | Joint Institute for Nuclear Research | Sungkyunkwan University | University of Warsaw | Istituto Nazionale di Fisica Nucleare-Laboratori Nazionali di Frascati | Space Regatta Consortium | Hokkaido University | Shinshu University | ISDC Data Centre for Astrophysics | Centre for Development of Advanced Technologies (CDTA) | IRAP | Fairfield University

    Cited 3|Views30
    Abstract
    JEM-EUSO is an international program for the development of space-based Ultra-High Energy Cosmic Ray observatories. The program consists of a series of missions which are either under development or in the data analysis phase. All instruments are based on a wide-field-of-view telescope, which operates in the near-UV range, designed to detect the fluorescence light emitted by extensive air showers in the atmosphere. We describe the simulation software ESAF in the framework of the JEM-EUSO program and explain the physical assumptions used. We present here the implementation of the JEM-EUSO, POEMMA, K-EUSO, TUS, Mini-EUSO, EUSO-SPB1 and EUSO-TA configurations in ESAF. For the first time ESAF simulation outputs are compared with experimental data.
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    【要点】：本文介绍了JEM-EUSO项目中的ESAF模拟和分析框架的开发成果，包括多种观测配置的模拟实现，并首次将ESAF模拟结果与实验数据进行对比。
    

    【方法】：文中详细描述了ESAF模拟软件的物理假设和实现过程，以及如何模拟JEM-EUSO项目下的不同观测配置。
    

    【实验】：实验使用ESAF模拟框架，对JEM-EUSO、POEMMA、K-EUSO、TUS、Mini-EUSO、EUSO-SPB1和EUSO-TA等配置进行模拟，并将模拟结果与实际观测数据进行了对比。
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