The JEM-EUSO mission: a space observatory to study the origin of Ultra-High Energy Cosmic Rays

M. Bertaina , E. Parizot , JEM-EUSO Collaboration
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引用次数: 8

Abstract

The Extreme Universe Space Observatory (EUSO) onboard the Japanese Experiment Module (JEM-EUSO) of the International Space Station (ISS) is an innovative space-based mission with the aim of detecting Ultra-High Energy Cosmic Rays (UHECRs) from the ISS, by using the Earth's atmosphere as a calorimeter viewed by a fluorescence telescope. An observatory able to produce an arrival direction map with more than several hundreds events above 5 × 1019 eV would give important information on the origin of the UHECRs and identify structures in the sky map that contain information about the source density and/or distribution. This is likely to lead to an understanding of the acceleration mechanisms with a high potential for producing discoveries in astrophysics and/or fundamental physics. The scientific motivations of the mission as well as the current development status of the instrument and its performance are reviewed.

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JEM-EUSO任务:研究超高能量宇宙射线起源的空间天文台
国际空间站(ISS)日本实验舱(JEM-EUSO)上的极端宇宙空间天文台(EUSO)是一项创新的天基任务,旨在通过荧光望远镜观察地球大气层作为量热计,探测来自国际空间站的超高能量宇宙射线(uhecr)。一个天文台如果能够制作一张包含超过数百个5 × 1019 eV以上事件的到达方向图,将提供关于uhecr起源的重要信息,并识别天空图中包含源密度和/或分布信息的结构。这可能会导致对加速机制的理解,这对天体物理学和/或基础物理学的发现具有很高的潜力。回顾了该任务的科学动机以及该仪器的发展现状及其性能。
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Contents Editorial Board Author index Hybrid Simulations of Particle Acceleration at Shocks Using optical lines to study particle acceleration at supernova remnants
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