Pierre Auger天文台北部的硬实时无线通信

R. Kieckhafer
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引用次数: 7

摘要

皮埃尔·奥格宇宙射线天文台使用大量的地面探测器来探测超高能量宇宙射线到达时产生的二次粒子阵雨。运行中的俄歇南站点使用基于塔的无线网络在站点和天文台校园之间进行通信。一个更大的俄歇北阵列的计划需要一个类似的系统。然而,各种因素使得直接站塔路由在俄歇北部不可行。因此,它将采用一种新的范例,即硬实时嵌入式网络无线架构(WAHREN),专为在硬实时截止日期下通过固定网络进行高可靠的消息传递而设计。本文描述了WAHREN的拓扑结构和协议,以及实时性能评估、形式化验证、试验台运行和马尔可夫可靠性建模。讨论了系统硬件开发和现场研发阵列的现状。
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Hard Real-Time wireless communication in the northern Pierre Auger Observatory
The Pierre Auger Cosmic Ray Observatory employs a large array of Surface Detector stations to detect the secondary particle showers generated by the arrivals of Ultra High Energy Cosmic Rays. The operational Auger South site uses a tower-based wireless network for communication between the stations and observatory campus. Plans for a larger Auger North array call for a similar system. However, a variety of factors have rendered direct station-to-tower routing infeasible in Auger North. Thus, it will employ a new paradigm, the Wireless Architecture for Hard Real-Time Embedded Networks (WAHREN) designed specifically for highly reliable message delivery over a fixed network, under hard real-time deadlines. This paper describes the WAHREN topology and protocols, as well as real-time performance evaluation, formal verification, testbed operation, and Markov reliability modeling. The status of system hardware development and an on-site Research and Development Array are also discussed.
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