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Radar Detection of UHECR Air Showers at the Telescope Array

机译:望远镜阵列中UHECR风淋的雷达检测

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Progress in the field of high-energy cosmic rays is currently limited by the rarity of the most interesting raysstriking the Earth. Indeed, the continuation of the field beyond the current generation of observatories may becomefinancially and practically impossible if new ways are not found to achieve remote coverage over large portions of theEarth's surface. We describe the development of an observatory based on such a new technique: the remote sensingvia bistatic radar technology of cosmic ray induced extensive air showers. We build on pilot studies performed byMARIACHI which have demonstrated that air shower radar echoes are detectable, the opportunity afforded by the locationof the Northern Hemisphere's largest "conventional" cosmic ray observatory (The Telescope Array) in radio-quiet westernUtah, and the donation of analog television transmission equipment to this effort by a local television station. We willpresent a description of the transmitter and receiver stations, as well as the most recent observational data from the bistaticradar observatory.
机译:当前,高能宇宙射线领域的进展受到最有趣的撞击地球的罕见性的限制。的确,如果找不到新的方法可以在大范围的地球表面实现远程覆盖,那么在当今的天文台之外,要继续扩展该领域在财务上和实际上是不可能的。我们描述了基于这样一种新技术的天文台的发展:通过宇宙射线引起的大范围风淋的双基地雷达遥感技术。我们以MARIACHI进行的试点研究为基础,这些研究表明,可以检测到空气淋浴雷达回波,北半球最大的“常规”宇宙射线天文台(望远镜阵列)位于安静的犹他州西部,并提供了类似物,从而提供了机会电视传输设备由本地电视台为此付出努力。我们将对发射器和接收器站以及双基地雷达天文台的最新观测数据进行描述。

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