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Auger ACCESS - Remote monitoring and controlling the auger experiment

机译:螺旋钻访问-远程监控螺旋钻实验

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Ultra high energy cosmic rays are the most energetic of subatomic particles in the universe. They are measured to have energies of up to 1020 eV and occur at a rate of about once per square kilometer and century. To increase the probability of detecting one of these events, a huge detector covering a large area is needed. During the last decades, the Pierre Auger collaboration [1] build up an observatory covering 3000 square kilometers of the Pampa Amarilla close to Malargüe for this purpose. Until now, the Auger experiment was controlled exclusively via the local network for security and performance reasons. As local operation is associated with high travel costs, the Auger ACCESS project was started in 2005 to find a secure, operable and sustainable solution for remote control and monitoring. This paper descibes the implemented solution, including Grid technologies for secured access and infrastructure virtualization for building up a fully featured testing environment for the Pierre Auger Observatory. Finally, measurement results are presented together with a specification of a remote control room and associated benefits for the future of the Auger experiment.
机译:超高能宇宙射线是宇宙中最活跃的亚原子粒子。据测量,它们的能量高达10 20 eV,并且每平方公里和每世纪出现一次。为了增加检测这些事件之一的可能性,需要覆盖大面积的巨大检测器。在过去的几十年中,皮埃尔·奥格(Pierre Auger)的合作[1]为此目的在天文台附近的马拉加(Malargüe)上建立了3000平方公里的潘帕阿马里拉(Pampa Amarilla)。到目前为止,出于安全和性能方面的考虑,Auger实验仅通过本地网络进行控制。由于本地运营与高昂的旅行成本相关联,因此,Auger ACCESS项目于2005年启动,旨在寻找一种安全,可操作且可持续的远程控制和监视解决方案。本文介绍了已实现的解决方案,包括用于安全访问的网格技术和用于为Pierre Auger天文台建立功能齐全的测试环境的基础架构虚拟化。最后,将介绍测量结果以及远程控制室的规格以及对俄格实验未来的益处。

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