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首页> 外文期刊>Nuclear Instruments & Methods in Physics Research >A prototype station for ARIANNA: A detector for cosmic neutrinos
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A prototype station for ARIANNA: A detector for cosmic neutrinos

机译:ARIANNA的原型站:宇宙中微子探测器

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The Antarctic Ross Ice Shelf Antenna Neutrino Array (ARIANNA) is a proposed detector for ultra-high energy astrophysical neutrinos. It will detect coherent radio Cherenkov emission from the particle showers produced by neutrinos with energies above about 1017 eV. ARIANNA will be built on the Ross Ice Shelf just off the coast of Antarctica, where it will eventually cover about 900 km2 in surface area. There, the ice-water interface below the shelf reflects radio waves, giving ARIANNA sensitivity to downward-going neutrinos and improving its sensitivity to horizontally incident neutrinos. ARIANNA detector stations each will contain 4-8 antennas, which search for pulses of 50 MHz to 1 GHz radio emission from neutrino interactions. We describe a prototype station for ARIANNA, which was deployed in Moore's Bay on the Ross Ice Shelf in December 2009, discuss the design and deployment, and present some initial figures on performance. The ice shelf thickness was measured to be 572 ± 6 m at the deployment site.
机译:南极罗斯冰架天线中微子阵列(ARIANNA)是一种提议的超高能天体中微子探测器。它将检测中微子产生的粒子阵雨的相干无线电Cherenkov发射,能量超过约1017 eV。 ARIANNA将建在南极海岸附近的罗斯冰架上,最终将覆盖约900平方公里的表面积。在那里,架子下方的冰水界面反射了无线电波,使ARIANNA对向下的中微子敏感,并提高了其对水平入射中微子的敏感度。每个ARIANNA检测站将包含4-8根天线,这些天线会搜索来自中微子相互作用的50 MHz至1 GHz无线电发射脉冲。我们描述了ARIANNA的原型站,该站已于2009年12月部署在罗斯冰架上的摩尔湾中,讨论了设计和部署,并提供了一些性能初步数据。在部署地点测得的冰架厚度为572±6 m。

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