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首页> 外文期刊>Nuclear Instruments & Methods in Physics Research >Tethered balloons for radio detection of ultra high energy cosmic neutrinos in Antarctica
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Tethered balloons for radio detection of ultra high energy cosmic neutrinos in Antarctica

机译:用于南极超高能宇宙中微子的无线电探测的系留气球

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We present a brief overview of experimental efforts in Antarctica to search for radio pulses from electron-hadron cascades produced by cosmic ultrahigh-energy neutrinos in Antarctic ice. Thus far, the essential features (energy thresholds, effective recording volumes, etc.) of Antarctic neutrino radio experiments can be classified according to the deployment scheme employed: either (1) on the surface of the glacier-RAMAND-type, (2) in holes in the ice at depths of several hundred meters-RICE-type or (3) on board of a stratospheric balloon at an altitude of 40 km-ANITA-type. We herein propose an alternative possibility, namely to use tethered balloons for placing the radio antennas at modest (compared to ANITA) altitudes above the ice surface (1-2 km). This configuration of antennas will reduce (as compared to ANITA) the energy threshold for detection of neutrinos and increase the observation time.
机译:我们简要概述了南极洲从南极冰中的宇宙超高能中微子产生的电子-强子级联中搜索无线电脉冲的实验工作。到目前为止,可以根据所采用的部署方案对南极中微子无线电实验的基本特征(能量阈值,有效记录量等)进行分类:(1)在冰川-RAMAND型表面上,(2)在数百米深的冰洞中-米型-或(3)在平流层气球上高度40公里-ANITA型。我们在此提出了一种替代的可能性,即使用系留气球将无线电天线放置在冰面(1-2公里)上方适度(与ANITA相比)的高度上。天线的这种配置将降低(与ANITA相比)检测中微子的能量阈值并增加观察时间。

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