A balloon-borne measurement of high latitude atmospheric neutrons using a licaf neutron detector

M. Kole, Y. Fukazawa, K. Fukuda, S. Ishizu, M. Jackson, T. Kamae, N. Kawaguchi, T. Kawano, M. Kiss, E. Moretti, M. Salinas, M. Pearce, S. Rydstrom, H. Takahashi, T. Yanagida
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Abstract

PoGOLino is a scintillator-based neutron detector. Its main purpose is to provide data on the neutron flux in the upper stratosphere at high latitudes at thermal and non-thermal energies for the PoGOLite instrument. PoGOLite is a balloon borne hard X-ray polarimeter for which the main source of background stems from high energy neutrons. No measurements of the neutron environment for the planned flight latitude and altitude exist. Furthermore this neutron environment changes with altitude, latitude and solar activity, three variables that will vary throughout the PoGOLite flight. PoGOLino was developed to study the neutron environment and the influences from these three variables upon it. PoGOLino consists of two Europium doped Lithium Calcium Aluminium Fluoride (Eu:LiCAF) scintillators, each of which is sandwiched between 2 Bismuth Germanium Oxide (BGO) scintillating crystals, which serve to veto signals produced by gamma-rays and charged particles. This allows the neutron flux to be measured even in high radiation environments. Measurements of neutrons in two separate energy bands are achieved by placing one LiCAF detector inside a moderating polyethylene shield while the second detector remains unshielded. The PoGOLino instrument was launched on March 20th 2013 from the Esrange Space Center in Northern Sweden to an altitude of 30.9 km. A description of the detector design and read-out system is presented. A detailed set of simulations of the atmospheric neutron environment performed using both PLANETOCOSMICS and Geant4 will also be described. The comparison of the neutron flux measured during flight to predictions based on these simulations will be presented and the consequences for the PoGOLite background will be discussed.
用licaf中子探测器在气球上测量高纬度大气中子
PoGOLino是一种基于闪烁体的中子探测器。它的主要目的是为PoGOLite仪器提供高纬度平流层上层热能和非热能中子通量的数据。PoGOLite是一种气球携带的硬x射线偏振计,其主要背景源来自高能中子。没有对计划飞行纬度和高度的中子环境的测量。此外,中子环境随着高度、纬度和太阳活动的变化而变化,这三个变量将在整个PoGOLite飞行过程中发生变化。开发PoGOLino是为了研究中子环境以及这三个变量对它的影响。PoGOLino由两个铕掺杂锂钙铝氟化(Eu:LiCAF)闪烁体组成,每个闪烁体夹在2个铋锗氧化物(BGO)闪烁晶体之间,用于否决伽马射线和带电粒子产生的信号。这使得即使在高辐射环境中也可以测量中子通量。通过将一个LiCAF探测器放置在减速聚乙烯屏蔽层内,而另一个探测器保持未屏蔽状态,可以实现对两个不同能带的中子的测量。PoGOLino仪器于2013年3月20日从瑞典北部的Esrange航天中心发射到30.9公里的高度。介绍了探测器的设计和读出系统。还将描述使用PLANETOCOSMICS和Geant4进行的一组详细的大气中子环境模拟。将介绍飞行期间测量的中子通量与基于这些模拟的预测的比较,并讨论对PoGOLite背景的影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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