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Analyses of cosmic ray induced-neutron based on spectrometers operated simultaneously at mid-latitude and Antarctica high-altitude stations during quiet solar activity

机译:基于光谱仪的宇宙射线感应中子在安静的太阳活动期间同时在中纬度和南极高空站工作的分析

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In this paper are described a new neutron spectrometer which operate in the Concordia station (Antarctica, Dome C) since December 2015. This instrument complements a network including neutron spectrometers operating in the Pic-du-Midi and the Pico dos Dias. Thus, this work present an analysis of cosmic ray induced-neutron based on spectrometers operated simultaneously in the Pic-du-Midi and the Concordia stations during a quiet solar activity. The both high station platforms allow for investigating the long period dynamics to analyze the spectral variation and effects of local and seasonal changes, but also the short term dynamics during solar flare events. A first part is devoted to analyze the count rates, the spectrum and the neutron fluxes, implying cross-comparisons between data obtained in the both stations. In a second part, measurements analyses were reinforced by modeling based on simulations of atmospheric cascades according to primary spectra which only depend on the solar modulation potential. (C) 2016 Elsevier B.V. All rights reserved.
机译:本文介绍了一种自2015年12月起在Concordia站(南极洲,圆顶C)运行的新型中子光谱仪。该仪器对包括在Pic-du-Midi和Pico dos Dias中运行的中子光谱仪的网络进行了补充。因此,这项工作提出了一种基于光谱仪的宇宙射线感应中子的分析方法,该光谱仪在安静的太阳活动期间同时在Pic-du-Midi和Concordia站中运行。这两个高台站平台都允许调查长期动态,以分析光谱变化和局部和季节性变化的影响,以及太阳耀斑事件期间的短期动态。第一部分专门分析计数率,频谱和中子通量,这意味着在两个站获得的数据之间存在交叉比较。在第二部分中,通过基于主要级光谱的大气级联模拟建立模型,从而加强了测量分析,该光谱仅取决于太阳调制电势。 (C)2016 Elsevier B.V.保留所有权利。

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