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Terrestrial Gamma-ray Flashes monitor demonstrator on CubeSat

机译:CubeSat上的地面伽玛射线闪烁监视器演示器

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摘要

The CubeSat mission with the demonstrator of miniaturized X-ray telescope is presented. The paper presents one of the mission objectives of using the instrument for remote sensing of the Terrestrial Gamma-ray Flashes (TGFs). TGFs are intense sources of gamma-rays associated with lightning bolt activity and tropical thunderstorms. The measurement of TGFs exists and was measured by sounding rockets, high altitude balloons or several satellite missions. Past satellite missions were equipped with different detectors working from 10 keV up to 10 MeV. The RHESSI mission spectrum measurement of TGFs shows the maximum counts per second around 75 keV. The used detectors were in general big in volume and cannot be utilized by the CubeSat mission. The presented CubeSat is equipped with miniaturized X-ray telescope using the Timepix non-cooled pixel detector. The detector works between 3 and 60 keV in counting mode (dosimetry) or in spectrum mode with resolution 5 keV. The wide-field X-ray "Lobster-eye" optics/collimator (depending on energy) is used with a view angle of 3 degrees for the source location definition. The UV detectors with FOV 30 degrees and 1.5 degrees are added parallel with the optic as a part of the telescope. The telescope is equipped with software distinguishing between the photons and other particles. Using this software the TGF's detection is possible also in the field of South Atlantic anomaly. For the total ionization dose, the additional detector is used based on Silicone (12-60 keV) and CdTe (20 keV - 1 MeV). The presented instruments are the demonstrators suitable also for the astrophysical, sun and moon observation. The paper shows the details of TGF's observation modes, detectors details, data processing and handling system and mission. The CubeSat launch is planned to summer 2016.
机译:介绍了带有微型X射线望远镜演示器的CubeSat任务。本文介绍了使用该仪器遥感地面伽玛射线闪光(TGF)的任务目标之一。 TGF是与雷电活动和热带雷暴有关的伽玛射线的强烈来源。存在TGF的测量,并通过探测火箭,高空气球或几次卫星飞行来测量。过去的卫星飞行任务都配备了从10 keV到10 MeV的不同探测器。 TGF的RHESSI任务频谱测量显示,每秒最大计数约为75 keV。所使用的探测器通常体积较大,不能被CubeSat任务使用。展示的CubeSat使用Timepix非冷却像素检测器配备了微型X射线望远镜。该检测器在计数模式(剂量测定)或光谱模式下以3 keV到60 keV的分辨率工作。宽视野X射线“龙虾眼”光学元件/准直仪(取决于能量)用于确定源位置的3度视角。将FOV为30度和1.5度的紫外线检测器与光学元件平行添加,作为望远镜的一部分。望远镜配备了可区分光子和其他粒子的软件。使用该软件,TGF的检测还可以在南大西洋异常领域进行。对于总电离剂量,使用基于有机硅(12-60 keV)和CdTe(20 keV-1 MeV)的附加检测器。所展示的仪器是同样适用于天体观测,日月观测的演示器。该文件显示了TGF的观测模式的详细信息,探测器的详细信息,数据处理和处理系统以及任务。 CubeSat计划于2016年夏季推出。

著录项

  • 来源
    《Cubesats and nanoisats for remote sensing》|2016年|99780D.1-99780D.7|共7页
  • 会议地点 San Diego CA(US)
  • 作者单位

    Aerospace Research and Test Establishment, Prague, Czech Republic;

    Rigaku Innovative Technologies Europe, Prague, Czech Republic,Czech Technical University, Prague, Czech Republic;

    Rigaku Innovative Technologies Europe, Prague, Czech Republic,Czech Technical University, Prague, Czech Republic;

    Aerospace Research and Test Establishment, Prague, Czech Republic;

    Czech Technical University, Prague, Czech Republic;

    Czech Technical University, Prague, Czech Republic;

    Czech Technical University, Prague, Czech Republic;

    Czech Technical University, Prague, Czech Republic;

    Czech Technical University, Prague, Czech Republic;

  • 会议组织
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    CubeSat; TGFs; X-ray; Timepix; Lobster eye;

    机译:立方体卫星TGFs; X射线Timepix;龙虾眼;

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