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Performance study of the gamma-ray bursts polarimeter POLAR

机译:伽马射线爆裂偏振仪偏振的性能研究

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The Gamma-ray Burst Polarimeter-POLAR is a highly sensitive detector which is dedicated to the measurement of GRB's polarization with a large effective detection area and a large field of view (FOV). The optimized performance of POLAR will contribute to the capture and measurement of the transient sources like GRBs and Solar Flares. The detection energy range of POLAR is 50 keV ~ 500 keV, and mainly dominated by the Compton scattering effect. POLAR consists of 25 detector modular units (DMUs), and each DMU is composed of low Z material Plastic Scintillators (PS), multi-anode photomultipliers (MAPMT) and multi-channel ASIC Front-end Electronics (FEE). POLAR experiment is an international collaboration project involving China, Switzerland and Poland, and is expected to be launched in September in 2016 onboard the Chinese space laboratory "Tiangong-2 (TG-2)". With the efforts from the collaborations, POLAR has experienced the Demonstration Model (DM) phase, Engineering and Qualification Model (EQM) phase, Qualification Model (QM) phase, and now a full Flight Model (FM) of POLAR has been constructed. The FM of POLAR has passed the environmental acceptance tests (thermal cycling, vibration, shock and thermal vacuum tests) and experienced the calibration tests with both radioactive sources and 100% polarized Gamma-Ray beam at ESRF after its construction. The design of POLAR, Monte-Carlo simulation analysis, as well as the performance test results will all be introduced in this paper.
机译:伽马射线突发偏振仪极性是一种高度敏感的检测器,其专用于使用大有效检测区域和大型视野(FOV)测量GRB的极化。极性的优化性能将有助于捕获和测量GRBS和太阳耀斑等瞬态源。极性的检测能量范围为50keV〜500 keV,主要由康普顿散射效果主导。极性由25个探测器模块化单元(DMU)组成,每个DMU由低Z材料塑料闪烁体(PS),多阳极光电倍增器(MAPMT)和多通道ASIC前端电子设备(费用)组成。极地实验是一项涉及中国,瑞士和波兰的国际合作项目,预计将于2016年9月推出中国太空实验室“天江 - 2(TG-2)”。随着合作的努力,极地经历了演示模型(DM)阶段,工程和资格模型(EQM)相位,验证模型(QM)相,现在已经建造了极性的全飞行模型(FM)。 Polar的FM已通过环境验收测试(热循环,振动,休克和热真空测试),并在其结构之后在ESRF下使用放射源和100%极化伽马射线束经历了校准测试。本文介绍了极地,Monte-Carlo仿真分析的设计,以及性能测试结果。

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