首页> 外文会议>Conference on X-Ray and Gamma-Ray Instrumentation for Astronomy XI 2-4 August 2000 San Diego, USA >The on-line quick-look analysis and archiving system for the calibration of the PICsIT high energy detector on the INTEGRAL satellite
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The on-line quick-look analysis and archiving system for the calibration of the PICsIT high energy detector on the INTEGRAL satellite

机译:在线快速分析和归档系统,用于在INTEGRAL卫星上校准PICsIT高能探测器

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The PiCsIT instrument is the high energy imager which together with a low-energy plane comprises one of the two main detectors of the INTEGRAL gamma-ray satellite due to be launched by ESA in late 2001. PICsIT consists of 8 identical modules of 512 Caesium Iodide (CsI) scintillation crystals. The calibration of the detection plane is performed at module level (in three parallel chains), and consists of characterising each pixel in terms of resolution, gain and efficiency to a very high precision. The high precision and large number of pixels leads to the production of very large amounts of data which then leads to the requirement for a system capable of accumulating at a very high bit-rate; of archiving the data in a suitable format for later analysis; of visualising these data as they are accumulated in a quick-look fashion in order to control the correct set-up of the test arrangement and the detector functionality during the test and of partially analysing these extremely large quantities of data on-line so as to obtain the results essential for proceeding with the test process in a rapid manenr and not to impede the data accumulation process. Herein we describe the test equipment currently in use for the flight model calibration.
机译:PiCsIT仪器是高能成像仪,它与低能平面一起构成定于2001年末由ESA发射的INTEGRALγ射线卫星的两个主要探测器之一。PICsIT由512个碘化铯的8个相同模块组成(CsI)闪烁晶体。检测平面的校准在模块级别(在三个平行链中)执行,包括以非常高的精度在分辨率,增益和效率方面表征每个像素。高精度和大量像素导致产生非常大量的数据,这又导致需要一种能够以非常高的比特率进行累积的系统;以适当的格式归档数据以供以后分析;可视化以快速查看的方式累积的这些数据,以便在测试过程中控制测试装置和检测器功能的正确设置,以及部分在线分析这些非常大量的数据,从而获得快速进行测试过程必不可少的结果,并且不会妨碍数据累积过程。在此,我们描述当前用于飞行模型校准的测试设备。

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