排序方式: 共有12条查询结果,搜索用时 15 毫秒
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Low temperature testing and neutron irradiation of a swept charge device on board the HXMT satellite
王于仨 陈勇 徐玉朋 杨彦佶 崔苇苇 李茂顺 刘晓艳 王娟 韩大炜 陈田祥 李承奎 霍嘉 李正伟 李炜 胡渭 张艺 陆波 朱玥 刘琰 吴帝 孙庆荣 张子良 《中国物理 C》2012,36(10):991-995
We present the low temperature testing of an SCD detector, investigating its performance such as readout noise, energy resolution at 5.9 keV and dark current. The SCD's performance is closely related to temperature, and the temperature range of -80 ℃ to -50 ℃ is the best choice, where the FWHM at 5.9 keV is about 130 eV. The influence of the neutron irradiation from an electrostatic accelerator with fluence up to 1×109 cm-2 has been examined. We find the SCD is not vulnerable to neutron irradiation. The detailed operations of the SCD and the test results of low temperature are reported, and the results of neutron irradiation are discussed. 相似文献
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星载数据管理系统的共模故障分析方法 总被引:1,自引:0,他引:1
数据管理系统是低能X射线望远镜进行数据传输和数据处理的关键电路模块,为提高可靠性采用冷贮备冗余设计,但冗余设计会引入由共模故障引起的失效。因此,结合空间应用的环境,在对低能X射线望远镜的数据管理系统的故障树分析的基础上,对其进行共模故障方法的研究。首先,针对数据管理系统进行传统故障树的构建;其次,确定数据管理系统的共模故障分析对象,分析共模故障产生的原因及机理;再次,对数据管理系统进行共模故障定量分析;最后,通过对比考虑共模故障和未考虑共模故障的定量结果,提出改进设计措施。通过对数据管理系统进行共模故障定性和定量分析,找出引起发生共模故障的主要原因,并提出改进措施,提高了星载数据管理系统的可靠性。 相似文献
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仪器的本底是空间天文观测项目实施过程中关注的一个重要内容,对于聚焦型空间X射线望远镜,仪器的粒子本底水平直接关系到观测灵敏度及本底重建的系统误差.因此,在仪器设计及工程实现迭代过程中,需要确定仪器粒子本底水平,保证其在可接受范围内.本文发展了一种基于面密度插值快速估计聚焦型空间X射线望远镜粒子本底的方法,该方法同时具有较高的本底估计精度和快的计算速度,适合于在望远镜方案设计的早期对各种设计方案的本底屏蔽效果进行快速估计并据此提出优化设计的建议,可以大大提高早期方案设计的有效性,对于聚焦型空间高能天文仪器的研制及其他类似领域具有一定的参考意义. 相似文献
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Charged Coupled Devices(CCDs) have been successfully used in several low energy X-ray astronomical satellites over the past two decades. Their high energy resolution and high spatial resolution make them a perfect tool for low energy astronomy, such as observing the formation of galaxy clusters and the environment around black holes. The Low Energy X-ray Telescope(LE) group is developing a Swept Charge Device(SCD) for the Hard Xray Modulation Telescope(HXMT) satellite. A SCD is a special low energy X-ray CCD, which can be read out a thousand times faster than traditional CCDs, simultaneously keeping excellent energy resolution. A test method for measuring the charge transfer efficiency(CTE) of a prototype SCD has been set up. Studies of the charge transfer inefficiency(CTI) with a proton-irradiated SCD have been performed at a range of operating temperatures. The SCD is irradiated by 3×108cm-210 MeV protons. 相似文献
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A readout system for X-ray CCDs based on an improved architecture is presented; by optimizing several critical circuit blocks along the analog signal chain, the conflict between the readout speed and readout noise is greatly alleviated. Using CCD47-10 as its target CCD, the readout system has achieved 8.6e- readout noise and 142 eV FWHM at 5.9 keV Mn m Kα under a pixel rate of 80 kHz. Also its performance of imaging has been investigated. 相似文献
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探测器的读出噪声是表征其性能的一个重要参数,它不仅限制了探测器的能量分辨,还影响探测器系统的动态范围。传统的CCD探测器信号读出部分都采用由模拟器件构成的相关双采样(Correlated Double Sampling,简称CDS)电路,这种方法已被证实能够有效抑制探测器噪声,但与此同时,由于CDS电路本身比较复杂,引入了新的噪声,它成为进一步减小读出噪声的一个屏障。为了消除模拟电路本身的噪声屏障,作者采用了一种基于高速ADC和FPGA的直接数字化读出方法,去除CDS电路,简化信号路径,由FPGA控制高速ADC对CCD探测器输出信号的参考电平和信号电平进行多次采样,用数值计算方法实现CDS功能,提高了信噪比,改善了探测器的性能。 相似文献
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正硬X射线调制望远镜(The Hard X-ray Modulation Telescope,简称:HXMT)是我国自主研制的第一颗X射线天文卫星,承载有高能X射线望远镜(20~250ke V,5000 cm2)、中能X射线望远镜(5~30ke V,952 cm2)、低能X射线望远镜(1~15ke V,384 cm2)以及空间环境监测器。HXMT具有扫描观测和定点观测两种工作模式,扫描观测可以进行宽波段大天区X射线巡天成像,定点观测可以研究黑洞、中子星等高能天体的多波段X射线快速光变,HXMT还可以监视天空的高能爆发现象。通过HXMT 相似文献
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杨彦佶 陆景彬 王于仨 陈勇 徐玉朋 崔苇苇 李炜 李正伟 李茂顺 刘晓艳 王娟 韩大炜 陈田祥 李承奎 霍嘉 胡渭 张艺 陆波 朱玥 马克岩 吴帝 刘琰 张子良 尹国和 王宇 《中国物理 C》2014,38(8)
The Low Energy X-ray Telescope is one of the main payloads on the Hard X-ray Modulation Telescope satellite.Swept charge devices(SCDs)are selected as detectors for the Low Energy X-ray Telescope.As SCDs are sensitive to proton irradiation,irradiation tests were carried out on the HI-13 accelerator at the China Institute of Atomic Energy.The beam energy was measured to be 10 MeV at the SCD.The proton fluence delivered to the SCD was 3×108protons/cm2over two hours.By comparing the performance before and after irradiation,it is concluded that proton irradiation affects both the dark current and the charge transfer inefficiency of the SCD.The energy resolution of the proton-irradiated SCD is 212 eV@5.9 keV at-60?C,while it before irradiated is 134 eV.Moreover,better performance can be reached by lowering the operating temperature of the SCD in orbit. 相似文献