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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   
2.
本文从FPGA器件内部最基本的CMOS单元出发,分析了器件功能失效时反相器输出波形随累积剂量的变化关系,进而研究Altera SRAM型FPGA器件60Co γ射线辐照后的总剂量辐射损伤效应.实验结果表明:由于场氧漏电和结构漏电的影响,随着累积剂量的增加输出波形发生畸变,峰峰值变为原来的十分之一左右,但输出波形还有相对的高低电平;同时,输出高电平不能保持原有的状态,迅速地向低电平转换,并且转换速度随着累积剂量的增加而加快,输出低电平相对初始值有一定程度抬高;由于栅氧厚度变薄,输出波形 关键词: 60Coγ')" href="#">60Coγ 总剂量辐射损伤效应 SRAM型FPGA CMOS单元  相似文献   
3.
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   
4.
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   
5.
为了考核FPGA器件空间使用时的抗辐射能力,对Altera SRAM型FPGA器件60Coγ辐照后的总剂量辐射损伤效应及退火效应进行了研究。通过不同模块实现相同的分频功能,比较了不同模块输出波形随总剂量、退火时间的变化关系;通过实现不同源程序所需的模块不同,比较了不同模块、不同源程序功耗电流随总剂量、退火时间的变化关系。分析了功耗电流在不同退火温度下恢复的原因,讨论了不同退火温度下功耗电流恢复幅度的差异。测量了输出端口的高低电平,分析了高低电平随总剂量、退火时间的变化关系。实验结果表明:氧化物正电荷的退火导致了不同退火温度下的功耗电流的恢复,并且浅能级亚稳态的氧化物正电荷的数量多于深能级氧化物正电荷的数量;随着退火时间的增加,功能恢复为突变过程,而功耗电流的恢复为渐变过程。  相似文献   
6.
低能X射线望远镜是硬X射线调制望远镜卫星的主要载荷之一,探测器采用CCD236.探测器的量子效率会影响能谱拟合和绝对流量,有必要对其进行标定.利用~(55)Fe放射源,以硅漂移探测器为标准探测器,标定了CCD236在Mn-K_α(5.899 keV)和Mn-K_β(6.497 keV)能量点处的量子效率,此能段在Fe线附近,对X射线天文观测有重要价值.考虑探测器的分裂事例后,Mn-K_α和Mn-K_β处的量子效率分别为71%和62%.在-95—-30?C工作温度范围内,CCD量子效率与温度无关.利用CCD236的结构及实测的量子效率,不考虑沟阻影响,得到耗尽层厚度为38μm.对CCD236施加不同的电压,其量子效率基本不变,表明其在两相驱动下高低电平的耗尽层厚度相等,进而说明CCD236一直工作在深耗尽状态,其耗尽层到了外延层和衬底层边界,已达最大值.  相似文献   
7.
Readout noise is a critical parameter for characterizing the performance of charge-coupled devices (CCDs), which can be greatly reduced by the correlated double sampling (CDS) circuit. However, a conventional CDS circuit inevitably introduces new noise since it consists of several active analog components such as operational amplifiers. This paper proposes a digital CDS circuit technique, which transforms the pre-amplified CCD signal into a train of digital presentations by a high-speed data acquisition card directly without the noisy CDS circuit, then implements the digital CDS algorithm through a numerical method. A readout noise of 3.3 e- and an energy resolution of 121 eV@5.9 keV can be achieved via the digital CDS technique.  相似文献   
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   
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