空间粒子辐射监测器用模拟信号源的实现

空间粒子辐射监测器需要有模拟信号源在其生产和测试、试验阶段对其进行电性能检测,并随其辗转于各测试场地。使用进口模拟信号源存在操作复杂、设备笨重及只有单路输出等问题,因此需要设计一种专用模拟信号源。根据空间粒子辐射监测器的要求自行研制的模拟信号源有多路模拟信号输出,且各路信号幅度可独立调节,并采用内部电源供电。经过测试验证,该模拟信号源可作为空间粒子辐射监测器的配套设备使用,性能优于原进口模拟信号源,其电路设计亦可为相关设备提供参考。     

光电池测光器在爆震波测量中的应用

爆震管内火焰的结构非常复杂且传播速度快,需要高精度、高响应时间的测试工具.本文在单爆震试验中采用光电池测光器和离子探针测量燃烧波.研究中以高频响压力传感器为参考依据,通过测量同一截面上压力传感器、光电池测光器和离子探针之间的触发顺序,以及光电池测光器与离子探针信号的持续时间,来验证光电池测光器在爆震波测量中的可行性与精度.结果表明:光电池测光器比离子探针更适合测量爆震管内火焰传播速度.      

The high precision gamma-ray spectrometer for lunar polar orbiter SELENE

The high precision gamma-ray spectrometer (GRS) is scheduled to be launched on the lunar polar orbiter of the SELENE mission in 2007. The GRS consists of a large Ge crystal as a main detector and massive bismuth germanate crystals as an anticoincidence detector. A Stirling cryocooler was adopted in cooling the Ge detector. The flight model of SELENE GRS has been completed and an energy resolution of 3.0 keV (FWHM) at 1.332 MeV has been achieved. The spectrometer aims to observe nuclear line gamma rays emitted from the lunar surface in a wide energy range from 100 keV to 12 MeV for one year and more to obtain chemical composition on the entire lunar surface. The gamma-ray data enable us to study lunar geoscience problems including crust and mantle composition, and volatile reservoirs at polar regions.     

末修姿控系统极性检测仪设计

为满足末修姿控动力系统与控制系统一致性和协调性检测而研制的末修姿控系统极性检测仪,能实时检测并显示末修姿控动力系统根据控制系统发出的控制指令按时序动作的情况,从而为控制系统提供可靠的判断数据,确保了末修姿控动力系统的正常工作。末修姿控系统极性检测仪使用方便,操作界面简单,可自动记录、保存检测数据,并可离线浏览、打印,自动化程度高;同时仪器内部嵌入控制信号模拟线路,可自动进行模拟自检测试,从而提高工作效率,减少设备投入,其便携式、小型化设计更适应了机动、灵活的使用需求。     

空间粉尘探测器研究进展

文章在系统地总结空间粉尘（微小空间碎片和微流星体）探测技术的基础上,重点分析了压电型探测器、半导体型探测器、电离型探测器、组合式探测器等的工作原理、技术特点及其应用,同时简要评述了空间粉尘探测技术的发展趋势。     

基于LabVIEW的单光子探测器量子效率测控软件设计

介绍了利用相关光子法测量单光子探测器量子效率的原理和测量系统,开发了一套用于该系统的测控软件。软件采用LabVIEW的标准状态机结构,使用 VISA串口程序库、ActiveX控件和报表生成器,编写了激光器控制、符合光子测量、测试报告生成等分支程序,实现控制状态机分支的切换,和其他各项功能的调用。实际应用表明,该软件测控系统运行可靠、界面友好,满足单光子探测器量子效率测量的要求。     

飞机结冰探测器安装位置研究

基于飞机结冰探测器安装要求,通过三维数值仿真,模拟了机头表面流场和水滴撞击特性.通过标定水滴遮蔽区和浓度增加区引入危险位置点的概念,对结冰探测器的安装位置进行了分析,模拟了安装位置处结冰探测器探头表面和飞机主要迎风部件表面的水滴收集特性和结冰特性,并进行对比分析.分析结果表明探头表面的最大收集系数、结冰强度和结冰程度等...     

First measurements of periodicities and anisotropies of cosmic ray flux observed with a water-Cherenkov detector at the Marambio Antarctic base

A new water-Cherenkov radiation detector, located at the Argentine Marambio Antarctic Base (64.24S-56.62 W), has been monitoring the variability of galactic cosmic ray (GCR) flux since 2019. One of the main aims is to provide experimental data necessary to study interplanetary transport of GCRs during transient events at different space/time scales. In this paper we present the detector and analyze observations made during one full year. After the analysis and correction of the GCR flux variability due to the atmospheric conditions (pressure and temperature), a study of the periodicities is performed in order to analyze modulations due to heliospheric phenomena. We can observe two periods: (a) 1 day, associated with the Earth’s rotation combined with the spatial anisotropy of the GCR flux; and (b) $～$ 30 days due to solar impact of stable solar structures combined with the rotation of the Sun. From a superposed epoch analysis, and considering the geomagnetic effects, the mean diurnal amplitude is $～$ 0.08% and the maximum flux is observed in $～$ 15 h local time (LT) direction in the interplanetary space. In such a way, we determine the capability of Neurus to observe anisotropies and other interplanetary modulations on the GCR flux arriving at the Earth.     

红外探测设备抗烟幕干扰试验及评估方法

红外探测设备抗烟幕干扰能力是其抗干扰能力的重要部分。常规方法对场地和实施要求很高,试验次数安排有限。文章对该试验设计的关键问题开展分析和研究,根据红外探测设备作用距离与目标能量的关系,采用"等效试验"构建外场静态试验干扰环境,并合理选择试验因素采用均匀设计方法进行试验设计,确定抗干扰试验方案和评估方法。该方案可指导试验获得科学合理有效的数据,从而实现烟幕干扰环境下红外探测设备的抗干扰能力的准确评估。     

A new approach for pulse amplitude measurement using Lagrange’s interpolation for radiation or particle detectors

In radiation detector signal processing, usually, the charge-sensitive preamplifier converts the small charge signal coming from the semiconductor-based detector into voltage form and then the signal is further amplified to measure the energy of the incoming radiation. The voltage pulse from a charge-sensitive preamplifier (CSPA) is amplified using a shaping amplifier which reduces the signal bandwidth. To achieve better energy resolution, precise measurement of the peak amplitude of shaping amplifier output is required. The signal processing methods are available in which the signal from the charge-sensitive preamplifier can be directly digitized using high-speed Analog to Digital Converters (ADC), and then further signal processing such as gain and shaping is carried out inside the Field Programmable Gate Arrays (FPGA). For multiple detector systems, digital signal processing methods are quite difficult to implement in Field Programmable Gate Arrays (FPGA). In this context, The development of an alternative technique is initiated that uses a charge-sensitive preamplifier, shaping amplifier, low sampling analog-to-digital converter, and FPGA, where LaGrange’s interpolation technique is implemented in FPGA to precisely measure the peak of the analog pulse. In this paper, the comparison of the proposed method with other pulse amplitude measurement techniques is discussed. Results show that the implemented technique gives similar energy resolution compared to digital pulse processing and standard peak detector-based techniques.