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...     

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。     

深空探测器定位在太阳系中特殊点上的有关问题

由于某些探测任务的需要,要将空间探测器定位在日-地空间的适当 位置上,日-地系统中的5个平动点就是首选的位置。因其平动点是否稳定关 系到探测任务能否完成,如果不稳定又如何采取轨控策略是任务的关键。鉴于 这一点,本文将阐明5个平动点的动力学特征,特别是对3个不稳定的共线平动 点Li(i=1,2,3),给出相应的轨控条件,并以仿真计算结果表明,采用一定的轨 控方式,可以使探测器保持在Li附近而不远离。     

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。     

基于微型光谱仪的光纤压力高速解调技术

为解决高超声速飞行器中大气压力传感系统的多通道、高精度、强环境适应性等技术需求问题,具有耐高温、易组网、高灵敏度、抗电磁干扰等优点的光纤压力传感技术成为航空航天压力传感领域的重要研究方向。提出一种基于微型光谱仪的光纤压力高速解调技术,该技术采用基于体相位光栅和线阵光电探测器的微型光谱仪作为光谱探测单元、Actel公司的片上SoC电路系统作为智能信息处理单元,融合数字滤波、线性拟合、曲线寻峰、信号重构等数据处理算法,完成光纤压力传感器高速解调系统研制,并搭建压力检测实验平台。试验结果表明:系统的压力测量范围优于260kPa,测量精度接近0.1%F.S.,分辨率为10Pa,动态响应可达5kHz。     

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。     

基于单光子探测器恢复时间的误码率分析

在深空激光通信中，为满足通信距离远、传输速率高的要求，常采用脉冲位置调制（Pulse Position Modula-tion， PPM）与单光子探测器（Single-Photon Detector， SPD）相结合的探测体制。本文从单光子探测器的恢复时间特性出发，推导了探测器单元探测概率和虚警概率模型，建立了基于信号或硬判决和最大计数硬判决的多元单光子探测器阵列误码率模型。仿真分析结果表明：在16-PPM调制和RS（15，8）编码（Reed-Solomon Codes，里德-所罗门编码）体制下，为实现1.22 Gbps的通信速率、误码率优于10^-7，当探测器单元数为4时，探测器恢复时间应≤3.2 ns；当探测器单元数为25时，探测器恢复时间应≤10 ns。     

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.     

厚壁碳/酚醛复合材料热压罐固化工艺优化

厚壁碳/酚醛复合材料在固化过程中容易产生较大的温度梯度,造成固化不均匀。为了解此类产品在固化过程中内部的温度变化和分布,通过在产品内部预埋热电偶的方式,开展了温度监测实验。同时采用DSC及凝胶实验对树脂的固化特性进行了分析。结果表明:在初期阶段的升温过程中,产品内部温度远低于罐体内的温度;酚醛树脂随着温度的升高,流动性能变好,在95~100℃时开始凝胶,出现聚合放热现象。依据以上实验结果对固化工艺进行了优化,主要包括延长各温度点的保温时间、延缓初期的升温速率、调整加全压的时机、增加树脂凝胶温度点的保温段。最后对优化后的固化工艺进行了验证,结果表明优化后的固化工艺合理,产品经超声波检测,内部缺陷大大减少,质量均一性得到了有效提高。