基于随机点模拟方法分析空间目标危险交会

基于SGP4模型在空间目标轨道预报中的应用, 在预报的位置速度信息和误差 信息基础上, 提出一种空间两目标碰撞预警的分析方法, 即随机点模拟方法. 与传统的交会平面积分方法相比, 其主要有两点不同: 一是在误差信息中考虑 了误差均值的影响, 即误差椭球不再以预报位置为中心分布; 二是在分析方 法上侧重于真实模拟可能的交会情形, 而不忽略任一方向上的误差. 通过算例分 析验证了该方法的可行性, 结果表明误差均值的非零性使得最大碰撞概率不 一定出现在预报的最近交会距离时刻. 同时仿真结果还表明, 两目标在相对速 度方向上的相对位置仍然存在误差, 这可能造成随机点模拟的碰撞概率计算 值较交会平面积分方法偏小. 不同的碰撞预警分析方法对应不同的预警门限, 根据文中实例, 初步确定10^-6为随机点模拟方法的红色预警值.     

嫦娥四号任务科学目标和有效载荷配置

嫦娥四号探测器由中继星、着陆器和巡视器组成.其科学目标为：月基低频射电天文观测研究,月球背面巡视区浅层结构探测研究以及月球背面巡视区形貌与矿物组分探测研究.共配置6台有效载荷设备,其中3台载荷设备配置在着陆器上,分别为降落相机、地形地貌相机和低频射电谱仪,其余3台配置在巡视器上,分别为全景相机、测月雷达和红外成像光谱仪.本文主要论述了嫦娥四号任务的科学目标、着陆区概况、有效载荷配置及系统设计、各有效载荷任务和主要技术指标等.     

航天器介质深层充电模拟研究

针对航天器介质深层充电问题,提出了一种基于蒙特卡罗模拟和充电动力学RIC模型的介质电荷分布及电场预估新方法,利用地面试验验证了其正确性.航天器介质平板充电过程被简化为屏蔽铝板与分层介质组成的Geant 4模型,通过统计方法计算出了实际入射束流下Teflon介质内的注入电流密度和剂量率分布曲线,利用RIC模型获得了背面接地时介质中的电荷密度和电场分布,利用脉冲电声法(PEA)对不同束流密度辐照下的Teflon内部空间电荷密度进行了测量.数值模拟和地面试验结果表明,Teflon在100 keV能量电子辐照下,电荷密度和电场随着束流密度的增加而不断增大,其电荷密度峰值位置约为0.042 mm,且背面接地时接地侧电场最大.由于Geant 4粒子输运模拟和RIC模型具有通用性,因此该方法适用于各种航天器介质材料.     

N-fold Bernoulli probability based adaptive fast-tracking algorithm and its application to autonomous aerial refuelling

Recently, deep learning has been widely utilized for object tracking tasks. However, deep learning encounters limits in tasks such as Autonomous Aerial Refueling (AAR), where the target object can vary substantially in size, requiring high-precision real-time performance in embedded systems. This paper presents a novel embedded adaptiveness single-object tracking framework based on an improved YOLOv4 detection approach and an n-fold Bernoulli probability theorem. First, an Asymmetric Convolutional Network (ACNet) and dense blocks are combined with the YOLOv4 architecture to detect small objects with high precision when similar objects are in the background. The prior object information, such as its location in the previous frame and its speed, is utilized to adaptively track objects of various sizes. Moreover, based on the n-fold Bernoulli probability theorem, we develop a filter that uses statistical laws to reduce the false positive rate of object tracking. To evaluate the efficiency of our algorithm, a new AAR dataset is collected, and extensive AAR detection and tracking experiments are performed. The results demonstrate that our improved detection algorithm is better than the original YOLOv4 algorithm on small and similar object detection tasks; the object tracking algorithm is better than state-of-the-art object tracking algorithms on refueling drogue tracking tasks.     

灵巧型大孔径四反星敏感器镜头设计

星敏感器镜头是星敏感器姿态轨道控制系统的重要组成部分，具有相对孔径大、工作谱段宽、绝对畸变低的特点，针对这些特点，在四反射镜初始结构的基础上，分析了镜头探测能力和相对孔径的关系，明确了镜头设计指标，利用非球面反射镜强大的像差校正能力，优化设计得到了全反射4反星敏感器镜头。镜头焦距170mm，轴向长度50mm，镜头F数2，等效入瞳直径51.2mm，圆视场±2.25°。镜头工作波段可由膜系决定，无色差，空间频率35lp/mm处传递函数优于0.6，畸变优于0.01%，弥散斑直径优于13μm，系统15μm范围内能量集中度优于80%，渐晕系数小于0.95，该镜头可用于亚像素精度的飞船姿态轨道控制系统，为星敏感器导航光学系统设计提供了参考。     

航天用FR4 材料的本征电导率测试

介质材料电导率是影响卫星充电过程的重要材料参数,它决定着航天器上电荷的分布状态以及电流平 衡建立的快慢。常规的电导率测量方法完全不考虑空间真实带电环境,其测试结果用于卫星带电防护设计将会产生 较大的误差。本文建立了用传统三电极法和电荷衰减法测试介质材料本征电导率的测试系统,对卫星常用的FR4 材 料进行了测试,测试结果与国外的结果相近。     

Si粉特性对反应烧结Si3N4多孔陶瓷的强韧性及介电性能的调控作用

Si₃N₄多孔陶瓷具有优异的力学性能、介电性能、热学性能和化学稳定性等，特别适用于高温、大载荷、强侵蚀环境下的宽频透波材料。反应烧结Si₃N₄多孔陶瓷在性能、工艺和成本方面优势显著，原料Si粉特性显著控制着其物相、显微结构、力学和介电性能。本文以不同粒径和纯度的Si粉为原料制备注凝成形、反应烧结Si₃N₄多孔陶瓷。结果表明，双粒径配料使素坯产生紧密堆积效应，其遗传并进一步演化出两级显微组织强韧化机制，双粒径配料5 & 45 μm时的弯曲强度和断裂功获得最大值109.94 MPa和990.74 J/m²。该值分别比单粒径配料5和45 μm时的值提高了111.42%、25.97%和46.55%、20.46%；介电常数和介电损耗分别约为4.20和0.007。注凝成形、反应烧结Si₃N₄多孔陶瓷可以兼顾力学性能和介电性能，适用于透波罩等异形、大尺寸构件。     

Biaxial tensile behavior of Ti-6Al-4V under proportional loading

The biaxial tensile behavior of isotropic Ti-6Al-4 V is characterized in this paper. A novel cruciform specimen was designed and optimized to achieve uniform stress and strain distribution within the gauge area. Biaxial tensile tests were conducted at three different loading ratios by the biaxial testing machine. The Digital Image Correlation (DIC) technique was applied to determine strain distribution, and a high-speed camera was employed to record the fracture process. An Inverse Analysis (IA) approach with a combined experimental and numerical method was proposed to determine the true stresses at the gauge section of the specimen during biaxial tensile tests. The results indicate that the initial yield locus can be described by the Cazacu criterion accurately, whereas the Mises criterion can predict better the strengthening behavior of Ti-6Al-4 V in the first quadrant in the principal stress space.     

CFRP/TC4叠层结构制孔技术对比实验

因CFRP、TC4材料的物理性能差异较大，导致CFRP/TC4叠层构件切削性能匹配性较差，钻削过程中存在界面损伤、CFRP孔壁损伤难以调控的问题。针对上述问题，本文采用变参数啄式钻削工艺、变参数钻削工艺和恒参数钻削工艺对CFRP/TC4叠层结构进行了制孔实验，并对不同工艺条件下的轴向力、界面质量、TC4的切屑形态、CFRP层孔壁质量进行了对比分析。结果表明：相对于其他两种钻削工艺，在变参数啄式钻削工艺条件下，TC4材料层轴向力明显较高，产生短带状和短螺旋状切屑；CFRP层出口和入口处的孔径更接近于名义孔径，孔壁缺陷较少，表面粗糙度相对较小。     

Hardware qualification for scientific ballooning missions

The European Stratospheric Balloon Observatory (ESBO) initiative aims at simplifying the access to stratospheric balloon missions. We plan to provide platforms and support with instrument design in order to support scientists. During the design process, the inevitable question of qualification for the harsh flight conditions arises. Unfortunately, there is no existing standard for qualification of stratospheric ballooning hardware. Thus, we developed a qualification procedure for use within ESBO and similar projects.In this paper, we present our analysis of the environmental conditions in the stratosphere. While conditions at typical balloon float altitudes are similar to the space environment, there are also some relevant differences. For example, the thermal environment is dominated by radiation and thermal conduction, but the remaining atmosphere still supports a certain amount of convection. The remaining atmospheric pressure in the stratosphere also leads to reduced arcing distances. Vibrational loads are far less than for space missions, but quasi-static or shock loads may occur. The criticality of radiation increases with mission duration.Based on the environmental conditions, we present the qualification procedures for ESBO, which are based on the European Cooperation for Space Standardization (ECSS) standards for space systems. Overtesting against too high requirements leads to overengineering, driving mission cost and mitigating the advantages of balloons over space missions. Therefore, we modified the ECSS standards to fit typical scientific ballooning missions over several days at altitudes up to 40 km. Furthermore, we analyzed design rules for space systems with regard to their relevance for scientific ballooning, including material and component selection. We present the experience from the hardware qualification process for the ESBO prototype STUDIO (Stratospheric UV Demonstrator of an Imaging Observatory). Even though boundary conditions are different for each individual mission, we aimed for a broader approach: We investigated more general requirements for scientific ballooning missions to support future flights.