基于强化学习的航空器机场智能静态路径规划

随着人工智能迅速发展以及“智慧机场”的提出,研究人工智能在机场如何有效地辅助机场管制人员,驾驶员指挥航空器在地面滑行具有重要意义。本文提出一种基于强化学习的滑行路径规划方法,构建航空器机场地面强化学习移动模型,并以海口美兰机场为案例采用 Python 内置工具包 Tkinter 进行场面仿真;在此基础上,考虑机场航空器滑行规则,采用 Off-Policy 中 Q-Learning 算法求解贝尔曼方程,实现航空器在 Model-based 环境中进行静态路径规划。结果表明：本文所提方法能够实现停机位到跑道出口智能静态路径规划     

采用排间界面静压约束伴随方法的多级压气机叶片优化

为解决伴随优化应用在多级压气机中出现的优化工况点漂移问题,在前期薄层N-S方程伴随方法基础上,对目标函数——出口熵增不仅施以质量流量、总压比约束,还添加排间界面静压展向分布作为新的约束条件.以某5级压气机为对象,对其中第1级转、静叶分别在首1.5级和全5级压气机环境下进行了优化.结果表明,施加排间界面静压展向分布约束能够显著解决优化工作点漂移问题,优化后5级压气机的效率提高0.4个百分点.      

Orbit Design for Twin-spacecraft Space VLBI

Space Very Long Baseline Interferometry (S-VLBI) is an aperture synthesis technique utilizing an array of radio telescopes including ground telescopes and space orbiting telescopes. It can achieve much higher spatial resolution than that from the ground-only VLBI. In this paper, a new concept of twin spacecraft S-VLBI has been proposed, which utilizes the space-space baselines formed by two satellites to obtain larger and uniform uv coverage without atmospheric influence and hence achieve high quality images with higher angular resolution. The orbit selections of the two satellites are investigated. The imaging performance and actual launch conditions are all taken into account in orbit designing of the twin spacecraft S-VLBI. Three schemes of orbit design using traditional elliptical orbits and circular orbits are presented. These design results can be used for different scientific goals. Furthermore, these designing ideas can provide useful references for the future Chinese millimeter-wave S-VLBI mission.      

航天器火工冲击技术研究进展

系统总结了国内外航天器火工冲击环境预示、地面试验和减冲击技术三个方面的研究进展,并分析了国内在以上三个方面与国外航天强国的差距。在此基础上,从我国航天工程实际需求出发,分析指出了今后航天器火工冲击领域应重点开展的研究方向。     

旋翼微多普勒特性实验分析

为分析旋翼及其主要部件的微多普勒效应特点,提出了一种通过微波暗室进行旋翼微多普勒效应测试的实验方法,并通过实例验证了实验方法的可靠性;两种桨叶不同桨叶片数的系列实验结果表明,旋翼的微多普勒特性通过频率把各个散射部件的回波能量分开,旋翼的片数和转速不影响微多普勒特性的分析估算,旋翼的微多普勒特性仅与其运动特性相关;结合直升机目标识别特征,采用短时傅里叶变换方法对实验数据进行微多普勒效应提取,分析了微多普勒效应与入射波和旋翼几何属性之间的关系,得到了旋翼微多普勒效应的频率特性、极化特性和宽频带特性.     

汽油机进气歧管流通性和均匀性数值模拟

进气歧管的流通性和均匀性对发动机性能产生重要影响.建立了某四缸汽油发动机的GT-power仿真模型,对进气歧管的气体流速进行了仿真计算;利用STAR-CD软件模拟计算了进气歧管不同进气角度时各支管内的气体压力和流速分布,分析了各支管的进气均匀性和充气系数.计算和分析结果表明,通过改变进气口方向和稳压腔容积等几何参数,可以提高进气歧管的气体流通性,改善进气歧管各支管内气体流动质量,使各支管内气体流量趋于均匀.计算结果为该进气歧管的改性设计提供了理论依据.      

基于XML的EtherCAT工业以太网协议解析技术

重点研究了基于可扩展标记语言(XML,eXtensible Markup Language)的EtherCAT工业以太网协议解析器技术和实现方法.介绍了EtherCAT协议报文格式和特点,分析了以太网数据侦听器和协议解析器的结构,针对通用以太网解析器在工业以太网领域应用的局限性,提出使用XML语言描述协议报文的方法,在此基础上开发出一种开放式、可重构的EtherCAT协议解析器.实验结果表明基于XML的协议报文描述方法及解析器能够有效地描述和解析EtherCAT协议报文,使用者可以根据解析对象格式使用XML语言自定义、修改和扩展协议解析规则,获得清晰、直观的解析结果.      

激光跟踪仪在交会对接微波雷达多径试验中的应用

交会对接微波雷达多径试验是在地面模拟两个飞行器在轨交会对接过程中由舱体表面及遮挡对微波信号造成反射干扰的一种试验,其目的是验证激光雷达系统功能及安装位置的合理性。在近20 m远的距离上,对飞行器舱体上的微波雷达天线和微波应答天线进行角度及距离的精确测量。文章通过对试验环境、测量项目分析及不同精测方案比对,采用激光跟踪仪直接测量舱体结构,获得了准确的基准数据,有助于指导微波雷达在飞船轨道舱上的精确安装和提高交会对接微波雷达多径试验的精度。激光跟踪仪首次应用于交会对接微波雷达多径试验,相比经纬仪在航天器基准测量中具有更大的优势。     

Gyrosynchrotron Radiation of Interplanetary CMEs

CMEs (Coronal Mass Ejections) are an important means of energy release in the solar corona. Solar Polar Orbit Radio Telescope (SPORT) is a mission being proposed for observing the propagation of interplanetary CMEs from solar polar orbit. The main payload onboard SPORT is a synthetic aperture interferometric radiometer, which receives radio emission of interplanetary CMEs. It is identified that there are mainly three radio emission mechanisms of CMEs, i.e., bremsstrahlung, gyrosynchrotron emission and plasma emission. Among these emission types, bremsstrahlung emission is the main emission mechanism of the high-density plasma clouds of interplanetary CMEs. Gyrosynchrotron emission is the continuous emission generated by high-energy electrons from CMEs, while plasma emission is the main mechanism of transient radio bursts from CMEs. In this paper, the gyrosynchrotron emission of interplanetary CMEs is focused on. Firstly, the mechanism of gyrosynchrotron emission is reviewed. Secondly, a review of the physical parameter models of background solar wind and interplanetary CMEs is presented. After these, the brightness temperature and polarization of gyrosynchrotron emission of interplanetary CMEs are calculated and analyzed. Finally, the detectability of gyrosynchrotron emission of interplanetary CMEs by radio meters is discussed briefly.