基于RBF网络的质量矩导弹姿态控制

研究了三轴稳定质量矩导弹姿态控制问题.建立了内部带有3个可移动滑块的数学模型.利用RBF(radial basis function)网络的快速自学习、自适应特性, 作为被控对象的模型, 不断调整PID控制器的参数, 协调控制滑块位置, 从而改变导弹的飞行姿态.最后讨论了滑块运动特性对系统性能的影响并对系统稳定性进行了分析.仿真结果表明该控制律在保证系统稳定的情况下有效地实现导弹的姿态调整, 并且提高了系统的动态响应品质.      

PDE在模拟冲压进气条件下的台架推力修正

研究射流模拟冲压进气条件下,气源喷口尺寸和气源压头对脉冲爆震发动机(PDE)地面台架测量推力的影响及消除外阻对测量推力的影响的措施.研究结果表明,由于PDE外阻存在使PDE地面台架测量推力偏小,采用PDE进气道前装承力锥的方法,可以消除PDE外阻对PDE地面台架试验推力测量的影响,获得PDE实际内流推力.在试验结果基础上,提出一个PDE地面台架试验内流推力修正公式并在试验中得到验证.      

Jet Vectoring Control Using a Novel Synthetic Jet Actuator

A primary air jet vectoring control system with a novel synthetic jet actuator (SJA) is presented and simulated numerically. The results show that, in comparison with an existing traditional synthetic jet actuator, which is able to perform the duty of either “push” or “pull”, one novel synthetic jet actuator can fulfill both “push” and “pull” functions to vector the primary jet by shifting a slide block inside it. Therefore, because the new actuator possesses greater efficiency, it has potentiality to replace the existing one in various appli- cations, such as thrust vectoring and the reduction of thermal signature. Moreover, as the novel actuator can fulfill those functions that the existing one can not, it may well be expected to popularize it into more flow control systems.     

空间轨道转移飞行器推进系统静态仿真分析

采用模块化方法建立了空间轨道转移飞行器推进系统的静态数学模型,用C语言开发出对应静态模型的仿真计算软件,应用该软件分别对N2O4/MMH、N2O4/UDMH、LO2/LH2、LO2/RP-1等推进剂组合推进系统进行静态仿真计算,并把计算结果导入相关质量模型,估算各系统在特定条件下的质量,再对上述几种推进系统进行单干扰因素分析,确定了敏感度较大的干扰因素。     

超燃冲压发动机性能初步研究

介绍了北京动力机械研究所进行的超燃冲压发动机初步研究。该方面研究包括超声速燃烧初步试验研究、双模态超燃冲压发动机燃烧室计算模拟和试验研究、高超声速进气道研究、超燃冲压发动机模型自由射流试验研究,获得了良好的高超声速进气道和超燃冲压发动机的工作性能。     

应用PIV技术测量压电型自耦合射流

 采用PIV对激励信号频率为300 Hz、 400 Hz和500 Hz的矩型出口自耦合射流流场进行测量,应用相位锁定技术,测得一个激励周期内12个相位的瞬时流场,并由120张瞬时流场图像的平均得到了射流流场时均流动特性。分析了3种频率下的流场结构,发现在当前实验条件下,射流的扩张半角近35°,稳定增长区的中心线速度随流向距离的-0.511次方变化。当频率为f=400 Hz时流量增长率高达4,动量增长率最高达4.5。当沿流向距离y/h>40后自耦合射流的动量呈下降趋势,这与定常二维平面射流动量保持不变的规律不同。     

Science objectives of the magnetic field experiment onboard Aditya-L1 spacecraft

The Aditya-L1 is first Indian solar mission scheduled to be placed in a halo orbit around the first Lagrangian point (L1) of Sun-Earth system in the year 2018–19. The approved scientific payloads onboard Aditya-L1 spacecraft includes a Fluxgate Digital Magnetometer (FGM) to measure the local magnetic field which is necessary to supplement the outcome of other scientific experiments onboard. The in-situ vector magnetic field data at L1 is essential for better understanding of the data provided by the particle and plasma analysis experiments, onboard Aditya-L1 mission. Also, the dynamics of Coronal Mass Ejections (CMEs) can be better understood with the help of in-situ magnetic field data at the L1 point region. This data will also serve as crucial input for the short lead-time space weather forecasting models.The proposed FGM is a dual range magnetic sensor on a 6?m long boom mounted on the Sun viewing panel deck and configured to deploy along the negative roll direction of the spacecraft. Two sets of sensors (tri-axial each) are proposed to be mounted, one at the tip of boom (6?m from the spacecraft) and other, midway (3?m from the spacecraft). The main science objective of this experiment is to measure the magnitude and nature of the interplanetary magnetic field (IMF) locally and to study the disturbed magnetic conditions and extreme solar events by detecting the CME from Sun as a transient event. The proposed secondary science objectives are to study the impact of interplanetary structures and shock solar wind interaction on geo-space environment and to detect low frequency plasma waves emanating from the solar corona at L1 point. This will provide a better understanding on how the Sun affects interplanetary space.In this paper, we shall give the main scientific objectives of the magnetic field experiment and brief technical details of the FGM onboard Aditya-1 spacecraft.     

充液航天器质量特性计算方法研究

充液航天器的质量特性对飞行动力学建模和控制设计有着重要影响。质量特性测量装置通常只能测出干重状态下航天器的质量特性，而充液状态下的航天器质量特性只能靠计算给出，其中如何计及各贮箱内液体的惯性张量是此类工程计算的难点。首先采用势流理论推导了任意形状贮箱内液体质量特性的一般表达式，包括全充液情况和部分充液情况，其中对部分充液情况考虑了自由液面小幅晃动的影响；然后采用三维有限元方法建立了液体质量特性的数值计算方法，并通过一个验证算例确认了该计算方法的有效性；最后应用该方法计算了一个充液航天器的质量特性，并研究了不同的液体处理方法对计算结果的影响。研究表明，工程上通常采用的“固化液体”处理方法所计算出来的转动惯量明显偏大，而所提出的计算方法具有更好的理论正确性和工程适用性。     

Analysis of a long-duration AR throughout five solar rotations: Magnetic properties and ejective events

Coronal mass ejections (CMEs), which are among the most magnificent solar eruptions, are a major driver of space weather and can thus affect diverse human technologies. Different processes have been proposed to explain the initiation and release of CMEs from solar active regions (ARs), without reaching consensus on which is the predominant scenario, and thus rendering impossible to accurately predict when a CME is going to erupt from a given AR. To investigate AR magnetic properties that favor CMEs production, we employ multi-spacecraft data to analyze a long duration AR (NOAA 11089, 11100, 11106, 11112 and 11121) throughout its complete lifetime, spanning five Carrington rotations from July to November 2010. We use data from the Solar Dynamics Observatory to study the evolution of the AR magnetic properties during the five near-side passages, and a proxy to follow the magnetic flux changes when no magnetograms are available, i.e. during far-side transits. The ejectivity is studied by characterizing the angular widths, speeds and masses of 108 CMEs that we associated to the AR, when examining a 124-day period. Such an ejectivity tracking was possible thanks to the multi-viewpoint images provided by the Solar-Terrestrial Relations Observatory and Solar and Heliospheric Observatory in a quasi-quadrature configuration. We also inspected the X-ray flares registered by the GOES satellite and found 162 to be associated to the AR under study. Given the substantial number of ejections studied, we use a statistical approach instead of a single-event analysis. We found three well defined periods of very high CMEs activity and two periods with no mass ejections that are preceded or accompanied by characteristic changes in the AR magnetic flux, free magnetic energy and/or presence of electric currents. Our large sample of CMEs and long term study of a single AR, provide further evidence relating AR magnetic activity to CME and Flare production.     

亚声速矩形射流的噪声辐射特性和声源分布

基于射流噪声模拟试验台，对出口面积相同的圆形喷口及宽高比分别为1、1.5、2、10的矩形喷口亚声速射流的远场噪声辐射特性和噪声源分布位置进行了较为系统的研究。通过远场噪声测量，获得了不同宽高比矩形喷口在不同方位角平面的射流噪声频谱分布结果相对于圆形射流的差异，揭示了矩形射流潜在的降噪潜力。通过基于波束成形算法的传声器阵列，得到了矩形射流噪声源峰值位置随频率的变化情况，系统分析了射流速度、方位角、宽高比等参数对矩形射流噪声源分布的影响。射流速度和方位角对矩形射流噪声源分布的归一化结果影响很小，而宽高比对矩形射流噪声源分布有较大影响：随着矩形宽高比的增加，矩形射流低频段噪声源向上游偏移，高频段噪声源向下游偏移。