星载赋形反射面数传天线优化设计

为了使星载赋形反射面数传天线的波束形状满足设计要求,应用Minimax算法对其进行了优化设计。首先基于几何光学原理得到反射面中截线的初始形状,然后采用Newton插值函数对中截线进行拟合并把插值函数的系数作为优化变量,最终利用Minimax算法对优化变量进行调整来使获得理想的赋形波束。通过对一个X波段赋形反射面天线优化结果的分析及与基于几何光学原理综合算法所得结果的对比,表明此方法的有效性和优越性。数值仿真结果表明：该方法能够保证覆盖角域内任意一点的增益均高于设计指标要求。     

基于MIMO圆阵雷达的二维DOA估计新算法

基于对均匀圆阵导向矢量的分析,将四元均匀圆阵作为多输入多输出(MIMO)雷达的发射阵,通过构造相应的二阶统计量并对其进行联合对角化获得了目标方位角和俯仰角的闭式解,以实现存在角度兼并时目标的二维到达方向(DOA)的估计,并保持原DOA矩阵方法无需二维谱峰搜索和参数配对等优点。仿真结果证明算法正确、可行。     

双极型磁选态单束铯束管内铯原子运动轨迹的算法改进

针对简化算法得到的铯原子运动轨迹精度不高的结果,通过分析磁选态单束铯束管内双极型选态磁铁的磁场分布,提出了不简化磁场梯度和有效磁矩,用布利厄施-施多厄方法求解铯原子运动方程的算法。用此算法得到的铯原子运动轨迹与通常采用的简化算法得到的轨迹相比,最大差异约为10 mm。此计算结果影响管内机械组件的安装对中位置,可用于束光学模拟计算,提高短期稳定度指标。     

一个带间隙连接结构对梁基频漂移影响研究

文章以一端夹支、另一端带套筒连接结构的梁作为研究对象,通过在连接结构中引入间隙非线性因素,分别研究了在连接结构处有无预紧力两种情况时在均布载荷作用下梁的非线性幅频响应。同时,利用改进的振型转化法及连续振型法对系统进行建模,采用伽辽金近似得到系统的非线性受迫振动方程;针对实际算例,用龙格-库塔法得到了其数值解,讨论了此算例梁的频率漂移结果,从而得到了对研究航天器地面振动试验中的频率漂移现象有价值的结论。     

同波束VLBI技术用于月球双探测器精密定轨及重力场解算

同波束VLBI通过同时观测两个探测器的多点频信号,可以得到两个探测器之间高精度的差分相位时延,日本月球探测计划SELENE充分体现了这一技术在月球探测器精密定轨中的贡献。本文针对采样返回的月球探测任务中,轨道器和返回器同时绕月飞行期间,研究利用同波束VLBI跟踪数据在探测器精密定轨和月球重力场仿真解算中的贡献。结果表明,加入同波束VLBI跟踪数据之后,探测器定轨精度有显著提高,改进超过一个量级。综合同波束VLBI跟踪数据解算得到的重力场模型相比于传统的USB双程测距测速数据,中低阶次位系数精度有明显改进,并且定轨精度有望能达到米级。
     

桨根柔性无铰旋翼桨叶气弹稳定性建模分析

建立了任意剖面无铰旋翼桨叶气弹稳定性分析模型,分析了复合材料柔性梁对无铰旋翼桨叶气弹稳定性的影响.将旋翼桨叶简化为二维截面特性线性分析和一维梁非线性分析,二维特性分析考虑了面内和面外翘曲,一维分析采用中等变形梁理论,考虑了剪切变形和与扭转相关的翘曲.采用准定常气动力,运用有限元理论,得出了无铰旋翼桨叶稳定性分析的有限元列式.研究了柔性梁不同铺层方式对气动弹性稳定性的影响.算例表明复合材料柔性梁铺层角对旋翼桨叶气动弹性稳定性影响明显,充分地利用这些影响变化规律,能够设计出更为先进的复合材料悬翼桨叶.      

基于某型振动式干燥机应力集中问题的强度分析

针对某型振动式干燥机模梁的应力集中问题,运用有限元理论和电测法对横梁进行了强度分析,找出了其产生破坏的原因。     

星载聚束式SAR天线波束指向控制分析

建立了波束控制条件下的星载聚束式SAR的天线指向及成像数学模型,证实天线波束指向被控造成回波信号的幅度调制,引起成对回波,从而影响成像质量.此外,分析了波束指向控制比率与测绘带方位宽度、图像动态范围的制约关系,提出设计星载聚束式 SAR天线波束指向控制比率的基本原则.最后,通过计算机仿真,验证了理论分析的正确性.      

Multiple-constraint cooperative guidance based on two-stage sequential convex programming

An improved approach is presented in this paper to implement highly constrained cooperative guidance to attack a stationary target. The problem with time-varying Proportional Navigation (PN) gain is first formulated as a nonlinear optimal control problem, which is difficult to solve due to the existence of nonlinear kinematics and nonconvex constraints. After convexification treatments and discretization, the solution to the original problem can be approximately obtained by solving a sequence of Second-Order Cone Programming (SOCP) problems, which can be readily solved by state-of-the-art Interior-Point Methods (IPMs). To mitigate the sensibility of the algorithm on the user-provided initial profile, a Two-Stage Sequential Convex Programming (TSSCP) method is presented in detail. Furthermore, numerical simulations under different mission scenarios are conducted to show the superiority of the proposed method in solving the cooperative guidance problem. The research indicated that the TSSCP method is more tractable and reliable than the traditional methods and has great potential for real-time processing and on-board implementation.     

The effect of solar and geomagnetic parameters on total electron content over Ankara,Turkey

In this study, the relationship between total electron content (TEC) and solar and geomagnetic parameters for Ankara station (39.7 N, 32.76 E), Turkey located in the mid-latitude ionosphere is investigated. In this context, F10.7 solar flux and Interplanetary Magnetic Fields (IMF) from solar parameters and Kp and Dst indices from geomagnetic parameters affecting on TEC are considered. The relationship between the variables is investigated by means of the statistical multiple regression model at the universal time (UT) (Local Time = UT + 2 h) 1200 and 2400 in the years when the 24th solar cycle was minimum (2007–2009) and maximum (2015). As a result, it is found that explainable rates by solar and geomagnetic parameters of TEC changes in 2007–2009 are lower than in 2015 at daytime, while the explainable rates in the solar minimum years are higher than those the maximum year at nighttime. To be higher than the solar maximum of explainable rate in the solar minimum years at nighttime may be related to the fact that the dynamics of the ionosphere is significantly different than expected in this deep minimum period. As expected in 2015, the relationship between TEC and independent parameters is greater at daytime than at nighttime.