基于IMM理论的大型舰船被动定位算法研究

针对相控阵导引头跟踪航母等大型舰船目标的要求,为了给雷达成像进行运动补偿、给目标识别提供更多的先验信息,必须对目标运动参数进行准确的估计,但是常规被动定位算法通常采用单一目标运动模型,难以适应大型军舰运动规律的多样化,导致模型不匹配,使得误差较大,难以对目标参数进行准确估计,为解决上述问题,提出了一种基于交互式多模型(IMM)理论的大型舰船被动定位方法,使用不同的模型来匹配舰船不同的运动状态。仿真结果表明,提出的方法与常规的被动定位算法相比,定位精度明显提高,且易于工程实现。     

双光束补偿扫描系统

提出一种新的高精度大型平面扫描仪。利用双光束补偿系统，扫描头由一特殊光路组成。当入射光通过此光路后，产生对称输出的两束光。当入射光发生角漂或扫描头发生摆动时，输出的两束光对称上下漂移，其中心线保持不变，故扫描形成的基准面保持不变，从而大大提高了测量精度。经实验证明，测量精度优于2．5×10－6。     

不可压缩橡胶薄膜受气压作用的大变形分析

分析了周边固定的橡胶薄膜受气压作用的轴对称问题，推导了基本方程，并得到了数值解，给出了薄膜的应力分布和形变特征。结果表明在大变形情况下，橡胶薄膜处于单向拉伸状态。     

数字近景摄影大尺寸三坐标测量系统V-STARS的测试与应用

介绍了数字近景摄影大尺寸柔性三坐标测量系统V—STARS的配置、测量原理和测量过程,对其三维坐标及平面度的测量重复性进行了实际测试,与激光跟踪仪进行了平面度的比对测试,并将V—STARS系统成功应用于某17m网状天线的型面测量与调整工程实践中。     

Two-level optimization approach for Mars orbital long-duration,large non-coplanar rendezvous phasing maneuvers

A relative dynamics equation-set based on orbital element differences with J₂ effects is derived, based on which a two-level approach is proposed to optimize the Mars orbital rendezvous phasing with a large difference in the initial ascending node. The up-level problem uses the revolution deviation between the target spacecraft and the chaser as the design variable, and employs a linear search to find the optimum. The low-level problem uses the maneuver revolutions, locations, and impulses as the design variables, and is solved using a hybrid genetic algorithm combined with sequential quadratic programming. To improve the solution accuracy, an iteration method is developed to satisfy the terminal constraints of the absolute numerical integration trajectory. Test cases involving Mars sample return missions with large initial node differences are presented, which show that the relative dynamics, two-level optimization model, and hybrid optimization algorithm are efficient and robust. Compared with previously published results, the total velocity increment has been further reduced by utilizing this proposed approach. It is found that a five-impulse plan requires the least quantity of propellant, and a propellant-optimal minimum rendezvous duration exists for this long-duration, large non-coplanar rendezvous problem.     

Damage assessment of large space structures through the variational approach

The present investigation is focused on the solution of a dynamic inverse problem which is concerned with the assessment of damage in large space structures by means of measured vibration data. This inverse problem has been presented as an optimization problem and has been solved through the use of the conjugate gradient method with the adjoint equation, also called the variational approach. When a high number of damaged elements has to be found and these elements are also severely damaged, it is shown that the use of an additional method is necessary in order to provide a better initial guess for the conjugate gradient method. A stochastic method, represented by the genetic algorithm method, has been chosen because it provides robust search in complex spaces and also reduces the chance of converging to local optima. The application of this hybrid approach showed that better results can be achieved, although the computational time for the application analyzed here could increase. The damage estimation has been evaluated using noiseless and noisy synthetic experimental data, and the reported results are concerned with a space truss structure.     

A preliminary Chandra X-ray spectroscopy of the supernova remnant N132D

We present the preliminary results of a Chandra X-ray study of N132D, a young shell-like supernova remnant (SNR) in the Large Magellanic Cloud. The equivalent width maps of emissions from O, Ne, Mg, Si, and S are provided. Spatially resolved spectral analysis for the small-scale regions were tentatively performed. X-ray spectra of the interior can be described with a single-thermal model. The faint interior regions have lower density, higher temperature above 1 keV than that of bright interior regions. The X-ray spectra along the shell can be phenomenally fitted with either a double-vpshock model or a vpshock + powerlaw model. If the non-thermal component is true, N132D would be listed as another X-ray synchrotron SNR.     

基于改进强跟踪ASCKF算法的SINS/GNSS组合对准方法

大方位失准角下的SINS/GNSS组合对准系统呈非线性,采用传统的卡尔曼滤波方法进行初始对准易导致对准精度下降甚至滤波发散。基于此,提出了一种基于改进强跟踪自适应平方根容积卡尔曼滤波算法的组合对准方法。该方法采用QR分解求取协方差的分解因子,并在状态预测方差阵的平方根更新中引入多重渐消因子调整滤波增益;同时,基于Sage-Husa自适应滤波,引入改进的时变噪声估计器实时估计噪声的统计特性。仿真结果表明,采用改进的滤波算法进行大方位失准角下的组合对准,对准精度明显提高。     

基于模型预测的轨道自主快速大机动控制

为改善太阳同步轨道(SSO)卫星轨道大机动经典控制方法的性能,提出了一种基于卫星动力学模型预测的轨道自主机动控制算法,用大推力轨控发动机开环控制加小推力器闭环修正进行控制。给出了制导策略和算法流程。理论分析和仿真结果表明,该控制算法适于卫星轨道自主快速机动控制,其轨控精度较高,收敛时间可满足快速性要求。     

柔性空间结构的分散模糊变结构控制

提出了一种适用于一类不确定大系统的分散变结构控制方法 ,并将该方法用于柔性空间结构的控制系统设计中。考虑到复杂大系统的系统关联及不确定因素复杂 ,在控制律中引入了模糊控制规则来确定分散控制律中的非线性分量大小 ,使控制系统设计时不需知道系统不确定变化及关联的具体情况 ,简化了控制器的设计。同时 ,模糊控制规则的引入还有效减弱了一般分散变结构控制系统的抖颤问题。所设计的控制系统可以保证柔性空间结构系统在未知参数摄动以及外界干扰情况下的稳定。数字仿真结果表明该方法的有效性。