基于强化学习的在轨目标逼近

从强化学习的角度,对在轨目标逼近问题进行研究,设计了一种整合制导与控制的端到端的算法.首先对在轨目标逼近问题进行数学建模;然后对强化学习算法原理进行简介,根据问题特点分析不同强化学习框架的优劣,确定以DDPG作为算法框架,并设计了基于强化学习的在轨目标逼近算法;最后通过仿真验证,分析了基于强化学习逼近算法的优劣性.     

脉冲星方位误差估计的两步卡尔曼滤波算法

为了克服钟差和卫星位置误差对脉冲星方位误差估计的影响，设计了两步卡尔曼滤波（TSKF）算法。首先，介绍了脉冲星方位误差估计的传统模型，并通过分析和仿真验证了钟差、卫星位置误差以及2种误差同时存在时会使脉冲星方位误差估计结果产生较大偏差。其次，在传统的估计模型中加入了钟差和卫星位置误差，并将钟差和钟差变化率增广为新的状态量，从而推导出包含2种误差的新模型，并证明了该模型的完全可观测性；根据该模型并按照两步卡尔曼滤波原理，得到了TSKF算法的步骤。最后，通过仿真表明:在钟差和卫星位置误差同时影响下，传统脉冲星方位误差估计算法偏差较大且发散；TSKF算法则能够有效隔离2种误差的影响，使赤经和赤纬误差估计达到0.2 mas之内的精度。      

微纳聚合体卫星的对称式重构规划算法

为解决微纳聚合体卫星变构过程中，聚合体各部分之间的动力学耦合导致的卫星整体姿态翻转或紊乱，提出了一种对称式变构规划算法。首先建立了铰链约束下的漂浮基多刚体系统动力学模型，研究了重构过程中各运动模块对本体姿态的影响，提出当每两个运动模块位置与转动方向满足对称性条件时，两者对本体姿态的影响可在一定程度上相互抵消。基于上述理论，在A*算法中引入最优分配度量和对称性判定，设计了并行对称重构规划算法。仿真结果表明，该规划算法可实现重构过程中多模块并行、对称运动，重构过程总步数较少，运动模块对本体姿态的影响小。     

Maximal admissible mode decision delay in terminal guidance

Mode decision-maker is a critical component in the logic-based Integrated Estimation and Guidance(IEG) system. For the best possible estimation and guidance performance, the mode decision delay of the mode decision-maker should be limited to a range as small as possible. This paper presents a numerical method for computing the maximal admissible mode decision delay that varies with time-to-go. Particular attention has been paid to highly maneuvering target interception in terminal guidance. The results of this research offer useful guidelines for the design of the mode decision-maker in IEG systems.     

空间低温杜瓦瓶凯夫拉支撑结构多约束优化设计

采用新型凯夫拉纤维作为某空间用小型低温杜瓦瓶的支撑材料，在验证其力学性能的基础上，设计了杜瓦瓶的支撑结构，建立了一种新的热力学耦合优化模型，给出支撑结构固有频率、热应力及发射环境下的约束条件，通过一种“离散点加密”新约束优化法计算出了支撑结构满足约束条件范围内的要求的最优设计参数。     

固体火箭冲压发动机设计点性能优化分析

针对冲压动力飞行器射程优化总体需求，提出了基于飞行器-发动机性能因子的评估方法，建立了固体火箭冲压发动机性能模型及优化设计流程，为总体与动力一体化优化设计提供了支撑。根据典型含硼贫氧推进剂性能分析结果可知，相同马赫数及余气系数下，高度对比冲的影响不明显；相同马赫数下，比冲随余气系数的增加先增加后减小；相同余气系数下，比冲随马赫数的增加而降低；飞发性能因子随马赫数、余气系数的增加先增加后降低，在一定条件下达到最大值。      

高温环境下大尺度薄壁结构的电性能优化设计

考虑温度引起的热变形和材料电磁参数变化对天线罩电性能的影响,基于口径积分-表面积分法(AI-SI)和有限元法(FEM),提出了高温环境下天线罩电性能分析方法;进而基于粒子群算法(PSO),建立了计及热效应的天线罩结构电性能优化流程。分别选取常温环境、均匀高温环境和非均匀高温环境三种典型工况,对比研究了温度对天线罩电性能的影响规律,并对天线罩电性能进行了优化,研究结果表明:高温会引起天线罩透波系数的下降和瞄准误差的上升,在天线罩优化设计中应重视温度对电性能的影响;计及热效应的天线罩结构电性能优化方法能显著提升天线罩的透波系数、降低瞄准误差,具有良好的优化效果。     

静压气浮轴承工程设计方法研究

静压气浮轴承是惯性器件测试平台回转支撑轴系的关键部件，其承载能力和回转精度对惯性器件测试的准确性有着重要的影响，目前，静压气浮轴承设计、计算过程复杂，为提高设计效率，简化设计方法，在满足静压气浮轴承性能的条件下，推导了静压气浮轴承工程计算公式，在此基础上，设计了一款双向止推空气轴承，确定了几何参数，计算了空气静压径向轴承、空气静压止推轴承的轴承承载力、刚度、耗气量及摩擦力矩，并与有限元仿真结果进行了对比分析，验证了该设计方法的有效性。     

Research on navigation of satellite constellation based on an asynchronous observation model using X-ray pulsar

Pulsar navigation is a promising navigation method for high-altitude orbit space tasks or deep space exploration. At present, an important reason for restricting the development of pulsar navigation is that navigation accuracy is not high due to the slow update of the measurements. In order to improve the accuracy of pulsar navigation, an asynchronous observation model which can improve the update rate of the measurements is proposed on the basis of satellite constellation which has a broad space for development because of its visibility and reliability. The simulation results show that the asynchronous observation model improves the positioning accuracy by 31.48% and velocity accuracy by 24.75% than that of the synchronous observation model. With the new Doppler effects compensation method in the asynchronous observation model proposed in this paper, the positioning accuracy is improved by 32.27%, and the velocity accuracy is improved by 34.07% than that of the traditional method. The simulation results show that without considering the clock error will result in a filtering divergence.     

Simulation and analysis of chemical release in the ionosphere

Ionospheric inhomogeneous plasma produced by single point chemical release has simple space-time structure, and cannot impact radio wave frequencies higher than Very High Frequency (VHF) band. In order to produce more complicated ionospheric plasma perturbation structure and trigger instabilities phenomena, multiple-point chemical release scheme is presented in this paper. The effects of chemical release on low latitude ionospheric plasma are estimated by linear instability growth rate theory that high growth rate represents high irregularities, ionospheric scintillation occurrence probability and high scintillation intension in scintillation duration. The amplitude scintillations and the phase scintillations of 150?MHz, 400?MHz, and 1000?MHz are calculated based on the theory of multiple phase screen (MPS), when they propagate through the disturbed area.