某型飞机角位移自动驾驶仪比例式控制规律设计与仿真

现代飞机越来越复杂的飞行任务对飞机控制系统性能提出了更高要求,而飞机控制系统性能的好坏与飞机自动驾驶仪控制规律设计的优劣关系密切.为此,对某型飞机自动驾驶仪的比例式控制规律进行了分析和设计,仿真研究了控制规律中的速率反馈及位置反馈的作用和选取原则,进而设计出性能良好的飞机角位移自动驾驶仪比例式控制规律.通过大量仿真比较...     

高超声速飞行器舵面热气动弹性分析方法研究

利用修正的牛顿碰撞理论建立平板舵热结构气动力计算模型,完成非定常气动力计算,利用有限元方法建立温度场影响下舵面结构动力学模型,进而完成颤振稳定性分析。研究结果表明高温会导致控制舵颤振稳定性向坏发展。     

超静定捆绑火箭传力路径的组合优化策略

为了获得新一代 大推力捆绑火箭捆绑方案的最优设计参数,针对超静定捆绑传力路径进行分析与优化设计。基于PATRAN的二次开发语言PCL对超静定捆绑火箭进行了参数化建模和仿真分析,并运用拉丁超立方试验方法对传力路径设计参数进行灵敏度分析。在此基础上提出了一种多目标粒子 群和序列二次规划算法的组合优化策略,确定了捆绑联接方案设计参数,实现了对捆绑联接装置和助推器结构载荷的高效优化。计算结果表明：组合优化策略能够将主捆绑联接结构的受力减少了30%左右,明显优于单独使用一种全局优化算法或局部优化算法的优化结果。本文研究成果将为新型捆绑火箭捆绑方案优化设计提供参考。     

直升机旋翼/机身气动干扰的计算方法

应用先进的自由尾迹分析方法,对旋翼／机身的气动干扰进行了计算。该方法建立在桨叶的二阶升力线模型、旋翼的全展自由尾迹模型、机身的源面元模型、旋翼的配平模型的基础上,通过迭代旋翼／尾迹在机身上的诱导速度和机身在桨盘平面、尾迹定位点的诱导速度,形成一个作耦合的综合分析模型。在该模型中,采用“数值解－分析解匹配”的方法建立了一贴近涡／面干扰模型来计入机身对尾迹畸变的影响。作为算例,分别计算了旋翼／机身组合     

原子氧与真空紫外线协同效应对有机涂层的降解作用

为研究真空紫外与原子氧的协同作用,进行了环氧树脂和有机硅树脂的原子氧/真空紫外交互的地面模拟实验,结果表明:在交互作用中,对有机涂层破坏的主导因素是原子氧,真空紫外线起到协同作用,在切断有机高分子材料化学键的同时,为原子氧提供了反应基,加速了原子氧的反应速率.对比真空紫外辐照和原子氧/真空紫外交互实验结果分析中可以发现,有机硅树脂是较好的耐真空紫外辐射和原子氧侵蚀的有机涂层材料.     

一种基于二次组阵的DOA估计方法

提出一种基于二次组阵的信号到达方向估计方法,在阵列中通过划分相互重叠的子阵对指定的空间区域进行空域滤波波束设计实现对空间信号的干扰抑制,提高期望信号的信干噪比。根据子阵间的位置关系对阵列进行二次组阵,用空间谱估计方法实现对各子阵输出期望信号的到达方向（DOA）估计。仿真结果表明：与常规谱估计方法相比,基于二次组阵的DO...     

中国空间技术研究院的标准化卫星平台

首先阐述卫星标准化的三种形式——通用化、系列化和组合化的基本概念和卫星平台实现标准化的必要性;其次介绍了国外公用平台的现状,提出建立卫星公用平台的基本原则;最后给出8种公用平台的自重、平台尺寸、可支承的有效载荷重量、总功率、有效栽荷可用功率、姿态控制精度、测控能力、推进剂携带量、设计工作寿命、与运载火箭的兼容性等主要性能参数及应用前景。     

Adaptive controller design for satellite attached by non-cooperative object

When non-cooperative body attachment occurs in space, the inertia of the new combination and the change of the system’s momentum are unknown. This uncertainty may lead to the instability of the spacecraft’s attitude control. In order to solve this problem, we propose an adaptive control scheme based on the inertia estimation of the new, combined system of non-cooperative body and satellite. This method can allow the new combination of different situations to reach a stable state with a high level of precision and speed. In this paper, the stability of the adaptive control scheme is proven by constructing a Lyapunov function. A simulation environment in which a non-cooperative body attaches to a satellite attaches to is constructed. The simulation shows that the attitude error converges to a small field when using the control scheme, regardless of unfavorable cases, including unknown inertia parameters, added momentum. In addition, the simulation results show the strong robustness of the control scheme for the new combination.     

Improvement of the GRACE star camera data based on the revision of the combination method

The new release of the sensor and instrument data (Level-1B release 02) of the Gravity Recovery and Climate Experiment (GRACE) had a substantial impact on the improvement of the overall accuracy of the gravity field models. This has implied that improvements on the sensor data level can still significantly contribute to arriving closer to the GRACE baseline accuracy. The recent analysis of the GRACE star camera data (SCA1B RL02) revealed their unexpectedly higher noise. As the star camera (SCA) data are essential for the processing of the K-band ranging data and the accelerometer data, thorough investigation of the data set was needed. We fully reexamined the SCA data processing from Level-1A to Level-1B with focus on the combination method of the data delivered by the two SCA heads. In the first step, we produced and compared our own combined attitude solution by applying two different combination methods on the SCA Level-1A data. The first method introduces the information about the anisotropic accuracy of the star camera measurement in terms of a weighing matrix. This method was applied in the official processing as well. The alternative method merges only the well determined SCA boresight directions. This method was implemented on the GRACE SCA data for the first time. Both methods were expected to provide optimal solution characteristic by the full accuracy about all three axes, which was confirmed. In the second step, we analyzed the differences between the official SCA1B RL02 data generated by the Jet Propulsion Laboratory (JPL) and our solution. SCA1B RL02 contains systematically higher noise of about a factor 3–4. The data analysis revealed that the reason is the incorrect implementation of algorithms in the JPL processing routines. After correct implementation of the combination method, significant improvement within the whole spectrum was achieved. Based on these results, the official reprocessing of the SCA data is suggested, as the SCA attitude data are one of the key observations needed for the gravity field recovery.     

滚转振荡指标在再入无人飞行器上的应用研究

深入研究了飞行品质规范中滚转振荡指标的物理意义,探讨了以侧滑相位描述滚转振荡指标的机理,分析了影响滚转振荡指标边界的三个因素。针对再入无人飞行器各飞行阶段,分析了滚转振荡指标的适用性。最后,基于方向舵交叉控制可以减小滚转速率振荡幅值比的控制策略,针对再入无人飞行器对滚转振荡指标的边界进行了初步拓展,为再入无人飞行器飞行品质指标的制定提供了一种思路。