有限推力下相对绕飞轨道的直接形成

提出了一种有限推力下主动航天器在完成轨道转移的同时形成相对目标航天器绕飞的方法。根据以改进春分点轨道根数表示的非奇异轨道摄动方程,用变分方法将问题转化为经典的最优控制,由相对运动动力学获得主动航天器实现绕飞须满足的终端约束条件,再用非线性规划求解。给出了求解模型。理论分析和仿真结果表明,该方法理论上可行,但为减少干扰产生的偏差,还需对绕飞形成过程中的导引率进行研究。     

固体火箭发动机前封头人工脱粘层烧蚀研究

从理论分析的角度出发．通过对人工脱粘层和绝热层所构成的槽缝燃气温度场与烧蚀的耦合计算，得出了人工脱粘层的烧蚀规律。在计算中，采用了隐式差分格式及控制容积法等计算技术，并采用了先进的烧蚀模型。为模拟发动机静止与飞行两种不同状态，本文对不同宽度的槽缝人工脱粘层的烧蚀进行了计算，对其进行了比较。本文所采用的方法可供今后人工脱粘层的设计参考。     

火箭基组合循环(RBCC)发动机性能分析

介绍了采用引射火箭模式的RBCC发动机工作原理,并在对其概念设计模型进行简化的基础上,进行了RBCC发动机系统性能分析,评估了RBCC发动机系统主要设计参数(发动机系统出口截面直径和燃料化学反应后的总温)的变化对其性能(推力、推力系数和比冲)的影响,认为:1)燃料经过加热后,推力和推力增益都上升了69.97%,比冲增加了180.18%;2)随着二次燃烧过程中燃烧室温度的上升,发动机的推力、推力增益和比冲得到了很大的提高,火箭发动机的性能得到了很好的改善;3)随着RBCC发动机系统出口截面直径的增加,尾气对发动机的反推力、推力增益以及比冲急剧下降,不利于其性能的改善。     

燃烧室新材料在卫星双组元低推力发动机上的应用

对有代表性、有发展前途的几种新材料进行比较 ,并根据应用新材料的低推力发动机燃烧室的结构特点 ,分析了不同冷却方式对双组元低推力发动机性能损失的影响 ,为双组元低推力发动机燃烧室的材料选择、加工工艺、设计优化提供参考。     

基于双量程推力传感器的精确测力技术

针对双量程推力传感器在使用中测试精度低的问题,结合传感器固有特性,开展了传感器动态特性分析及误差补偿方法的研究。通过有限元分析和力锤冲击试验,结合结构分析获得了双量程力传感器等效二自由度和三自由度动力学模型。利用近似求积数值法对冲击力试验输出信号进行补偿,获得了接近标准信号的测试结果,对该补偿方法进行了有效性验证。结果显示:本方法对发动机试验的推力信号进行了补偿,推动了单室双推力发动机推力的精确测量,为双推力发动机的推力测试提供了有效途径。     

单OSV服务多卫星的转移轨道优化研究

利用混合法解决了有限推力作用下单OSV服务多卫星的转移轨道优化问题.首先从OSV携带燃料的角度出发,初步筛选出在其服务范围内的服务对象,基于双脉冲交会假设,确定了服务序列以及时间节点;其次针对每一段转移轨道,利用Pontryagin极小值原理推导出最优控制律,设定开-关-开的发动机工作方式,将初始协态变量和开关机时间进行参数化处理,采用遗传算法对非线性规划问题进行求解;最后对整条轨道进行拼接优化.仿真结果表明,混合法对协态变量初值猜测敏感性小,降低了搜索最优转移轨道的难度,且控制轨线光滑.     

A lunar cargo mission design strategy using variable low thrust

A design technique for a near optimal, Earth–Moon transfer trajectory using continuous variable low thrust is proposed. For the Earth–Moon transfer trajectory, analytical and numerical methods are combined to formulate the trajectory optimization problem. The basic concept of the proposed technique is to utilize analytically optimized solutions when the spacecraft is flying near a central body where the transfer trajectories are nearly circular shaped, and to use a numerical optimization method to match the spacecraft’s states to establish a final near optimal trajectory. The plasma thruster is considered as the main propulsion system which is currently being developed for crewed/cargo missions for interplanetary flight. The gravitational effects of the 3rd body and geopotential effects are included during the trajectory optimization process. With the proposed design technique, Earth–Moon transfer trajectory is successfully designed with the plasma thruster having a thrust direction sequence of “fixed-varied-fixed” and a thrust acceleration sequence of “constant-variable-constant”. As this strategy has the characteristics of a lesser computational load, little sensitivity to initial conditions, and obtaining solutions quickly, this method can be utilized in the initial scoping studies for mission design and analysis. Additionally, derived near optimal trajectory solution can be used as for initial trajectory solution for further detailed optimization problem. The demonstrated results will give various insights into future lunar cargo trajectories using plasma thrusters with continuous variable low thrust, establishing approximate costs as well as trajectory characteristics.     

过失速下俯敏捷性及纵向控制效能需求研究

结合飞行安全和作战效能需求,对过失速战斗机的大迎角/过失速迎角下俯敏捷性指标及纵向控制效能需求进行了研究.为了满足飞行品质和过失速敏捷性指标要求,采用非线性动态逆方法设计了某推力矢量飞机快回路和慢回路飞行控制律.在此基础上,根据过失速下俯敏捷性和滚转敏捷性指标要求,对所需的最小俯仰推力矢量偏角进行了计算分析,所得结果对先进战斗机的设计有一定的参考价值.     

Sailing at the brink – The no-limits of near-/now-term-technology solar sails and SEP spacecraft in (multiple) NEO rendezvous

Near-Earth object (NEO) in-situ exploration can provide invaluable information for science, possible future deflection actions and resource utilisation. This is only possible with space missions which approach the asteroid from its vicinity, i.e. rendezvous. This paper explores the use of solar sailing as means of propulsion for NEO rendezvous missions. Given the current state of sail technology, we search for multiple rendezvous missions of up to ten years and characteristic acceleration of up to 0.10 mm/s². Using a tree-search technique and subsequent trajectory optimisation, we find numerous options of up to three NEO encounters in the launch window 2019–2027. In addition, we explore steerable and throttleable low-thrust (e.g. solar-electric) rendezvous to a particular group of NEOs, the Taurid swarm. We show that an acceleration of 0.23 mm/s² would suffice for a rendezvous in approximately 2000 days, while shorter transfers are available as the acceleration increases. Finally, we show low-thrust options (0.3 mm/s²) to the fictitious asteroid 2019 PDC, as part of an asteroid deflection exercise.