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.     

Single-event upset in geostationary transfer orbit during solar-activity maximum period measured by the Tsubasa satellite

This paper reports single-event upset (SEU) occurrence related to the space radiation environment in geostationary transfer orbit during solar-activity maximum period measured by the Tsubasa satellite. Most SEUs are measured in the inner radiation belt, indicating that they are mainly caused by trapped protons. Thus, the spatial distribution and the temporal variation of the SEU count correlate well with those of trapped protons. The peak SEU rate appears around L = 1.4. The transition point from SEUs caused by trapped protons to those caused by galactic cosmic rays is around L = 2.6. During the experiment period, increased SEU count was sometimes detected due to solar and geomagnetic events outside the inner radiation belt.     

Lyapunov-based switched-gain impact angle control guidance

To hit stationary ground targets in specified direction, a nonlinear impact angle control guidance law based on Lyapunov stability theory is proposed. The proposed law ensures the convergence of the heading angle and the miss distance to guarantee a successful engagement. The impact angle can be adjusted by varying a single parameter. And the maximum value of acceleration has been analyzed to get the proper range for control parameter. Considering the achievable impact angle set is limited, an additional phase is added to form a two-phase control strategy. The first phase is to establish a proper initial condition for the second phase, and the second phase is to hit the target with a certain impact angle. An analysis of the proper selection of control parameters to expand the achievable impact angle set is presented. The performance of the proposed guidance law is illustrated with simulations.     

静偏心对挤压油膜阻尼器减振特性影响的 数值分析

由于装配误差或重力等原因,挤压油膜阻尼器在实际使用中难以避免产生静偏心。为了研究静偏心对挤压油膜阻尼器减振特性的影响,基于广义雷诺方程推导出静偏心条件下挤压油膜阻尼器雷诺方程并建立了静偏心挤压油膜阻尼器-转子系统的动力学模型,随后运用数值积分获取静偏心下转子系统的非线性响应。研究表明:转子进动半径随着静偏心增大而减小;静偏心显著影响转子轴心轨迹,静偏心时转子轴心轨迹在大多数转速下近似为椭圆而不再是圆,静偏心下突加不平衡响应瞬态振幅远高于无静偏心条件下瞬态振幅。     

基于空间隔离的低轨卫星系统频谱共享方法

随着业务需求的全球性增长,传统低频波段有限的频谱资源已不能满足低轨（LEO）卫星的业务承载要求,采用Ka频段的LEO星座系统设计成为了主流。然而,采用Ka频段的LEO星座系统不可避免地会对同频段已经存在的静止轨道（GEO）卫星系统产生干扰。首先,通过基于空间隔离的干扰规避方法,采用对LEO与GEO的频谱共用系统设置隔离角来进行上下行场景的干扰消除,使该LEO系统能满足国际电信联盟（ITU）对同频段内通信干扰的约束条件;然后,通过引入GEO带的概念,分析并研究了干扰规避区域的确定方法和其对LEO星座密度的影响。最后,通过仿真得出了干扰隔离角、GEO带与LEO星座密度的关系,得到了在采用隔离角的方式进行干扰避让时满足LEO星座系统业务不中断所需要的最小卫星数量,对LEO星座设计具有一定的指导意义。      

一种多目标区域多轨道星座设计方法

在有限资源条件下,针对多目标区域的对地观测问题是航天器轨道设计、在轨任务规划中的重要问题。卫星效能的充分发挥基于科学的卫星星座设计。围绕多区域多轨道星座设计问题:首先,结合运载器实际能力,确定轨道类型和设计变量;然后,根据轨道外推、星下点轨迹、探测区域等算法,提出重访时间的计算方法,以最大重访时间作为星座性能指标,采用多层嵌套变量搜索方法实现星座设计;最后,对 1个具体任务进行实例设计。结果表明,采用该方法能够设计出满足指标要求的星座,具有可行性。     

液体火箭发动机基于非线性理论的稳定性分析方法

以液氧/煤油单台空间发动机的起动过程和平稳工况为研究对象,在改变推力室喷管喉部直径的情况下,运用非线性领域中的分析方法,对系统在整个相空间的表现行为作了全局分析比较。综合考虑相空间吸引子、李雅普诺夫指数以及分维数,提出了一种新的研究系统稳定性分析方法——轨道稳定性分析法。该方法具有几何学直观的优点,易于在计算机上实现。