火星进入段纵向脱敏局限性分析与三自由度脱敏设计

针对火星进入段制导存在的“进入状态偏差”问题进行脱敏轨迹设计研究,以增强制导鲁棒特性,提升末端状态精度。首先分析倾侧角反转逻辑对弱机动能力航天器制导精度的影响,结果表明, 存在倾侧角调整性能约束时,反转逻辑会引起末端状态偏差并使系统对进入状态偏差敏感度上升,当制导采用现有纵向脱敏方法时其影响尤为突出,会导致严重失效问题;然后在解决敏感度传播奇异问题的基础上提出三自由度脱敏设计。其主要思路是轨迹优化中采用三自由度动力学方程,而敏感度罚项仍由纵向敏感度传播方程得出。蒙特卡洛仿真结果表明本文方法对进入状态偏差具有显著增强的鲁棒性能。     

不同粒径颗粒在涡轮流道内沿程温度及其与叶片的撞击特性研究

涡轮叶片表面的颗粒沉积会影响其气动性能和冷却效率,因此很有必要开展颗粒在流道内的运动、温度及其在涡轮叶片表面的撞击特性研究。基于离散相模型,采用CFD数值模拟了涡轮流道内的燃气流动以及不同粒径颗粒在涡轮流道内的运动轨迹与沿程温度变化,并获得了颗粒与涡轮叶片的撞击特性。模拟结果表明,随着颗粒粒径由1μm增加至200μm,颗粒在涡轮流道内的随流性变差,颗粒在流道内的撞击、反弹现象加剧,这促使颗粒在流道内的运动路程整体呈上升趋势;颗粒粒径的增大还会导致颗粒散热能力下降,促使颗粒的沿程温降逐渐降低;同时,颗粒粒径的增大会导致颗粒在导叶片表面的撞击系数上升,而动叶则与之相反。     

基于Bi-LSTM 的无人机轨迹预测模型及仿真

传统轨迹预测模型存在模型简化较大、考虑因素较少等问题。结合飞行轨迹连续性、时序性、交互性 的特点,提出基于双向长短期记忆(Bi-LSTM)神经网络的轨迹预测模型,将入侵者的位置、姿态和两机的相对 信息同时作为轨迹预测模型的输入,更加符合真实轨迹变化规律;对建立的基于 Bi-LSTM 的轨迹预测模型采 用综合考虑动量和速度的自适应调整学习步长的学习算法进行训练;并与基于 Elman神经网络的轨迹预测模 型进行仿真对比分析。结果表明:与基于 Elman神经网络的轨迹预测模型相比,所提模型在不同方向预测200 个点的平均绝对误差不超过4m,三维预测效果更优,可以较为准确地进行轨迹预测。     

用加速度计的积分遥测量计算弹道参数及轨道要素

文章提供利用运载火箭特征点(关机点,入轨点等)的有关加速度计的积分遥测量计算该点的弹道参数和轨道要素的计算方法。     

基于脱靶量数据的发射系航迹参数求解方法

针对当前海态巡航飞行试验末段外测无法跟踪测量的实际问题,基于现有脱靶量测量系统,建立了利用某脱靶量测量数据到发射系的转换模型。此模型将脱靶量测量数据统一到发射系航迹中,有利于航迹分析工作。并建立了转换结果的误差估计模型,误差模型充分考虑了脱靶量测量误差、靶船定位误差以及靶船航向角误差。利用仿真数据对转换模型及误差模型进行了计算验证。结果表明,位置误差满足精度要求。该方法对延拓外测处理时段具有积极意义。     

基于逆多项式轨迹成形法的小推力轨道设计

轨迹成形法是一种基于反向设计思想的轨道设计方法,它假设待研究的轨道呈现某一形状,利用数学曲线进行逼近从而得到设计结果.逆多项式轨迹成形法为小推力地球转移轨道设计和数值求解最优轨迹过程中初值的选取提供了新的研究思路.首先结合轨道动力学方程和逆多项式曲线模型给出了轨迹成形法的设计过程,并在考虑时间约束的情况下对小推力转移轨道进行设计.仿真结果表明逆多项式轨迹成形法适宜于小推力转移轨道设计,并且其设计结果是一组近优解,可以作为求取精确最优轨迹的初值猜测.     

基于逆动力学的柔性连杆机械臂的混合模糊控制

利用假设模态法建立了柔性连杆机械臂的逆动力学方程,提出了一种并行于常规开环逆动力学控制的混合模糊控制方法对其进行末端轨迹跟踪。设计的控制器由两部分组成,一部分为根据结构的逆动力学以及机械臂末端所需跟踪的轨迹计算出控制力;另一部分为通过末端位置的实测与给定轨迹的偏差,利用一个辅助模糊控制对控制量进行调整,构成输出反馈部分。通过数字仿真,并与常规模糊控制结果的比较,表明借助于结构逆动力学,可以降低模糊控制器对知识库的需求,获得较好的控制稳态性能。     

Trajectory optimization of multiple asteroids exploration with asteroid 2010TK7 as main target

In this study, the Earth’s Trojan asteroid 2010 TK₇ is selected as the rendezvous target. The multiple flyby sequence of asteroid exploration was proposed by optimizing the probe’s orbit. Impulsive maneuvers and low-thrust propulsion were used respectively to design the trajectories of the multiple asteroids exploration mission. Under impulsive maneuvers, gravity assist technique was adopted to reduce fuel consumption. First a reference orbit with only 2010 TK₇ as the rendezvous target was designed. Then five asteroids near the reference orbit were selected as candidates. Finally, we obtained a multiple asteroids exploration sequence of three asteroids based on gravity assist technique and genetic algorithm, and an additional velocity impulse of 0.4?km/s was required. In the subsequent section, a sixth-degree inverse polynomial shape-based method is applied to the low-thrust trajectory design of 2010 TK₇, and the exploration sequence under the action of low-thrust propulsion was provided.     

Titan’s new pole: Implications for the Huygens entry and descent trajectory and landing coordinates

The European Space Agency’s Huygens probe separated from the NASA Cassini spacecraft on 25 December 2004, after having been attached for a 7-year interplanetary journey and three orbits around Saturn. The probe reached the predefined NASA/ESA interface point on 14 January 2005 at 09:05:52.523 (UTC). It performed a successful entry and descent sequence and softly landed on Titan’s surface on the same day at 11:38:10.77 (UTC) with a speed of about 4.54 m/s. Since the publication of the official project entry and descent trajectory reconstruction effort by the Descent Trajectory Working Group in 2007 (referred to as DTWG#4) various other efforts have been performed and published. This paper presents an overview of the most relevant reconstructions and compares their methodologies and results. Furthermore, the results of a new reconstruction effort (DTWG#5) are presented, which is based on the same methodology as DTWG#4 but takes into account new estimates of Titan’s pole coordinates which were derived from radar images of different Cassini Titan flybys. It can be shown that the primary effect can be observed in the meridional direction which is represented by a stark southward shift of the trajectory by about 0.3 deg. A much smaller effect is seen in the zonal direction (i.e., less than 0.01 deg in the west to east direction). The revised probe landing coordinates are 192.335 deg W and 10.573 deg S. A comparison of these coordinates with results of recent landing site investigations using visual and radar images of the Cassini VIMS instrument shows excellent agreement of the two independently derived landing coordinates, i.e., longitude and latitude residuals of respectively 0.035 deg and 0.007 deg.     

基于自适应高斯伪谱法的SGCMG无奇异框架角轨迹规划

针对采用SGCMG作为姿态执行机构的小卫星,在大角度机动过程中SGCMG系统易陷入奇异的问题,提出了一种基于自适应Gauss伪谱法的SGCMG无奇异框架角轨迹快速规划方法。该算法综合考虑到实际工程应用中存在的SGCMG框架角受限、框架角速度受限,奇异量度受限,星体机动角速度受限以及星体初始和终端状态受限等约束条件,将卫星大角度机动问题看成满足上述一系列约束条件和边界条件同时实现某一性能指标最优的最优控制问题。然后,结合自适应高斯伪谱法与非线性规划技术,求解带有边界约束与路径约束的最优化问题,获得实现性能指标最优的无奇异SGCMG系统轨迹。仿真结果表明：该算法能够在25s的时间内给出顺利实现大角度机动并满足所有约束条件,同时近似精度优于10 -3 的高精度平滑轨迹。