Dynamics of a spacecraft and normalization around Lagrangian points in the Neptune–Triton system

The problem of a spacecraft orbiting the Neptune–Triton system is presented. The new ingredients in this restricted three body problem are the Neptune oblateness and the high inclined and retrograde motion of Triton. First we present some interesting simulations showing the role played by the oblateness on a Neptune’s satellite, disturbed by Triton. We also give an extensive numerical exploration in the case when the spacecraft orbits Triton, considering Sun, Neptune and its planetary oblateness as disturbers. In the plane a × I (a = semi-major axis, I = inclination), we give a plot of the stable regions where the massless body can survive for thousand of years. Retrograde and direct orbits were considered and as usual, the region of stability is much more significant for the case of direct orbit of the spacecraft (Triton’s orbit is retrograde). Next we explore the dynamics in a vicinity of the Lagrangian points. The Birkhoff normalization is constructed around L₂, followed by its reduction to the center manifold. In this reduced dynamics, a convenient Poincaré section shows the interplay of the Lyapunov and halo periodic orbits, Lissajous and quasi-halo tori as well as the stable and unstable manifolds of the planar Lyapunov orbit. To show the effect of the oblateness, the planar Lyapunov family emanating from the Lagrangian points and three-dimensional halo orbits are obtained by the numerical continuation method.     

导引头量测故障下的增量式三维制导律设计

考虑导引头量测故障下拦截机动目标的末制导问题,以提高制导系统的鲁棒性、降低制导增益、减小系统残差、避免视线角速率剧烈振荡/发散为目的,基于增量式控制方法设计了一种具有鲁棒增强特性的三维末制导律。首先,将末制导问题转化为零化视线角速率的控制问题。其次,通过弹目相对距离及视线角速率定义辅助变量,给出传统的滑模制导律作为设计参考。然后,基于增量式非线性动态逆滑模控制方法,充分挖掘视线角加速度估计信息及上一采样时刻的制导指令,得到增量式三维鲁棒制导律。最后,在目标机动及导引头量测故障下,分析并比较了两种制导律所产生的系统残差。理论分析及多工况仿真结果表明,增量式制导律不仅对目标机动及大范围失效的导引头量测故障具有强鲁棒性,而且所需制导增益也较小,同时避免了末端视线角速率严重发散的问题     

LYAPUNOV-TYPE STABILIZATION FOR NONLINEAR UNCERTAIN SYSTEMS AND NONLINEAR H~∞ CONTROL

ＬＹＡＰＵＮＯＶ┐ＴＹＰＥＳＴＡＢＩＬＩＺＡＴＩＯＮＦＯＲＮＯＮＬＩＮＥＡＲＵＮＣＥＲＴＡＩＮＳＹＳＴＥＭＳＡＮＤＮＯＮＬＩＮＥＡＲＨ∞ＣＯＮＴＲＯＬＦｅｉＳｈｕｍｉｎ（ＲｅｓｅａｒｃｈＩｎｓｔｉｔｕｔｅｏｆＡｕｔｏｍａｔｉｏｎ，ＳｏｕｔｈｅａｓｔＵ...     

自旋火箭姿态运动的稳定性分析和数学仿真

本文主要对自旋火箭姿态运动的稳定性进行了分析,并给出了数学仿真结果。飞行试验结果表明,稳定性分析和数学仿真是正确、可靠的。     

Event-triggered attitude control of spacecraft

The problem of spacecraft attitude stabilization control system with limited communication and external disturbances is investigated based on an event-triggered control scheme. In the proposed scheme, information of attitude and control torque only need to be transmitted at some discrete triggered times when a defined measurement error exceeds a state-dependent threshold. The proposed control scheme not only guarantees that spacecraft attitude control errors converge toward a small invariant set containing the origin, but also ensures that there is no accumulation of triggering instants. The performance of the proposed control scheme is demonstrated through numerical simulation.     

遗传算法在机翼气动优化设计中的应用

把最优化方法与机翼的气动力求解相结合,进行跨音速机翼的气动优化设计。采用最优化方法为遗传算法,机翼的气动力由三维欧拉方程的数值解来提供。与基准机翼相比较,优化设计的机翼其气动性能有较大幅度的提高,表明遗传算法在机翼优化设计中的可行性和有效性     

涡轮叶栅端壁区流动的实验研究

本文在大尺寸低速开式叶栅传热风洞中对一种高压涡轮导向叶栅中的流场进行了实验研究。采用五孔针对5个雷诺数下的叶栅端壁区三维流场进行了测量,并用线簇和小球浮动法对5个工况的流动进行了流场显示。实验结果表明:马蹄涡压力面分支在向吸力面运动的过程中,破坏了来流附面层的结构,在马蹄涡压力面分支之后,叶栅通道中产生了一个新的从压力面到吸力面的新附面层,新附面层的厚度小于来流附面层厚度;三维流动区约占叶栅通道的40%;雷诺数的增大将增强端壁区的三维流动。从流场显示图片可以观测叶片吸力面靠近端壁的角涡形成与发展,以及吸力面上的三角形区域;流场显示的通道涡大小与流场测量结果吻合。本文的实验结果有助于分析端壁表面和叶片表面换热特性的形成机理。      

“风云一号” B 卫星姿态控制系统

“风云一号”气象卫星姿态控制系统采用了三轴稳定对地定向的主动控制方案。已发射了两颗（Ａ、Ｂ）卫星,其中Ｂ星是在Ａ星主控系统的基础上,增加了一个完整的备份系统,采取一系列冗余措施并设计全方位姿态重新捕获的故障对策。经飞行试验及在轨故障应急处理证明,系统设计是完善和成功的,其中反作用飞轮控制、偏置动量控制、磁章动进动和飞轮卸载控制、全方位姿态重新捕获方案在中国是首次采用,均取得了较好的飞行效果,为长寿命卫星姿态控制系统的设计积累了宝贵经验。     

机载红外搜索跟踪系统关键技术分析

概述了红外搜索跟踪系统的组成及主要技术特点,对红外成像系统中的红外望远光学系统、红外探测器组件等进行了分析;探讨了稳定与瞄准系统实现方案;对图像跟踪器中的跟踪算法及工程实现中采取的措施进行了论述。     

Alternative transfer to the Earth–Moon Lagrangian points L4 and L5 using lunar gravity assist

Lagrangian points L4 and L5 lie at 60° ahead of and behind the Moon in its orbit with respect to the Earth. Each one of them is a third point of an equilateral triangle with the base of the line defined by those two bodies. These Lagrangian points are stable for the Earth–Moon mass ratio. As so, these Lagrangian points represent remarkable positions to host astronomical observatories or space stations. However, this same distance characteristic may be a challenge for periodic servicing mission. This paper studies elliptic trajectories from an Earth circular parking orbit to reach the Moon’s sphere of influence and apply a swing-by maneuver in order to re-direct the path of a spacecraft to a vicinity of the Lagrangian points L4 and L5. Once the geocentric transfer orbit and the initial impulsive thrust have been determined, the goal is to establish the angle at which the geocentric trajectory crosses the lunar sphere of influence in such a way that when the spacecraft leaves the Moon’s gravitational field, its trajectory and velocity with respect to the Earth change in order to the spacecraft arrives at L4 and L5. In this work, the planar Circular Restricted Three Body Problem approximation is used and in order to avoid solving a two boundary problem, the patched-conic approximation is considered.