某导弹武器系统可靠性优化

给出了系统可靠性与费用的关系 ,建立了某导弹武器可靠性优化模型 ,用MonteCarlo方法解决了此问题。     

考虑燃料均衡的卫星编队队形重构技术

在卫星编队队形重构过程中,如何在实现编队整体燃料消耗较少的同时使得各子卫星燃料消耗均衡,能够有效地提高卫星编队整体的寿命。提出了一种基于虚拟中心位置可变的卫星编队队形重构新方法。该方法以虚拟中心位置为寻优变量,以首末脉冲时刻可优化的双脉冲规划作为单星轨道机动策略,将编队队形重构问题转化为混合0-1数学规划问题。仿真结果表明,该优化算法在实现整体燃料次优的同时,兼顾了各星当前的燃料剩余水平,实现了各子卫星的燃料均衡。     

分布式小卫星SAR系统GMTI模式构形优化

对分布式小卫星SAR系统地面动目标检测GMTI模式的研究目前正处于广泛探索阶段。如何评价一个分布式卫星系统的GMTI能力，编队构形对GMTI到底有怎样的影响，怎样设计编队使系统GMTI能力最强等问题是文章讨论的内容。从盲速比例的角度出发，提出对系统的GMTI功能进行衡量的定量指标，分析编队构形方式对该指标的具体影响，寻找GMTI模式下可能的编队优化方法。     

基于Simulink的导弹三通道弹道仿真模型

运用MATLAB的Simulink工具箱建立起了导弹三通道弹道仿真模型 ,并给出一定条件下的弹道仿真结果 ,以此证明模型建立的正确性、实用性及兼容性。     

A joint mid-course and terminal course cooperative guidance law for multi-missile salvo attack

Salvo attacking a surface target by multiple missiles is an effective tactic to enhance the lethality and penetrate the defense system. However, existing cooperative guidance laws in the mid-course or terminal course are not suitable for long- and medium-range missiles or stand-off attacking. Because the initial conditions of cooperative terminal guidance that are generally generated from the mid-course flight may not lead to a successful cooperative terminal guidance without proper mid-course flight adjustment. Meanwhile, cooperative guidance in the mid-course cannot solely guarantee the accuracy of a simultaneous arrival of multiple missiles. Therefore, a joint mid-course and terminal course cooperative guidance law is developed. By building a distinct leader-follower framework, this paper proposes an efficient coordinated Dubins path planning method to synchronize the arrival time of all engaged missiles in the mid-course flight. The planned flight can generate proper initial conditions for cooperative terminal guidance, and also benefit an earliest simultaneous arrival. In the terminal course, an existing cooperative proportional navigation guidance law guides all the engaged missiles to arrive at a target accurately and simultaneously. The integrated guidance law for an intuitive application is summarized. Simulations demonstrate that the proposed method can generate fast and accurate salvo attack.     

绳系卫星部署阶段的动力学分析

绳系卫星系统部署阶段末时刻状态决定着其编队飞行的初始状态，为了研究不同因素对绳系卫星系统部署阶段运动的影响，本文建立了一种简单的平面哑铃模型，将系绳视作有阻尼的弹簧，两个卫星视作刚体，考虑重力梯度力矩。通过仿真，发现系绳释放的速度和副星推力是影响绳系卫星系统部署阶段稳定性的主要因素。     

基于量子行为鸽群优化的无人机紧密编队控制

随着军事、民用需求的提高和相关领域的技术推动，无人机编队协同作业已成为当今人们逐渐关注的焦点。无人机紧密编队是指无人机间侧向距离在1~2倍翼展内的编队，因其可有效改善编队中无人机的气动性能而备受瞩目。基于无人机紧密编队条件下的气动耦合效应，建立三维空间下的状态空间方程描述双机相对运动，并推导了紧密编队条件下的双机最优编队构型，在此构型下将人工势场法和编队控制相结合作为控制系统中的间接控制环，并针对基本鸽群优化算法的寻优缺陷利用量子行为规则对其进行改进，将改进后的鸽群优化算法和无人机控制量结合作为控制系统中的直接控制环，最后通过仿真对比验证了此控制系统对于紧密编队控制的有效性。     

战术导弹的一种自校正控制

本文探讨自校正控制理论在战术导弹控制中的应用。采用一种渐近的最小方差自校正控制方案设计导弹自动驾驶仪回路。该方案通过设计自校正控制器的极点和可调增益,使控制器稳定,并能兼顾闭环系统的动态特性,也可使输出方差趋于最小。在两种参考输入信号情况下进行仿真,结果表明,与经典控制情况相比,该方案具有较强的抑制干扰能力,能克服参数变化对系统控制性能的影响,提高了系统的跟踪性能。     

立方体星的技术发展和应用前景

系统论述了立方体星技术发展的三个阶段;从2010-2013年已成功发射的立方体星与纳卫星中挑选了10颗典型卫星,研究分析其技术水平、应用价值和特点优势;并重点论述了立方体纳卫星的应用;最后预测了立方体纳卫星的未来应用前景。     

Diversity of Comets: Formation Zones and Dynamical Paths

The past dozen years have produced a new paradigm with regard to the source regions of comets in the early solar system. It is now widely recognized that the likely source of the Jupiter-family short-period comets (those with Tisserand parameters, T > 2 and periods, P, generally < 20 years) is the Kuiper belt in the ecliptic plane beyond Neptune. In contrast, the source of the Halley-type and long-period comets (those with T < 2 and P > 20 years) appears to be the Oort cloud. However, the comets in the Oort cloud almost certainly originated elsewhere, since accretion is very inefficient at such large heliocentric distances. New dynamical studies now suggest that the source of the Oort cloud comets is the entire giant planets region from Jupiter to Neptune, rather than primarily the Uranus-Neptune region, as previously thought. Some fraction of the Oort cloud population may even be asteroidal bodies formed inside the orbit of Jupiter. These comets and asteroids underwent a complex dynamical random walk among the giant planets before they were ejected to distant orbits in the Oort cloud, with possible interesting consequences for their thermal and collisional histories. Observational evidence for diversity in cometary compositions is limited, at best. This revised version was published online in June 2006 with corrections to the Cover Date.