自循环机匣处理周向覆盖比例和喷嘴轴向位置对轴流压气机扩稳效果的影响

为了揭示自循环机匣处理周向覆盖比例和喷嘴轴向位置对扩稳效果的影响规律,在固定引气位置于叶顶阻塞区域的前提下,设计了6个不同周向覆盖比例和4个不同喷嘴轴向位置的自循环机匣处理结构,并以一个高亚声速轴流压气机转子为研究对象进行了数值模拟。结果表明:随着周向覆盖比例增大,压气机的综合稳定裕度先增大后减小,峰值效率则单调降低,综合稳定裕度改进量最大的周向覆盖比例为90%,兼顾扩稳效果和效率损失的最佳周向覆盖比例为30%。随着喷嘴位置由叶顶前缘沿轴向逐渐前移,压气机的扩稳效果变化不大,但效率有所提升,而且喷嘴位置越往前移,效率提升越多。     

采用多重交点判别的传感器网络覆盖控制协议

在保证一定的覆盖质量前提下,延长传感器网络生存时间,提出一种以充分必要条件判断网络节点冗余性的分布式覆盖控制协议.该协议通过多重交点判别法则(MIER,Multi-Intersection Estimation Rule)对无线传感器网络进行分布式节点的动态休眠控制,从理论上证明了MIER法则是判断网络节点冗余性的充分必要条件,能保证目标区域不出现覆盖盲点同时使活跃节点数降至最低.实验表明,MIER法则比CCP法则有了很大改进,消除由于法则本身引起的盲点数目,能更好的运用于覆盖控制协议中,更为准确的判断节点是否应该工作或休眠,是判别节点是否冗余的充分必要条件;同时比Ottawa法则更加高效的减少整个网络功耗,延长网络寿命.     

社交网络中谣言传播动力学研究

社交网络已成为谣言发酵与传播的主要媒介之一,因此有必要研究谣言在社交网络上的传播规律。本文结合时空滞后、空间扩散、媒体报道等因素对社交网络中谣言传播的影响,建立新的社交网络谣言时空传播模型。利用偏泛函微分方程理论,给出模型的稳定性以及发生Hopf分岔的判别条件。数值仿真显示时滞可以影响模型的收敛速度及改变模型的稳定性,同时,媒体对社交网络谣言的深度报道可以极大地减小网络中谣言传播者密度,并扩大系统的稳定区域。 最后,给出一些社交网络谣言传播控制策略。     

无人机中继平台覆盖区域统计模型

针对中继信号覆盖区域确定性模型没有考虑信道随机衰落影响的问题,提出了一种基于中断概率的无人机（UAVs）中继平台信号覆盖半径统计模型。通过将中继链路建模为包含路径损耗、阴影衰落和多径衰落的复合分布模型,推导获得中继信号覆盖半径的概率分布,并给出一种利用中断概率数值求解覆盖半径的方法。仿真结果表明,信道衰落对覆盖半径影响非常大,当中断概率小于10%时,覆盖半径仅为无衰落信道时的一半。研究结果对移动自组织网络（MANETs）中的中继网络的无人机最优布置、飞行策略以及网络性能评估等具有重要的参考价值。     

基于布尔感知模型的边界线多重覆盖算法

无线传感器网络监视预警系统的区域边界具有特殊重要性,针对节点的布尔感知模型,根据节点感知圆盘的相互关系,可将整条边界线划分为不可再分割的可数个最小曲线段,利用改进的贪婪式算法研究了集中式多重覆盖算法和分布式多重覆盖算法,通过仿真实验,验证了多重覆盖带来的高检测概率以及高覆盖概率。     

间接Legendre伪谱法的欠驱动航天器姿态运动轨迹跟踪

针对仅带有两组喷气推力器的非轴对称欠驱动刚性航天器,提出一种基于间接Legendre伪谱法的姿态运动轨迹跟踪控制算法。首先采用Legendre伪谱法(LPM)离线规划出系统的最短时间姿态机动参考轨迹。接着将实际运行轨迹与参考轨迹之间的偏差作为变量,根据Pontryagin极小值原理必要条件把系统姿态运动跟踪问题转化为一个两点边值问题(TPBVP)。最后采用 Legendre-Gauss-Lobatto(LGL)点将此两点边值问题离散转化为一个线性方程组来求解,避免了对传统Riccati微分方程的积分运算。数值仿真校验了本文基于间接Legendre伪谱法的姿态运动轨迹跟踪控制算法的有效性。     

Fuel-optimal and Energy-optimal guidance schemes for lunar soft landing at a desired location

Two guidance schemes (i) fuel-optimal (ii) energy-optimal to realize soft landing at a desired location on the moon are developed using the optimal control laws. The optimal control laws are obtained by solving a two-point boundary value problem formulated based on Pontryagin’s principle. The guidance laws, adapted from the optimal control laws, are obtained as a function of unknown co-state variables. Differential Transformation (DT) technique is employed to determine the unknown co-states at each time instant of landing trajectory using the information on the current vehicle state, target landing site (loaded on-board apriori) and the time-to-go. The numerical integration of co-state dynamics is avoided due to the DT based approach. The time-to-go, a critical parameter for any guidance scheme, is computed and updated real time using a simple strategy which uses the current and end states. The simple strategy for time-to-go works well even when the shape of the trajectory is nonlinear. Extensive analysis is carried out to evaluate and compare the proposed guidance schemes. Further, the proposed schemes are compared with other popular guidance schemes. The DT based proposed schemes help quantify the landing masses for fuel-optimal and energy-optimal objectives. Other features of the proposed schemes are that they do not assume constant gravity field and independent of reference trajectory.     

中低轨红外预警星座基于自由段跟踪的单星覆盖性能

推导了中低轨天基红外星座中单颗卫星基于自由段跟踪时的空域覆盖体积与星下黑体积,研究了其随轨道高度变化的规律,分析了存在切地角影响时的体积变化,并进行了计算。     

Dust Environment Modelling of Comet 67P/Churyumov-Gerasimenko

Dust is an important constituent of cometary emission; its analysis is one of the major objectives of ESA’s Rosetta mission to comet 67P/Churyumov-Gerasimenko (C–G). Several instruments aboard Rosetta are dedicated to studying various aspects of dust in the cometary coma, all of which require a certain level of exposure to dust to achieve their goals. At the same time, impacts of dust particles can constitute a hazard to the spacecraft. To conciliate the demands of dust collection instruments and spacecraft safety, it is desirable to assess the dust environment in the coma even before the arrival of Rosetta. We describe the present status of modelling the dust coma of 67P/C–G and predict the speed and flux of dust in the coma, the dust fluence on a spacecraft along sample trajectories, and the radiation environment in the coma. The model will need to be refined when more details of the coma are revealed by observations. An overview of astronomical observations of 67P/C–G is given, because model parameters are derived from this data if possible. For quantities not yet measured for 67P/C–G, we use values obtained for other comets, e.g. concerning the optical and compositional properties of the dust grains. One of the most important and most controversial parameters is the dust mass distribution. We summarise the mass distribution functions derived from the in-situ measurements at comet 1P/Halley in 1986. For 67P/C–G, constraining the mass distribution is currently only possible by the analysis of astronomical images. We find that both the dust mass distribution and the time dependence of the dust production rate of 67P/C–G are those of a fairly typical comet.     

侦察卫星星座覆盖性能仿真分析软件设计

为了快速、便捷分析天基侦察系统的对地覆盖性能,开展综合对比分析,设计开发天基侦察卫星星座对地覆盖性能仿真分析系统。仿真系统基于VS2010平台开发,通过软件交互接口调用STK引擎完成计算,使用Matlab编译的库函数完成仿真数据处理及可视化输出。仿真系统采用Redis数据库实现输入参数和仿真结果的存储,并提供与外部程序静态和动态交互功能。仿真系统提供独立仿真和协同仿真两种工作方式,可独立运行分析星座覆盖性能,也可作为其它仿真系统的一部分,在外部命令控制下运行。经应用测试,该系统可以快速、有效完成卫星星座对地面目标的覆盖性能对比分析,为天基侦察系统星座构型设计论证提供支撑。