Optimization of geosynchronous satellite constellation for independent regional navigation and positioning in Middle East region

Regional Navigation and positioning systems using geosynchronous satellites are emerging for different parts of the world. Optimal constellation geometry achievement for a set of geosynchronous satellites is a key sector in designing of such systems. Genetic algorithm is applied for optimization of constellations with 6 and 7 satellites which is to be used in Middle East region where these systems have been deprived of. Based on the fact that the coverage criterion is not sufficient enough to guarantee a good navigation service, positioning process by the satellite systems is discussed and the performance of the system on the basis of position dilution of precision is collected as the fitness criterion. Placing the satellites in groups to pass over the same ground track is applied as a constraint to the genetic algorithm. By simulation, performance of the best obtained results and GPS are compared in terms of position dilution of precision, visibility and the required epochs (time span) to resolve the ambiguities with a 99% success rate, in this region. Also, capability of the GA for such problems is demonstrated.     

On the large-scale structure of the tail current as measured by THEMIS

The magnetic field structure and the spatial characteristics of the large-scale currents in the magnetospheric tail were studied during quiet and moderately disturbed geomagnetic conditions in 2009. The magnetic field of the currents other than the tail current was calculated in terms of a paraboloid model of the Earth’s magnetosphere, A2000, and was subtracted from measurements. It was found on the base of obtained tail current magnetic field radial distribution that the inner edge of the tail current sheet is located in the night side magnetosphere, at distances of about 10 R_E and of about 7 R_E during quiet and disturbed periods respectively. During the disturbance of February 14, 2009 (Dst_min ∼ −35 nT), the B_x and the B_z component of the tail current magnetic field near its inner edge were about 60 nT, and −60 nT that means that strong cross-tail current have been developed. The tail current parameters at different time moments during February 14, 2009 have been estimated. Solar wind conditions during this event were consistent with those during moderate magnetic storms with minimum Dst of about −100 nT. However, the magnetospheric current systems (magnetopause and cross-tail currents) were located at larger geocentric distances than typical during the 2009 extremely quiet epoch and did not provide the expected Dst magnitude. Very small disturbance on the Earth’s surface was detected consistent with an “inflated” magnetosphere.     

基于轮询的高级在轨系统多路复用包时延分析

目前的高级在轨系统(AOS,Advanced Orbiting Systems)多路复用研究主要以仿真为主,很少有文献给出专门的理论分析.针对基于轮询的AOS多路复用包时延进行研究,通过采用排队论中非空竭限量服务的休假排队系统建立模型,并采用循环再生法进行分析,得到了多路复用包时延计算公式,并给出包时延的下限值.仿真结果表明,在包到达率取值分别为1,2,3包/s,在各种不同的下行速率(范围240~330 bit/s)之下,包时延的仿真值曲线均高于理论下限值曲线,从而论证了理论推导的正确性.研究结果可以为工程设计提供一定的参考作用.     

航天项目管理——高技术复杂项目管理

航天项目是高技术项目。航天项目管理是高技术复杂项目管理。人的动机和行为的不确定性以及高新技术的挑战是复杂性的重要根源。高技术项目组织管理需要系统思维,高技术系统研制要采用系统工程方法。系统思维和系统工程方法是项目管理者应对复杂管理局面的有效方法。     

基于模型的系统工程方法在载人航天任务中的应用探讨

针对基于文档的航天任务设计中设计数据分散、一致性差、跟踪难度大等问题,引入了基于模型的系统工程(MBSE)方法。首先,介绍了MBSE方法理念,即通过构建图形化的模型来支持系统的需求捕获、设计、分析、验证和确认等全生命周期活动。然后,给出了MBSE方法的一般工作流程,即先构建系统的需求模型,用于指导功能模型、物理架构模型等的构建,按照事先制定好的逻辑规则建立模型间的关系,依靠模型间的关系实现设计过程中的关联性分析、参数查询等工作。最后,应用MBSE方法于载人飞船交会对接任务中。结果表明,此方法改善了人员沟通,提高了设计效率,降低了设计风险,可为MBSE方法在航天任务设计中的进一步应用提供参考。     

捷联式天线稳定平台动力学建模与仿真分析

对于体积有限制的战术导弹应用,导引头天线伺服系统的体积受到严格限制,传统的速率陀螺稳定平台的应用受到挑战,为此提出采用捷联稳定方式来解决视线稳定问题.根据弹载捷联式天线平台的结构特点及稳定原理,应用坐标变换方法,完整地建立了两自由度捷联式天线平台的运动学与动力学模型.通过分析平台框架运动学耦合关系,表明捷联稳定方式与速率陀螺稳定方式的基本区别在于信息的获取和控制方式上,速率陀螺稳定方式是一种直接硬件稳定方法,而捷联稳定方式是一种软件补偿方法.在此基础上,对框架动力学耦合特性进行了数值仿真,结果表明:弹体对框架的耦合较强,需要进行弹体解耦,而框架之间的交叉耦合相对较弱,实际设计时可以忽略.所得结果为进一步研究捷联式天线稳定平台提供了理论基础,也为小型化导引头视线稳定平台系统的工程设计提供了一种解决方案.     

复杂网络的灰点及灰度分析(英文)

依据对复杂网络和灰色系统理论的相关分析,提出了复杂网络中的灰点问题,认为灰点分为存在而未知的灰点和演化灰点两类,并给出了相关定义。进一步给出复杂网络灰度问题的相关描述,将网络灰度分为相对灰度和绝对灰度,并分别进行了证明。     

离散广义Markov跳变系统的镇定性

针对转移概率部分未知情况下的离散时间广义Markov跳变系统,研究了系统的稳定性和镇定性。转移概率部分未知的情况包含了转移概率完全已知和完全未知两种特殊情况,具有更广泛的实际意义。首先利用线性矩阵不等式方法,将离散Markov跳变系统的结论推广到离散广义Markov跳变系统,提出了使开环系统随机稳定的充分条件;在此基础上,进一步提出了闭环系统可镇定的判据,并表示为线性矩阵不等式形式;最后,通过仿真算例验证了所提方法的有效性。     

大型导弹车工作模态识别研究及应用

针对大型导弹车在运输状态下的动态特性识别问题,设计制作了能够反映大型导弹车主要动力学特征的简化模型,使用最小二乘复指数法（LSCE）对简化模型进行了动态特性识别,对识别结果进行了分析和评估,并将最小二乘复指数法应用到真实大型导弹车运输状态的模态识别中。可为大型导弹车运输状态下的动力学特性分析提供参考。     

Universal scaling laws for fully-developed magnetic field turbulence near and far upstream of the Earth’s bow shock

We analyze the multifractal scaling of the modulus of the interplanetary magnetic field near and far upstream of the Earth’s bow shock, measured by Cluster and ACE, respectively, from 1 to 3 February 2002. The maximum order of the structure function is carefully estimated for each time series using two different techniques, to ensure the validity of our high-order statistics. The first technique consists of plotting the integrand of the pth order structure function, and the second technique is a quantitative method which relies on the power-law scaling of the extreme events. We compare the scaling exponents computed from the structure functions of magnetic field differences with the predictions obtained by the She–Lévêque model of intermittency in anisotropic magnetohydrodynamic turbulence. Our results show a good agreement between the model and the observations near and far upstream of the Earth’s bow shock, rendering support for the modelling of universal scaling laws based on the Kolmogorov phenomenology in the presence of sheet-like dissipative structures.