自组织网络中的分布式能量感知拓扑控制算法

为了有效利用无线自组织网络的能量,将最小连通支配集和计算几何学相结合,提出了一种自组织网络中的分布式能量感知拓扑控制算法.首先选举能量寿命较长的节点构建能量感知最小连通支配集,保证支配节点有充足的能量完成路由转发任务.之后在能量感知最小连通支配集上面构建Delaunay三角剖分,降低节点数据发送能耗,保证链路的能量有效性和网络拓扑的平面性.在原有连通支配集失效的情况下,选举能量寿命较长的替代节点进行拓扑重构,实现动态网络能量均衡.仿真结果表明,本算法在获得小的支配集的同时延长了网络寿命.      

大气闪烁对近似无衍射激光通信系统的影响

在近似无衍射激光通信系统中,大气湍流的作用导致接收端光强起伏不定,这将对通信系统的误码率产生影响.以光强起伏的概率分布为基础,忽略系统中的其他噪声,推导出折射率结构常数、通信距离和激光波长等影响因素与误码率的关系式.通过计算机模拟,研究了误码率随折射率结构常数的变化规律,讨论了一定湍流强度下通信距离和激光波长对误码率的影响,并以10-9为误码率标准,确定了通信距离的允许范围.结果表明,合理地选择天气和日照条件、减小通信距离以及选择长波长的激光器可以减弱大气湍流对误码率的影响.      

多级协同项目执行中的资源冲突检测与管理

以航空航天型号工程项目为背景,针对多级协同项目中的资源冲突问题,利用基于时间约束网络的冲突检测算法实现了多级协同项目中的资源冲突检测,该算法建立了任务关系的时间约束网络模型,给出了基于模型的线性化、实例化方法和检测判据.针对资源冲突的检测结果表达及冲突信息的管理提出多视图表达方式,建立了基于UML的信息模型.基于研究结果设计开发了项目资源管理原型系统,以某航天项目任务的管理为例进行了验证,表明了研究结果的有效性.      

滑橇甲板助飞的力学机理分析

针对飞机在滑橇甲板上起飞的特点,基于力多边形的变化过程,以及甲板形状对飞机俯仰转动的作用,分析了飞机性能和品质与甲板参数的适配关系,说明了飞机在低速离舰初期迎角建立的力学机理.迎角的建立综合3个方面的效果:曲面甲板提供正向俯仰角速度,使迎角增加;前轮离舰释放载荷、后轮尚未离舰的过程中,甲板支反力提供低头力矩,使离舰初期俯仰角速度减小;离舰初期升力不能平衡重力,加速度指向前下方,轨迹向下弯曲,速度下偏使迎角增加.对航母/舰载机/起落架多体动力学系统进行数值仿真,结果表明分析合理.      

基于Bayes统计模型的卫星融合定轨方法研究

根据目前天基导航系统现状,结合中国对低、中轨卫星精密定轨的要求,给出了天地基信息融合定轨的原理;结合卫星待估融合参数的先验信息,提出了基于Bayes统计模型的卫星精密定轨方法;在卫星观测的线性化融合模型中引入观测噪声,利用概率估计融合模型,根据Bayes理论进行卫星状态改进量的最大后验估计,并分析了Bayes估计方法的定轨精度;依据期望融合的待估改进量方差最小规则建立了相应的参数求解算法;最后以导航融合测控系统中测距和测速数据的融合定轨为例进行了仿真实验,表明该融合方法能够得到很好的定轨效果。     

航空泵试验台驱动变结构控制

飞机液压系统泵源需进行地面试验,采用变频调速器＋异步电机＋增速箱的驱动形式是航空泵进行地面试验最先进有效的方法之一.建立了矢量控制变频调速驱动下航空泵试验台驱动系统的数学模型,针对航空泵试验时由于负载变化泵转速不能保持恒定的问题,采用积分滑模面的滑模变结构控制策略,并构造Lyapunov函数证明其稳定性.为降低输出抖振现象,提出采用模糊控制监督下的滑模变结构控制和伪微分反馈(PDF, Pseudo Derivative Feedback)控制相结合的控制策略,仿真及实验结果表明,该控制方法有很高的控制精度,在保持滑模变结构控制鲁棒性强的前提下降低了输出抖振现象.      

Tropospheric wet refractivity tomography using multiplicative algebraic reconstruction technique

Algebraic reconstruction techniques (ART) have been successfully used to reconstruct the total electron content (TEC) of the ionosphere and in recent years be tentatively used in tropospheric wet refractivity and water vapor tomography in the ground-based GNSS technology. The previous research on ART used in tropospheric water vapor tomography focused on the convergence and relaxation parameters for various algebraic reconstruction techniques and rarely discussed the impact of Gaussian constraints and initial field on the iteration results. The existing accuracy evaluation parameters calculated from slant wet delay can only evaluate the resultant precision of the voxels penetrated by slant paths and cannot evaluate that of the voxels not penetrated by any slant path. The paper proposes two new statistical parameters Bias and RMS, calculated from wet refractivity of the total voxels, to improve the deficiencies of existing evaluation parameters and then discusses the effect of the Gaussian constraints and initial field on the convergence and tomography results in multiplicative algebraic reconstruction technique (MART) to reconstruct the 4D tropospheric wet refractivity field using simulation method.     

Predicting performance in manually controlled rendezvous and docking through spatial abilities

Manually controlled rendezvous and docking (manual RVD) is a challenging space task for astronauts. This study aims to identify spatial abilities that are critical for accomplishing manual RVD. Based on task analysis, spatial abilities were deduced to be critical for accomplishing manual RVD. 15 Male participants performed manual RVD task simulations and spatial ability tests (the object-manipulation spatial ability and spatial orientation ability). Participants’ performance in the test of visualization of viewpoints (which measures the spatial orientation ability) was found to be significantly correlated with their manual RVD performance, indicating that the spatial orientation ability in the sense of perspective taking is particularly important for accomplishing manual RVD.     

Stability of relative equilibria of the full spacecraft dynamics around an asteroid with orbit–attitude coupling

The full dynamics of spacecraft around an asteroid, in which the spacecraft is considered as a rigid body and the gravitational orbit–attitude coupling is taken into account, is of great value and interest in the precise theories of the motion. The spectral stability of the classical relative equilibria of the full spacecraft dynamics around an asteroid is studied with the method of geometric mechanics. The stability conditions are given explicitly based on the characteristic equation of the linear system matrix. It is found that the linearized system decouples into two entirely independent subsystems, which correspond to the motions within and outside the equatorial plane of the asteroid respectively. The system parameters are divided into three groups that describe the traditional stationary orbit stability, the significance of the orbit–attitude coupling and the mass distribution of the spacecraft respectively. The spectral stability of the relative equilibria is investigated numerically with respect to the three groups of system parameters. The relations between the full spacecraft dynamics and the traditional spacecraft dynamics, as well as the effect of the orbit–attitude coupling, are assessed. We find that when the orbit–attitude coupling is strong, the mass distribution of the spacecraft dominates the stability of the relative equilibria; whereas when the orbit–attitude coupling is weak, both the mass distribution and the traditional stationary orbit stability have significant effects on the stability. We also give a criterion to determine whether the orbit–attitude coupling needs to be considered.     

Satellite-observed biological variability in the equatorial Pacific during the 2009–2011 ENSO cycle

The event of 2009–2011 El Niño Southern Oscillation (ENSO) provides an opportunity to gain insight into the biological variability of the equatorial Pacific Ocean for an entire ENSO cycle with satellite and in situ observations. Even though El Niño and La Niña in general led to respectively weakened and enhanced chlorophyll-a concentration and net primary production (NPP) along the equatorial Pacific Ocean during the 2009–2011 ENSO cycle, biological responses were highly disparate along the equator and attributed to different driving mechanisms. In the eastern equatorial Pacific east of 150°E, the El Niño-La Niña biological change was in general small except for the transition period even though sea surface temperature (SST) showed over ∼5 °C drop from El Niño to La Niña. In the central-eastern (170°W–140°W) equatorial Pacific, moderate change of biological activity is attributed to the changes of thermocline driven by the eastward propagating equatorial Kelvin waves and changes of zonal currents and undercurrents. Highest biological response in this ENSO cycle was located in the central (170°E–170°W) and central-western (150°E–170°E) equatorial Pacific with quadruple chlorophyll-a concentration and over ∼400 mg C m⁻² d⁻¹ increase of NPP from El Niño in 2009 to La Niña in 2010. However, spatial pattern of ENSO biological variability as represented with NPP is not exactly the same as chlorophyll-a variability. Wind-driving mixing of nutrients and eastward advection of the oligotrophic warm pool waters are attributed to this significant biological variability in this region.