SOFT IMAGE SEGMENTATION BASED ON CENTER-FREE FUZZY CLUSTERING

Image segmentation remains one of the major challenges in image analysis.And soft image segmentation has been widely used due to its good effect.Fuzzy clustering algorithms are very popular in soft segmentation.A new soft image segmentation method based on center-free fuzzy clustering is proposed.The center-free fuzzy clustering is the modified version of the classical fuzzy C-means ( FCM ) clustering.Different from traditional fuzzy clustering , the center-free fuzzy clustering does not need to calculate the cluster center , so it can be applied to pairwise relational data.In the proposed method , the mean-shift method is chosen for initial segmentation firstly , then the center-free clustering is used to merge regions and the final segmented images are obtained at last.Experimental results show that the proposed method is better than other image segmentation methods based on traditional clustering.     

基于仅光学观测的短弧关联分析方法

初始轨道确定是空间目标编目的一个重要部分,尤其在光学仅角度观测下是极具挑战性的.光学观测在短弧的情况下很难进行有效的初轨确定,解决短弧问题的一个重要手段是将不同时刻获取到的短弧数据进行关联匹配,找到属于同一个目标的观测数据.以容许域的方法为基础,通过找到拟合多组观测数据的最优轨道的方式来确定角度预测值和角度测量真实值之...     

中性气体释放人工产生气辉

电离层中分子性的离子与电子的复合要比氧离子与电子的辐射性复合快得多,因此火箭发动机产生的尾气和空间等离子体主动实验中主动释放的中性气体会对电离层有很大的影响,这么大的电离层扰动现象在过去的实验中经常可以观测到.根据中性气体在热层背景中的扩散方程,考虑电离层F区主要的离子化学反应,研究了H2,H2O和CO2气体在电离层高度上的扩散过程和电离层对所释放气体的响应,计算了气辉的体发射系数和发射强度.结果表明,中性气体在电离层高度上扩散非常迅速,在F区的一些高度上,主要正离子成分由O+转变为其他分子离子,且在释放过程中伴随气辉发射,发射气辉的波长和特征与释放物质的种类有关.      

Thermal Stresses and Cracks During the Growth of Large-sized Sapphire with SAPMAC Method

本文利用有限元法对冷心放肩微量提拉法(SAPMAC)生长大尺寸蓝宝石单晶过程中的热应力进行了模拟计算,应用临界缺陷理论解释了裂纹的萌生与扩展机理。研究表明,晶体内的热应力主要与晶体生长速率,环境温度和结晶取向有关;较大热应力多出现在结晶界面,放肩、收尾以及直径急剧变化等位置;最大热应力总是出现在籽晶与新生晶体的界面附近。裂纹将在临界缺陷位置产生,并在应力作用下沿a或m面扩展。计算结果与实验结果基本吻合,通过晶体生长系统和生长工艺的改进,对晶体的开裂问题得到了有效的抑制。     

电离层F层中舒曼共振现象的检测

利用Ａｕｒｅｏｌ－３卫星在电离层Ｆ层高度上（６５０ｋｍ左右）对电离层电场扰动与电子密度扰动的观测进行分析处理,在高纬电离层Ｆ层高度上可以检测到舒曼共振现象。根据等离子体参数,可以认为,发生在这个高度上的舒曼共振现象与Ｌ模式的波传播有关,舒曼共振的基频是与电子密度的大尺度不规则性有关,谐波分量与正向密度梯度相关。     

跨流区超低轨航天器快速气动力计算方法

超低轨飞行器常工作在过渡流区中,过渡流区中气动特性多变,建模困难,目前缺少较好的快速气动力计算方法。在面元法的基础上,提出了设计迎风单元筛选算法与logistics-log桥函数,对连续流区与自由流区结果进行加权,实现超低轨卫星的气动力估算。在方法验证中,对圆柱与钝头双楔体在宽努森数(Kn)范围下的气动力进行测算,发现结果与直接模拟蒙特卡洛法(DSMC)数据一致。对典型超低轨飞行器地球重力场和海洋环流探测卫星(GOCE)的气动力进行分析,发现GOCE随着姿态变化阻力变化明显,需要舵面或陀螺仪进行姿态控制;在不同高度下的阻力量级变化大,在超低轨运行时需要动力系统维持高度。     

飞机最优巡航条件的确定

续航性能是飞机的主要战术技术指标之一。从飞机巡航段航程的基本公式出发，利用导数求极值的性质，推导出确定飞机巡航爬升和平流层内最佳巡航条件的方程，证明了最优巡航马赫数出现在飞机阻力增加区段，最优巡航高度存在于飞机阻力最小处。最后以某型飞机的巡航爬升条件和平流层平飞最优马赫数和高度的确定作为算例，说明用此方法确定飞机巡航条件，将使飞机获得最大航程。     

大气层内动能拦截弹的变增益鲁棒姿控系统设计研究

当调度参数快速变化时,基于传统方法设计的系统可能会变得不稳定。针对这个原理缺陷,应用变增益鲁棒控制理论设计参数较快变化的动能拦截弹。首先建立了导弹动力学模型,然后介绍并推证了基于状态反馈的二次H∞性能稳定定理,为了保证闭环系统具有满意的动态性能,引入了闭环极点区域配置技术,最后的仿真表明,该方法具有良好的跟踪切换能力,预期的动态响应能力并可保证系统全局稳定。     

Furthering our understanding of electrostatic solitary waves through Cluster multispacecraft observations and theory

Nonlinear isolated electrostatic solitary waves (ESWs) are observed routinely at many of Earth’s major boundaries by the Wideband Data (WBD) plasma wave receivers that are mounted on the four Cluster satellites. The current study discusses two aspects of ESWs: their characteristics in the magnetosheath, and their propagation in the magnetosheath and in the auroral acceleration (upward current) region. The characteristics (amplitude and time duration) of ESWs detected in the magnetosheath are presented for one case in which special mutual impedance tests were conducted allowing for the determination of the density and temperature of the hot and cold electrons. These electron parameters, together with those from the ion experiment, were used as inputs to an electron acoustic soliton model as a consideration for the generation of the observed ESWs. The results from this model showed that negative potential ESWs of a few Debye lengths (10–50 m) could be generated in this plasma. Other models of ESW generation are discussed, including beam instabilities and spontaneous generation out of turbulence. The results of two types of ESW propagation (in situ and remote sensing) studies are also presented. The first involves the propagation of bipolar type ESWs from one Cluster spacecraft to another in the magnetosheath, thus obtaining the velocity and size of the solitary structures. The structures were found to be very flat, with large scale perpendicular to the magnetic field (>40 km) and small scale parallel to the field (<1 km). These results were then discussed in terms of various models which predict such flat structures to be generated. The second type of propagation study uses striated Auroral Kilometric Radiation (SAKR) bursts, observed on multiple Cluster satellites, as tracers of ion solitary waves in the upward current region. The results of all studies discussed here (pulse characteristics and ESW velocity, lifetime, and size) are compared to in situ measurements previously made on one spacecraft and to theoretical predictions for these quantities, where available. The primary conclusion drawn from the propagation studies is that the multiple spacecraft technique allows us to better assess the stability (lifetime) of ESWs, which can be as large as a few seconds, than can be achieved with single satellites.     

Hill区域内基于推广的Poincaré映射的低能逃逸/捕捉轨道

给出了Hill区域内基于推广的Poincare映射的低能逃逸轨道的计算.文中的推广的Poincare映射需要在相空间中选取两个(而非一个)与流相截的面,即将包含某个天平动点的截面通过轨道来映射到近拱点的通道面上的,在数值上通过总变差减小的Runge-Kutta方法来实现两个相面之间的映射.捕捉轨道则可由Hill三体模型的对称性直接导出.最后,关于Rhea的二维、三维的逃逸和捕捉轨道的仿真结果验证了该方法的精度和鲁棒性.