Conceptual model about the interaction between El Ni(n)o/ Southern Oscillation and Quasi-Biennial Oscillation in far west equatorial Pacific

Interaction between the Quasi-Biennial Oscillation in far west equatorial Pacific (QBOWP) and the El Nino/Southern Oscillation (ENSO) is studied using a new conceptual model. In this conceptual model, the QBOWP effects on ENSO are achieved through two ways: (1) the oceanic Kelvin wave along equatorial Pacific, and (2) the Atmospheric Walker Circulation anomaly, while ENSO effects on QBOWP can be accomplished by the atmospheric Walker Circulation anomaly. Diagnosis analysis of the model results shows that the Atmospheric bridge (Walker circulation) plays a more important role in interaction between the ENSO and QBOWP than the oceanic bridge (oceanic Kelvin wave along equatorial Pacific); It is found that by the interaction of the ENSO and QBOWP, a free ENSO oscillation with 3-5 years period could be substituted by a oscillation with the quasi-biennial period, and the dominant period of SST anomaly and wind anomaly in the far west equatorial Pacific tends to be prolonged with enhanced ENSO forcing. Generally, the multi-period variability in the coupled Atmosphere-Ocean System in the Tropical Pacific can be achieved through the interaction between ENSO and QBOWP.     

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Weak stability boundary trajectories for the deployment of lunar spacecraft constellations

Suitable lunar constellation coverage can be obtained by separating the satellites in inclinations and node angles. It is shown in the paper that a relevant saving of velocity variation ΔV can be achieved using weak stability boundary trajectories. The weakly stable dynamics of such transfers allows the separation of the satellites from the nominal orbit to the required orbit planes with a small amount of ΔV. This paper also shows that only one different set of orbital parameters at Moon can be reached with the same ΔV manoeuvre starting from a nominal trajectory and ending at a fixed periselenium altitude. In fact, such a feature is proved to be common to other simpler dynamical systems, such as the two- and three-body problems.     

基于不同轨道高度iHCO通信卫星的CAPS星座优化研究

基于通信卫星的导航系统可以利用比地球静止轨道（Geostationary Earth Orbit,GEO）高约200 km的倾斜高圆轨道（inclined Highly Circular Orbit,iHCO）通信卫星组成导航星座.结合两种轨道高度的倾斜高圆轨道通信卫星,仿真分析了利用倾斜高圆轨道卫星组成的中国区域定位系统（Chinese Area Positioning System,CAPS）的导航性能,并讨论了利用倾斜高圆轨道卫星组成的中国区域定位系统实现中国区域覆盖的最佳星座布局.     

基于星座图改进的QAM盲均衡算法

针对多模辅助算法均方误差高的缺点,提出了两种基于星座图改进的盲均衡算法.首先利用16QAM星座图信息,增加多模辅助算法代价函数中信号点的均衡数目,得到改进的多模辅助算法,与多模辅助算法相比,改进后的算法稳态均方误差更低,而且收敛速度略有提高;其次将改进的多模辅助算法和判决引导算法相结合,根据均方误差调整两种算法的比例,得到的混合算法进一步降低了稳态均方误差.水声信道仿真结果表明:提出的两种算法都可以有效地降低均方误差,适用于对精度要求较高的场合.     

Contrasting Regional Responses of Indian Summer Monsoon Rainfall to Exhausted Spring and Concurrently Emerging Summer El Ni?o Events

The inverse relationship between the warm phase of the El Ni?o Southern Oscillation(ENSO) and the Indian Summer Monsoon Rainfall(ISMR) is well established. Yet, some El Ni?o events that occur in the early months of the year(boreal spring) transform into a neutral phase before the start of summer, whereas others begin in the boreal summer and persist in a positive phase throughout the summer monsoon season. This study investigates the distinct influences of an exhausted spring El Ni?o(springtime)...     

导航星座抗毁组网结构研究

为提高整个二代导航卫星网络的抗毁性能,对其抗毁组网结构进行了研究。基于分群管理、链路冗余与修补方法,提出并设计分析了一种基于GEO星层、MEO星层以及地面节点联合组网的二代导航卫星网络组网结构,根据快照周期内位置固定的方法对星座中MEO星层进行分群管理,设计其群首的备份选择机制,以及群首MEO替代失效群管理者GEO机制,提高了星座网络的通信链路的抗毁性。通过分析二代导航卫星网络中数据传输过程与类型,设计网络结构中群内、星层以及整个二代导航星座的通信链路,特别是对星座中MEO星层的通信链路进行充分的冗余设计,启用视距范围内间隔失效卫星间次相邻卫星节点链路连接的链路设计,并同时提高了整个二代导航卫星网络的通信性能和通信容量,可以满足各种不同业务需求的数据包传输。     

导航星座抗毁路由方法与技术研究

基于分群管理、群首备份、链路冗余、链路修补的二代导航卫星网络组网结构,提出并设计了一种基于GEO星层、MEO星层、地面节点联合组网的抗毁路由算法（DRRA）。基于二代导航动态卫星网络中卫星移动的动态卫星网络中,提出的DRRA算法在定位信号稳定、数据包路由抗毁、数据包路由最短延时等方面具有优势,并分析了其主要原因。     

地震电磁卫星星座轨道优化设计

根据地震监测任务对电磁卫星的需求．利用点数字仿真方法和遗传算法优化设计了电磁卫星星座。由4颗卫星组成的电磁卫星星座之空间分辨率约为700km．覆盖全球的观测用时周期为12小时。     

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