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.      

基于遗传进化算法反演吸波结构电磁参数

对多层吸波结构中未知参数层的电磁参数进行了反演.根据传输线理论确立的多层结构电磁参数与反射/透射系数的关系,建立正向反射率计算模型,根据自由空间法原理搭建的测试平台测量得到多层吸波材料不同入射角度下的反射率信息,利用改进的遗传进化算法获取了多层吸波结构中未知参数层的电磁参数.在遗传进化过程中,采用高斯随机数代替基本遗传算法的均匀随机数,避免了传统网络参数法厚度谐振、多值性问题和基本遗传算法易陷入局部最优点的问题.与传统传输/反射法结果的比较,验证了这种方法的可靠性.这种方法同时适用于计算高、低损耗介质材料的电磁参数.      

H.264中多模式运动估计算法优化

针对H.264标准的多模式运动估计算法编码模式复杂、计算量大的不足,通过对H.264参考模型JM10中运动估计算法的分析,提出了一种利用时间、空间相关性的模式选择算法和结合一维绝对差值和(SAD,Sum of Absolute Difference)的高效匹配准则,将串行全搜索的运动估计算法改进为并行部分搜索的运动估计算法,把一维SAD和二维SAD匹配准则结合使用,从模式选择和编码速度两个方面对原算法进行优化.实验结果表明:与参考模型JM10的运动估计算法相比,提出的优化算法在恢复质量(用峰值信噪比表征)平均下降0.03 dB、码速率增加不超过1.5%的前提下,编码速率提高20%~30%,表明了该算法在恢复质量略有下降的情况下明显提高了编码速度.      

飞机飞行控制律/操纵效率器多学科优化设计

基于近似模型和遗传算法,针对多操纵面布局飞机提出一种对全包线飞行控制律和操纵效率器几何形状与位置进行多学科优化的设计方法.该方法采用力矩控制方式进行控制,应用鲁棒增益调参方法设计全包线飞行控制系统,利用试验设计方法和径向基神经网络响应面获取近似的气动学科模型和控制学科模型,在近似模型基础上由遗传算法获得优化的设计参数并最终获得优化的控制律和操纵效率器.以某多操纵面布局无尾飞机为例进行计算机飞行仿真验证,结果表明该方法具有可行性.      

Antideuteron based dark matter search with GAPS: Current progress and future prospects

The General Antiparticle Spectrometer (GAPS) is a new approach to the indirect detection of dark matter. It relies on searching for primary antideuterons produced in the annihilation of dark matter in the galactic halo. Low energy antideuterons produced through Standard Model processes, such as collisions of cosmic-rays with interstellar baryons, are greatly suppressed compared to primary antideuterons. Thus a low energy antideuteron search provides a clean signature of dark matter. In GAPS antiparticles are slowed down and captured in target atoms. The resultant exotic atom deexcites with the emission of X-rays and annihilation pions, protons and other particles. A tracking geometry allows for the detection of the X-rays and particles, providing a unique signature to identify the mass of the antiparticle. A prototype detector was successfully tested at the KEK accelerator in 2005, and a prototype GAPS balloon flight is scheduled for 2011. This will be followed by a full scale experiment on a long duration balloon from Antarctica in 2014. We discuss the status and future plans for GAPS.     

Finite element reconstruction approach for on-orbit spacecraft breakup dynamics simulation and fragment analysis

Breakup model is the key area of space debris environment modeling. NASA standard breakup model is currently the most widely used for general-purpose. It is a statistical model found based on space surveillance data and a few ground-based test data. NASA model takes the mass, impact velocity magnitude for input and provides the fragment size, area-to-mass ratio, velocity magnitude distributions for output. A more precise approach for spacecraft disintegration fragment analysis is presented in this paper. This approach is based on hypervelocity impact dynamics and takes the shape, material, internal structure and impact location etc. of spacecraft and impactor, which might greatly affect the fragment distribution, into consideration. The approach is a combination of finite element and particle methods, entitled finite element reconstruction (FER). By reconstructing elements from the particle debris cloud, reliable individual fragments are identified. Fragment distribution is generated with undirected graph conversion and connected component analysis. Ground-based test from literature is introduced for verification. In the simulation satellite targets and impactors are modeled in detail including the shape, material, internal structure and so on. FER output includes the total number of fragments and the mass, size and velocity vector of each fragment. The reported fragment distribution of FER shows good agreement with the test, and has good accuracy for small fragments.     

Optimization of communication network topology for navigation sharing among distributed satellites

Navigation sharing among distributed satellites is quite important for coordinated motion and collision avoidance. This paper proposes optimization methods of the communication network topology to achieve navigation sharing. The whole communication network constructing by inter-satellite links are considered as a topology graph. The aim of this paper is to find the communication network topology with minimum communication connections’ number (MCCN) in different conditions. It has found that the communication capacity and the number of channels are two key parameters affecting the results. The model of MCCN topology for navigation sharing is established and corresponding method is designed. Two main scenarios, viz., homogeneous case and heterogeneous case, are considered. For the homogeneous case where each member has the same communication capacity, it designs a construction method (Algorithm 1) to find the MCCN topology. For the heterogeneous case, it introduces a modified genetic algorithm (Algorithm 2) to find the MCCN topology. When considering the fact that the number of channels is limited, the Algorithm 2 is further modified by adding a penalized term in the fitness function. The effectiveness of these algorithms is all proved in theoretical. Three examples are further tested to illustrate the methods developed in this paper.     

北极黄河站极光亚暴期间低热层大气中性风研究

极光亚暴是地球空间基本的能量输入、耦合及耗散过程,其对低热层大气中性风的影响不容忽视,对这一问题进行深入研究具有重要意义.2010年11月,中国北极黄河站(78.92°N,11.93°E)安装了一台自主研制的全天空法布里-珀罗干涉仪(FPI)并开始进行正常观测,为中国首次获得了极光亚暴期间的FPI观测数据.根据2012年越冬期间的观测情况,对2012年11月12-14日及12月09-11日两个极光亚暴事件期间的数据进行处理,计算得到了5级干涉环对应的风场.亚暴期间风场变化与地磁活动变化的对比分析表明,风速的剧烈变化可能是由地磁活动剧烈扰动造成的.针对2012年11月13日00:00UT-02:00UT和2012年12月10日05:00UT-07:30UT的亚暴事件,将全天空相机拍摄到的极光图像与FPI干涉图像对应的视线风场进行对比分析.结果表明在极光活动中,视线风速加强的方向与极光弧的方向垂直,而在极光弧的平行方向,风速相对较小.     

用于识别两颗故障卫星的RAIM算法

提出了一种可以识别两颗故障卫星的接收机自主完好性监测算法.将最优奇偶矢量法应用于两颗故障卫星识别,指出由于故障偏差可能会抵消而使得正确识别率较低.对最优奇偶矢量法进行了改进,利用对单颗卫星故障敏感的最优奇偶矢量对所有可能的两颗故障卫星组合分别构造两个新的奇偶矢量,用于两颗故障卫星的检测和识别.计算机仿真结果显示,改进后的算法与直接利用最优奇偶矢量法相比,可以显著提高两颗故障卫星正确识别率,识别率可超过90%.同时,改进算法的奇偶矢量构造方法简单,计算量将减少90%以上,更有利于工程实现.      

单相流体回路在卫星热控制中的应用研究

单相流体回路系统是航天器主动热控技术中的一种重要方式,文章概述了流体回路的工作原理及理论基础,总结了单相流体回路的设计思路,设计了一个可参考的流体回路方案,在SINDA/FLUINT中建立数值仿真模型进行分析计算,并评价了其应用性能,结果显示,将单相流体回路系统应用于卫星,可取得很好的控温效果。