高阶矩谱分析与空间等离子体非线性相互作用识别

利用高阶矩统计分析方法对ＡＵＲＥＯＬ－３卫星观测数据进行分析处理，所涉及的信号分别为ＥＬＦ频率范围内的电场扰动Ｅｈ（ｔ）和等离子体密度波动δＮｅ／ｎｅ（ｔ），处理结果表明：利用高阶矩谱分析方法可以很好地识别空间等离了波－粒相互作用过程中的非线性成分     

非金属电热膜材料及工艺分析

本文论述了制作电热膜的工艺过程.对电热膜的材料、烧结工艺及使用寿命进行了试验,获得了有价值的结论.并论述了提高电热膜产品寿命应注意的问题.     

疲劳学的研究进展

随机疲劳、混沌疲劳及复合材料疲劳寿命估算属疲劳学研究的三个重要前沿。给出了疲劳损伤的动态概率分布；对混沌疲劳进行了初步探索；且给出了用于复合材料疲劳寿命估算的损伤演化方程。     

随机疲劳累积损伤可靠性分析模型

将疲劳损伤累积过程看作是能量耗散的不可逆过程，从随机过程的角度，研究了各类随机损伤累积法则均应满足的若干必要条件，对目前已有的一些概率型疲劳损伤累积法则的统计相容性进行了较为系统的理论分析，建立了一类不依赖于疲劳寿命具体分布形式的随机疲劳累积损伤可靠性分析模型。     

High energy radiation from the direction of the galactic black hole Sgr A

X-ray observations indicate that the Galactic black hole Sgr A^∗ is inactive now, however, we suggest that Sgr A^∗ can become active when a captured star is tidally disrupted and matter is accreted into the black hole. Consequently the Galactic black hole could be a powerful source of relativistic protons with a characteristic energy ∼10⁵² erg per capture. The diffuse GeV and TeV γ-rays emitted in the direction of the Galactic Center (GC) are the direct consequences of p–p collisions of such relativistic protons ejected by very recent capture events occurred ?10⁵ yr ago. On the other hand, the extended electron-positron annihilation line emission observed from GC is a phenomenon related to a large population of thermalized positrons, which are produced, cooled down and accumulated through hundreds of past capture events during a period of ∼10⁷ yr. In addition to explaining GeV, TeV and 511 keV annihilation emissions we also estimate the photon flux of several MeV resulting from in-flight annihilation process.     

在MATLAB中模拟平稳随机过程

叙述了平稳随机过程理论的基本定义,以及运用实谱分解方法模拟平稳随机过程的原理.全面分析了在微型计算机上使用MATLAB软件模拟平稳随机过程的注意事项,包括:信号源的选取,仿真算法和相应参数的设置,由于功率谱密度的不同定义而需要进行相应的调整等3个方面.结合大气紊流和航空母舰在海上的随机运动的2个实例,给出了在MATLAB中模拟类似过程的方法,并对结果进行了检验.分析表明在MATLAB中能够较好地模拟平稳随机过程.      

Interstellar hydrogen bonding

This paper reports the first extensive study of the existence and effects of interstellar hydrogen bonding. The reactions that occur on the surface of the interstellar dust grains are the dominant processes by which interstellar molecules are formed. Water molecules constitute about 70% of the interstellar ice. These water molecules serve as the platform for hydrogen bonding. High level quantum chemical simulations for the hydrogen bond interaction between 20 interstellar molecules (known and possible) and water are carried out using different ab-intio methods. It is evident that if the formation of these species is mainly governed by the ice phase reactions, there is a direct correlation between the binding energies of these complexes and the gas phase abundances of these interstellar molecules. Interstellar hydrogen bonding may cause lower gas abundance of the complex organic molecules (COMs) at the low temperature. From these results, ketenes whose less stable isomers that are more strongly bonded to the surface of the interstellar dust grains have been observed are proposed as suitable candidates for astronomical observations.     

非线性动力Alfven波的演化

本文讨论了非线性动力Alfven波在1＞＞β＞＞me／mi条件下形成孤子解的限制条件，表明只有亚Alfven速度才能形成压缩型孤子．由动力Alfven波孤子和湍流产生的极大纵向电子速度不会超过本底电子热速度，但由此产生的纵向电场在小尺度范围可以很强，这可能对太阳风的能量传输与粒子加速产生一定影响．     

一种新型水溶性芯模的制备和性能

概述了金属模具不易脱模的形状复杂的复合材料结构件成型中遇到的工艺技术难题,着重对水溶性芯模的制备工艺特点和性能进行了研究,并将所制得的水溶性芯模成功的用于树脂基复合材料结构件的制造中。结果表明,水溶性芯模的各项性能满足复杂异型复合材料结构件制造的要求。     

基于HMDP的无人机三维路径规划

路径规划是UAV(Unmanned Aerial Vehicle)自主飞行的重要保障.初步建立了基于MDP(Markov Decision Processes)的全局路径规划模型,把UAV的路径规划看作是给定环境模型和奖惩原则的情况下,寻求最优策略的问题;为解决算法时空开销大、UAV航向改变频繁的缺点,提出一种基于状态聚类方法的HMDP(Hierarchical Markov Decision Processes)模型,并将其拓展到三维规划中.仿真实验证明:这种简单的规划模型可以有效解决UAV的三维全局路径规划问题,为其在实际飞行中的局部规划奠定了基础.