Fourier变换的基本格式与PSD非参数估计

以传统Fourier变换为基础的非参数估计方法是振动工程研究中PSD估计的重要方法。文章以周期图法为例,研究Fourier变换基本格式的不同对PSD非参数估计结果的影响。首先介绍了Fourier变换常见的几种基本格式及其对应的PSD非参数估计计算公式;然后基于PSD的物理内涵,分析、证明多种不同形式的PSD估计公式的同时存在是一种人为误解,只有惟一的一种PSD估计结果才是具有典型物理意义的;最后给出了Fourier变换的一种通用格式及其PSD估计计算公式。     

萤火一号火星探测计划的科学目标

与其他行星相比火星是与地球最为相似, 也是最有可能在其上发现地球以外生命现象的一颗行星, 因此特别受到人类的关注. 近年来, 有国家已经发射了火星探测器, 并启动了载人火星探测研究计划. 中国是世界上第五个具备自主发射人造卫星的国家, 也是世界上第三个具备自主开展载人航天活动的国家. 但是中国在深空探测领域才刚刚起步. 2007年中俄两国签署了联合探测火星计划, 俄罗斯负责将中国研制的一颗微小卫星------萤火一号发送至火星轨道. 萤火一号将开展自主探测, 并与俄罗斯的火卫一探测器开展联合探测. 本文综述了萤火一号任务提出的科学背景及科学目标, 简要介绍了为实现科学目标配置的有效载荷, 以及入轨后的主要探测任务, 并对其科学探测结果进行了初步的展望.      

空间环境天基探测现状与需求分析

天基空间环境探测是了解空间环境状态及变化规律的重要手段, 同时也是保障人类空间活动安全的空间环境预报业务的重要数据来源. 为了促进中国空间环境天基探测的发展和合理布局, 本文分析总结了空间环境天基探测的现状、特点以及能够服务于空间天气预报的业务监测能力情况, 从空间环境业务保障角度分析了空间环境天基探测的需求, 并对中国天基空间环境探测的发展思路进行了初步探讨分析.      

TDLAS测量甲烷／空气预混平面火焰温度和H2O浓度

基于可调谐二极管激光器吸收光谱技术（YDLAS）建立了温度和H2O浓度测量系统,利用光谱数据库Hitran2004在1393nm附近选择了在500～1300K有很高测温灵敏度的两条水吸收线：7168．437cm^-1,7185．597cm^-1。在1kHz的扫描频率下,利用直接吸收-扫描波长法对甲烷／空气预混平面火焰进行测量,并进行边界层修正,与热电偶的对比结果显示,在温度区间1100～1350K,两者最大相差80K（6．7％）;水蒸气组分浓度与计算值平均相差小于0．02（10％）．     

Ozone variability related to several SEP events occurring during solar cycle no. 23

Data from geostationary operational environmental satellite (GOES) series were used to identify intense solar energetic particle (SEP) events occurred during the solar activity cycle no. 23. We retrieved O₃, NO, NO₂, HNO₃, OH, HCl and OHCl profiles coming from different satellite sensors (solar occultation and limb emission) and we looked for the mesospheric/stratospheric response to SEPs at high terrestrial latitudes. The chemistry of the minor atmospheric components is analysed to evaluate the associated odd nitrogen (NO_x) and odd hydrogen (HO_x) production, able to cause short (h) and medium (days) term ozone variations. We investigated the effects of SEPs on the polar atmosphere in three different seasons, i.e., January 2005, April 2002 and July 2000. The inter-hemispheric variability of the ozone, induced by the SEP series of January 2005, has been compared with the effects connected both to larger and quite similar events. We found that during SEP events: (i) solar illumination is the key factor driving SEP-induced effects on the chemistry of the polar atmosphere; (ii) even events with limited particle flux in the range 15–40 MeV are able to change the abundance of the minor constituents in the mesosphere and upper stratosphere.     

Interactions of solar wind plasma with dust grains: Effects of strong plasma anisotropy

In this paper we re-examined the fundamental physics of charging of a dust particle in the moon environment by tenuous anisotropic solar wind plasma. The majority of work on dusty (complex) plasmas is largely concerns with laboratory plasmas, in which charging process of dust grains is very fast, thus making practical the working concept of dynamically equilibrium floating potential and grain charge. However, solar wind plasma parameters are considerably different at the moon orbit, and we found the characteristic charging time of lunar dust grains to be considerably longer, ranging from 3 to 4.6 min for micron size particles, and up to 7.6 h for 10-nm grains, depending on the value of plasma streaming velocity. These findings make it clear that the transient stage of charging process is important in the moon environment, and equilibrium floating potential and grain charge could be considered as long time asymptotic values. For this reason we re-formulated the moon dust charging process as an inherently time-dependent problem and derived the time-dependent charging equation for the grain potential for general case of anisotropic solar wind plasma. Using the results of our kinetics analysis we found that the distribution of charge density over grain surface submerged into solar wind plasma is highly anisotropic, thus making the OML model, which is based on the assumption of isotropic distribution of surface charge density, not applicable to the grain charging problem by the solar wind plasma.     

Web环境下协同装配系统的并发控制

通过对网络环境下协同装配操作的分析,总结了客户端执行结果不一致、多客户端误抓零件、多客户端同时装配同一零件、合理并行装配受阻以及装配约束冲突等5种并发装配冲突.提出了一种层次混合并发冲突控制模型(HCM,Hierarchical Hybrid Concurrency Conflict Control Model),HCM分上下两层,集成了4种并发控制策略,采用将具有装配语义的命令进行传输实现并发控制.上层采用基于全局装配序列的并发控制策略,整体上避免了前两种并发冲突;下层集成了装配操作序列化、系统加锁和用户解锁以及建立装配约束库等策略,消解了后3种并发冲突.基于HCM开发了一个原型系统,并结合实例验证了该系统的灵活性和有效性.     

腹下后置大偏距S弯进气道气动特性试验研究

对一种腹下后置大偏距S弯进气道进行高速风洞试验研究,得到了该进气道的工作特性:(1)随着流量系数的增加,进气道出口总压恢复系数略有下降,稳态周向畸变指数、紊流度和综合畸变指数均上升;当流量系数较大或较小时,进气道出口气流总压脉动均存在局部峰值。(2)在试验研究范围内,来流马赫数和侧滑角的变化对进气道性能影响不大;随着迎角的增大,总压恢复系数有所上升,畸变指数有所下降。(3)进/发匹配点处,进气道出口气流总压脉动功率谱密度分布呈现白噪声特征,对进气道/发动机匹配工作是有利的。     

镍基合金钼元素可见光谱数字化分析技术研究

使用可见光谱数字化自动分析系统对镍基合金中Mo元素可见光谱进行了分析测定,研究了镍基合金中Mo元素的Mo550.65nm和M588.83nm分析谱线组的特征,探索了镍基合金中Mo元素的数字化分析技术.结果可用于镍基合金中Mo元素的定性、定量分析和牌号鉴别.     

应用数据挖掘关联技术研究温湿度 对冲击谱试验的影响

冲击谱试验随机性强,难度较大,必须了解环境温度、湿度对试验的影响。通过对数据预处理并建立冲击谱试验评价模型,应用数据挖掘中关联分析方法提取数据背后隐藏的有用知识,获得了温度、湿度对冲击谱试验各个调试因素的影响,并分析了其间存在的某种规律性,找出了适用于冲击谱试验的环境温度、湿度范围。研究结果可为今后的产品冲击环境试验提供有力的技术支持,进一步提高冲击谱试验的试验质量和试验中的产品安全性。