Phase Space Density Analysis of Energy Transport in the Earth’s Magnetotail

Two energetic events in the Earth’s magnetotail detected by Geotail are examined with detailed analysis of three-dimensional velocity phase space density. It is found that the occurrence of multiple ion components is high during these dynamic episodes. Different populations evolve independently of each other, suggesting particles from multiple activity sites contributing to the observed phase space density. The transport properties with consideration of multiple components are evaluated, with the result showing significant differences from those based on a single fluid approach. This comparison indicates that precise evaluation of the energy and magnetic flux transport of energetic events in the magnetotail requires resolving individual populations in the phase space density.     

复合材料锥壳0°铺层的自动铺放成型方法研究

研究了一种基于自动铺带技术的复合材料锥壳0°铺层成型方法：根据锥壳构件尺寸将等宽预浸带数控分切成预定尺寸的直角梯形预浸带片，按特定方式铺放到锥壳表面并使每两片拼成一个等腰梯形单元，多个等腰梯单元形构成锥壳的0°铺层；并针对这种成型方法设计了一种实现锥壳0°铺层自动成型的装置。采用该方法及其设备可以实现锥壳0°铺层的自动化制造，提高成型效率、降低废料率、稳定工艺质量，降低装备制造成本。     

The Grain Impact Analyser and Dust Accumulator (GIADA) Experiment for the Rosetta Mission: Design, Performances and First Results

The Grain Impact Analyser and Dust Accumulator (GIADA) onboard the ROSETTA mission to comet 67P/Churyumov–Gerasimenko is devoted to study the cometary dust environment. Thanks to the rendezvous configuration of the mission, GIADA will be plunged in the dust environment of the coma and will be able to explore dust flux evolution and grain dynamic properties with position and time. This will represent a unique opportunity to perform measurements on key parameters that no ground-based observation or fly-by mission is able to obtain and that no tail or coma model elaborated so far has been able to properly simulate. The coma and nucleus properties shall be, then, clarified with consequent improvement of models describing inner and outer coma evolution, but also of models about nucleus emission during different phases of its evolution. GIADA shall be capable to measure mass/size of single particles larger than about 15 μm together with momentum in the range 6.5 × 10⁻¹⁰ ÷ 4.0 × 10⁻⁴ kg m s⁻¹ for velocities up to about 300 m s⁻¹. For micron/submicron particles the cumulative mass shall be detected with sensitivity 10⁻¹⁰ g. These performances are suitable to provide a statistically relevant set of data about dust physical and dynamic properties in the dust environment expected for the target comet 67P/Churyumov–Gerasimenko. Pre-flight measurements and post-launch checkouts demonstrate that GIADA is behaving as expected according to the design specifications. The International GIADA Consortium (I, E, UK, F, D, USA).     

A Thermodynamic Approach to the Magnetospheric Complexity: The Role of Fluctuations

Recent studies evidenced that the magnetotail dynamics looks like the one of an avalanching system. This fact has been related with a near criticality dynamics and modelled by singular diffusion and transport equations. Here, we discuss some features of the Earth’s magnetotail dynamics using a thermodynamic approach. In detail we discuss the role played by fluctuations in singular diffusion and relaxation processes from a non-equilibrium thermodynamics point of view. Moreover, the emergence of non-Gaussian statistics is discussed in the framework of the thermodynamics of composite systems.     

β Cep stars from a spectroscopic point of view

In this review we present the current status of line-profile-variation studies of β Cep stars. Such studies have been performed for 26 bright members of this class of pulsating stars in the past 25 years. We describe all these currently available data and summarize the interpretations based on them in terms of the excited pulsation modes. We emphasize that line-profile variations offer a much more detailed picture of the pulsational behaviour of pulsating stars compared to ground-based photometric data. The latter, however, remain necessary to unravel the often complex frequency pattern and to achieve unambiguous mode identification for multiperiodic β Cep stars and also to derive the pulsational properties of the faint members of the class. We highlight the statistical properties of the sample of 26 stars for which accurate spectroscopic studies are available and point out some future prospects. This revised version was published online in June 2006 with corrections to the Cover Date.     

Direct integration methods in dynamic problems of structural mechanics

A method of direct integration with respect to time is proposed to solve dynamic problems of structural mechanics and comparison with the well-known methods is presented.     

月面冯·卡门撞击坑的着陆选址和科学探测目标浅析

冯·卡门（Von Kármán）撞击坑位于月球背面南极—艾肯（South Pole-Aitken,SPA）盆地中部,是中国“嫦娥4号”计划的优先级较高的探测目标。对该撞击坑的着陆和探测,有助于揭示月球形成和演化的一些关键问题,在月球科学研究中具有重大的意义。论文概要总结了冯·卡门撞击坑的研究意义和科学价值;结合LRO卫星LOLA数据、Clementine UV-VIS数据、GRAIL数据、“嫦娥2号”卫星CELMS等数据,简要分析了冯·卡门撞击坑的地形、成分、深部结构和亮?%rater are analyzed with LRO satellite LOLA data,Clementine UV-VIS data,GRAIL data,and Chang''E-2 CELMS data and their scientific meanings are also presented. Finally,combined with our results and the previous prospects about theVon Kármán crater,three candidate landing sites and the possible scientific discoveries are proposed.     

基于伪寿命的加速退化机理一致性边界检验

根据寿命型随机变量的加速机理一致性条件,提出一种基于伪寿命的加速退化机理一致性边界检验方法,通过由低到高逐一对各个加速应力水平下的退化机理一致性进行检验,来确定加速退化机理一致性的边界应力水平.针对工程常用的两类寿命型分布——对数正态分布和Weibull分布,分别以对数标准差和形状参数为退化机理表征量,在产品伪寿命估计的基础上建立了退化机理表征量齐性检验的F统计量,导出了退化机理一致性检验拒绝域的解析式,给出了退化机理一致性边界检验的具体步骤.该方法能够充分利用多个应力水平下表征产品退化机理一致的横向信息,有效提高了检验的精度.以某镀膜平板玻璃热退化机理一致性边界温度的确定为例,分析说明了该方法的合理性与有效性.     

45#钢微动疲劳特性的研究

微动疲劳发生于两零件的接触表面间，紧密接触表面间的微辐滑动是产生微动疲劳的重要因素。微动疲劳导致零部件的强度显著降低，是引发意外失效事故的重要原因之一，因此研究材料的微动疲劳特性具有重要的理论和工程应用价值。本文研究了45^#钢在室温下的微动疲劳特性，通过采用宏观力学试验与微观结构分析相结合的方法探讨了45^#钢微动疲劳破坏的机理。通过对试验结果进行分析，确定了显著影响微动疲劳特性的重要因素，从而加深了对微动疲劳过程的认识，而且其中一些结果可以推广应用到其他材料上去。     

落儿岭-土地岭断裂几何结构及晚第四纪活动特征初探

落儿岭-土地岭断裂是东大别地区重要的发震构造,然而限于自然地理条件等因素,前人对其的研究并不充分。本文以发生多次中强地震的落儿岭-土地岭断裂为研究对象,在高精度卫星影像解译的基础上,通过详细的野外地质地貌调查,尤其是对典型断层剖面进行分析,研究落儿岭-土地岭断裂的断错地质地貌特征、几何结构及活动特征。通过野外调查并结合其他资料分析认为落儿岭-土地岭断裂为发育于大别造山带内部的一条走向NE、向NW陡倾的断裂带。依据地质地貌特征及地震活动性,断裂可以划分为杨树沟-黑石渡段和黑石渡-横塘岗乡段两个几何段落。断裂最新活动时代为中更新世晚期—晚更新世早期,断裂最新活动继承了中生代以来的运动方式,以兼具右旋走滑的拉张正断为主。