等质量异形粒子超高速撞击侵蚀

用数值方法模拟双锥，圆柱，椭球、圆锥和倒圆锥五类等质量异形铝粒子五种高宽比共２５种粒子对半无限铝靶的超高速撞击侵蚀，撞击速度为４ｋｍ／ｓ，给出了坑深、坑径、坑形参数和坑体积随粒子形状及高宽比的变化曲线。结果与非圆球异形粒子超高速撞击侵蚀计算有重要参考价值。     

2000年行星际南向磁场事件及相关CME的若干分析

根据WIND飞船的观测资料，讨论了2000年发生的南向磁场（BS）事件，分析了它们的源，发现12次事件中11次的源是日冕物质抛射（CME）。运用从地球向太阳时间倒推的方法和LASCO，EIT195A的观测资料，确定了这些CME。它们都是快速CME，伴有行星际激波，都具有晕状（Halo)形态，它们在日面上发生的位置是在一个不对称的区域内。还分析了5个强南向磁场（BS≥20nT)事件，发现它们的CME源，或者具有很高的能量，或者抛射方向正对地球，或者是具有叠加效应的CME系列，分析表明，在我们所讨论的太阳活动高年，大的行星际扰动和强地磁暴与高速流的联系并不密切。     

磁云—高速流相互作用的数值模拟

对１９７８年８月２７至２８日期间观测到的磁云与尾随高速流的相互作用进行数值模拟，基本拟合了１ＡＵ处的观测剖面。模拟结果表明，磁云－高速流系统将导致前向快，慢激波和后向快激波的形成。     

粒子云侵蚀问题实验研究中动能通量模拟的意义

本文首先将粒子云侵蚀条件下的驻点表面后退分解为无粒子烧蚀部分、粒子云引起的烧蚀增量部分和粒子撞击物面引起的直接侵蚀部分。然后研究了表面能量平衡关系,给出了粒子云引起的烧蚀增量表达式。最后分三类讨论粒子与飞行器的碰撞:(1)完全弹性碰撞(不符合实际);(2)完全非弹性碰撞;(3)部分弹性碰撞。对于后两种碰撞,本文分析了动能通量模拟适用的条件。     

Experimental investigation on silica dust lofting due to charging within micro-cavities and surface electric field in the vacuum chamber

The charged dust particles can be mobilized electrostatically by the repulsion between the adjacent grains and the surface electric field due to the incoming electron current and the charge accumulation within the micro-cavities. In this study, the experimental results of the initial vertical launching velocities and the maximum dust heights are compared with the estimated values for the lofted spherical dust grains by the patch surface charging equations. Silica particles with the sizes between <6 and 45?µm in radius are loaded on a graphite plate, and they are exposed to the electron beam with 450?eV energy under 4?×?10^?3?Pa vacuum chamber pressure. During the first set of the experiments, the dust samples are tested without an initial compression process and an additional horizontal electric field. Second, the dust samples are compressed by two different weights in order to increase the packing density under approximately 780.7?Pa and 3780?Pa. Finally, the dust grains are placed between the two parallel aluminum plates to apply approximately 2000?V/m and 4800?V/m horizontal electric field. A high-speed camera is used to record the transportation of the dust grains together with a microscopic telescope, and the results point out that the patch surface dust-charging model estimations are in agreement with the first experiments. On the other hand, the dust particles from the compressed samples are lofted with higher velocities than the estimations, and the number of the dust lofting observations decreases significantly, which demonstrates the importance of the micro-cavities and the increased charging requirement to overcome the contact forces. When the horizontal electric field is present, the initial vertical launching velocities are measured to be lower than the other experiments, which can be attributed to the decreased charging requirement for the dust lofting as a result of inter-particle collisions and rolling motion. According to the experimental results, the electrostatic dust transportation can be controlled not only by the ambient plasma and the solar irradiation on the airless planetary bodies, but also by the surface properties such as the contact surfaces between the dust grains, the number of the micro-cavities related to the packing density, and the presence of the horizontal electric field contributing to the external forces by other particle motions.     

边缘计算在电机远程运维系统中的应用探讨

介绍了边缘计算的基本概念及与云计算的对比。针对电机远程运维需求,介绍了电机远程运维系统的架构及主要功能。在描述边缘侧设备与远程运维平台的数据交互过程的基础上,详细阐述了边缘计算在电机远程运维系统中的应用。     

无网格法耦合RNG k-ε湍流模型在亚、跨声速翼型黏性绕流中的数值模拟

基于移动最小二乘无网格方法,耦合RNG(Re-Normalisation Group)k-ε湍流模型求解雷诺平均Navier-Stokes方程。采用AUSM(Advection Upstream Splitting Method)+-up迎风格式求解数值通量,应用在高度各向异性点云结构中取得良好结果的点云重构技术结合移动最小二乘法拟合空间导数,并用三阶SSP(Strong Stability Preserving)型Runge-Kutta显式时间推进格式求解离散后的控制方程。在此基础之上,实现了对NACA0012、RAE2822翼型亚、跨声速黏性绕流的数值模拟,给出了翼型表面压力系数分布曲线、不同位置处的平均速度剖面、马赫数等值线等计算结果,并与实验值及相关文献数值模拟结果进行比较,结果吻合较好。表明所发展的结合点云重构技术的无网格方法耦合RNGk-ε湍流模型能够成功模拟翼型亚、跨声速黏性绕流,验证了所提算法的有效性,并拓展了无网格方法求解湍流流动的途径。     

民机飞行结冰参数的模拟与校准

结冰问题的研究对于民用飞机设计十分重要,采用结冰风洞试验是主要的方法之一,欧美国家有很多成熟的结冰风洞用于型号研究。结冰风洞中需要对很多参数进行控制,其中水雾参数精确控制的难度很大,而且一般通过间接方法来进行测试校准,往往误差较大,导致不同结冰风洞试验结果往往有所差异。文章介绍了在意大利宇航中心的IWT 结冰风洞完成的冰风洞校准试验,对结冰风洞水雾参数校准方法进行了阐述,为民机结冰风洞研究提供参考。     

云计算环境下动态用户行为认证的机制、模型与分析

在云计算中,终端用户对云资源软硬件的影响和破坏远比目前用户利用因特网进行资源共享要严重的多,因此相对于用户的身份,用户的行为是否真实可信是云计算研究的一个重要内容。提出了户行为认征的机制,包括行为认证集的确立、行为证据的获得、行为认证的策略,建立相应的随机Petri网模型,并通过量化瞬时变迁的实施概率来模拟不同的认证选择,利用系统达到稳定状态时位置中的平均标记数来评价认证效果,为云计算的安全应用奠定理论和实践基础。     

A Revisit of the Phobos Events

The magnetic field disturbances detected by the Phobos-2 spacecraft in 1989 have been suggested to be caused by a ring of dust and/or gas emitted from the Martian moon, Phobos. The physical nature of these ``Phobos events' is examined using results from related investigations over the last twenty years. It is concluded that there is no clear evidence at present to support the association of magnetic field disturbances in the solar wind with Phobos. The situation will be further clarified taking advantage of the multi-spacecraft observations of the Yinghuo-1(YH-1), Mars Express and MAVEN missions beginning in 2012. It is expected that many novel features of solar wind interaction with Phobos (and possibly also Deimos) itself will also be revealed.