模拟弹塑性碰撞的修正SPH方法

从基本的无网格光滑粒子法SPH(Smoothed Particle Hydrodynamics)近似出发,修正了模拟固体力学中大变形弹塑性碰撞的SPH方法.在边界处采用修正的边界条件,弹塑性分析过程中采用增量理论计算应力,迭代过程中用守恒光滑法进行滤波修正消除拉力不稳定.对SPH方法进行了程序实现,给出了杆弹塑性碰撞的算例.计算分析表明,SPH方法节点的影响域较大、精度较相同节点间距有限元法的结果有一定差距,但是通过增加粒子数量可以提高SPH的精度,保持了其简单性和计算大变形的特性.      

大冲击测量中高频能量的影响分析

大冲击测量时,高g值激励中存在远高于测量频率之上的分量,会造成加速度计数据零漂、非线性甚至损坏;系统分析了高频能量对加速度计的影响以及产生影响的机理,试验验证了机械滤波器可有效滤除高频能量,改善压电加速度计零漂问题,并根据分析和试验结果提出相应的解决措施。     

无人集群试验评估研究现状分析及理论方法

无人集群试验评估是促进无人集群技术从理论走向实践的重要桥梁。与传统的作战系统相比,无人集群系统具有自主协同、能力涌现、智能对抗等特点,这已大大超出传统作战系统试验评估的范畴。针对上述现实需求,本文旨在综述美国和中国在推进集群试验评估方面所进行的开创性工作的基础上,主要对无人集群试验评估的概念内涵、发展现状进行了讨论分析;结合课题组在航空集群作战领域的研究基础,探讨无人集群试验评估的主要内容和可行的技术路线,为军事装备的信息化升级和智能化转型奠定基础。     

铝合金联装架焊接残余应力和变形数值模拟

基于SYSWELD有限元分析软件,以某新型战术型号铝合金联装架为产品对象,选取支撑框配对组件、弹位组件和立方体组件为典型结构件进行焊接残余应力和变形数值模拟,以期表征铝合金联装架焊接过程的残余应力分布和变形趋势。结果表明:焊缝及其附近热影响区的Von-Mises应力较高,甚至超过了5A06铝合金材料的常温屈服强度;支撑框组件焊后最大变形出现于长矩形管中央,约为6.44 mm;弹位组件的焊接变形整体表现为凹向三维结构内腔,焊接变形也多集中在长矩形管上,最大变形约为5.21 mm。另外,采用对称分散焊过程产生的焊接变形量小于逐条焊缝焊接过程,但焊接残余应力趋势则相反。     

CCD在零件几何尺寸测量方面应用的研究

本文介绍了ＣＣＤ用于测量零件几何尺寸的探讨,设计制作了测量系统,取得一批实验数据,经过分析提出了改进的方案,为今后在这方面的进一步研究奠定了基础。     

Slow Solar Wind: Observations and Modeling

While it is certain that the fast solar wind originates from coronal holes, where and how the slow solar wind (SSW) is formed remains an outstanding question in solar physics even in the post-SOHO era. The quest for the SSW origin forms a major objective for the planned future missions such as the Solar Orbiter and Solar Probe Plus. Nonetheless, results from spacecraft data, combined with theoretical modeling, have helped to investigate many aspects of the SSW. Fundamental physical properties of the coronal plasma have been derived from spectroscopic and imaging remote-sensing data and in situ data, and these results have provided crucial insights for a deeper understanding of the origin and acceleration of the SSW. Advanced models of the SSW in coronal streamers and other structures have been developed using 3D MHD and multi-fluid equations.However, the following questions remain open: What are the source regions and their contributions to the SSW? What is the role of the magnetic topology in the corona for the origin, acceleration and energy deposition of the SSW? What are the possible acceleration and heating mechanisms for the SSW? The aim of this review is to present insights on the SSW origin and formation gathered from the discussions at the International Space Science Institute (ISSI) by the Team entitled “Slow solar wind sources and acceleration mechanisms in the corona” held in Bern (Switzerland) in March 2014 and 2015.     

Book reviews

The general significance of streamers of the solar corona is discussed in the frame of our knowledge of the solar wind phenomenon and the large-scale solar magnetic structure. Thermodynamical and geometric parameters of streamers observed and measured at total solar eclipses are reviewed. Both the low part (in the form of a helmet with a cusp) and the external part (in the form of a stalk extended at many solar radii) are considered. The modelling of streamers starts with the analysis of effects produced by the solar wind flow on a magnetic structure. Facts and arguments are presented in favor of a model with a current sheet and reconnection processes going on along the axis of the streamer, especially in the non-collisional part of the radially extended streamer. Further development of the Pneuman and Kopp (1971) model is discussed, including difficulties occurring in the interpretation of a stationary solution. An empirical model satisfying observations is presented. Future researchs on streamers were discussed with emphasis on observations to be done with the space-borne coronagraphs on the SOHO spacecraft.     

叶栅相似流场存在性与唯一性

本文应用相似理论讨论了二维平面全位势方程及其不同程度的线化方程所描述的流场 ,当进口马赫数不同时 ,是否存在唯一与该马赫数对应的相似流场 ,即相似流场对进口马赫数的存在性与唯一性问题。其结果可为叶栅流场的相似变换提供部分理论依据。     

保角变换在复杂外形网格生成中的应用

保角变换在二维翼型网格生成中已经得到了大量的应用。本文描述保角变换方法生成三角翼翼身组合体，全机标模的计算网格，最后，对实用 残击机外形的网格生成也做了有效的尝试。