可伸缩挠性结构的稳定控制

对于挠性梁收缩过程的不稳定性,提出了边界控制方案,并设计了相应的控制律。受控结构的振动能量总是被耗散,系统的阻尼被增强,从而挠性梁的伸展过程、收缩过程和平台保持过程都被稳定化。     

刚性太阳电池阵基板的研究

文章简要地叙述碳纤维复合材料刚性太阳电池阵基板的结构设计,理论分析,模态试验和振动试验。理论分析和试验结果比较一致。通过试验还解决了基板各种复合材料的力学性能测试问题,取得了必要的数据。     

γ-TiAl基自生复相材料的显微组织特征

研究了添加硼、硅、碳的 γ-TiAl基自生复相材料的显微组织特征.在压力4?GPa、温度1?273?K、反应合成时间60?min的条件下,通过粉末间的原位置换放热反应制备了样品.研究发现:Ti-Al-B三元合金含有TiAl相、Ti₃Al相和TiB₂相;Ti-Al-Si三元合金含有TiAl相、Ti₃Al相和Ti₅(Al,Si)₃相;Ti-Al-C三元合金含有TiAl相和Ti₃AlC相;Ti-Al-B-Si四元合金含有TiAl相、Ti₃Al相、TiB₂相和Ti₅(Al,Si)₃相;Ti-Al-B-C四元合金含有TiAl相、Ti₃AlC相和TiB₂相;Ti-Al-B-Si-C五元合金含有TiAl相、Ti₃AlC相、TiB₂相和Ti₅(Al,Si)₃相,其组织非常相似于预先设计的组织.在此基础上就不同相对性能的影响进行了分析.     

一类线性不确定大系统的分散变结构控制

研究了具有参数摄动、关联影响和外界干扰等不确定性因素影响的线性大系统的分散控制问题,在假设系统不确定性有界且满足一定匹配条件的前提下,提出了一种分散变结构滑模控制算法,并给出了消颤方案和控制受限的解决方法.该算法结构简单计算量小,同时闭环系统具有较好的动态特性和较强的鲁棒性,数字仿真表明了该算法的有效性.      

基于RTI的PDM框架实现策略

近年来,随着分布交互仿真技术的不断发展,解决仿真系统互操作和重用的高层体系结构的提出,以及ＰＤＭ技术的广泛应用和面临的新的挑战,提出了基于ＲＴＩ的ＰＤＭ框架技术,采用ＲＴＩ作为框架的运行支撑系统,以及通过联邦的运行方式,支持企业的动态联盟。阐述了基于ＲＴＩ的ＰＤＭ框架的特点,并对其实现的策略和应用作了有意义的研究。     

多维驱动微型振动平台的研制

一种以压电元件为驱动源,结合柔性铰链机构的微型振动平台,通过计算机设计控制电压波形,对其进行三维振动控制.通过实验证明,该机构具有良好的波形跟踪性能,易于实现复杂控制波形,适用于微型机械的动态性能测试.     

Fractal Structure of the Heliospheric Plasma Sheet at the Earth''''s Orbit

An analysis of the data from the Wind and IMP-8 spacecraft revealed that a slow solar wind, flowing in the heliospheric plasma sheet, represents a set of magnetic tubes with plasma of increased density (N > 10cm-3 at the Earth's orbit). They have a fine structure at several spatial scales (fractality), from 2°-3°(at the Earth's orbit, it is equivalent to 3.6-5.4h, or (5.4-8.0)×106km) to the minimum about 0.025°, i.e. the angular size of the nested tubes is changed nearly by two orders of magnitude. The magnetic tubes at each observed spatial scale are diamagnetic, i.e. their surface sustains a flow of diamagnetic (or drift) current that decreases the magnetic field within the tube itself and increases it outside the tube. Furthermore, the value of β= 8π[N(Te + Tp)]/B2 within the tube exceeds the value of βoutside the tube. In many cases total pressure P = N(Te + Tp) + B2/8πis almost constant within and outside the tubes at any one of the aforementioned scales.     

Non-Thermal Processes in Cosmological Simulations

Non-thermal components are key ingredients for understanding clusters of galaxies. In the hierarchical model of structure formation, shocks and large-scale turbulence are unavoidable in the cluster formation processes. Understanding the amplification and evolution of the magnetic field in galaxy clusters is necessary for modelling both the heat transport and the dissipative processes in the hot intra-cluster plasma. The acceleration, transport and interactions of non-thermal energetic particles are essential for modelling the observed emissions. Therefore, the inclusion of the non-thermal components will be mandatory for simulating accurately the global dynamical processes in clusters. In this review, we summarise the results obtained with the simulations of the formation of galaxy clusters which address the issues of shocks, magnetic field, cosmic ray particles and turbulence.     

L10结构金属间化合物空位形成能

L1₀结构CoPt和FePt 薄膜因其高磁各向异性而成为新一代超高磁记录密度材料.采用Miedema理论计算了多种L1₀结构金属间化合物的空位形成能.研究结果表明:在这些金属间化合物中可能形成的空位类型,如FeNi和MnNi合金中易形成Ni空位;FePt和FePd合金中易形成Fe空位;CoPt合金中易形成Co空位;NiPt合金中易形成Ni空位;MnPt合金中易形成Pt空位;MnPd和MnHg合金中易形成Mn空位;MnRh合金中易形成Rh空位.这一研究结果为进一步研究开发高性能的磁性薄膜提供了理论依据.     

Simulation Techniques for Cosmological Simulations

Modern cosmological observations allow us to study in great detail the evolution and history of the large scale structure hierarchy. The fundamental problem of accurate constraints on the cosmological parameters, within a given cosmological model, requires precise modelling of the observed structure. In this paper we briefly review the current most effective techniques of large scale structure simulations, emphasising both their advantages and shortcomings. Starting with basics of the direct N-body simulations appropriate to modelling cold dark matter evolution, we then discuss the direct-sum technique GRAPE, particle-mesh (PM) and hybrid methods, combining the PM and the tree algorithms. Simulations of baryonic matter in the Universe often use hydrodynamic codes based on both particle methods that discretise mass, and grid-based methods. We briefly describe Eulerian grid methods, and also some variants of Lagrangian smoothed particle hydrodynamics (SPH) methods.