虚拟供应链在中小企业集群中的可靠性分析

文章通过对两种不同企业集群组织形式的比较,重点探讨了形成企业竞争优势的企业虚拟组织的机理及结构功能.以关系型同质中小企业集群为研究对象,基于供应链虚拟一体化的思路,对其竞争优势进行研究,同时提出这种组织模式可能存在的潜在问题并加以理论上的证明,力求找到适合我国中小企业现状的发展之路.     

Linux 2．6内存保护机制研究

基于Intel i386平台处理器和Linux 2.6内核源代码,从硬件内存保护和虚拟内存保护两个方面分析了最新的Linux内存保护机制,其中硬件内存保护机制包括段式映射阶段的访问控制、页式映射阶段的访问控制以及最新内存保护NX(No eXecute)技术,虚拟内存保护机制包括虚拟区间保护、虚拟区间加锁和Hole技术.最后进一步讨论了增强Linux内存保护的方案.     

虚拟现实系统中三维视觉几何建模

三维视觉建模是建立虚拟现实系统的基础,文中主要研究了虚拟现实系统中对象形状的建造方法、纹理映射的数学建模,并对其常用算法进行了比较分析。     

基于小波分析的虚拟仪器

以小波分析原理为基础,开发出可视化和可操作的虚拟仪器,用于处理实验数据与药物分析.应用小波变换实现数据消噪,利用LabVIEW 和MATLAB软件开发出虚拟仪器.用该仪器可实现对数据进行消噪;在不经分离的情况下,对药物实现多组分的含量测定及对实验结果进行分析和预测,采用的方法和开发的软件在药学领域有其独到的应用价值.     

飞行控制系统虚拟原型技术

 在综述虚拟原型技术的基础上,研究飞行控制系统虚拟原型机以及采用虚拟原型技术后飞控系统的设计方法。提出了飞控系统设计,特别是飞控计算机设计中,基于虚拟原型技术的 3个层次应用,分析了构筑虚拟原型机需要重点解决的一些问题。     

Magnetosphere Imaging Instrument (MIMI) on the Cassini Mission to Saturn/Titan

The magnetospheric imaging instrument (MIMI) is a neutral and charged particle detection system on the Cassini orbiter spacecraft designed to perform both global imaging and in-situ measurements to study the overall configuration and dynamics of Saturn’s magnetosphere and its interactions with the solar wind, Saturn’s atmosphere, Titan, and the icy satellites. The processes responsible for Saturn’s aurora will be investigated; a search will be performed for substorms at Saturn; and the origins of magnetospheric hot plasmas will be determined. Further, the Jovian magnetosphere and Io torus will be imaged during Jupiter flyby. The investigative approach is twofold. (1) Perform remote sensing of the magnetospheric energetic (E > 7 keV) ion plasmas by detecting and imaging charge-exchange neutrals, created when magnetospheric ions capture electrons from ambient neutral gas. Such escaping neutrals were detected by the Voyager l spacecraft outside Saturn’s magnetosphere and can be used like photons to form images of the emitting regions, as has been demonstrated at Earth. (2) Determine through in-situ measurements the 3-D particle distribution functions including ion composition and charge states (E > 3 keV/e). The combination of in-situ measurements with global images, together with analysis and interpretation techniques that include direct “forward modeling’’ and deconvolution by tomography, is expected to yield a global assessment of magnetospheric structure and dynamics, including (a) magnetospheric ring currents and hot plasma populations, (b) magnetic field distortions, (c) electric field configuration, (d) particle injection boundaries associated with magnetic storms and substorms, and (e) the connection of the magnetosphere to ionospheric altitudes. Titan and its torus will stand out in energetic neutral images throughout the Cassini orbit, and thus serve as a continuous remote probe of ion flux variations near 20R _S (e.g., magnetopause crossings and substorm plasma injections). The Titan exosphere and its cometary interaction with magnetospheric plasmas will be imaged in detail on each flyby. The three principal sensors of MIMI consists of an ion and neutral camera (INCA), a charge–energy–mass-spectrometer (CHEMS) essentially identical to our instrument flown on the ISTP/Geotail spacecraft, and the low energy magnetospheric measurements system (LEMMS), an advanced design of one of our sensors flown on the Galileo spacecraft. The INCA head is a large geometry factor (G ∼ 2.4 cm² sr) foil time-of-flight (TOF) camera that separately registers the incident direction of either energetic neutral atoms (ENA) or ion species (≥5^∘ full width half maximum) over the range 7 keV/nuc < E < 3 MeV/nuc. CHEMS uses electrostatic deflection, TOF, and energy measurement to determine ion energy, charge state, mass, and 3-D anisotropy in the range 3 ≤ E ≤ 220 keV/e with good (∼0.05 cm² sr) sensitivity. LEMMS is a two-ended telescope that measures ions in the range 0.03 ≤ E ≤ 18 MeV and electrons 0.015 ≤ E≤ 0.884 MeV in the forward direction (G ∼ 0.02 cm² sr), while high energy electrons (0.1–5 MeV) and ions (1.6–160 MeV) are measured from the back direction (G ∼ 0.4 cm² sr). The latter are relevant to inner magnetosphere studies of diffusion processes and satellite microsignatures as well as cosmic ray albedo neutron decay (CRAND). Our analyses of Voyager energetic neutral particle and Lyman-α measurements show that INCA will provide statistically significant global magnetospheric images from a distance of ∼60 R _S every 2–3 h (every ∼10 min from ∼20 R _S). Moreover, during Titan flybys, INCA will provide images of the interaction of the Titan exosphere with the Saturn magnetosphere every 1.5 min. Time resolution for charged particle measurements can be < 0.1 s, which is more than adequate for microsignature studies. Data obtained during Venus-2 flyby and Earth swingby in June and August 1999, respectively, and Jupiter flyby in December 2000 to January 2001 show that the instrument is performing well, has made important and heretofore unobtainable measurements in interplanetary space at Jupiter, and will likely obtain high-quality data throughout each orbit of the Cassini mission at Saturn. Sample data from each of the three sensors during the August 18 Earth swingby are shown, including the first ENA image of part of the ring current obtained by an instrument specifically designed for this purpose. Similarily, measurements in cis-Jovian space include the first detailed charge state determination of Iogenic ions and several ENA images of that planet’s magnetosphere.This revised version was published online in July 2005 with a corrected cover date.     

基于VXI总线的检测软件设计

基于VXI总线和虚拟仪器技术，研制开发了用于外场的模拟式电子控制器检测软件，并对软件开发的过程和要求进行了分析，重点解决了程序设计中的需求分析和模块化设计问题。     

基于虚拟目标点制导的误差分析

基于标准弹道确定的虚拟目标点位置在弹道小扰动的情况下能够确保闭路制导的精度,但是在弹道大扰动时,虚拟目标点位置修正误差变大,能否保证闭路制导的精度值得探讨。通过给弹道一个大扰动进行了弹道仿真,结果表明,弹道大扰动会引起闭路制导的方法误差变大。     

利用虚拟仪器实现角速度波动率的采集和处理

利用NI 的PXI-6281高速数据采集卡来完成角速度波动信号的采集,借鉴信号失真度的概念,分析角速度反馈信号的基波和高次谐波大小,求取高次谐波与基波幅值比,作为角速度波动率.     

电子商务中虚拟现实的应用

针对虚拟现实技术在电子商务等领域的广泛应用，阐述了虚拟现实的概念、几种实现方法的原理。给出了用杰图造型师软件实现面向景点的三维全景图和面向物体的三维全景图的方法和步骤；分析了连接www网的场景描述语言—VRML的语言结构，编辑方法和VRML的常用浏览器软件，这样用键盘或鼠标任意改变视角来观看在网页上展示的各种产品。总结了虚拟现实技术未来的应用领域和应用前景，以及受成本、硬件、带宽、模拟环境等因素的影响可以选择不同的技术形式。