洪都集团企业级信息系统数据备份策略研究

分析了洪都集团当前企业级信息系统数据备份系统中存在的问题,结合目前的主流数据备份策略,提出了基于SAN(存储局域网)的高速、可靠、安全的洪都集团新的企业级信息系统数据备份策略。     

基于CORBA的分布式网络管理的研究

详细地介绍了将CORBA这种面向对象地分布式中间件用于网络管理的方法,着重探讨在实现基于CORBA的分布式网络管理中的关键的技术-CORBA/SNMP网关,通过CORBA/SNMP网关实现CORBA域与SNMP域的透明通信。     

基于图像识别的发动机内窥智能检测系统研究

介绍了一种基于图像识别技术的航空发动机内窥检测的新方法，采用最大类间方差法计算二值化分割的最佳阈值，并将提取的图像特征输入神经网络进行分层识别，最后由专家系统对损伤程度进行了诊断。通过现场测试，证明了该方法的有效性和实用性．     

应用ART1神经网络仿真车间分组

阐述了ART1神经网络在制造单元设计过程中形成零件族的基本方法,并在基于MATLAB的软件平台上,利用其神经网络工具箱对生产过程中的实际情况进行了仿真和应用。     

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.     

基于线性神经网络的滑油金属含量预测

利用神经网络方法对某型航空发动机滑油监控系统中需重点监控的金属元素含量建立了网络，并根据该模型对其含量变化趋势进行了预测分析。某部队通过对不同实测数据的检验证明，可根据该模型的预测结果预报金属含量是否超标。     

基于Hopfield神经网络和KS函数的优化设计研究

介绍了Hopfield神经网络优化的原理。将神经网络的求解转化为非线性微分方程组的初值问题，并利用MATLAB提供的微分方程组求解器进行计算。对于多约束优化问题，KS函数的包络凝聚特性可以简化约束条件，其光滑可微特性又方便了问题的求解。将其运用于非线性约束规划和某型飞机总体参数优化问题，算例表明此方法是有效的。     

网络计费数据采集方法与应用实现

计费功能是网络管理中一个重要的基本功能,如何快速准确的采集到用户的相关计费数据,是实现高效计费功能的关键。本文通过对IP用户和拨号用户接入方式和适用计费协议分析,提出用SNMP协议命令读写路由器计费相关的MIB值和在网络底层中"侦听-转发"IP数据包的设计思想,进行用户计费数据地采集。在Windows平台上用VC++工具实现了网络计费数据采集功能模块,此模块具有一定的应用价值。     

直升机涡环状态试验数据处理研究

采用神经网络误差反向传播算法,以旋翼涡环状态试验数据为基础,研究了桨叶负扭度对直升机涡环状态特性的影响,分析了负扭度变化对旋翼扭矩、拉力平均值及脉动幅度的影响。计算结果表明,神经网络模型能够准确预测桨叶负扭度对直升机涡环状态的影响。     

基于APIHOOK技术的个人防火墙

在深入研究APIHOOK(Application programming interface HOOK)技术及其实现．并综合各种木马的行为特征的基础上构建防火墙。该防火墙的原理是借助APIHOOK技术用自编的DLL函数替代部分系统函数。新的函数实现了注册表监视，文件监视，网络监视和其他高级操作的监视。一旦发现类似木马的行为，就会根据用户可定制的规则实时作出反应。该防火墙能详细记录程序的行为，因此高级用户还可以用它来分析木马。由于该防火墙是针对木马行为特征的，因此其优点是可以预防目前一般防火墙不能预防的未知木马和新一代木马。实际的木马攻击试验证明，该防火墙能够很好地预防木马。