风力机翼型的多学科设计优化

为了解决优化计算和流场分析耦合求解的难题,并实现优化流程的自动化运行,采用多学科优化设计框架软件,针对风力机专用翼型运行工况,对低雷诺数航空翼型NACA 4412的气动性能进行优化设计。软件集成了翼型生成、网格划分、流场分析、优化计算4个模块。其中,流场计算采用N-S方程求解;优化方法为多岛遗传算法。优化结果表明,优化后翼型有较高的升力系数和相对大的升阻比,其升阻比提高了15.9%。该方法可以实现多学科领域的精确分析和整个优化循环过程的自动化运行,也能为其他气动外形的优化设计提供参考。     

一种惯组外场标定振动干扰的分离方法

惯组在外场进行标定时常会受到地基振动的干扰,这种干扰会对惯组的测试精度造成极大的影响.为解决这一问题,根据工程实际需要,提出了一种基于经验模态分解和数字信号滤波技术相结合的惯组输出振动干扰分离方法.首先利用经验模态分解将受振动干扰的惯组输出分解成若干本征模态分量,然后采用低通滤波器对高频分量进行滤波,对低频分量相应区段做幅值修正,最后将处理过的各分量叠加,即重构出消除振动干扰的信号.相对于传统的剔除野值后的平滑滤波方法,新方法保证了数据信息的完整性,有效降低了振动干扰的不利影响,提高数据信息的可靠性和真实性.仿真实验和工程实践表明,该方法对外场的瞬时振动干扰有较强地分离能力.     

凸曲面的离散求交算法及其在飞机设计上的应用

构建精确的目标外形是飞机设计的必要条件。本文给出了凸曲面离散求交的算法，在飞机设计中采用此方法，能够得到机身机翼交线的准确位置。     

基于修正角模型的平显工作状态仿真研究

研究了在某型平显仿真训练器中实现平显工作状态仿真的方法。首先介绍了平显工作画面,分析了瞄准环及其构成修正角的原理;然后通过对工作式和各相关参数的计算,建立了平显的瞄准环及其修正角的模型,并给出了计算瞄准环环心位置和直径的基本关系式;最后讨论了用VisualC++编程实现平显工作画面中公共符号和瞄准环仿真的方法。通过建立修正角模型,可使实现的平显仿真工作画面在外观上和操作特性上与实际平显工作状态一致。     

一个拼音汉字自动转换系统的设计与实现

给出了拼音汉字转换的定义，并建立了一个带调拼音词句到汉字语句的自动转换系统。它由五个部分组成，自动分词模块，词法分析模块，句法和语义分析模块，语义修饰模块和显示模块。其中句法分析是系统的核心，在比较各种方法的基础上选择了扩充转移网络模型，使ＡＴＮ的优点和音字转换的特点得到较好的结合，测试结果表明，系统的正确转换率达到９７％。     

基于C/S和B/S混合模式上机实验一体化系统的研究

基于C／S和B／S混合模式上机实验一体化系统的研究就是要解决当前上机教学中急需的计算机电子化管理的问题。该项目的完成除了对计算中心计算机基础课程上机实验适用以外，其它相关专业课程的上机教学和各种计算机课程综合训练等也同样适用，项目的完成对于提高上机实验环节的教学质量具有重要作用，因此具有实际意义。     

Performance of a simple Closed Aquatic Ecosystem (CAES) in space.

A simple Closed Aquatic Ecosystem (CAES) consisting of single-celled green algae (Chlorella pyrenoidosa, producer), a spiral snail (Bulinus australianus, consumer) and a data acquisition and control unit was flown on the Chinese Spacecraft SHENZHOU-II in January 2001 for 7 days. In order to study the effect of microgravity on the operation of CAES, a 1 g centrifuge reference group in space, a ground 1 g reference group and a ground 1 g centrifuge reference group (1.4 g group) were run concurrently. Real-time data about algae biomass (calculated from transmission light intensity), temperature, light and centrifugation of the CAES were logged at minute intervals. It was found that algae biomass of both the microgravity group and the ground 1 g-centrifuge reference group (1.4 g) fluctuated during the experiment, but the algae biomass of the 1 g centrifuge reference group in space and the ground 1 g reference group increased during the experiment. The results may be attributable to influences of microgravity and 1.4 g gravity on the algae and snails metabolisms. Microgravity is the main factor to affect the operation of CAES in space and the contribution of microgravity to the effect was also estimated. These data may be valuable for the establishment of a complex CELSS in the future.     

Interleaved boost converter with zero diode reverse-recovery loss

A three-phase interleaved continuous-inductor-current-mode (CICM) boost converter with zero diode reverse-recovery loss is proposed. In the converter, the di/dt of the output rectifiers is controlled by an integrated magnetic component. All the output rectifiers can be turned off softly and a very high efficiency is obtained. The equivalent-circuit model of the integrated inductors, the operation principle of the converter, and the design issues are discussed. Simulation and experimental results are presented.     

Physics of Substorm Growth Phase,Onset, and Dipolarization

A new scenario of substorm growth phase, onset and dipolarization during expansion phase and the corresponding physical processes are presented. During the growth phase, as a result of enhanced plasma convection, the plasma pressure and its gradient continue to be enhanced over the quiet-time values in the plasma sheet. Toward the late growth phase, a strong cross-tail current sheet is formed in the near-Earth plasma sheet region, where a local magnetic well is formed. The equatorial plasma beta (β _eq ) can reach a local maximum with value larger than 50 and the cross-tail current density can be enhanced to over 10nA/m² as obtained from 3D quasi-static magnetospheric equilibrium solutions for the growth phase. The most unstable kinetic ballooning instabilities (KBI) are expected to be located in the tailward side of the strong cross-tail current sheet region. The field lines in the most unstable KBI region map to the transition region between the region-l and region-2 currents in the ionosphere, which is consistent with the observed initial brightening location of the breakup arc in the intense proton precipitation region. The KBI explains the AMPTE/CCE observations that a low frequency instability with a wave period of 50–75 seconds is excited about 2–3 min prior to substorm onset and grows exponentially to a large amplitude at the onset of current disruption (or current reduction). At the onset of current disruption higher frequency instabilities are excited so that the plasma and electromagnetic field fluctuations form a strong turbulent state. Plasma transport takes place due to the strong turbulence to relax the ambient plasma pressure profile so that the plasma pressure and current density are reduced and the ambient magnetic field intensity increases by more than a factor of 2–3 in the high-β _eq region and the field line geometry recovers from tail-like to dipole-like – dipolarization.