一种基于实体模型的三轴数控加工刀轨生成算法

实体模型是几何造型的高级模型，它具有完整的曲面拓扑关系，国内基本实体模型的数摈加工算法的需求日渐迫切，本文提出了一种适合实体模型的三轴数控加工刀位轨迹生成算法；首先根据加工行距作一组平行于刀轴的平面，与模型的待加工表面求交，得到一系列交线，再根据加工步长规划另一组与上述平面垂直且平行于刀轴的平面，与上述交线求交，得到一交点网格，判断刀具与数据点的位置关系从而得到刀位轨迹。     

飞机穿越微下击暴流风切变的智能控制

在应用模糊逻辑建模与辨识方法建立微下击暴流风切变模型的基础上，根据恒定俯仰姿态改出微下击暴流的飞行引导策略，提出了一种改出微下击暴流风切变的模糊反馈控制系统，并将遗传算法应用于该模糊逻辑控制器的设计。结果表明，本文提出的建模方法能够更真实地反映出飞机穿越微下击暴流风场的动态特性；采用模糊逻辑控制器，可使得飞机在穿越微下击暴流风场时具有较好的改出性能；另外，遗传算法的应用对已设计的模糊逻辑控制器进行了优化，进一步改善了飞机穿越微下击暴流的性能。     

基于批生产的逐段式车间作业调度算法

探讨了离散作业型（Job shop）车间中的作业调度的分阶段模型，并根据离散作业调度的阶段性提出了基于作业状态空间的逐段式车间作业调度算法，通过对一个实际车间作业调度仿真比较，此算法运算速度比最短加工时间（SPT）和最少工作量剩余（LWR）算法快，其调度结果在实际作业车间具有可执行性。     

一种新颖组合变换器拓扑研究与应用

基于电源模块并联和串联的思想，提出了一种新颖双管正激组合变换器拓扑，克服了双管正激变换器副边二极管电压应力过高，输出电压和电流脉动大，只能应用于输出中低压场合的缺点，具有副边二极管电压应力低，可靠性高，原边开关管电流应力低，输出电压和电流脉动小，磁芯元件体积小等优点，本文对该新颖组合变换器进行分析，仿真和实验，表明适合应用于输入中，高电压，输出高压，大电流场合，并成功应用于某型飞机6KVA逆变器前级变换器，各项技术指标均符合设计要求。     

加权电压控制多路输出正激变换器的研究

研究了一种经济实用的多路输出DC／DC变换器的输出电压控制方法－加权电压控制，该方法可有效地改善多路输出变换器输出的稳态稳压精度和动态响应性能，对应用加权电压控制的两路输出正激变换器进行直流稳态分析，得出直流稳态等效电路模型和输出电路压数学表达式，分析了加权因子对输出电压的影响，给出了设计加权因子的原则和设计方法，通过样机实验，验证了该方法能够较好地实现多路输出稳压指标。     

快速可重构信息系统的框架研究(英文)

变化和重构是快速可重构信息系统 (RRIS)的两个核心概念 ,RRIS对变化的适应或演化能力使它优于传统信息系统。本文首先提出 RRIS的体系结构 ,然后以 RRIS框架为重点 ,讨论框架的定义、分类及设计 ,研究框架的构成、构成元素 (业务构件 )的设计及构件如何在构架的组织下协调地安插在 CORBA的软总线上 ,实现类似硬件IC的即插即用。构件在框架上即插即用的灵活机制及热点构件 (反映变化 )的灵活运用 ,提高了框架的可扩展性、可定制性 ,从而提高了 RRIS适应变化的可重构性。     

Nitrogen fixation on early Mars and other terrestrial planets: experimental demonstration of abiotic fixation reactions to nitrite and nitrate

Understanding the abiotic fixation of nitrogen is critical to understanding planetary evolution and the potential origin of life on terrestrial planets. Nitrogen, an essential biochemical element, is certainly necessary for life as we know it to arise. The loss of atmospheric nitrogen can result in an incapacity to sustain liquid water and impact planetary habitability and hydrological processes that shape the surface. However, our current understanding of how such fixation may occur is almost entirely theoretical. This work experimentally examines the chemistry, in both gas and aqueous phases, that would occur from the formation of NO and CO by the shock heating of a model carbon dioxide/nitrogen atmosphere such as is currently thought to exist on early terrestrial planets. The results show that two pathways exist for the abiotic fixation of nitrogen from the atmosphere into the crust: one via HNO and another via NO(2). Fixation via HNO, which requires liquid water, could represent fixation on a planet with liquid water (and hence would also be a source of nitrogen for the origin of life). The pathway via NO(2) does not require liquid water and shows that fixation could occur even when liquid water has been lost from a planet's surface (for example, continuing to remove nitrogen through NO(2) reaction with ice, adsorbed water, etc.).     

New insights into Titan's organic chemistry in the gas and aerosol phases.

Titan, the largest satellite of Saturn, with a dense atmosphere very rich in organics, and many couplings in the various parts of its "geofluid", is a reference for studying prebiotic chemistry on a planetary scale. New data have been obtained from experiments simulating this organic chemistry (gas and aerosol phases), within the right ranges of temperature and a careful avoiding of any chemical contamination. They show a very good agreement with the observational data, demonstrating for the first time the formation of all the organic species already detected in Titan atmosphere including, at last, C4N2, together with many other species not yet detected in Titan. This strongly suggests the presence of more complex organics in Titan's atmosphere and surface, including high molecular weight polyynes and cyanopolyynes. The NASA-ESA Cassini-Huygens mission has been successfully launched in October 1997. The Cassini spacecraft will reach the Saturn system in 2004 and become an orbiter around Saturn, while the Huygens probe will penetrate into Titan's atmosphere. In situ measurements, in particular from Huygens GC-MS and ACP instruments, will provide a detailed analysis of the organics present in the air, aerosols, and surface. This very ambitious mission should yield much information of crucial importance for our knowledge of the complexity of Titan's chemistry, and, more generally for the field of exobiology.     

一种新的射频仿真目标位置控制方法与软件研究

针对射频目标仿真系统中目标位置的控制，本文通过对国内外目标位置控制的常用方法进行研究，提出一种新的通用目标位置控制方法，该方法适用于任何天线分布的面阵。利用这种新的方法编写了基于三元阵天线阵面的射频仿真目标位置控制软件，实现对多目标在天线阵面上多种轨迹运动下的高速准确的定位，并能实时监视目标的运动状态和运动轨迹。