异型封闭腔辐射几何学问题

讨论了解决异型封闭腔辐射几何学问题的几种方法:异型封闭腔内,表面间可见性的判断方法;优化异型封闭腔角系数计算的方法;确定异型封闭腔内定向辐射的壁面辐射源的方法.计算了两种结构喷管封闭腔内的角系数,并从角系数的互换性和完整性定理验证了方法的正确性和有效性,为异型封闭腔的辐射计算解决了几何问题.     

The fundamental parameters of the central stars of eight WR ring nebulae

We describe work that has recently been completed on deriving the fundamental parameters of eight WR stars through the photoionization modelling of their surrounding nebulae using non-LTE WR flux distributions. The resulting effective temperatures range from 57 000–71 000 K for the WN4-5 stars and <30 000–42 000 K for the WN6-8 stars. The derived stellar parameters are compared with those obtained from stellar emission line modelling. We find good agreement for the hot early WN stars, indicating that the non-LTE WR flux distributions have essentially the correct shape in the crucial far-UV region. We find lower temperatures for the four cooler late WN stars, particularly for the two WN6 stars. For the nebulae surrounding these stars, we find that the model flux distributions produce too much nebular ionization. We suggest that these discrepancies arise because of the lack of line-blanketing in the WR atmospheres. For the WO1 central star of G2.4+1.4, with strong nebular He II 4686 A emission, we derive a temperature of 105 000 K, somewhat less than previous estimates. The positions of our eight WR stars on the H-R diagram are compared with the evolutionary tracks of Maeder (1990) for solar metallicity. In common with previous workers, we find that our derived luminosities are too low, giving an initial mass range of 25–40 M, below that expected for the majority of WR stars.     

Energetic particles at high latitudes

We review work on diffusion coefficients of energetic particles with an attempt to extract implications on their behaviour at high latitudes. In the ecliptic plane results from solar energetic particle propagation between the Sun and about 5 AU can be described by an effective radial mean free path _r which is approximately constant as a function of distancer. When particle propagation in three dimensions in the heliosphere is considered it is not sufficient to consider _r only. Jovian electrons can be used as probes to determine the parameters of three-dimensional diffusion. In the polar regions diffusion is dominated by its parallel component. Some predictions how should vary with latitude are discussed. For different choices of this variation we present expectations for intensity-time profiles of solar particle events during the Ulysses polar passages.     

鱼雷发射控制系统测试设备的设计与实现

介绍了鱼雷发射控制系统测试设备的功能和工作原理,给出了测试设备的硬件构成和软件设计方法,并分析设计中所采用的关键技术,采用LabWindows/CVI作为软件开发平台,具有良好的人机界面.     

制导火箭弹制导控制系统精益设计方法

制导火箭弹在陆军未来战争中正发挥越来越重要的作用，制导控制系统设计是制导火箭弹研制的核心和难题。提出了一种适用于制导火箭弹制导控制系统的精益设计方法，将设计过程分为数据处理环节、自动驾驶仪设计环节、制导律设计环节和六自由度仿真分析环节4个部分，并将标准化和基于模型的思想体现在精益化设计软件中，从而给出了一条可以又快又好地完成系统设计的技术途径。     

非线性主轴降维映射法在固体火箭发动机设计优化中的应用

为在二维或三维空间中表达固体火箭发动机高维设计空间,引入非线性主轴降维映射法对多维非线性设计优化问题进行降维处理。以某大型固体火箭发动机设计问题为例,将10变量4有效约束优化问题降维映射到二维空间进行研究,拟合的非线性主轴降维映射模型中,目标函数和约束函数的相对误差控制在1.5%以内。研究表明,非线性主轴降维映射法具有发现多变量非线性优化数学模型本征特性的特点,能对设计变量重要性排序;通过降维展示设计空间全景,为优化算法和优化初始点优选提供了直观、有力的工具;优化轨迹实时展示为优化算法性质研究及算法切换提供了依据;根据优化轨迹从优化结果在降维空间中的位置能够判断优化结果是否具有全局最优解特性。     

稳态等离子体推力器磁场设计与数值分析

首先分析了稳态等离子体推力器性能对磁场的要求，据此介绍了磁路系统的工程设计原则和方法；然后，采用ANSYS大型有限元分析软件对一个具体的稳态等离子体推力器在额定工况下的磁场进行了计算，获得了满意的结果，通过对结果的分析获得了对有关现象的直观深入的认识，为所计算具体推力器的改进设计提供了线索；同时，也证实了以ANSYS为软件平台的稳态等离子体推力器磁路系统计算机数值仿真辅助设计的可行性和有效性。     

一种基于Agent的武器装备保障性评估系统的设计

运用Agent技术设计了一种武器装备保障性评估系统。首先介绍了装备保障性评估的任务、功能和工作流程,然后研究了Agent的内部结构和工作原理;最后依据武器装备保障性评估流程,设计了保障性评估系统总体结构,阐述了运行原理。     

联合应用现代优化方法与S2流面计算进行多级涡轮的气动设计

本文联合应用S2流面正问题计算和多级局部优化设计对某三级涡轮进行多级气动优化设计。优化联合采用人工神经网络和遗传算法,流场计算采用全三维粘性流N-S方程求解,计算网格采用H-O-H型网格,即入口段、出口段采用H型网格,叶片区域采用O型网格。通过优化,总效率提高1.1%,总体性能提高,达到设计要求。     

基于CORBA实现专业领域软件在网络环境下的集成

如何有效地将已有系统集成或移植到新系统中 ,是集成系统开发中提出的一个重要问题。本文基于CORBA技术探讨如何实现遗留系统集成的方法 ,并通过实例重点阐述如何将已有的系统封装成CORBA对象的步骤。