旋翼三维非定常跨音速绕流的数值模拟

 利用小扰动位势方程，用有限差分方法求解了旋翼跨音速流场。导出了严格的三维非定常位势方程远场无反射边界条件，并成功地用于数值计算中，缩小了物理求解域的空间尺度。采用了贴体坐标和网格加密技术，以得到合理的非均匀网格分布。应用较少的网格点数成功地计算了无升力情况下旋翼的三维非定常亚、跨音速绕流流场，得到了与实验结果符合良好的数值解     

Solar mass flow in fine-scale structures

Observations of transient and steady velocities at chromospheric, transition region and coronal temperatures in the quiet Sun and coronal holes are reviewed. The relevance of fine-scale structures in governing the mass balance of the solar atmosphere is stressed. At present, a coherent picture of these mass flows does not exist. However, the current observational base of transition region and coronal velocity information is limited but should greatly improve with measurements from the SOHO satellite.     

事故与熵—事故发生可能性计算的新方法

本文从熵增加的观点描述了事故的本质,剖析了人机系统的实质与特性,提出了风险熵与事故势的概念,给出了计算风险熵与故事势的方法.结果表明,系统具有二重性.在系统运行期间,系统具有封闭体系的特性;在休整期间.系统具有开放体系的特性.事故是运行系统的必然发展趋势,是一种自发过程,是运行系统的固有属性.由于在系统熵增的过程中信息与能量的交换,所以可以把事故定义为系统熵增加的结果.避免事故发生的原理是不断向系统输入信息或负熵以抵消系统内部的熵增加.     

大迎角涡流的同步迭代算法

 基于多重线涡模型(MLVM),本文建立了一种计算机时少、收敛性强的适用于大迎角涡流势流数值模拟的迭代算法。采用本文算法,首次得到了迎角直到60°的旋转体涡流的收敛解。计算出的空气动力数据与实验结果吻合。     

无粘跨声速绕流的有限元法和界积分方程的某些进展

本文对无粘跨声速绕流的有限元法和边界积分方程法的目前进展,特别是对提高跨声速流算法效率起着主要作用的成果,例如普适元素和块结构有限元网格生成技术有限元解法的多重网格技术、SUPG有限元法、GRMES算法和可压流的完全边界积分方程法等方面作了回顾和评介。     

柔性飞艇主气囊湿模态分析及试验研究

大型柔性飞艇是临近空间“长驻空”重要平台,具有重要的国防及民用价值,是近年来浮空器结构工程领域研究的热点之一。主气囊是柔性飞艇核心结构部件,为了研究大型柔性飞艇主气囊周边流场对其模态性能的影响,将柔性飞艇主气囊内、外气体视为不可压缩流体,将空气随囊体振动的影响作为附加质量添加到囊体结构中,采用基于势流理论的附加质量计算...     

解批量问题的模拟退火算法

多品种、有能力约束的批量问题是多品种批量生产中生产计划的关键性问题.这一问题就是要确定:在每一期生产多少产品以使得所用费用最少且满足已知的每一期的需求量.本文设计了一种模拟退火算法的实现形式,通过大量的算例分析表明,该算法具有良好的寻优特性与运算效率.      

类构件潜在可重用性预测技术

首先分析了Judith Barnard类构件潜在可重用性预测模型,针对其不足提出了改进意见.在此基础上,将"类构件"的概念进行扩展,提出了"可重用类群"的概念及相应的判定算法,该技术使得对类构件潜在可重用性的预测更加合理、准确.      

感应式表面电位探针的研制

本文描述了感应式表面电位探针原理及实验方法;给出了探针在大气和真空中输出信号大小与表面电位、距离、以及感应片面积之间的关系。为探针设计提供了必要的数据。     

Plasma electron temperature variability in lunar surface potential and in electric field under average solar wind conditions

The Moon is immersed in plasma environment. The most interesting challenge of the lunar plasma– field environment is that it is alternatively dominated by the extended but variable outer atmosphere of the Earth – the magnetosphere – and by the extended but highly variable solar atmosphere – the solar wind. Understanding the plasma environment and its interaction with the lunar surface will be beneficial to both manned and robotic surface exploration activities and to scientific investigations. Presented is a preliminary map of variations of lunar surface electric potential over the day side and night side using probe equations and a discussion on dust dynamics in this E-field structure using the data from Electron Reflectometer in Lunar Prospector spacecraft during 1998–1999. On the day side, potential is around 5 V and on the night side it reaches up to −82 V. On the night side region, only highly energetic electrons can overcome this large negative potential. The variation at electron temperature (T_e) strongly reflects in the surface potential. The potential reaches to a value of −82 V for T_e = 58 eV. Surface charging causes the electrostatic transport of charged dust grains. Dust grain size of 0.1 μm shows a levitation height of 4.92 m on lunar day side, 748 m on terminator region and 3.7 km on the night side. The radius of maximum sized grain to be lofted, R_max, peaks at the terminator region (R_max = 0.83 μm). At the transition region dust levitation is almost absent. This region is most suited for exploration activities as the region is free from hazards caused by lunar dust.