翼身组合体的变可信度优化设计

基于信赖域思想,发展了一种变可信度优化设计方法组织和管理不同可信度模型,有效利用低可信度模型建立近似模型,进行优化设计,高可信度模型仅修正优化近似模型,使最终优化结果收敛到高可信度模型上.采用全位势边界层有粘无粘迭代方法作为低可信度模型,多重网格Navier-Stokes方程方法作为高可信度模型,对翼身组合体进行优化设计,优化结果表明:发展的变可信度优化方法优化效率高,且能保证优化精度,具有实际的工程应用价值.     

叶片全三维反问题优化设计方法

基于数值求解Navier-Stokes方程,对叶轮机械叶片全三维反问题优化设计方法进行研究.反问题给定叶片表面的静压分布反求叶型,假设叶表网格点有虚拟移动速度,迭代过程中根据叶表的实际静压和目标静压之差来修改叶型.对单排叶栅进行了反问题设计,并给出了初步的优化算例,结果能很好地满足目标静压分布,验证了该方法的有效性,计算的时间和精度也适合进行工程应用.      

自动组卷系统试题数据库的设计与实现

目的为了在自动组卷系统中合理地保存试题和试卷;方法利用数据库函数简化字段生成操作,在组卷后较好的保存试卷信息;结果提出一种试题数据库设计方案,能够合理保存试题;结论在实际使用中取得较好的效果。     

涡轮多学科优化中的气动设计技术探讨

通过对涡轮多学科优化的分析,讨论了多学科优化中的气动设计技术.提出了基于叶栅特征参数和贝塞尔函数的二维叶栅参数化造型方法,并结合积叠轴的掠、弯形成三维复杂几何叶片成型技术.通过对气动优化过程中的数学模型分析,给出了一般要求的约束条件,并根据不同阶段的气动设计和约束条件提出了分阶段嵌套优化方法.针对三维气动计算,对商用软件CFX进行了二次开发,实现了三维计算的自动分网、建模、求解和后处理.最后,结合具体算例完成的优化设计结果表明,其涡轮效率提高了约2.3%,工作叶片数减少13.21%,叶片叶身总质量下降8.96%.      

太阳帆航天器移位轨道设计

研究了太阳帆日心移位轨道的稳定性、控制律设计及轨道拼接。将柱坐标形式的太阳帆动力学方程在参考移位轨道附近线性化,得到线性变分方程。分析线性变分方程的特征值在复数平面上的位置就可以得到移位轨道的稳定性条件。设计了太阳帆日心移位轨道的控制律,并证明了控制律满足稳定性条件。该控制律仅要求太阳帆在移位轨道飞行时姿态角α保持不变。此外,太阳帆移位轨道可以与开普勒轨道相互转化,也可以与移位轨道之间相互拼接。     

苏联／俄罗斯数据中继卫星系统评述

在全面收集相关资料的基础上,对苏联／俄罗斯中继卫星系统发展历史和现状给出了较为准确和明晰的描述,并从专业的角度对卫星星座、轨道位置、有效载荷及平台特性、服务范围和在轨运营等重要内容作出了技术评论。其结果对评价我国在这一领域中的成就和研发下一代卫星均具有参考价值。     

Magnetospheric disturbances associated with the 13 December 2006 solar flare and their ionospheric effects over North-East Asia

We present an observational study of magnetospheric and ionospheric disturbances during the December 2006 intense magnetic storm associated with the 4В/Х3.4 class solar flare. To perform the study we utilize the ground data from North–East Asian ionospheric and magnetic observatories (60–72°N, 88–152°E) and in situ measurements from LANL, GOES, Geotail and ACE satellites. The comparative analysis of ionospheric, magnetospheric and heliospheric disturbances shows that the interaction of the magnetosphere with heavily compressed solar wind and interplanetary magnetic field caused the initial phase of the magnetic storm. It was accompanied by the intense sporadic E and F2 layers and the total black-out in the nocturnal subauroral ionosphere. During the storm main phase, LANL-97A, LANL 1994_084, LANL 1989-046 and GOES_11 satellites registered a compression of the dayside magnetosphere up to their orbits. In the morning–noon sector the compression was accompanied by an absence of reflections from ionosphere over subauroral ionospheric station Zhigansk (66.8°N, 123.3°E), and a drastic decrease in the F2 layer critical frequency (foF2) up to 54% of the quite one over subauroral Yakutsk station (62°N, 129.7°E). At the end of the main phase, these stations registered a sharp foF2 increase in the afternoon sector. At Yakutsk the peak foF2 was 1.9 time higher than the undisturbed one. The mentioned ionospheric disturbances occurred simultaneously with changes in the temperature, density and temperature anisotropy of particles at geosynchronous orbit, registered by the LANL-97A satellite nearby the meridian of ionospheric and magnetic measurements. The whole complex of disturbances may be caused by radial displacement of the main magnetospheric domains (magnetopause, cusp/cleft, plasma sheet) with respect to the observation points, caused by changes in the solar wind dynamic pressure, the field of magnetospheric convection, and rotation of the Earth.     

GNSS-R concept extended by a fine orbit tuning

Small changes in semimajor axis of the orbits selected for the GNSS-R [R as Reflectometry] satellites, so-called fine orbit tuning, known from the ESA’s Gravity and steady-state Ocean Circulation Explorer mission, can dramatically increase the number of nadir and off-nadir reflecting points and, in turn, can enhance the capability of the concept of bistatic altimetry (GNSS Reflectometry) without additional costs. The application of our suggestion is feasible for a satellite which will be equipped by thrusters for the orbit keeping. During the mission lifetime several orbit tunings are feasible, just to transfer from one to another orbit. Then we can study short-periodic or longer-periodic features, according to scientific goals defined for the mission. The shortest cycles (few days), corresponding to the required revisit time (defined by ESA), may be subcycles of much longer cycles (repeat periods).     

Removing orbital debris with lasers

Orbital debris in low Earth orbit (LEO) are now sufficiently dense that the use of LEO space is threatened by runaway collision cascading. A problem predicted more than thirty years ago, the threat from debris larger than about 1 cm demands serious attention. A promising proposed solution uses a high power pulsed laser system on the Earth to make plasma jets on the objects, slowing them slightly, and causing them to re-enter and burn up in the atmosphere. In this paper, we reassess this approach in light of recent advances in low-cost, light-weight modular design for large mirrors, calculations of laser-induced orbit changes and in design of repetitive, multi-kilojoules lasers, that build on inertial fusion research. These advances now suggest that laser orbital debris removal (LODR) is the most cost-effective way to mitigate the debris problem. No other solutions have been proposed that address the whole problem of large and small debris. A LODR system will have multiple uses beyond debris removal. International cooperation will be essential for building and operating such a system.     

聚酰亚胺/无机氧化物复合薄膜的制备与耐原子氧性能

分别以锆酸四丁酯、钛酸四丁酯和正硅酸乙酯为氧化物前驱体,利用溶胶凝胶法制备了一系列聚酰亚胺/无机氧化物复合薄膜,在原子氧地面模拟设备中进行了原子氧暴露实验,原子氧累计通量约为3.1×10²⁰ atom/cm².分别考察了无机氧化物种类和含量对复合薄膜力学性能和耐原子氧性能的影响.结果表明,无机氧化物在聚酰亚胺基体中的分散形态对其力学性能影响很大;原子氧暴露后,聚酰亚胺薄膜表面分别形成了富锆、富钛和富硅的保护层,质量损失率减小,耐原子氧性能明显提高.