马赫数4一级下颔式混压进气道试验

对一种Ma=4一级下颔式混压进气道进行了试验,得到了该类进气道的气动特性,结果表明:①在Ma=3.5,攻角和偏航角为零时,随着出口反压的增加,进气道总压恢复系数先升高后降低,临界状态下进气道总压恢复系数最高;②攻角和偏航角为零时临界状态时,随着来流马赫数的增加,进气道的总压恢复系数呈线性下降趋势;③有攻角或偏航角的状态下进气道的总压恢复系数有所下降;④进气道在由反压引起的不起动过程中具有再起动特性,再起动过程中无迟滞廻路现象.      

卫星点波束天线的多目标指向优化研究

卫星天线波束常常需要同时覆盖特定区域内多个目标,为保证目标接收卫星信号的增益要求,需对其指向进行优化。以我国某卫星点波束天线为研究对象,将天线功率辐射模型引入卫星指向计算模型中,完成了指向目标的增益计算。运用最优化原理分析了多目标指向增益优化模型,在无约束条件下,指向增益最优点在标称三目标构成的三角形重心位置;有约束条件下,最优点在满足相应约束下偏离无约束最优点。多目标指向优化理论研究对点波束天线的高精度指向及确保目标的通信特性提供了适用的工程模型,具有极强的工程应用价值。     

基于DEA-Malmquist指数的辽宁高技术产业创新效率评价

高技术产业在辽宁省经济发展中占有举足轻重的地位.如何使辽宁高技术产业又好又快发展,提高辽宁自主创新能力,转变经济增长方式,是亟待解决的问题.基于DEA-Malmquist指数方法,对辽宁高技术产业不同行业的全要素效率、技术效率变化和技术进步情况进行了分析,发现了辽宁高技术产业发展中存在的问题与不足.     

复杂时变激励下失谐叶盘瞬态强迫响应分析

提出一种高效的失谐叶盘瞬态强迫响应分析方法,不同于传统的数值积分方法,该方法推导出瞬态强迫响应的解析表达式,能更为高效地预测失谐叶盘的瞬态强迫响应。首先,对叶盘的高保真有限元模型进行减缩建模,在精确地描述叶盘结构的动力学特性的前提下,极大的减少了模型的自由度数目。其次,模拟加速旋转的涡轮叶盘经过复杂流场时叶片表面上的气动载荷,并建立叶盘固有频率和振型随转速变化的数学函数;通过共振分析确定叶盘共振的转速区间并分析引起共振的激励阶次成分。最后,计算了不同旋转加速度和阻尼下叶盘的瞬态强迫响应,并对叶盘的失谐幅值放大因子进行研究。应用本办法对某86个叶片的涡轮叶盘进行了数值分析,结果表明,相同阻尼水平下,叶盘的瞬态强迫响应幅值随旋转加速度增加而降低,失谐幅值放大因子在瞬态条件下大于稳态条件下,最高可达30%。     

The Magnetic Field of Mercury

The magnetic field strength of Mercury at the planet’s surface is approximately 1% that of Earth’s surface field. This comparatively low field strength presents a number of challenges, both theoretically to understand how it is generated and observationally to distinguish the internal field from that due to the solar wind interaction. Conversely, the small field also means that Mercury offers an important opportunity to advance our understanding both of planetary magnetic field generation and magnetosphere-solar wind interactions. The observations from the Mariner 10 magnetometer in 1974 and 1975, and the MESSENGER Magnetometer and plasma instruments during the probe’s first two flybys of Mercury on 14 January and 6 October 2008, provide the basis for our current knowledge of the internal field. The external field arising from the interaction of the magnetosphere with the solar wind is more prominent near Mercury than for any other magnetized planet in the Solar System, and particular attention is therefore paid to indications in the observations of deficiencies in our understanding of the external field. The second MESSENGER flyby occurred over the opposite hemisphere from the other flybys, and these newest data constrain the tilt of the planetary moment from the planet’s spin axis to be less than 5°. Considered as a dipole field, the moment is in the range 240 to 270 nT-R _M ³ , where R _M is Mercury’s radius. Multipole solutions for the planetary field yield a smaller dipole term, 180 to 220 nT-R _M ³ , and higher-order terms that together yield an equatorial surface field from 250 to 290 nT. From the spatial distribution of the fit residuals, the equatorial data are seen to reflect a weaker northward field and a strongly radial field, neither of which can be explained by a centered-dipole matched to the field measured near the pole by Mariner 10. This disparity is a major factor controlling the higher-order terms in the multipole solutions. The residuals are not largest close to the planet, and when considered in magnetospheric coordinates the residuals indicate the presence of a cross-tail current extending to within 0.5R _M altitude on the nightside. A near-tail current with a density of 0.1 μA/m² could account for the low field intensities recorded near the equator. In addition, the MESSENGER flybys include the first plasma observations from Mercury and demonstrate that solar wind plasma is present at low altitudes, below 500 km. Although we can be confident in the dipole-only moment estimates, the data in hand remain subject to ambiguities for distinguishing internal from external contributions. The anticipated observations from orbit at Mercury, first from MESSENGER beginning in March 2011 and later from the dual-spacecraft BepiColombo mission, will be essential to elucidate the higher-order structure in the magnetic field of Mercury that will reveal the telltale signatures of the physics responsible for its generation.     

飞行器变质心控制及性能分析

在合理简化基础上,推导了滑块运动与飞行器姿态角运动之间的关系,分析了配平攻角产生机理及条件;同时还深入分析了轴向位置、横向偏移量、质量比等滑块结构参数对配平攻角的影响;以及不同配平条件下弹道落点偏差情况。结果表明,气动阻力与系统质心偏移弹体纵轴是产生配平攻角两个必要因素,系统静稳定是产生配平攻角的前提条件;轴向位置决定了系统静稳定裕度,与配平攻角呈反比关系;横向偏移量改变控制力矩的力臂,与配平攻角呈正比关系;质量比对力臂和系统静稳定裕度均有影响,与配平攻角呈线性或非线性正比关系;变质心控制能力主要体现在低空段。     

基于故障行为模型的产品寿命分析方法

针对传统可靠性工程方法无法满足高可靠长寿命需求产品设计与分析要求的现状。本文充分考虑引起产品寿命分散性的内因和外因的不确定性,在产品功能模型或数字样机模型的基础上,结合产品的故障行为模型,建立了一种基于产品故障行为模型的产品寿命分析方法。在该方法中,内因参数与外因参数的分散性分别可以用相应的概率密度函数来表示,都是通过对实际使用情况和生产条件的估计得到的,因此,按照这种方法评估得到的产品寿命特征,能够弥补基于故障物理的可靠性预计方法无法体现产品正常使用条件的不足。      

军工高安全软件数值型运行时错误分析方法

提出一种抽象解释和有界模型验证的数值型运行时错误分析方法.利用抽象解释方法分析程序数值变量范围,获得每个程序点达到不动点的变量初步值范围信息.根据待分析的运行时错误类型,在相关需要检测的程序点处将数值变量取值信息转化为断言或假设形式插入程序中,将带有断言和假设的程序转化为布尔公式,验证其可满足性,进而验证断言的正确性.实验证明,该方法与现有方法相比,在精度和效率两方面都有良好的表现.     

超临界压力下湍流区碳氢燃料传热研究

碳氢燃料的传热特性对于再生冷却超燃发动机的传热设计至关重要.采用电热管开展了正十烷的传热特性实验,燃料压力约4.0MPa.利用一维流动的质量和能量守恒关系,对管道内燃料的传热进行了分析.采用多元线性回归的方法获得了正十烷在湍流区的传热关联式,通过外壁温的计算与测量的对比,验证了实验获得的湍流传热关联式的适用性.     

Digital signal processing and numerical analysis for radar in geophysical applications

Numerical solutions for signal processing are described in this work as a contribution to study of echo detection methods for ionospheric sounder design. The ionospheric sounder is a high frequency radar for geophysical applications. The main detection approach has been done by implementing the spread-spectrum techniques using coding methods to improve the radar’s range resolution by transmitting low power. Digital signal processing has been performed and the numerical methods were checked. An algorithm was proposed and its computational complexity was calculated.