三脉冲冷原子陀螺仪中基于内态演化的拉曼光光强补偿算法

由于在复杂环境中拉曼光功率不稳定会导致原子脉冲的宽度发生改变,从而影响陀螺仪的测量精度.通过对冷原子干涉仪的干涉全过程进行建模,计算得出了陀螺仪在拉曼光改变情形下输出相位的解析表达式,即建立了拉曼光在非近共振条件下强度变化时陀螺仪的输出值与外界载体运动之间的关系.与此同时,基于该解析表达式提出了一种对拉曼光光强的补偿算...     

汽车双横臂独立悬架参数优化与仿真研究

针对国内某轿车双横臂独立悬架系统，运用ADMAS／View模块建立了双横臂式悬架模型，利用ADMAS／Insight模块对建立的双横臂式独立悬架进行了优化分析。优化结果分析表明：通过悬架参数优化设计，使前悬架性能有了较大的提高。     

大展弦比运输机标模高升力构型设计与评估

介绍了中国航空工业空气动力研究院基于分层策略遗传算法的多段翼型优化设计工具和高升力构型计算评估方法,参照国内外大展弦比运输机指标为FL-9增压风洞设计了高升力构型标模,为检验标模气动性能,在法国ONERA F1风洞进行了一系列风洞试验和采用UNSMB平台进行了数值模拟。结果显示计算结果与试验结果有着较好的一致性,设计方案具有较好的增升效果。     

Decision-making of Aircraft Optimum Configuration Utilizing Multidimensional Game Theory

As multi-discipline coupling and components interference often affect the aircraft configuration decision-making and analysis during conceptual design process, this article presents an approach of multidimensional game theory based on aircraft components to deal with this problem. The idea is that the configuration decision-making process is regarded as the game for different disciplines and technologies, and the aircraft components are players. The payoff function with highest total gain means that according to the game protocols and multidimensional theory, the optimal aircraft configuration within the strategy set will be chosen. The decision-making model is applied to conceptual design process of the high altitude long endurance (HALE) unmanned aerial vehicle (UAV) based on the assessment of technological risk. The obtained optimum configuration is quite consistent with the current HALE UAV development trends. Thus, taking into account the coupling and interference factors, the multidimensional gaming model based on aircraft components will be an effective analysis method in the decision-making process of aircraft optimum configuration.     

CLVD 法制备C/C复合材料工艺探索研究

研究了采用化学液气相沉积法制备C／C复合材料的工艺过程，分析了不同预制件、温度、浸泡时间等工艺参数对致密速度、效果的影响，并总结出了一套快速高效的致密方法。     

航空软件配置管理系统设计和关键技术研究

从军工软件配置管理的需求出发,结合国军标的开发库、受控库和产品库的三库配置管理体系,阐述某自主知识产权的＂航空软件配置管理系统＂的总体设计思路,指出该配置管理系统实现的关键技术为软件配置库的存储设计方法和文件的增量存储和差异比较技术。说明系统软件配置库的存储设计思路和方案,采用编辑图和贪心算法实现文件的增量存储和差异比较技术的解决方案。总结系统的特点和优点,说明系统下一步发展及扩充的几个方向。     

运动基航天飞行模拟器信号缩比策略

对于大幅值的输入信号,三阶多项式缩比法易产生信号畸变且参数配置复杂;而Hermite缩比函数法的触发速度较慢.提出两种改进的缩比方法:基于三阶多项式缩比法的最优参数配置法和加入线性缩比的非线性缩比法.前一种方法通过参数的优化配置最大化稳定区,以防止信号的畸变;后一种方法则利用线性缩比的特性将缩比度限制在稳定区内.仿真结果表明:线性缩比的加入可以防止三阶多项式缩比法信号的畸变;最优配置参数法应用方便且整体效果较好.为航天飞行模拟提供了更有效的缩比策略.     

A Structured Mesh Euler and Interactive Boundary Layer Method for Wing/Body Configurations

To compute transonic flows over a complex 3D aircraft configuration, a viscous/inviscid interaction method is developed by coupling an integral boundary-layer solver with an Eluer solver in a ＂semi-inverse＂ manner. For the turbulent boundary-layer, an integral method using Green＇s lag equation is coupled with the outer inviscid flow. A blowing velocity approach is used to simulate the displacement effects of the boundary layer. To predict the aerodynamic drag, it is developed a numerical technique called far-field method that is based on the momentum theorem, in which the total drag is divided into three component drags, i.e. viscous, induced and wave-formed. Consequently, it can provide more physical insight into the drag sources than the often-used surface integral technique. The drag decomposition can be achieved with help of the second law of thermodynamics, which implies that entropy increases and total pressure decreases only across shock wave along a streamline of an inviscid non-isentropic flow. This method has been applied to the DLR-F4 wing/body configuration showing results in good agreement with the wind tunnel data.     

增升状态下的全机位流数值模拟

研究了势流理论下的全机增升装置复杂外形气动力数值计算方法,该方法以低阶面元法为基础,具有计算量小、速度快的优点.复杂流动的粘性效应主要通过附面层粘性修正技术加以体现.采用该方法对某增升装置翼身组合体外形压力分布特性进行计算,并和风洞实验数据相比较,验证了方法的正确性和实用性.在此基础上对某型飞机真实复杂外形的压力分布特性进行了计算,为复杂外形飞行器增升装置的初步设计、方案选型与评估提供了非常理想的工程技术手段.     

Solar cycle and latitude dependence of high-beta suprathermal plasma conditions in interplanetary space between 1.3 and 5.4 AU

The analysis of energetic particles and magnetic field measurements from the Ulysses spacecraft has shown that in a series of events, the energy density contained in the suprathermal tail particle distribution is comparable to or larger than that of the magnetic field, creating conditions of high-beta plasma. In this work we analyze periods of high-beta suprathermal plasma occurrences (β_ep > 1) in interplanetary space, using the ratio (β_ep) of the energetic particle (20 keV to ∼5 MeV) and magnetic field energy densities from measurements covering the entire Ulysses mission lifetime (1990–2009) in order to reveal new or to reconfirm some recently defined interesting characteristics. The main key-results of the work are summarized as follows: (i) we verify that high-beta events are detected within well identified regions corresponding mainly to the vicinity of shock surfaces and magnetic structures, and associated with energetic particle intensity enhancements due to (a) reacceleration at shock-fronts and (b) unusually large magnetic field depressions. (ii) We define three considerable features for the high-beta events, concentrated on the next points: (a) there is an appreciable solar-activity influence on the high-beta events, during the maximum and middle solar-cycle phase, (b) the annual peak magnitude and the number of occurrences of high events are well correlated with the sunspot number, (c) the high-beta suprathermal plasma events present a spatial distribution in heliographic latitudes (HL) up to ∼±80°, and a specific important concentration on the low (−25° ? HL < −6°, 6° < HL ? 25°) and median (−45° ? HL < −25°, 25° < HL ? 45°) latitudes. We also reconfirm by a statistical analysis the results of Marhavilas and Sarris (2011), that the high-beta suprathermal plasma (β_ep > 1) events are characterized by a very large parameter β_ep (up to 1732.5), a great total duration (406 days) and a large percentage of the Ulysses-mission lifetime (which is equal to 6.34% of the total duration with usable measurements, and 11.3% of the duration in presence of suprathermal particles events).