机翼对自转旋翼机纵向稳定性的影响

为了研究机翼对自转旋翼机纵向稳定性的影响,针对某复合式自转旋翼机,建立了基于状态空间法描述的非线性全量方程数学模型。该模型包含自转旋翼、机身、螺旋桨、机翼和尾翼的气动模型、动态入流模型和稳定性分析模型。运用该模型对比研究了样例自转旋翼机和样例复合式自转旋翼机的纵向稳定性。研究结果表明：机翼的增加对于浮沉模态和短周期模态稳定性是有利的;对于旋翼转速模态稳定性是不利的,在设计复合式自转旋翼机时可以考虑增加旋翼桨尖配重来提高此模态的稳定性。机翼的纵向位置对自转旋翼机的纵向稳定性有显著影响。在机翼纵向位置能满足配平约束条件下,机翼纵向位置越靠后,迎角稳定性越好,但旋翼转速稳定性越差。在设计复合式自转旋翼机时,机翼纵向位置的选择要综合考虑这两个因素进行折中。     

基于零空间的改进直接分配法

直接分配法是解决操纵面冗余飞行器控制分配的一种有效方法,但直接分配法只能对指定方向上误差最小目标进行优化,这种缺点限制了直接分配法的应用。零空间可以在保持转矩不变的前提下对控制量进行调节,利用这种特性,在三维转矩直接分配的基础上,通过对零空间坐标K进行数学规划可以使其他性能指标达到最优。推导证明,控制量最小问题和阻力最小问题分别可以转化为对坐标K的线性规划与二次规划问题。仿真结果表明,给出的基于零空间的改进直接分配法可以实现控制量最小和阻力最小控制分配。     

柔性接头有效摆心漂移特性

设计了带缠裹式防热套的柔性接头,弹性件和防热套材料均采用硅橡胶.研究了柔性接头有效摆心和几何球心的关系,采用2阶四项式Mooney-Rivlin模型模拟弹性件的本构关系,利用ANSYS软件分别仿真计算柔性接头在压强为0,9MPa下不同摆角条件的有效摆心和几何球心漂移,得到了两者的漂移包络线,把仿真的有效摆心漂移结果与试验测量值进行比较,并利用间隙碰撞试验验证了几何球心漂移仿真结果的准确性,在此基础上研究了有效摆心漂移的原因.结果表明:摆心包络线的仿真结果与试验结果吻合较好,有效摆心和几何球心是两个不同的概念,柔性接头的有效摆心漂移在半径为2.5mm,高为1.4mm的圆柱包络面内,而几何球心的漂移在半径为0.013mm,高为0.6mm的圆柱包络面内,有效摆心漂移是由接头各层增强件和弹性件的变形不同引起的.      

波束波导馈电系统在深空探测天线应用中的关键技术研究

针对波束波导馈电系统在深空探测天线应用中存在的电小尺寸镜面绕射引起波束波导传输效率降低,不同极化工作时波束指向不一致,以及TE21模跟踪时坐标转换等问题,进行深入研究并给出相应的解决方案或数学模型.通过优化椭球镜M5的曲率,解决了电小尺寸镜面绕射使波束波导传输效率下降问题,使S频段的传输效率提高约4％,35 m天线副反射面的截获效率增加约11％,天线增益提高0.7 dB;给出天线束峰值位置随方位、俯仰角变化的数学模型,提出了中值补偿方法,使天线左右旋极化峰值不一致增益损失减小约0.16 dB,并给出TE21模跟踪时的坐标转换数学模型.这些方法和数学模型已成功应用于实际工程中,并取得了良好的效果.     

基于我国深空站三向测量模式的数据精度分析

为了验证我国深空站三向测量模式的正确性,以同步星跟踪试验中的测量数据为基础,建立了站间同步修正算法和三向测量观测模型,通过与同步卫星的精密星历反算测量值比较,得到了测量数据的标定参数,结果表明,我国深空站测控能够实现dm级的测量精度,明显优于“嫦娥二号”测量的水平;同时利用测量数据进行定轨策略分析,最终实现了10 m量级的同步卫星定轨精度.分析结果为“嫦娥三号”探测器实施有效测控提供了依据.     

面向持续战域感知的近空间飞行器技术

未来战争呈全空域立体化发展趋势,近空间的深入探索和有效利用日益受到重视.本文从热力学特性和电离特性角度,概述了近空间大气环境.重点以持续的战域感知为军事应用背景,介绍了现有的C4ISR能力,进而归纳评述了相关近空间飞行器的技术发展、工程设计、概念应用.分析指出,近空间无人HALE飞机具有填补持续的C4ISR能力中所有空缺的潜力.     

The effect of realistic surface properties on low temperature space observatories

We highlight the effect on space-telescope temperatures of thedirectionality of the radiative properties of materials, by showing results from a Monte-Carlo simulation of telescope cooling. The need for further measurements of directional properties is stressed.     

Space weather: its effects and predictability

Terrestrial technology is now, and increasingly, sensitive to space weather. Most space weather is caused by solar storms and the resulting changes to the Earth's radiation environment and the magnetosphere. The Sun as the driver of space weather is under intense observation but remains to be adequately modelled. Recent spacecraft measurements are greatly improving models of solar activity, the interaction of the solar wind with the magnetosphere, and models of the radiation belts. In-situ data updates the basic magnetospheric model to provide specific details of high-energy electron flux at satellite orbits. Shock wave effects at the magnetopause can also be coarsely predicted. However, the specific geomagnetic effects at ground level depend on the calculation of magnetic and electric fields and further improvements are needed. New work on physical models is showing promise of raising geomagnetic and ionospheric predictability above the synoptic climatological level. This revised version was published online in August 2006 with corrections to the Cover Date.     

Real-Time Specifications of the Geospace Environment

We report the recent progress in our joint program of real-time mapping of ionospheric electric fields and currents and field-aligned currents through the Geospace Environment Data Analysis System (GEDAS) at the Solar-Terrestrial Environment Laboratory and similar computer systems in the world. Data from individual ground magnetometers as well as from the solar wind are collected by these systems and are used as input for the KRM and AMIE magnetogram-inversion algorithms, which calculate the two-dimensional distribution of the ionospheric parameters. One of the goals of this program is to specify the solar-terrestrial environment in terms of ionospheric processes, providing the scientific community with more than what geomagnetic activity indices and statistical models provide. This revised version was published online in August 2006 with corrections to the Cover Date.     

显示彩色矢量汉字的方法

给出了一种根据TTF字形轮廓数据描绘汉字轮廓的方法,解决了彩色矢量汉字显示的问题。