涡流阀变推力发动机涡流室涡流结构分析

为了研究涡流阀变推力发动机涡流室流动,利用建立的径向压强测试实验装置和三维数值计算模型,进行了涡流室压强分布和涡流结构的研究,获得了涡流室径向压强分布及涡流室旋涡结构.研究结果表明,涡流室内压强分布呈现出中心较小区域变化剧烈,而其余大部分区域变化不明显的现象;流场中心区域存在涡核结构,减小了喷管有效喉部面积,即实现推力...     

Cosmic Rays at High Heliolatitudes

The Ulysses spacecraft has been the first to orbit the Sun over its poles and to explore the heliosphere at these high heliolatitudes. It has now completed two fast latitude scans, one at solar minimum and one at solar maximum. Since its launch in October 1990, this mission has led to several surprising discoveries concerning energetic particles, cosmic rays, Jovian electrons, the solar wind, the heliospheric magnetic field and the global features of the heliosphere. This review addresses mainly the propagation and modulation of cosmic rays and other charged particles, from both an observational and theoretical point of view, with emphasis on what has been learned from exploring the inner heliosphere to high heliolatitudes. This is done for solar minimum and maximum conditions. The review is concluded with a summary of the main scientific discoveries and insights gained so far from the Ulysses mission.     

等腰梯形脉宽调制波控制的变频器研究

介绍了一种斜边占π/5的等腰梯形脉宽调制波,从理论上证明了采用这种PWM(PulseWidth Modulation)波控制的变频器,能消除输出电压的5次谐波分量,使输出电压谐波分量小,电流波形好,系统运行时转矩脉动小,可靠、平稳、噪声低.已将这种控制技术应用于某种列车风扇异步电机的变频调速,实验结果与理论分析相吻合.     

ACARS原理分析

本文着重分析了 ACARS 工作原理,论证了调制体制的优越性,对微机控制下链信息发射的软件流程进行了模拟设计。     

DVOR副载波上60Hz调幅现象及一种消弱方式的分析

以理论与实践相结合为出发点，着重分析了ＤＶＯＲ信号副载波上存在着的６０Ｈｚ调幅现象，指出边带天线间的“寄生辐射效应”是危及ＤＶＯＲ信号质量的主嵰蛩兀⒁源宋行钠饰隽耍粒祝粒担保男停模郑希以谏杓萍鞍沧暗魇怨讨形跽庵窒窒蠖扇〉氖侄渭霸怼     

载体角运动对旋转捷联惯导误差的影响分析

旋转捷联惯导系统采用旋转调制误差补偿技术对陀螺仪和加速度计误差进行调制,可以提高系统导航精度。在简要分析旋转调制误差补偿机理基础上,研究了单轴旋转方案中载体常值旋转和周期旋转2种角运动模式对导航误差的影响。结果表明：载体特定角运动对旋转捷联惯导的误差补偿效果有一定影响,且单轴正反转停方案中误差补偿效果所受影响相对较小。     

Cosmic ray modulation with a Fisk-type heliospheric magnetic field and a latitude-dependent solar wind speed

The effect of a latitude-dependent solar wind speed on a Fisk heliospheric magnetic field [Fisk, L. A. Motion of the footpoints of heliospheric magnetic field lines at the Sun: implications for recurrent energetic particle events at high heliographic latitudes. J. Geophys. Res. 101, 15547–15553, 1996] was first discussed by Schwadron and Schwadron and McComas [Schwadron, N.A. An explanation for strongly underwound magnetic field in co-rotating rarefaction regions and its relationship to footpoint motion on the the sun. Geophys. Res. Lett. 29, 1–8, 2002. and Schwadron, N.A., McComas, D.J. Heliospheric “FALTS”: favored acceleration locations at the termination shock. Geophys. Res. Lett. 30, 41–1, 2003]. Burger and Sello [Burger, R.A., Sello, P.C. The effect on cosmic ray modulation of a Parker field modified by a latitudinal-dependent solar wind speed. Adv. Space Res. 35, 643–646, 2005] found a significant effect for a simplified 2D version of a latitude-dependent Fisk-type field while Miyake and Yanagita [Miyake, S., Yanagita, S. The effect of a modified Parker field on the modulation of the galactic cosmic rays. In: Proceedings of 30th International Cosmic Ray Conference. Merida, Mexico, vol. 1, 445–448, 2007] found a smaller effect. The current report improves on a previous attempt Hitge and Burger [Hitge, M., Burger, R.A. The effect of a latitude-dependent solar wind speed on cosmic-ray modulation in a Fisk-type heliospheric magnetic field. In: Proceedings of 30th International Cosmic Ray Conference. Merida, Mexico, vol. 1, pp. 449–450, 2007] where the global change in the solar wind speed and not the local speed gradient was emphasized. The sheared Fisk field of Schwadron and McComas [Schwadron, N.A., McComas, D.J. Heliospheric “FALTS”: Favored acceleration locations at the termination shock. Geophys. Res. Lett. 30, 41–1, 2003.) is similar to the current Schwadron–Parker hybrid field. Little difference is found between the effects of a Parker field and a Schwadron–Parker hybrid field on cosmic-ray modulation, in contrast to the results of Burger and Sello and Miyake and Yanagita [Burger, R.A., Sello, P.C. The effect on cosmic ray modulation of a Parker field modified by a latitudinal-dependent solar wind speed. Adv. Space Res. 35, 643–646, 2005 and Miyake, S., Yanagita, S. The effect of a modified Parker field on the modulation of the galactic cosmic rays. In: Proceedings of 30th International Cosmic Ray Conference. Merida, Mexico, vol. 1, pp. 445–448, 2007]. The two-dimensional approximation used by these authors is therefore inadequate to model the complexities of the actual three-dimensional field. We also show that a Fisk-type field with a latitude-dependent solar wind speed (Schwadron–Parker hybrid field) decreases both the relative amplitude of recurrent cosmic ray intensity variations and latitude gradients and yields similar constants of proportionality for these quantities as for the constant solar wind speed case.     

多路导航信号恒包络处理技术

现代化的导航系统需要在一个频段发射多路导航信号以提高频谱利用率。直接组合的复合信号不是恒包络,在通过饱和状态功率放大器时会产生AM/PM失真,从而影响整个导航系统的定位精度。为了解决这个问题,需要增加互调分量,把信号处理成恒包络复合信号。文章在分析GPS和GALILEO系统导航信号恒包络处理方法的基础上,给出了我国导航卫星系统恒包络处理方法的建议。     

基于多组合窗函数的NLFM信号匹配滤波器设计

文章研究了在相位逗留原理的基础上采用由多种窗函数线性组合得到的组合窗设计NLFM信号的波形与脉冲压缩滤波器,重点分析了组合窗函数的组合参数及窗函数数量对NLFM信号脉冲压缩结果的影响。仿真结果表明,在一定条件下对基于三种窗函数线性组合的组合窗设计的NLFM信号进行谱修正滤波后,主副瓣比（RMS）可提高4．6～8．9dB,而主瓣展宽和主瓣损失变化较小。     

导弹无线电引信电磁脉冲效应仿真

以LFM导弹无线电引信为研究对象,以Ansoft软件为仿真平台,建立无线电引信天线模型和电路模型,通过计算机仿真对高功率微波(HPM)干扰导弹无线电引信的效应进行了研究。仿真结果表明,在高功率电磁脉冲作用下,混频器和滤波器上分布的电压很高,而进入执行级的电压很低,达不到启动电压的幅度。