The waves observed in the ARAKS-East experiment

Experimental results of the Wave measurements over frequency range 0.1–5.0 MHz during the second launch of the ARAKS Experiment (15.02.75) are reported. The differences between the results of the first and the second launches are discussed.     

俄罗斯卫星制造产业概览(下)

二、拉沃奇金科研生产联合体拉沃奇金科研生产联合体(NPO LA)是俄罗斯另一家大型航天公司。该公司在发展俄航天技术,特别是在行星际空间探索中起着重要的作用,同时还从事科学卫星和地球观测卫星的研制。2.1发展简况拉沃奇金联合体建于1937年4月,当时主要是设计制造军用飞机。S.     

大机动飞行情况下姿态控制系统的设计

本文针对目前战术导弹广泛使用捷联系统这个现状,以及对大机动飞行器采用姿态角误差反馈进行控制有时出现的奇异问题,提出并研究了基于四元数进行大机动战术导弹姿态控制系统的设计问题.首先,给出了大机动飞行情况下基于四元数描述的弹体动力学模型,然后,基于非线性控制系统综合方法设计了姿态控制系统,并验证了系统的稳定性.研究结果表明,基于四元数进行姿态控制系统的设计,既解决了姿态角表示法存在的奇异性问题,又可减少捷联计算机的计算量,对战术导弹具有重要实际意义.最后,通过数值仿真验证了本文提出方法的有效性.     

成像光谱仪编程选择波段数据采集系统的研究

随着成像光谱仪的发展,遥感数据量越来越大,这对电子学系统中的数据采集、传输和处理带来了一定的困难。基于目前技术和数据的实用性两方面考虑,采用编程选择波段的方法能够很好地解决数据量日益增大的问题,国内外的一些方案中已经对此有了一定的设想,即通过遥控指令改变波段数目、光谱取样间隔或波段的重组,这一切都要求有一个灵活性强、通用性好的数据采集系统,能够对不同的选择情况正确地收集用户所需的数据。文中对数据采集的可行性进行了研究,并提出了一个较为容易实现的方案。     

基于流场函数的变刚度层合板铺放设计

文章提出了一种新的变刚度铺层轨迹设计方法,即采用一对互相共轭的标量场函数实现复合材料变刚度铺层的轨迹定义和铺层设计。最后,通过有限元建模和算例对比方法,对直线铺放层合板和变刚度铺放层合板进行压缩特征值屈曲分析和非线性屈曲分析,得出变刚度铺放层合板的屈曲特性比直线铺放层合构件提高约23．62％,y方向的屈曲变形位移减小为直线铺层构件的59．47％,大幅度提高了构件的抗压缩屈曲特性,同时也验证了该设计方法的可行性和实用价值。     

直接数字式合成技术之研究

直接数字式合成(DDS)技术,是近几年来发展迅速的一种频率合成新技术。DDS具有输出相对带宽宽、频率转换时间短、频率分辨力高且输出相位连续、可产生宽带正交信号,易集成等优点。在通信、雷达、遥控遥测、电子对抗、电子扩频以及现代化的仪器仪表工业等许多电子领域显示出广泛的应用前景。本文介绍了直接数字式合成技术的特点及其应用情况,阐述了DDS的基本原理并对其在应用中的一些合成方法做了相互对比。     

多坐标系下目标跟踪的联合滤波

针对雷达目标观测和处理在不同的坐标系下完成,本文提出了联合滤波算法来跟踪机动目标。该算法以卡尔曼滤波器为基础,直角坐标系下和极坐标系下的算法相联合,不仅克服了两种坐标系下滤波算法的不足,而且对机动目标有很好的跟踪效果。仿真实验结果表明了该算法的有效性。     

Application of small-size antennas for estimation of angles of arrival of HF signals scattered by ionospheric irregularities

A modification of the Doppler Interferometry Technique is suggested to enable estimating angles of arrival of comparatively broadband HF signals scattered by random irregularities of the ionospheric plasma with the use of small-size weakly directional antennas. The technique is based on the measurements of cross-spectra phases of the probe radiation recorded at least in three spatially separated points. The developed algorithm has been used to investigate the angular and frequency-time characteristics of HF signals propagating at frequencies above the maximum usable one (MUF) for the direct radio path Moscow-Kharkiv. The received signal spectra show presence of three families of spatial components attributed, respectively, to scattering by plasma irregularities near the middle point of the radio path, ground backscatter signals and scattering of the sounding signals by the intense plasma turbulence associated with auroral activations. It has been shown that the regions responsible for the formation of the third family components are located well inside the auroral oval. The drift velocity and direction of the auroral ionosphere plasma have been determined. The obtained estimates are consistent with the classical conception of the ionospheric plasma convection at high latitudes and do not contradict the results of investigations of the auroral ionosphere dynamics using the SuperDARN network.     

Results of solar observations by the CORONAS-F payload

The CORONAS-F mission experiments and results have been reviewed. The observations with the DIFOS multi-channel photometer in a broad spectral range from 350 to 1500 nm have revealed the dependence of the relative amplitudes of p-modes of the global solar oscillations on the wavelength that agrees perfectly well with the earlier data obtained in a narrower spectral ranges. The SPIRIT EUV observations have enabled the study of various manifestations of solar activity and high-temperature events on the Sun. The data from the X-ray spectrometer RESIK, gamma spectrometer HELICON, flare spectrometer IRIS, amplitude–temporal spectrometer AVS-F, and X-ray spectrometer RPS-1 have been used to analyze the X- and gamma-ray emission from solar flares and for diagnostics of the flaring plasma. The absolute and relative content of various elements (such as potassium, argon, and sulfur) of solar plasma in flares has been determined for the first time with the X-ray spectrometer RESIK. The Solar Cosmic Ray Complex monitored the solar flare effects in the Earth’s environment. The UV emission variations recorded during solar flares in the vicinity of the 120-nm wavelength have been analyzed and the amplitude of relative variations has been determined.