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.     

太空原位制造和修复技术研究现状分析

概述了太空原位制造和修复技术（In—situ Fabrication and Repair,ISFR）的概念和特点,并结合该技术的发展背景,介绍了国内外以选择性激光烧结和电子束熔融技术为代表的太空原位制造、空间钎焊修复、太空基地建筑构建等方向发展现状及趋势。结合我国空间技术事业发展,提出充分借鉴国外相关技术成果,围绕主要应用材料,重点开展空间环境适应性和应用验证研究,并探索利用模拟月壤开展太空原位制造技术研究的设想与建议。     

飞机下滑波束导引系统设计及仿真

下滑波束导引系统是飞机在自动着陆时所采用的一种重要无线电波束导引系统。首先,简要阐述了下滑波束导引系统的基本工作原理;然后,对导引系统的运动学环节及下滑耦合器进行分析,对飞机下滑波束导引系统结构进行设计;最后,在MATLAB平台下,对所设计的下滑波束导引系统进行大量仿真研究。仿真结果显示。所设计的下滑波束导引系统结构是合理的,其控制系统是稳定的,且其稳态性能也得到改善。     

基于PSO算法的半球谐振陀螺惯导系统陀螺温度补偿方法

针对半球谐振陀螺受温度影响出现零位漂移的问题，以测温电路温度为基准，建立温度频率函数实时解算温度，提出一种基于粒子群优化(PSO)算法的半球谐振陀螺惯导系统陀螺温度补偿方法。在求解温度时，需要先将温度频率函数转换为一元三次方程，存在测试计算量大的问题。引入逆向拟合思想，建立频率温度函数，提高陀螺输出温度实时性和降低测试计算量，替代了传统陀螺测温硬件电路，为惯导系统轻小型设计提供新思路。考虑温度变化、温度变化率以及两者的交叉项，建立温度补偿模型，引入PSO算法求解模型系数。温度试验结果表明，在温箱温度为-40~50 ℃内，补偿后的半球谐振陀螺的零偏稳定性较补偿前提升了46％。     

确定无约束梁耦合振型的一种途径

无约束梁耦合振动问题属于单柔体动力学问题,确定无约束梁耦合振型对于分析梁的振动性质具有重要意义。首先给出单柔体动力学的拟变分原理,然后分析无约束梁耦合振动的特点,应用单柔体动力学的拟变分原理建立了确定无约束梁耦合振型的一种途径。应用这种途径求解无约束梁耦合振动的奇数次振型和偶数次振型。最后,讨论了有关问题。     

某型飞机平尾管梁轴承轴向间隙问题的分析

分析某型飞机平尾管梁安装轴承轴向间隙产生的原因及轴承间隙加大对飞机使用的影响，并提出了排故和设计改进措施。     

Antenna pattern control of planar arrays for long distance communications

As an alternative to standard antennas and due to the advent of low-cost digital processors and materials, adaptive antenna arrays are increasingly considered for applications in long distance communications. The pattern beam control potentialities provide the performance improvement of the communication systems. In this context, this work presents a technique that permits to synthesize the antenna pattern of a planar array. Considering that the relationship between the array factor and the array excitations for the far field region is a Fourier transform in the appropriate variables, the non-uniform sampling procedure is extended for planar arrays. These arrays permit a further control of the antenna pattern since two dimensions of space are used. The technique considers a number of array factor points equal to the array size, which is used to impose appropriated values in the antenna pattern. The produced array factor passes through those points with the desired values, which allows the synthesis of antenna patterns with appropriated characteristics. The theory is presented in order to develop the necessary direct expressions to calculate the array excitation. The array factor can be obtained using the inverse Fourier transform. As application examples, with this technique it is possible to define the level of each sidelobe of the antenna pattern, to control the main beam and to impose nulls in prescribed directions of the pattern.     

Theory of fragmented energy release in the Sun

The magnetic energy released inside an active region is closely related to its formation and evolution. Following the evolution of a collection of flux tubes inside the convection zone and above the photosphere we can show that many nonlinear structures (current sheets, shock waves, double layers etc.) are formed. We propose in this review that coronal heating, flares and particle acceleration are due to the interaction of the plasma with these nonlinear structures. Approaching active regions as a driven complex dynamical system we can show that several coherent ensembles of the nonlinear structures will appear spontaneously. The statistical analysis of these structures is a major problem in solar physics. We can also show that many observed large scale structures are the result of the convolution of non-observable fragmentation in the energy release process.     

Distribution and variability of accelerated electrons at Mars

We investigate accelerated electrons observed by Mars Global Surveyor (MGS), using data from the Electron Reflectometer (ER) instrument. We find three different types of accelerated electron events. Current sheet events occur over regions with weak or no crustal fields, have the highest electron energy fluxes, and are likely located on draped magnetotail fields. Extended events occur over regions with moderate crustal magnetic fields, and are most often observed on closed magnetic field lines. Localized events have the lowest energy fluxes, occur in strong magnetic cusp regions, and are the most likely kind of event to be found on open magnetic field lines. Some localized events have clear signatures of field-aligned currents; these events have much higher electron fluxes, and are preferentially observed on radially oriented open magnetic field lines. Electron acceleration events, especially localized events, are similar in many ways to events observed in the terrestrial auroral zone. However, physical processes related to those found in the terrestrial cusp and/or plasmasheet could also be responsible for accelerating electrons at Mars.     

商用航空发动机转子部件的电子束焊接

现代商用航空发动机具有长寿命、高可靠性等要求,这对电子束焊接头的设计、制造及检测均提出了更高的要求。介绍了航空发动机转子部件电子束焊接结构及接头设计形式、检测要求,指出了针对商用航空发动机转子电子束焊需开展的研究工作。