梯形Halbach永磁阵列空心直线同步电动机特性的解析计算与优化

提出了一种新型的双边不对称梯形永磁空心直线电动机。首先使用等效磁荷法建立了梯形单块磁体的三维空间磁场解析模型,再由叠加原理得到双边Halbach阵列空心电机的气隙磁密三维模型。在考虑线圈横向端部效应的基础上,推导出电机运行过程中的反电动势与电磁推力的表达式。利用解析模型分析了梯形磁体阵列气隙磁密谐波分布的规律,并对其进行优化;三维有限元仿真结果表明所提解析模型具有较高的准确度,同时采用经过优化的梯形阵列定子,可以达到提高气隙磁密正弦性从而减小推力波动的目的。     

基于旋转轴向阵列的风扇宽频噪声实验

航空发动机降噪研究迫切需要一种叶轮机械管道内宽频噪声测量方法来指导降噪设计。本文通过对阵列测量的声压信号进行互相关分析,得到管道内顺流和逆流传播的模态声功率结果。安装在风扇实验台进口段的传声器阵列由2排周向间隔180°的轴向阵列组成,每排阵列有14个等间距的传声器。阵列安装在可周向旋转的测量段上,实验中测量段每隔6°旋转一次,共获得840个测点位置的声场信号。结果表明入射波与反射波最大可相差10dB。模态分解结果表明,转静干涉模态是转子通过频率及其谐频处的主导模态。利用不同参考信号计算出的声场结果相同,说明该实验测试方法对参考信号位置没有特殊要求,进一步说明该方法有很好的适用性。     

直升机旋翼电磁特性模拟新技术

针对直升机电磁散射特性无源模拟的技术瓶颈,基于直升机桨叶的结构特点和雷达回波特性,提出一种基于小散射源阵列的新型旋翼散射特性增强技术,通过阵列合成公式和数值仿真分析了散射源阵列的雷达散射截面（RCS）的峰值大小、波峰数目、波峰位置、主瓣宽度等特性。同时,将该技术应用于国内某型无人直升机旋翼,设计了原理样机,并在微波暗室里对其电磁特性进行测试。测试结果与理论仿真结果吻合较好,验证了本方案的有效性和可行性,为试验模拟技术提供有力支持。     

大型卫星太阳能帆板的分布式振动控制

针对大型卫星太阳能帆板（LSSP）振动主动控制器设计复杂、在轨扩展不易且容错性能有限等问题,提出一种适用于模块化结构的分布式振动控制方法。首先,根据LSSP的结构特点划分控制子模块,建立面向分布式控制的子模块动力学模型,并结合卡尔曼滤波算法设计各子模块线性二次最优振动控制器;然后,考虑各子模块之间的测量信息交互,提出应用于LSSP整体结构的分布式振动控制系统并分析闭环系统稳定性。最后,给出数值仿真算例以验证所提控制方法的有效性。结果表明,采用可扩展的分布式控制器,LSSP的振动能够得到有效抑制,且控制系统的容错性能良好。     

基于互相关和混沌振子阵列的转子早期碰擦故障检测

为了提高早期故障检测的准确性和有效性,提出了运用互相关去噪和构建混沌振子阵列,通过阵列扫描实现早期微弱故障的多个特征频率信号检测的方法.该方法将经过互相关去噪后的信号送入到混沌振子检测阵列中,让其作为混沌检测系统周期策动力的一部分,通过混沌检测系统相轨迹变化检测出表征同一微弱故障的多个频率信号.飞机转子系统早期碰擦故障检测为例验证了该方法的可行性.      

The Composition of the Solar Wind in Polar Coronal Holes

The solar wind charge state and elemental compositions have been measured with the Solar Wind Ion Composition Spectrometers (SWICS) on Ulysses and ACE for a combined period of about 25 years. This most extensive data set includes all varieties of solar wind flows and extends over more than one solar cycle. With SWICS the abundances of all charge states of He, C, N, O, Ne, Mg, Si, S, Ar and Fe can be reliably determined (when averaged over sufficiently long time periods) under any solar wind flow conditions. Here we report on results of our detailed analysis of the elemental composition and ionization states of the most unbiased solar wind from the polar coronal holes during solar minimum in 1994–1996, which includes new values for the abundance S, Ca and Ar and a more accurate determination of the ²⁰Ne abundance. We find that in the solar minimum polar coronal hole solar wind the average freezing-in temperature is ∼1.1×10⁶ K, increasing slightly with the mass of the ion. Using an extrapolation method we derive photospheric abundances from solar wind composition measurements. We suggest that our solar-wind-derived values should be used for the photospheric ratios of Ne/Fe=1.26±0.28 and Ar/Fe=0.030±0.007.     

Johannes Geiss’ Investigations of Solar, Heliospheric and Interstellar Matter

Johannes Geiss is a world leader and foremost expert on measurements and interpretation of the composition of matter that reveals the history, present state, and future of astronomical objects. With his Swiss team he was first to measure the composition of the noble gases in the solar wind when in the late 1960s he flew the brilliant solar wind collecting foil experiments on the five Apollo missions to the moon. Always at the forefront of the art of composition measurements, he with his colleagues determined the isotopic and elemental composition of the solar wind using instruments characterized by innovative design that have provided the most comprehensive record of the solar wind composition under all solar wind conditions at all helio-latitudes. He discovered heavy interstellar pickup ions, from which the composition of the neutral gas of the Local Interstellar Cloud is determined, and the “Inner Source” of pickup ions. Johannes Geiss played a key role both in the in-situ measurements and modeling of molecular ions in comets, and the interpretation of these data. He and co-workers measured the composition of plasmas in the magnetospheres of Earth and Jupiter. Here we highlight Johannes Geiss’ many discoveries and seminal contributions to our knowledge of the composition of matter of the Sun, solar wind, interstellar gas, early universe, comets and magnetospheres.     

Long-Term Fluences of Solar Energetic Particles from H to Fe

Data from ACE and GOES have been used to measure Solar Energetic Particle (SEP) fluence spectra for H, He, O, and Fe, over the period from October 1997 to December 2005. The measurements were made by four instruments on ACE and the EPS sensor on three GOES satellites and extend in energy from ∼0.1 MeV/nuc to ∼100 MeV/nuc. Fluence spectra for each species were fit by conventional forms and used to investigate how the intensities, composition, and spectral shapes vary from year to year.     

单脊波导裂缝天线面阵的研制

分析了某机载雷达单脊波导裂缝天线面阵的结构特点和制造要点.在此基础上拟定了天线面阵精密制造流程,并阐述了其中的关键工艺措施.     

MEO导航卫星在轨放气产生的干扰力矩研究

摘要： 针对多颗MEO导航卫星太阳翼展开后产生比较明显的干扰力矩,对卫星稳定控制产生了一定影响的现象,本文根据动力学模型、姿态、角速度和飞轮转速变化,给出了干扰力矩计算方法,并结合多颗卫星在轨遥测数据进行计算,得出放气期间产生的干扰力矩.通过使用此干扰力矩进行仿真得出,卫星模拟器结果和在轨表现基本一致.此研究有助于优化卫星飞控流程,并指导卫星放气孔设计.