基于神经网络的时频域雷达信号调制参数估计

针对常规时频分析方法对多分量雷达信号分析的不足,提出一种基于神经网络的时频域多分量雷达信号调制参数估计新方法.把多分量雷达信号的时频分布作为灰度图像,通过神经网络训练得到高分辨率时频平面图,然后在时频域实现雷达信号各分量的调制参数估计,相对于时频重排等方法,其对时频分布的处理不需要关于各分量信号的先验知识.仿真实验表明,该方法在得到比时频重排方法更高分辨率时频图的基础上,能够较准确地估计各分量雷达信号调制参数.     

Validation of IRI-2012 TEC model over Ethiopia during solar minimum (2009) and solar maximum (2013) phases

This paper investigates the capacity of the latest version of the International Reference Ionosphere (IRI-2012) model in predicting the vertical Total Electron Content (vTEC) over Ethiopian regions during solar minimum (2009) and solar maximum (2013) phases. This has been carried out by comparing the IRI-2012 modeled and experimental vTEC inferred from eight ground based dual frequency GPS (Global Positioning System) receivers installed recently at different regions of the country. In this work, the diurnal, monthly and seasonal variation in the measured vTEC have been analyzed and compared with the IRI-2012 modeled vTEC. During the solar minimum phase, the lowest and highest diurnal peak of the experimental vTEC are observed in July and October, respectively. In general, the diurnal variability of vTEC has shown minimum values around 0300 UT (0600 LT) and maximum values between around 1000 and 1300 UT (1300 and 1600 LT) during both solar activity phases. Moreover, the maximum and minimum monthly and seasonal mean hourly vTEC values are observed in October and July and in the March equinox and June solstice, respectively. It is also shown that the IRI-2012-model better predicts the diurnal vTEC in the time interval of about 0000–0300 UT (0300–0600 LT) during the solar minimum phase. However, the model generally overestimates the diurnal vTEC except in the time interval of about 0900–1500 UT (1200–1800 LT) during the solar maximum phase. The overall result of this work shows that the diurnal vTEC prediction performance of the model is generally better during the solar minimum phase than during solar maximum phase. Regarding the monthly and seasonal prediction capacity of the model, there is a good agreement between the modeled and measured monthly and seasonal mean hourly vTEC values in January and December solstice, respectively. Another result of the work depicts that unlike the GPS–TEC the IRI-2012 TEC does not respond to the effect resulted from geomagnetic storms.     

CCPT系统中基于副边阻抗调制技术的反向信号与能量叠加传输技术研究

为了解决金属环境条件下的无线供电和信号传输需求，提出了一种基于电容耦合方式的无线能量和信号并行传输方案。通过建立E类放大器的数学模型，分析电容耦合系统的传输特性和阻抗影响机理，设计了适用于E类放大器结构的调制与解调电路，并通过仿真验证了电路的可行性，为CCPT系统从能量传输到信号回传提供了系统性的理论指导。     

螺旋波电推进羽流电磁矢量控制的原理性验证

推进器羽流的电磁矢量控制是基于电磁位形的改变使得喷射的羽流改变方向。为了原理性验证电推进羽流电磁矢量控制技术，针对螺旋波电推进器，开展了磁场位形调制仿真设计和试验验证。说明了电磁矢量调制线圈能够改变磁场位型，并且在试验过程中验证了等离子体羽流随磁场位型变化而产生的羽流方向偏转。在周期性磁场调制过程中，验证了等离子体密度参数随之周期性涨落。螺旋波电推进羽流方向最大偏转角度60°，可控偏转频率15Hz，说明了电推进羽流电磁矢量控制的可行性。     

基于伪随机码相位调制和外差探测的高精度激光测速测距系统研究

为在远距离范围内实现高精度的激光测速测距，提出了一种联合利用伪随机码相位调制和外差探测技术的激光测速测距方法，并搭建了实验验证平台。当激光出射功率为2mW、参考光功率为117 、调制速率为100MHz、单周期内伪随机码序列长度为81.9 时，该系统在对位于约8 m处、径向速度约为1.4 m/s的目标进行测试时，可以实现0.138m的测距精度，以及4.16cm/s 的测速精度。实验结果证实，该套系统可实现高精度的径向速度和距离测量，且系统工作状态为长脉宽低峰值功率，为远距离的激光测速测距系统设计开辟了一条新途径。     

Spectra of the two official GLEs of solar cycle 24

Based on ground-level data and on satellite data we determine in this work the observational spectrum of both, the Ground Level Enhancement of May 17, (2012) the so-called GLE71 and the Ground Level Enhancement of September 10, 2017 (GLE 72). We describe a simplified method to obtain the experimental spectrum at ground level. Data of the GLE71 and GLE72 indicate the presence of two different populations, each one with a different energy spectrum. On the other hand, we explore the kind of phenomena that take place at the source in these two particular events. In contrast with other methods based on the temporal synchronization between electromagnetic emissions of flares and coronal mass ejections (CME), here we develop an alternative option based on the study of the accelerated particles, by adjusting our theoretical spectra to the observational spectra. The main results of this work are the derivation of the source and acceleration parameters involved in the generation process. These results lead us to construct possible scenarios of particle generation in the source for each one of the two studied GLEs.     

航天器太阳圆面速度差/太阳视方向组合导航

针对航天器，尤其是深空探测器的自主导航问题，提出了一种新的太阳圆面速度差天文量测信息，该信息利用太阳的较差自转所造成的太阳圆面各点速度不同的特性，是探测器当前位置的函数，其几何本质是一个探测器的位置圆锥。在此基础上，基于太阳圆面速度差和太阳视方向互补的特性，提出了一种太阳圆面速度差/太阳视方向组合导航新方法，将太阳圆面速度差与太阳视方向2种量测量结合起来，实现了量测量之间的优势互补，进一步提高了导航性能。以太阳探测器为例进行了仿真，仿真结果表明相比较于单独用太阳圆面速度差或太阳视方向的导航方法，基于太阳圆面速度差/太阳视方向的组合导航方法精度分别提升了10.2%和16.0%。此外，还分析了光谱仪精度、采样周期和光谱仪数量对导航性能的影响，为深空探测自主导航提供了新的理论与方法。     

含多间隙柔性可展帆板动力学建模及仿真

为研究柔性和多级铰链间隙对帆板展开过程动力学特性的影响，以月球车两级往复可展太阳帆板为研究对象，采用修正Coulomb模型表述摩擦力，通过接触碰撞力描述间隙，运用有限元法进行帆板柔性化，进而建立多间隙-柔性耦合的动力学模型。采用变步长伦哥库塔法进行数值求解，模拟帆板展开过程，分析了多间隙和柔性对帆板质心加速度、铰链间隙碰撞力等参数的影响。结果表明，在保证展开机构刚度要求的前提下，帆板柔性可补偿因铰间隙引起的加速度波动，减弱间隙处碰撞的剧烈程度，减小碰撞力幅值，进而改善帆板展开机构的动态特性。研究结果可用于指导月球车两级往复可展太阳帆板等同类型的可展机构动态优化设计。     

太阳电池片间隙区域充电电场的数值计算

高压太阳电池阵在空间带电粒子环境中易发生静电放电,特别是太阳电池片间隙区域存在着诱发二次放电的风险。文章建立了太阳电池片间隙区域充电模型,基于静电理论研究了计算太阳电池片间隙区域充电电场的算法。数值计算结果表明:太阳电池片间隙区域两侧,充电电场呈对称分布;玻璃盖片与基底之间存在明显的电位差,且玻璃盖片的电位高于其他部位。     

UltraFlex太阳电池阵的结构优化

以提高圆形太阳电池阵的展开过程稳定性和固有频率为优化目标,以UltraFlex太阳电池阵为模型,采用有限元软件SAMCEF对其进行结构优化。以承重梁材料、斜梁开口高度、斜梁位置、梁截面高度及厚度5种结构参数为优化变量,进行了多种工况的展开动力学仿真和模态计算。经分析发现,结构展开后期太阳毯与支撑梁拉扯会导致支撑梁剪切应力激增;梁材料、斜梁位置与支撑梁截面高度对太阳电池阵的展开过程稳定性影响较大;当梁材料为碳纤维,斜梁位置为1100 mm,梁截面高度为20 mm时,展开过程稳定性最好;斜梁位置和承重梁截面厚度对结构固有频率影响较大;当斜梁位置为900 mm或1100 mm、承重梁截面厚度从3 mm增至3.5 mm时,系统固有频率涨幅最大,由此带来的质量增加可以接受。