套筒天线组成的宽带干涉仪测向圆阵研究

为提高宽带干涉仪测向圆阵性能,首次提出了利用套筒天线代替常规加载宽带偶极子作为测向阵列单元.利用Fourier变换结合矩量法分析了套筒天线组成的测向圆阵的电磁特性,并利用HFSS软件对部分仿真结果进行了验证.在得出阵列电磁特性的基础上再运用基于空间距离的相关数据处理方法统计分析了测向圆阵性能.研究结果表明,相对于常规测向圆阵,由于套筒天线构成的测向圆阵增益高、消除了广义谐振现象,使测向圆阵的灵敏度、测向精度均得到较大提高.相应地模糊度减小、稳健性能增强.     

Correlation analysis of PCB and comparison of test-analysis model reduction methods

The validity of correlation analysis between finite element model（FEM） and modal test data is strongly affected by three factors, i.e., quality of excitation and measurement points in modal test,FEM reduction methods, and correlation check techniques. A new criterion based on modified mode participation（MMP） for choosing the best excitation point is presented. Comparison between this new criterion and mode participation（MP） criterion is made by using Case 1 with a simple printed circuit board（PCB）. The result indicates that this new criterion produces better results. In Case 2, 35 measurement points are selected to perform modal test and correlation analysis while 9 selected in Case 3.System equivalent reduction expansion process（SEREP）, modal assurance criteria（MAC）, coordinate modal assurance criteria（CoMAC）, pseudo orthogonality check（POC） and coordinate orthogonality check（CORTHOG） are used to show the error introduced by modal test in Cases 2 and 3. Case 2 shows that additional errors which cannot be identified by using CoMAC can be found by using CORTHOG.In both Cases 2 and 3, Guyan reduction, improved reduced system（IRS） method, SEREP and Hybrid reduction are compared for accuracy and robustness. The results suggest that the quality of the reduction process is problem dependent. However, the IRS method is an improvement over the Guyan reduction, and the Hybrid reduction is an improvement over the SEREP reduction.     

空间监视中设备级数据-目标对应关系确定方法

基于各测量弧段的方位、俯仰,通过数学变换和多项式拟合,实现以拟合系数为特征量表征该弧段的观测。进而通过比较观测值与理论值的拟合系数,完成数据-目标对应关系的确定,达到简化设备级数据-目标对应关系快速确定的目的。     

差分VLBI在深空导航中应用接收机信号形式的选择

讨论了差分VLBI系统在深空探测中应用的几个问题，就标校接收机的带宽设计进行了分析，提出了目标接收机在应用中可能的三种信号形式，并分析了三种信号形式在深空探测中应用的可能性，验算了每种信号形式的性能，并对将来可能使用形式进行了探讨。     

Measuring air traffic complexity based on small samples

Air traffic complexity is an objective metric for evaluating the operational condition of the airspace.It has several applications,such as airspace design and traffic flow management.Therefore,identifying a reliable method to accurately measure traffic complexity is important.Considering that many factors correlate with traffic complexity in complicated nonlinear ways,researchers have proposed several complexity evaluation methods based on machine learning models which were trained with large samples.However,the high cost of sample collection usually results in limited training set.In this paper,an ensemble learning model is proposed for measuring air traffic complexity within a sector based on small samples.To exploit the classification information within each factor,multiple diverse factor subsets (FSSs) are generated under guidance from factor noise and independence analysis.Then,a base complexity evaluator is built corresponding to each FSS.The final complexity evaluation result is obtained by integrating all results from the base evaluators.Experimental studies using real-world air traffic operation data demonstrate the advantages of our model for small-sample-based traffic complexity evaluation over other stateof-the-art methods.     

用于速度测量的硬件相关仪

相关法测量速度已经发展了多年。由于相关运算计算量很大，软件实现时，对于大速度系统，受运算速度所限，其实时性及精度都不甚理想。为此，本文介绍１种用硬件实现相关运算的方法，并给出硬件相关仪结构及与８０９８单片机的接口框图。     

信道相关性对分集合并接收性能的影响

简介分集接收的主要方式 ,定量分析信道相关性对分集接收性能的影响。特别针对 Rayleigh信道模型中最大比合并和选择合并在各分集支路相关时的性能作了仔细研究 ,给出仿真结果 ,验证各分集支路相关性越小 ,分集效果越好的结论。在最大比合并下 ,当各路平均信噪比与门限相比较小时 ,各分集支路越相关 ,输出信噪比超过门限的概率越大。     

Emission heights of coronal bright points on Fe XII radiance map

The study of coronal bright points (BPs) is important for understanding coronal heating and the origin of the solar wind. Previous studies indicated that coronal BPs have a highly significant tendency to coincide with magnetic neutral lines in the photosphere. Here we further studied the emission heights of the BPs above the photosphere in the bipolar magnetic loops that are apparently associated with them. As BPs are seen in projection against the disk their true emission heights are unknown. The correlation of the BP locations on the Fe XII radiance map from EIT with the magnetic field features (in particular neutral lines) was investigated in detail. The coronal magnetic field was determined by an extrapolation of the photospheric field (derived from 2-D magnetograms obtained from the Kitt Peak observatory) to different altitudes above the disk. It was found that most BPs sit on or near a photospheric neutral line, but that the emission occurs at a height of about 5 Mm. Some BPs, while being seen in projection, still seem to coincide with neutral lines, although their emission takes place at heights of more than 10 Mm. Such coincidences almost disappear for emissions above 20 Mm. We also projected the upper segments of the 3-D magnetic field lines above different heights, respectively, on to the tangent x–y plane, where x is in the east–west and y in the south–north direction. The shape of each BP was compared with the respective field-line segment nearby. This comparison suggests that most coronal BPs are actually located on the top of their associated magnetic loops. Finally, we calculated for each selected BP region the correlation coefficient between the Fe XII intensity enhancement and the horizontal component of the extrapolated magnetic field vector at the same x–y position in planes of different heights, respectively. We found that for almost all the BP regions we studied the correlation coefficient, with increasing height, increases to a maximal value and then decreases again. The height corresponding to this maximum was defined as the correlation height, which for most bright points was found to range below 20 Mm.     

六端口校准结果的误差相关性分析

本文认分析六端口校准标准的误差对核准结果精确度的影响出发,指出提供一套标准,实际上是提供了一个拟合的反射系数平面,它与理想的反射系数平面间由一个分式线性变换相联系。系统真实结参数的四个复参数是理想平面上的点,而实际核准结果则是拟合平面上的点。因此,校准所得结参数与真实结参数相比存在着误差相关性。而且,结参数中的三个实参数与各复参数问同样存在着误差相关性。     

利用AE指数重构磁层相空间—对存在问题的讨论

1引言由于磁层的物理过程受到太阳风到电离层诸多过程的影响并包含了许多空间和时间尺度，因此磁层是个相当复杂的系统．人们希望通过新的非线性科学理论了解这一系统的基本参数．因而许多学者纷纷用目前能较好反映磁层活动的极光电集流指数AE（或AL）及常用的相空间重构方法对磁层进行研究．他们利用不同时间段的AE指数和GP方法I’域SVD法l’］得到的吸引子的关联维在2－4之间，因此，认为磁层是一个具有低维吸引子的动力学系统．然而有人用修正的QP法l’］详细计算了多个时间段AE指数的关联维，发现计算的关联继大小依赖于磁层的活…