Results of Photometric and Polarimetric Observations of the Fuor V1057 Cyg from the Time of an Outburst to the Present

Observations of the brightness, color, and polarization of the fuor V1057 Cyg over more than 30 years are presented and briefly discussed. Variability of the linear polarization was found.     

A Critical review of theoretical models of negatively polarized light scattered by atmosphereless solar system bodies

About a dozen physical mechanisms and models aspire to explain the negative polarization of light scattered by atmosphereless celestial bodies. This is too large a number for the reliable interpretation of observational data. Through a comparative analysis of the models, our main goal is to answer the question: Does any one model have an advantage over the others? Our analysis is based on new laboratory polarimetric and photometric data as well as on theoretical results. We show that the widely used models due to Hopfield and Wolff cannot realistically explain the phase-angle dependence of the degree of polarization observed at small phase angles. The so-called interference or coherent backscattering mechanism is the most promising model. Models based on that mechanism use well-defined physical parameters to explain both negative polarization and the opposition effect. They are supported by laboratory experiments, particularly those showing enhancement of negative polarization with decreasing particle size down to the wavelength of light. According to the interference mechanism, pronounced negative branches of polarization, like those of C-class asteroids, may indicate a high degree of optical inhomogeneity of light-scattering surfaces at small scales. The mechanism also seems appropriate for treating the negative polarization and opposition effects of cometary dust comae, planetary rings, and the zodiacal light.     

A Compact Explicit Difference Scheme of High Accuracy for Extended Boussinesq Equations

Presented here is a compact explicit difference scheme of high accuracy for solving the extended Boussinesq equations.For time discretization,a three-stage explicit Runge-Kutta method with TVD property is used at predicting stage,a cubic spline function is adopted at correcting stage,which made the time discretization accuracy up to fourth order;For spatial discretization,a three-point explicit compact difference scheme with arbitrary order accuracy is employed.The extended Boussinesq equations derived by Beji and Nadaoka are solved by the proposed scheme.The numerical results agree well with the experimental data.At the same time,the comparisons of the two numerical results between the present scheme and low accuracy difference method are made,which further show the necessity of using high accuracy scheme to solve the extended Boussinesq equations.As a valid sample,the wave propagation on the rectangular step is formulated by the present scheme,the modelled results are in better agreement with the experimental data than those of Kittitanasuan.     

硬致密泥岩钻进的新型复合片钻头的研究与应用

介绍了一种新型齿形的复合片钻头，在硬致密泥岩中钻进，与常规复合片钻头相比，具有很高的钻进效率和高的钻头寿命，解决了泥岩钻进效率低的难题。     

对综合测井曲线解释的几点体会

本文阐述了在地质找矿中从地质角度对综合测井曲线解释的重要性；指出了测井曲线的一般特点和特殊优点；尤其对致密钙质岩石在测井曲线上的表现形式及其厚度确定做了深入研究；分析了测井曲线解释存在的问题；最后提出了几点建议。     

基于波导结构的紧凑型电介质加载双极化天线研究

本文提出了一款基于波导结构的紧凑型电介质加载双极化天线.通过采用在传统波导内加载电介质材料的方法,可以有效减小波导尺寸,从而达到天线小型化的目的.针对波导结构口径天线高后瓣辐射的问题,本文提出了一种在波导金属壁上添加矩形槽孔的方法,该方法的原理不同于扼流环结构.相比之下,矩形槽孔具有结构简单、尺寸小、加工方便等优点.通过电磁场全波仿真分析,可以发现所提出的天线具有阻抗带宽宽（大于40%）、增益高（8.6±0.6 dBi）、辐射性能稳定等优点,有很大的潜力,可以应用在如卫星通信等X波段的各种应用场景中.     

低剖面紧凑的圆盘加载单极子天线

本文介绍了一种低剖面小型化圆盘加载单极子天线.通过盘加载的方式,在中心频率5.8 GHz处,首先将单极子天线的剖面从大约12.9 mm（0.25λ₀）降低到2 mm（0.039λ₀）,实现了低剖面的特性.加载在单极子天线上方的圆盘,尺寸大概为21 mm（0.41λ₀）,因此天线具有结构紧凑的特点.接着,为了使天线具有良好的匹配,在加载圆盘四周加入4个接地通孔,并且在馈电端口加入集总电感.最终,天线在中心工作频率5.8 GHz处实现了反射系数-15 dB的匹配性能.     

国外大都市区管理的实践及其借鉴

大都市政府和都市议会是发达国家对大都市区和都市连绵区进行宏观管理的重要机构，本文简要介绍了各种类型的大都市政府和都市议会的形成与发展，在此基础上提出了我国相应的宏观管理机构为城镇密集区政府和都市区规划局，最后，对我国城镇密集区规划管理的可行性与规划管理体系问题进行了讨论。     

点态性质与一致性质的一个新关系

为了研究点态性质和一致性质之间的关系,应用紧性性质在拓扑意义下得到逐点有界性质蕴含一致有界性质的结论,并将其推广到连续函数族的情况.基于Baire定理,得到完备度量空间中的逐点收敛性质可导出一致有界性质的结论.