Filamentary structures in planetary nebulae

We have studied small-scale, filamentary features in 14 planetary nebulae and found that some structures are recurrent and shaped like the letters V and Y, with the apex or stem pointing toward the central parts of the nebula. Two such filaments containing dust, one in NGC 3132 and one in NGC 7293, were investigated in more detail. The mass and density of the filaments were obtained from extinction measurements, and their physical properties were derived. We propose that the structures are confined by magnetic fields, and derive magnetic field strengths of about 10⁻⁸ T, in line with earlier estimates. We also estimate the magnitude of the electric currents that we expect are generated in these dynamic systems. We propose a theory where the magnetic fields control the sculpting and evolution of small-scale filaments. This theory demonstrates how the substructures may form magnetized flux ropes that are twisted around each other, in the shape of double helices. Similar structures, and with similar origin, are found in many other astrophysical environments.     

频率可切换的矩形缝隙环频率选择表面

基于金属屏上周期排列的缝隙单元结构的通带特性,提出矩形缝隙环(Rectangular Slot Ring,RSR)加载短路线的单元结构实现频率可调频率选择表面(Frequency Selective Surface,FSS).谐振缝隙单元开路与短路时相对应的谐振频率分别为13 GHz和15 GHz.RSR-FSS选用Rogers RO4003介质作为基板,按照12×12的方阵进行周期排列,利用全波电磁仿真软件CST对其进行了电磁传输特性仿真.最终,通过实验验证了该频率选择表面在Ku波段通过连通和断开短路线可以进行频率的切换.     

传统星座的五帝座考证

中国传统星座中的紫微垣五帝内座和太微垣五帝座,都是古人为天上最高统治者天帝,在一年不同的五时处于不同方位处理政务而设的坐位。将五帝座作黄帝和四方之帝的坐位是“纬书”类的附会,与星座命名的本义相悖,由此造成不必要的混乱,一直延续至今,因此就有必要进行考证,给予澄清。     

“SZ-4”飞船高度计天线指向角反演方法

利用2003年2月7到8日“SZ-4”高度计的波形数据,经过波形数据预处理(波形为1 s的平均、去除热噪声和波形归一化)后,对海面回波波形后沿进行拟合,计算出了高度计天线的指向角,结果表明,“SZ-4”飞船高度计天线的指向角几乎全部在0.024°以内,天线指向在计算时间内比较稳定.     

不同天线组合对GPS姿态测量精度的影响分析

GPS姿态确定的精度不仅与单历元基线解算精度有关,还受基线长度和天线布设结构的影响。探讨了GPS姿态测量系统中基线长度和天线布设结构与姿态测量精度的关系。仿真结果表明:增加航向基线长度,能够提高航向角和俯仰角的精度,增加横向基线长度,能提高横滚角的精度;当基线长度一定时,将两基线正交布设,横滚角的精度最高。     

四酸溶矿——电感偶合等离子体发射光谱法测定钼矿中的钼

为了适应地质找矿和地质大普查工作对矿样测定速度和正确度的要求,对钼矿样品中的钼的测定方法进行试验,探讨在敞开体系中用盐酸+硝酸+氢氟酸+高氯酸的四酸溶矿体系消解钼矿样品,使用电感耦合等离子发射光谱仪(ICP-AES)测定钼的方法。     

基于CorelDRAW的地图注记自动化配置方法研究

作为制图者与用图者间信息传递的桥梁,地图注记辅助地图符号,对制图要素的名称、种类、性质和数量特征等进行了标识和说明,是地图不可或缺的组成部分。曲线、文字编辑功能极强的CorelDRAW软件颇受制图人员青睐,尤其在注记配置工作中扮演着重要角色。文章从点、线、面三个角度对地图注记配置进行了理论探析,同时基于CorelDRAW 15．0 Type Library控件和VBA环境进行了二次开发,智能化地实现了点注记的四点定位、线注记的适合路径、封闭面域的构建和自定义面注记的添加,对提高地图制图的效率和美化图面效果具有十分重要的意义。     

Array Configurations That Tile the Plane

Future radiotelescopes need ever increasing sensitivity. With the limits of receiver sensitivity being reached this can only be achieved by increasing collecting area. The increase in antenna numbers and the multi-resolution capabilities of these telescopes, such as the SKA, means a significant departure from existing designs is needed. In this article, some fundamental designs for antenna arrays that uniformly sample the UV plane are presented. The SKA is used to provide target specifications. The designs presented allow asymmetric configurations providing more freedom for site selection. They also allow a direct tradeoff between field of view and correlator complexity. This revised version was published online in July 2006 with corrections to the Cover Date.     

常德1631年大震事件的多场点群发式构造模型

根据对常德1631年地震事件的史料鉴别,尤其是江陵为典型七度震害这一事实,运用震声传播方向和地光物理场以及地震烈度衰减关系,拟合推断此地震事件的序列主要由安乡北6 3/4级地震、常德北太阳山7级地震、澧县6级地震、大庸6级地震和澧县—安乡6 1/2级地震组成,相应的地震地质背景是江汉—洞庭地区晚更新世以来的剩余形变呈四象限分布。若考虑地震-构造相关分布为“Z”字型,则该地震事件的主控构造——太阳山断裂带东断裂具左旋走滑的力学机制。根据区域地震—构造相关发展过程,常德大震事件可视为1668年郯城8 1/2级地震的前震序列组成部分。     

导航卫星天线相位中心误差标定方法研究现状及发展趋势

卫星天线相位中心误差是影响GNSS高精度定位定轨的重要误差源,实用中需要对其精确标定。随着北斗卫星导航系统的建设发展,如何对卫星天线相位中心误差进行更为精确的标定应引起人们的重视。为此,本文首先简要介绍了各卫星导航系统的卫星天线情况,而后系统总结了导航卫星天线相位中心误差标定方法的发展历程和研究现状,指出了未来卫星天线相位中心误差标定方法的发展趋势,相关研究成果对我国北斗卫星天线相位中心误差的标定方法研究具有参考意义。