TLM法在二维非均匀介质电磁场计算中的应用

传输线模型方法(Transm ission Line Modeling,TLM)是近年来发展起来的描述快速电磁场现象的分支。我们将TLM方法应用于二维介质电磁场的计算,并且详细地阐述了该算法的实现过程。在数值实验中,分别使用TLM法、有限差分法计算各向同性介质中的静电场的分布,通过对结果进行对比分析,证明了TLM方法具有较高的精度,并且用TLM方法计算电磁场相当直观。同时,还用TLM法计算了在二维非均匀各向同性介质中,点电流源情况下研究区域中的电位分布,其结果较为理想。     

Positional error curves band of a planar line segment within GISs

1 Introductionffe well-for Meanboha Eno(MSRE),having advanop of talculang ndy,has bo widdyed to m the W of pont ednates inGIS' NY and gedop. N, it is Me tDtw the opiW eno Of a pont in whitw dirm-tion, while in praedce there is ned tO for the value ofghH or Of a trint in a peial boon SUCh asthe uha diW. The or curve of a glnt is ableto W twl the diAnbution wttiOn of twnt eno.ln an arbtw dich and it is the nd efhaive edfor dedbing forhed rm Of odnts in SUrVopng..mpneenng(Mithel, 1983…     

基于栅格数据提取主骨架线的新算法

详细介绍了基于栅格数据的面状地物主骨架线的提取算法。该算法具有较快的处理速度和较强的适应性及内存需求少的优点 ,同时用该算法所提取的主骨架线为最优 (最长 )骨架线 ,可用于面状地物注记的自动配置。     

数字栅格地图的制作

阐述了数字栅格地图制作的技术流程 ,并对技术流程的关键技术问题作了详细的阐述。从方法上解决了扫描过程中因阈值选择不当而出现的断线、粘连现象 ,从原理上介绍了几何纠正。最后从方法上介绍了彩色数字栅格地图的色彩归一化。     

GS型重力仪面板常数测定的研究

系统分析了GS - 1 5 - 2 1 6重力仪多次在重力基线场标定的结果 ,并与厂家给出的面板常数进行对比 ,认为GS型重力仪的面板常数存在长期变化 ,应定期重新标定 ;检修或工作状态的变化也会引起面板常数的改变 ;面板常数是仪器测程的函数 ,必须分段标定以便拟合一条常数曲线 .     

South Segment of Minjiang Fault and Diexi Earthquake in 1933

Diexi earthquake(M7.5)in 1933 is a great event that occurred at the east border of Qinghai- Xizang Plateau in the 20th century.There are obviously different opinions about the shape ofisoseismal lines and the genetic fault of this earthquke.Based on the study of the newlyfound north-south trending active fault and ground fissures of Diexi earthquake,this papertends to hold that,as the southward extension of Miujiang fault,this north-south trendingactive fault might be the genetic fault of this event.     

低密度钻井液的开发与应用

ＤＭＺ低密度无固相钻井液主要由水、高分子聚合物（防塌剂）、天然高分子物质（降滤失剂）配制而成,其密度稳定在０．９９９～１．００４ｇ／ｃｍ＾３之间,具有良好的防塌护壁和絮凝能力,能有效解决小口径绳索取心钻探中出现的钻杆内结泥皮、携带岩粉能力差、失水量高等问题。     

Optical observations of the Be/X‐ray transient system KS 1947+300

ROTSE‐IIId observations of the Be/X‐ray transient system KS 1947+300 obtained between September 2004 and December 2005 make it possible to study the correlation between optical and X‐ray activity. The optical outburst of 0.1 mag was accompanied by an increase of the X‐ray flux in the 2004 observations. A strong correlation between the optical and X‐ray light curves suggests that the neutron star directly accretes from the outflowing material of the Be star. The nearly zero time lag between X‐ray and optical light curves suggests a heating of the disk of Be star by X‐rays. No optical brightening and X‐ray enhancement was seen in the 2005 observations. There is no indication of an orbital modulation in the optical light curve. (© 2007 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

红外源IRAS 05437-0001和IRAS 05351+3549的CO分子谱线观测研究

利用紫金山天文台青海观测站13.7米射电望远镜对红外源IRAS05437-0001和IRAS05351+3549附近区域进行了CO(J=1-0)的分子谱线观测.发现在这两个源的方向都有很强的CO发射,CO谱线还有明显的线翼成分,这暗示两个红外源存在分子外流.同时还获得了每个源5＇×5＇的成图.通过对高速气体的空间分布的观测和分析,认为这两个源为分子外流源.其中IRAS05437-0001附近区域的外流结构比较复杂,可能这一区域的外流是多极的.IRAS05351+3549附近的外流结构较简单.从两个源的红外光谱分类以及外流的动力学时标得出都是年轻星(年龄～105yrs).通过对这两个外流源的参数估算,得出两个外流源的质量损失率.