Third Body Perturbations of Double Stars

We report on the different results concerning the stability of the hierarchical triple systems where a close binary is accompanied by a third star. There are different possible approaches to answer the question of the stability limits for such triple stars: the most direct investigations can be undertaken in integrating numerically the respective equations of motion for many different initial conditions. It is then difficult to take into account all the important parameters like eccentricities, inclination, phases and masses. Analytical approaches and qualitative methods are more approriate to deal with this problem; the respective results confirm the numerically found results that: 1. for prograde orbits the ratio semimajor axis of the inner orbits to the periastron position of the outer orbit is approximately 3.2 2. for retrograde orbits this ratio is just some 10 percents smaller 3. the results are not sensitive in what concerns the masses involved 4. There is a tendency that the inclinations and eccentricities change slightly the stability limits mentioned above. This revised version was published online in August 2006 with corrections to the Cover Date.     

FLOW DIRECTION AND BRANCHING GEOMETRY AT JUNCTIONS IN DENDRITIC RIVER NETWORKS*

Automatic determination of flow direction from a partial view of a drainage network is a problem, notably in remote sensing. The main approach to determining which river link is pointing downstream uses spatial reasoning based on local features at junctions. Theoretical and empirical works on junction angles suggest that the two consecutive links which bound the most acute angle are the upstream links. This rule was tested using 2279 river junctions digitized from 19 dendritic drainage networks and was correct in nearly 90% of the cases. This result is better than that obtained from the decision table designed by Haralick, Wang et al. (1985) for the same purpose.     

藏北若拉岗日结合带中的浅变质地层及其锆石SHRIMP U-Pb年龄测定

通过对拉竹龙-西金乌兰湖-金沙江结合带西段若拉岗日一带的地层重新解体厘定,填绘出一套以白云母石英片岩、石英岩、变质石英砂岩为主的绿片岩相浅变质地层。该浅变质地层可与羌塘地块之上的浅变质岩系玛依岗日组对比。对浅变质地层的碎屑锆石进行U-PbSHRIMP年龄测定,认为所获得的最小年龄值524Ma代表了该套地层沉积时代的下限,再结合该地区出露未变质的泥盆纪地层这一事实,将这套浅变质岩系的形成时代置于早古生代。     

GPS三频载波相位组合误差分析及选择方法

本文首先从GPS双差模型出发，给出了三频载波组合的基本形式，依据该形式，得到了组合波长表达式，并分析了电离层误差和观测噪声对三频组合的影响。由这些误差特性，给出了三频线性组合系数的选取方法，并给出了一些常用的线性组合形式，分析了它们的优缺点。最后，简单介绍了目前主要的三频模糊度解算方法CIR和TCAR。     

巷道交岔点的三维建模及实现

针对巷道交岔点建模的难点问题,采用基于巷道底板中线加载巷道断面的方式绘制单一巷道体,提出了根据巷道设计参数的方式对柱墙式交岔点进行建模。并依据穿尖式交岔点和马门头中两条巷道自然相交的特征,对二者进行建模。最后通过C#结合DirectX的编程方式进行验证,结果表明所绘制的巷道交岔点外观规整并形成连通。     

塔中涡动资料不同坐标旋转方法比较分析

坐标旋转是涡动协方差(EC)通量观测数据后处理当中必须进行的步骤,本文利用塔克拉玛干沙漠腹地塔中西面标校站自然沙丘上3 m高度和塔中本站32 m高度2009年4—10月湍流通量数据,对比分析了不同坐标旋转方法在塔中通量观测数据中的应用。结果表明,塔克拉玛干沙漠腹地塔中湍流各通量在旋转订正前后差别不显著,不订正造成的通量计算误差1%。塔中32 m和塔中西站3 m通量计算误差,与两个站点的采集仪器架设高度差别较大有关。即使对于相对平坦的下垫面,也必须要进行倾斜校正,以修正地势、仪器振动、安装倾斜等产生的虚假信息。本研究对塔中涡动资料进行旋转时采用了二次坐标旋转方法。此结果为塔克拉玛干沙漠腹地EC通量观测的风速仪倾斜校正提供参考。     

涡度相关仪倾斜订正方法的比较及应用

利用973暴雨项目2002年在安徽肥西观测的涡度相关资料,针对目前涡度相关法中存在的仪器倾斜误差问题,采用两种倾斜订正方法计算湍流参数并进行对比分析.结果表明,三次坐标轴旋转倾斜订正方法和平面拟合方法均可以对仪器倾斜引起的误差进行坐标旋转订正,有效剔除仪器倾斜引起的侧向应力的影响,以及仪彝倾斜时水平方向风速引起的虚假湍流通量,提高了湍流通量的计算精度.两种倾斜订正方法各有一定适用条倬,平面拟合方法优于三次坐标轴旋转倾斜订正方法.     

皖西白大山群的发现及其地质意义

皖、豫交界的白大山－茶庵一带，出露一套碎屑岩夹碳酸盐岩地层，以往被置于青白口系八公山群。近期笔者等赴该地再次进行了调查和研究，结果发现该群地层组合内含有大量球藻类和植物碎片化石，这些微古植物分子在国内外多见于下古生代。并从岩石组合特征对比分析，认为该套地层属志留－泥盆系的可能性最大。对这套地层及微古植物的发现，具有两方面重要的地质意义：１．过去对华北地台南缘从未见有这个时代地层的报导，这就为该区地层填补了一个空白；２．从已采获的微古植物组合及岩性组合特征等分析，这有可能对华北地台南缘的岩相古地理图及地史发展等问题，进行一些必要的改写与补充。     

氧气反应模式-电感耦合等离子体串联质谱法测定土壤中的镉

应用电感耦合等离子体质谱法(ICP-MS)分析土壤中的镉元素时,锆的氢氧化物、钼的氧化物、锡的同位素会对镉造成严重的干扰,导致准确测定土壤中镉的难度较大.本文采用电感耦合等离子体串接质谱法(ICP-MS/MS),选取无同质异位素干扰的111 Cd为分析谱线,在MS/MS模式下碰撞反应池中通入的氧气可以与94Zr16O1...