基于浮游有孔虫重建的南海北部400 ka以来上层水体结构变化及其对东亚季风的响应

现代南海上层水体结构具有鲜明的季节特征,反映了季节性风场通过动力与热力过程施加的强烈影响;这种风场对上层水体结构的调控同样存在于地质历史时期,借此,长时间尺度上的东亚季风强度变化能够在南海沉积中留下记录,对相关高分辨率样品的研究继而可以从海洋的角度发掘出新的季风信息,成为对现有古季风资料的重要补充。本研究利用南海北部岩芯总长为50.8 m的MD12-3432站位（19°16.88'N,116°14.52'E;水深2125 m）高分辨率沉积样品,通过浮游有孔虫属种组合及其转换函数恢复了400 ka以来冬、夏季海水表层温度及温跃层深度,并对其进行频谱分析,同时对比现代观测资料及黄土粒度等古季风记录,讨论了海表温度、温跃层深度变化与东亚季风强度、表层环流格局等因素的关系。结果表明,晚更新世以来南海北部海表温度具有显著的100 ka冰期-间冰期旋回,冬季海表温度降幅可达8℃,是冰期冬季风增强与表层环流变化的共同结果。此外,冬季海表温度与温跃层深度重建结果均具有明显的67 ka周期,可能代表了东亚冬季风风速在南海北部的变化周期。同时,温跃层深度中未出现100 ka周期,可能指示冰期-间冰期旋回中表层环流的变化对其影响较弱,温跃层的加深主要由东亚冬季风的增强造成。

     

走滑断裂带中挤压阶区内部剪切构造初探

野外地质调查和航片立体镜下解译发现,小江断裂带北段蒙姑和东支大营盘两个挤压阶区内部发育有剪切构造,它们在地表主要表现为断裂槽地、断层陡坎、地裂缝等。挤压阶区内部剪切构造和拉张阶区内部剪切构造一样,是阶区形成后,随着走滑断裂的进一步活动而形成的新生性构造     

Analysis of the positive ionospheric response to a moderate geomagnetic storm using a global numerical model

Current theories of F-layer storms are discussed using numerical simulations with the Upper Atmosphere Model, a global self-consistent, time dependent numerical model of the thermosphere-ionosphere-plasmasphere-magnetosphere system including electrodynamical coupling effects. A case study of a moderate geomagnetic storm at low solar activity during the northern winter solstice exemplifies the complex storm phenomena. The study focuses on positive ionospheric storm effects in relation to thermospheric disturbances in general and thermospheric composition changes in particular. It investigates the dynamical effects of both neutral meridional winds and electric fields caused by the disturbance dynamo effect. The penetration of short-time electric fields of magnetospheric origin during storm intensification phases is shown for the first time in this model study. Comparisons of the calculated thermospheric composition changes with satellite observations of AE-C and ESRO-4 during storm time show a good agreement. The empirical MSISE90 model, however, is less consistent with the simulations. It does not show the equatorward propagation of the disturbances and predicts that they have a gentler latitudinal gradient. Both theoretical and experimental data reveal that although the ratio of [O]/[N₂] at high latitudes decreases significantly during the magnetic storm compared with the quiet time level, at mid to low latitudes it does not increase (at fixed altitudes) above the quiet reference level. Meanwhile, the ionospheric storm is positive there. We conclude that the positive phase of the ionospheric storm is mainly due to uplifting of ionospheric F2-region plasma at mid latitudes and its equatorward movement at low latitudes along geomagnetic field lines caused by large-scale neutral wind circulation and the passage of travelling atmospheric disturbances (TADs). The calculated zonal electric field disturbances also help to create the positive ionospheric disturbances both at middle and low latitudes. Minor contributions arise from the general density enhancement of all constituents during geomagnetic storms, which favours ion production processes above ion losses at fixed height under day-light conditions.     

Lymanα forests and the evolution of the universe

The Lyα forest absorption lines in the spectra of quasars are interpreted as caused by the crossings of the light beam with the walls of a bubble structure (expanding with the Hubble flow only). Then, the typical separation between the absorption lines is proportional to the mean size of the bubbles. The variable factor is the expansion rate H[z]. The Friedmann regression analysis of the observed line separations determines the density parameter ω₀ and the normalized cosmological term λ₀ = λc²/3H²₀ of the appropriate cosmological model: ω₀ = 0.014 ± 0.002, λ₀ = 1.080 ± 0.006. Depending on the Hubble parameter this method reveals the values of the present mean matter density pm,0 = 2.6 h² · 10⁻²⁸ kg m⁻³ and of the cosmological constant Λ = 3.77 h² · 10⁻⁵² m⁻² (with h = H₀/(100 km/s·Mpc)). According to our analysis all models with Λ = 0 must be excluded. The curvature of space is positive. The curvature radius R₀ is 3.3 times the Hubble radius (c/H₀). The age t₀ is 2.8 times the Hubble age (H₀⁻¹).     

Invariant manifolds, phase correlations of chaotic orbits and the spiral structure of galaxies

In the presence of a strong   m = 2  component in a rotating galaxy, the phase-space structure near corotation is shaped to a large extent by the invariant manifolds of the short-period family of unstable periodic orbits terminating at L ₁ or L ₂. The main effect of these manifolds is to create robust phase correlations among a number of chaotic orbits large enough to support a spiral density wave outside corotation. The phenomenon is described theoretically by soliton-like solutions of a Sine–Gordon equation. Numerical examples are given in an N -body simulation of a barred spiral galaxy. In these examples, we demonstrate how the projection of unstable manifolds in configuration space reproduces essentially the entire observed bar–spiral pattern.     

基于三角网的"种子法"多边形生成

将传统上广泛使用的“种子法”和“矢量求交法”的思想相结合 ,提出了一种基于约束Delaunay三角网结构的多边形生成算法。详细描述了该方法的基本思想 ,在实验基础上分析了算法的特点。     

经济信息管理系统分析与研究

根据经济信息管理系统的组织特征与建立原则 ,提出经济信息管理系统的结构模式与建立步骤。     

流域地形自动分割研究

本文提供了基于栅格数字高程模型（ＤＥＭ）提取流域空间结构,进行流域自动分割的技术方法。该方法包括地貌形态结构定义、流域结构定义和算法设计３个部分。基于本文设计的算法,可以从ＤＥＭ提取完整的汇流网络和分水线网络,两者组成的多边形集把流域分割成具有拓扑结构的多个子汇流区,这个子汇流区集作为存贮流域信息的基本地貌单元,是流域信息进入地学数据库的框架,也是进行空间分布式机理──过程流域分析模型的基础。并以山西离石黄土丘陵沟壑区的王家沟流域为试验区,获得了较为满意的结果。     

移动GIS在广州市文化遗产普查中的应用研究

采用移动GIS可以实现文化遗产信息管理的准确性、及时性、科学性,可以提高文化遗产保护及考古工作的科技含量与管理水平。本文介绍了基于GIS终端的文化遗产信息快速采集技术,通过统一的内、外业调研平台改变了以往内外业工作割裂的模式,外业现场采集的文化遗产空间信息和属性信息可以直接导入到最终的内业数据管理平台,减少了中间环节,达到提高文化遗产信息采集作业效率和采集数据快速入库的目的。     

大型射电望远镜背架精密安装技术

对65 m射电望远镜的背架安装做了尝试,取得较满意的结果.针对天线背架尺寸大、质量重、焊接变形大、几何精度要求高等特性,采用全站仪工业测量系统实现背架的快速、无接触、高精度定位测量,点位测量精度优于1 mm;采用独特的施工工艺和焊接技术,最大限度控制焊接变形,最终点位偏差优于1.5 cm.提出基于设计坐标系建立安装测量...