The FAST/SKA site selection in Guizhou province

Many karst depressions with diameters of 300 m to 500 m, suitable for constructing Arecibo-style radio telescopes, were identified in the south of Guizhou Province by Remote Sensing (RS) and Geographic Information System (GIS) technologies together with field investigations. Fundamental topography and landform databases were established for 391candidate depressions, and using GIS the3-dimensional images of depressions, at a scale of 1:10000, were then simulated to fit a spherical antenna. This revised version was published online in July 2006 with corrections to the Cover Date.     

浅析宁波盆地膏盐地层的时代──兼对“宁波盆地北部的长河群”之时代质疑

宁波盆地地下揭示的一套包含暗色膏硝质泥岩、泥质白云岩在内的紫红、灰紫色泥岩、棕褐色砂砾岩、细砂岩和玻屑凝灰岩的地层，均称方岩组，内含膏盐并具油色显示。对其时代有早、晚白垩世和早第三纪之认识，笔者从70～90年代地质工作中所获化石分析认为，虽然宁波盆地这一层位含化石不丰，但从分布及数量上比较，相对占优势的应该是孢粉和植物化石，其时代意见也较为一致，指示为早白垩世。     

Some Problems with Slow Rotation of CP Stars

Some difficulties in explaining the slow rotation of CP stars are discussed. The most likely hypotheses are (1) a loss of angular momentum involving a magnetic field during “pre-main sequence” evolution and (2) the slow rotation existed from the very start of the creation of these stars. The braking hypothesis is supported by only one property of CP stars— the lower the mass of the star is, the greater the difference between its average rotation velocity vsini and that of normal stars. On the other hand, there is another property— the lower the rotation speeds of CP stars are, the greater their fraction among normal stars. The latter property supports the hypothesis that the lower the initial rotation speed of a star is when it is created, the greater the probability will become chemically peculiar. This property is inherent in chemically peculiar stars both with and without a magnetic field. It is proposed that the cause of the slow rotation of CP stars must be sought in the very earliest phases of their formation, as should the cause of the separation into chemically peculiar magnetic, chemically peculiar nonmagnetic, and normal stars.__________Translated from Astrofizika, Vol. 48, No. 2, pp. 229–245 (May 2005).     

MERLIN Images of Five Compact Symmetric Object Candidates at 1.6 GHz

1 INTRODUCTIONCompact Symmetric Objects (CSOs) are powerful and compact sources (overall size <1 bpc) with lobe emission on both sides of the central engine. The small size of these sourcesis almost certainly to be attributed to the youth of the sources themselves (ages < 104 yr) andnot due to a dense coallning medium (Readhead 1996). The unification scenario assumes thatCSOs evolve into compact steep spectrum (CSS) sotirces and then into Fanaroff-Riley type 11objects (Fanti 1995). …     

基于AHP法和灰色模式识别理论的海底管道系统路由定量风险评估

根据海底管道路由潜在风险的特点及风险类型,提出了一种将层次分析法（AHP法）和灰色模式识别理论相结合的海底管道系统路由定量风险评估方法,该方法利用AHP确定风险评价指标体系,运用灰色模式识别理论,建立识别结果标准,并结合实际工程进行计算,计算结果表明该方法是可行的.     

二维动画地图表示方法的研究与应用

本文根据动画地图表示内容和常用动画技术的特点,对二维动画地图的表示方法进行了探讨。归纳了基于空间分布特征的表示方法、基于动画地图用途的表示方法和基于动画技术的表示方法及其分类,并讨论了影响选择表示方法的因素和几种表示方法相互配合的应用规律,对动画地图可视化的理论与技术的研究有一定参考。     

基础电子地图显示的关键技术

电子地图在走向产业化、实用化的过程中,人们越来越感到电子地图的显示所产生的问题不能被忽视。目前,对电子地图显示缺少系统的研究,特别是从理论、技术和实际应用层面相结合的研究还比较少见。因此,在分析基础电子地图显示存在问题的基础上,以地图制图理论为指导,研究了基础电子地图的显示特点,提出了基础电子地图显示研究的理论框架,并针对基础电子地图自适应变焦显示、可视化表达以及显示风格转换系统的研制等关键问题进行了探讨和实践。     

Galileo开放服务导航电文特点分析

介绍了Galileo系统开放服务接口控制文件中导航信号及电文的概况,并在如何满足导航电文中各种不同参数数据的时效性、如何缩短用户接收机导航数据接收时间、如何支持多系统互操作等方面对其特点进行了分析介绍。     

250kaB.P.以来西太平洋暖池中心区——Ontong Java海台古生产力演化

多年平均表层水温超过28℃的"西太平洋暖池",是全球海平面高度的加热中心和大气三大环流的辐散中心。为评价西太平洋暖池中心区域海洋生物泵的演化特征、规律与机制,本文以位于热带西太平洋暖池核心区——Ontong Java海台的WP7柱状样为材料,通过提取浮游有孔虫^δ13C组成、底栖有孔虫群落和钙质超微化石下透光带属种Florisphaera profunda相对百分含量变化等指标,反演该区250kaB.P.以来的古生产力的演化历史。研究结果表明,250kaB.P.以来西太平洋暖池中心区的古生产力演化与地球轨道变化控制的冰期-间冰期旋回以及岁差控制的太阳辐照率密切相关。在冰期-间冰期尺度上,西太平洋暖池中心区距今250ka以来的生产力变化间冰期明显低于冰期,而且在间冰期阶段生产力相对稳定,冰期波动幅度较大。在冰期或间冰期背景下显著的岁差周期是该区古生产力演化的又一重要特征。而且在岁差波段生物生产力的变化可能领先极地冰体积变化2～4ka左右。热带东西太平洋的古生产力演化在冰期-间冰期变化和岁差尺度上存在ENSO式的变动机制,而且二者互相调谐,产生了似30ka和19ka周期,并出现了"半30ka周期"和半岁差周期。此外,WP7孔Neogloboqudrina dutertrei的^δ13C显示在MIS 1/2,MIS 3/4和MIS 5e/6的冰期向间冰期的过渡期的冰消期阶段存在变轻事件,可能与数千年尺度的大洋环流演化有关。