N■no综合区对研究ENSO的效果评估

通过生成一个新的Ni(n)o1-4综合区,并以它的SSTA来确定El Ni(n)o事件.经过数据对比处理和指数相关分析后,论证了合成区的合理和可行性.     

非开挖管理软件的设计与开发

利用VisualBasic 6．0语言开发非开挖管理软件,选择Microsoft Office Access 2000作为软件的数据库系统。该软件从公司领导层到公司各部门到作业班组,按照管理需求对非开挖工程数据资料的操作流程进行切合实际的逻辑设计,形成施工主体技术参数、相关辅助信息和人力、物力、财力数据的有机综合管理系统。而且可以直接从窗体输入数据资料,相应的输出Excel、Word形式的数据资料,方便了工程进展情况的查看和资料的整理。软件中根据非开挖工程的要求,相对应的窗体之间创建了关联。软件可以在Windows 9X操作平台下运行,具有窗体友好、操作方便、运行可靠稳定等优点。     

六盘山群沉积物磁化率记录的早白垩世气候变化

白垩纪气候环境研究对认识现今全球环境格局的形成具有重要意义,现有的白垩纪环境变化记录均来自海洋沉积物,本文通过对我国中部六盘山地区六盘山群地层沉积与岩石磁化率测量分析,获得了128.15～115.82Ma期间陆相沉积物记录的气候变化信息。结果显示磁化率值总体较低,以125Ma为界大致可以分为前低后高两个阶段;结合岩石磁学测量及沉积相、岩石中铁含量与磁化率变化关系分析,认为岩石磁化率主要与源区磁性矿物的种类及含量有关,据此揭示六盘山地区在该时间段气候总体为干热环境,并可分为128.15～125Ma间气候相对湿热和125～115.82Ma间气候相对温湿两个阶段。磁化率记录的这种气候转变与海洋沉积物记录的全球海平面温度变化趋势一致,但相对海平面温度由升高到降低的转折时间提前约1.7Ma。     

Relationships between carbon isotope evolution and variation of microbes during the Permian–Triassic transition at Meishan Section, South China

This paper investigates kerogen carbon isotopes, the difference between carbonate and kerogen carbon isotopes (Δ¹³C_carb-kero = δ ¹³C_carb − δ ¹³C_kero) and the difference between carbonate and n-C₁₉ alkane compound-specific carbon isotopes (Δ¹³C_carb-n-C19 = δ ¹³C_carb − δ ¹³C _n-C19) during the Permian–Triassic transition at Meishan, South China. The results show that kerogen carbon isotopes underwent both gradual and sharp shifts in beds 23–25 and 26–29, respectively. The differences between carbonate and organic carbon isotopes, both the Δ¹³C_carb-kero and Δ¹³C_carb-n-C19, which are mainly affected by CO₂-fixing enzyme and pCO₂, oscillated frequently during the Permian–Triassic transition. Both the variations of Δ¹³C_carb-n-C19 and Δ¹³C_carb-kero coupled with the alternation between cyanobacteria and green sulfur bacteria indicated by biomarkers. The episodic low values of Δ¹³C_carb-n-C19 corresponded to episodic blooms of green sulfur bacteria, while the episodic high values of Δ¹³C_carb-n-C19 corresponded to episodic blooms of cyanobacteria. The relationships between the variation of carbon isotopes and biota show that the microbes which flourished after the extinction of macroorganism affected the carbon isotope fractionation greatly. Combining the carbon isotope compositions and the pattern of size variation of the conodont Neogondolella, this paper supposes that anoxia of the photic zone at bed 24 was episodic and it would be caused by the degradation of terrigenous organic matters by sulfate reducing bacteria in the upper water column. Considered together with results from previous research, the high resolution variation of the biogeochemistry presents the sequence of the important geo-events during the Permian–Triassic crisis.     

基于GIS的雷电灾害监测预警与数据处理系统

针对雷电灾害涉及的关键问题,基于ArcEngine开发平台,结合大型网络数据库sqlServer2005与空间数据库模型GeoIataBase,设计了具有3层逻辑结构的系统构架方案,构建了基于GIS的雷电监测预警与数据处理系统。该系统有效地将各种雷电数据与GIS平台进行无缝对接,并整合雷电预测模式,实现各种雷电数据基于GIS的实时监测处理与预测预警以及高效组织、存储与管理,满足各种雷电信息查询处理分析的需求;为气象部门对雷电灾害天气的监测、预报预警以及各种数据基于地理信息的处理分析等提供了有效的可视化平台,同时也为GIS与气象专业领域的结合进行了有益的探索。     

从2009年度Nature杂志看气候变化研究进展

<正>英国Nature杂志是世界著名的自然科学类综合学术期刊,代表着自然科学各门学科的最前沿研究动态。在大气科学及相关领域研究中,气候变化一直是Nature杂志最关心的内容。随着气候变化加剧、社会瞩目度的不断上     

广西龙州地区双层含铝岩系地质特征与找矿意义

对龙州地区合山组和都安组铝土岩（矿）层进行系统采样分析，并与堆积铝土矿进行对比研究，结合含铝岩系岩性与矿物特征发现，合山组、都安组铝土岩（矿）矿石矿物无显著差异，主要为一水硬铝石、高岭石、（鲕）绿泥石，其次为赤铁矿（针铁矿）集合体和碎屑物（岩屑、玻屑、砾屑），普遍存在大量（铁）凝胶。常量、微量、稀土元素特征及相关图解显示，合山组、都安组铝土岩（矿）均可能为该区堆积铝土矿的矿源层。Ni-Cr图解显示合山组铝土岩（矿）可能来自与火山物质有关的玄武岩，都安组铝土岩（矿）来源于卡斯特岩溶，堆积铝土矿除部分落入玄武岩、碳酸盐岩区以外，大多位于页岩、板岩内，表明该区堆积铝土矿存在多源性。微量元素Be、Ga、Sr、Ba含量与Sr/Ba、V/Zr、Zr/Cu含量比值等沉积环境元素特征表明该区原生铝土岩（矿）沉积环境为陆相；δCe分析显示铝土岩（矿）沉积环境有所差异，合山组表现为氧化环境，都安组则表现为还原环境。Th、U含量及Th/U含量比值显示该区铝土岩（矿）成矿以混合作用为主，并经历了较强的风化作用；δEu分析表明合山组、都安组铝土岩（矿）分别形成于被动大陆边缘与活动大陆边缘。合山组、都安组含铝岩系均发育不同程度的铝土岩（矿）层，都安组铝土岩（矿）部分样品已达工业边界指标，可作为沉积铝土矿勘查的主要目的层。     

The color properties of compact groups of main galaxies from the SDSS Data Release 4

In order to compare color statistical properties of member galaxies in compact groups with those of field galaxies, we use a compact group (CG) sample which contains 4217 CGs extracted from the MAIN galaxy sample of the SDSS Data Release 4 (SDSS4), and construct a random group sample which has the same distributions of redshift and number of member galaxies as those of the CG sample. It turns out that the mean colors of galaxies in CGs are redder than those of galaxies in random groups. Additionally, we also find that member galaxies in real CGs have a smaller dispersion of colors than those in random groups-at least for g-r, r-i, and i-z colors. Published in Astrofizika, Vol. 50, No. 1, pp. 29–37 (February 2007).     

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