中国春季土壤湿度与东亚夏季风的关系

利用1981～2002年全国土壤湿度资料,利用相关分析发现东亚夏季风和河套地区及西南地区春季土壤湿度之间存在较大的正相关,利用这两个区域的春季土壤湿度定义了一个标准化春季土壤湿度指数（SMI）,结果发现：（1）SMI和东亚夏季风的强弱相关较好。高指数年东亚季风区低空西南夏季风气流和高层东风气流明显偏强,表明这一年夏季风偏强,低指数年则相反;（2）强SMI年,西太平洋副热带高压位置偏北,强度偏弱,西风扰动带偏北,有利于夏季风北推,不利于北方冷空气南下与之交汇,使得锋区偏北,位于华北、东北地区。弱SMI年则反之;（3）SMI能够较好地反映东部地区夏季降水,在强SMI年,长江流域降水明显偏少,而华北和河套地区的降水明显增多,而弱SMI年正好相反,这与东亚夏季风降水的环流形势也较为吻合（;4）SMI指数存在明显的4～6年和准2年的周期振荡,但其振幅和周期又有明显的周期变化。在对东亚夏季风强度的预报能力上,负的SMI对弱东亚夏季风的预报能力要强于正SMI对强东亚夏季风的预报能力。     

Hafnium Isotope and Trace Element Constraints on the Nature of Mantle Heterogeneity beneath the Central Southwest Indian Ridge (13{degrees}E to 47{degrees}E)

Hafnium isotope and incompatible trace element data are presentedfor a suite of mid-ocean ridge basalts (MORB) from 13 to 47°Eon the Southwest Indian Ridge (SWIR), one of the slowest spreadingand most isotopically heterogeneous mid-ocean ridges. Variationsin Nd–Hf isotope compositions and Lu/Hf ratios clearlydistinguish an Atlantic–Pacific-type MORB source, presentwest of 26°E, characterized by relatively low _Hf valuesfor a given _Nd relative to the regression line through all Nd–Hfisotope data for oceanic basalts (termed the ‘Nd–Hfmantle array line’; the deviation from this line is termed_Hf) and low Lu/Hf ratios, from an Indian Ocean-type MORB signature,present east of 32°E, characterized by relatively high _Hfvalues and Lu/Hf ratios. Additionally, two localized, isotopicallyanomalous areas, at 13–15°E and 39–41°E,are characterized by distinctly low negative and high positive_Hf values, respectively. The low _Hf MORB from 13 to 15°Eappear to reflect contamination by HIMU-type mantle from thenearby Bouvet mantle plume, whereas the trace element and isotopiccompositions of MORB from 39 to 41°E are most consistentwith contamination by metasomatized Archean continental lithosphericmantle. Relatively small source-melt fractionation of Lu/Hfrelative to Sm/Nd, compared with MORB from faster-spreadingridges, argues against a significant role for garnet pyroxenitein the generation of most central SWIR MORB. Correlations between_Hf and Sr and Pb isotopic and trace element ratios clearly delineatea high-_Hf ‘Indian Ocean mantle component’ that canexplain the isotope composition of most Indian Ocean MORB asmixtures between this component and a heterogeneous Atlantic–Pacific-typeMORB source. The Hf, Nd and Sr isotope compositions of IndianOcean MORB appear to be most consistent with the hypothesisthat this component represents fragments of subduction-modifiedlithospheric mantle beneath Proterozoic orogenic belts thatfoundered into the nascent Indian Ocean upper mantle duringthe Mesozoic breakup of Gondwana. KEY WORDS: mid-ocean ridge basalt; isotopes; incompatible elements; Indian Ocean     

基于表格的通用管理信息系统的设计

作者提出了一种表格式通用管理信息系统的设计方案,介绍了系统的设计思想、主要工作流程、系统各组件的功能、作用及相互关系等还详细介绍了系统主要数据库的设计。     

水对三峡库区滑带（体）土直剪强度参数的弱化规律研究

通过对三峡库区典型滑带不同状态的原位直剪对比试验,研究了粘土、粉质粘土及土石混合体三类滑带（体）土在不同含水状态下的直剪强度参数及c,φ值随含水率的变化规律。在大量的数据基础上建立了滑带（体）土c,φ值与含水率之间的经验关系,分析了水对不同性质的滑带（体）土的作用机理,得出了蓄水或者含水率变化后滑带（体）土c,φ值的经验公式,量化了含水率变化（水位涨落）对直剪强度参数的弱化程度。     

面向粮情检测数据的可视化研究与应用

现阶段的粮仓检测数据以表格、图片或者文字描述为主,可视化程度较低,缺乏对粮情信息的直观立体表达.为了解决当前存在的数据表达形式单一,直观性不强等问题,将温度传感器检测到的温度数值和激光扫描仪获取的散点空间坐标进行数据处理与分析,利用三维可视化的方法,使用开源的Web端可视化引擎,将检测的粮情数据生成浏览器端的三维模型.通过Web端建立的粮仓三维可视化模型,不仅提高了粮情信息的可视化程度,并且方便仓储管理人员实时监测仓库粮情的动态变化情况.     

基于PPK的龙口水位测量及自适应提取方法研究

在系统分析龙口水域水文特点的基础上,基于GPS PPK测量技术,设计并研制出了浮球漂流水位连续测量系统。对系统测量数据的处理方法进行了详细研究。将该系统及数据处理算法应用于龙口水域截流区的连续水位测量和提取中,取得了理想的效果。     

水电项目对越南硒圣河地区社会经济发展及环境保护的影响

硒圣河是湄公河的主要分支之一,其集水区地形条件和水资源量均对水电开发十分有利。此外,无论从物种多样性还是生物量来看,硒圣河水生生物资源非常丰富。鱼类是当地人们的重要食物来源,粗略估计鱼类物种数量可能在200-300种之间,目前具有详细记录的鱼类大约为120种。截至目前,从越南境内硒圣河上游至越-柬边界总共开发了6个水电项目,兴建了一座4A级硒圣调蓄水库。流经柬埔寨的硒圣河部分,依据发展规划将兴建3座水电站,即硒圣5号电站（硒圣1号电站以下）、硒圣3号电站、硒圣2号电站。硒圣河水电项目对区域（越南和柬埔寨）社会经济的影响体现在：为地处偏远和困难的集水区创造了新的能源资源,改善了交通系统和农村地区的生活条件。与此同时,这些水电项目也对该区域自然环境产生了重大影响。例如,改变了下游流动机理变化,导致下游河道淤积,对沿河生态系统也产生了一定影响。     

A Statistical Analysis of X1- and X2- or Higher-Class Flares during Solar Cycles 21∼23

The X1- and X2- or higher class ?ares in solar cycles 21, 22, and 23 from 1986 to 2008 have been analyzed statistically in this paper. It is found in the statistical study that the number of the X1-class ?ares accounted for 52.71% of total X- and higher class ?ares, while, the number of the X2- and higher class ?ares accounted for 47.29% of total X- and higher class ?ares. No matter whether the X1- and X2- or higher class ?ares, most of them occured in the descending phases of the solar cycles. Moreover, the weaker the intensity of the solar cycle, the higher the ratio of the ?ares occurred in the descending phase of the solar cycle, and the stronger the intensity of solar ?ares, the higher the ratio of the ?ares occurred in the descending phases of the solar cycles. In addition, the phase difference between the peak of the smoothed monthly mean number of sunspots and that of the X-class ?ares has been calculated, which shows that the smoothed monthly mean number of the X1-class ?ares had a very noticeable time advance of 1 month with respect to that of sunspots in the cycles 21 and 22, but there was a time lag of 13 months in the cycle 23, while, for the X2- and higher class ?ares, there was a time lag of 9 months in the cycle 21, but a one-month time advance existed in the cycle 22, and again a time lag of 32 months appeared in the cycle 23.