渤海盆地辽东湾地区古近系烃源岩成熟演化模拟

古近系是辽东湾地区的主力烃源岩层系, 包括孔店组(Ek)-沙河街组四段(Es⁴)、沙河街组三段(Es³)、沙河街组一、二段(Es1-2)、东营组三段(Ed³)4套烃源岩, 它们主要分布在该地区的3个凹陷(辽西、辽中和辽东)的各个次洼中。在沉积和构造发育史的基础上, 结合烃源岩地球化学和热史等参数对烃源岩成熟演化进行模拟。对辽中凹陷各洼陷典型井区的烃源岩演化模拟表明辽中凹陷不同洼陷内各烃源岩层系的成熟演化历史存在明显差异:在东营组沉积末期,Es⁴-Ek烃源岩普遍进入生油门限,现今,基本上处于高-过成熟阶段;在馆陶组沉积末期,Es³和Es^-2烃源岩普遍进入生油门限,Ed³烃源岩部分进入生油门限,现今,Es³和Es^-2烃源岩在辽中凹陷的部分地区达到生油高峰期。同时, 利用Basinview软件模拟了辽东湾地区古近系4套烃源岩的成熟演化历史, 表明在盆地演化过程中同一套烃源岩在辽东湾地区不同凹陷进入生油门限和达到生油高峰及生气阶段的时间存在差异。研究成果可以为该地区深凹区的烃源岩预测与评价和计算烃源岩体积、生、排烃量等提供重要参数,这对指导该地区的油气资源勘探具有重要意义。      

Data Analysis of Chang’E-1 Gamma-Ray Spectrometer and Global Distribution of U, K, and Th Elemental Abundances

Gamma-ray spectrometer (GRS) is one of the main payloads on the Chang’E-1 (CE-1) lunar probe, mainly aimed to detect the elemental abundances and distributions on the lunar surface. At 03:58 on 28 November 2007, it performed the first observation of the lunar gamma rays. As of 24 October 2008, 2105?h of effective gamma rays spectra had been acquired by CE-1 GRS, which covers the whole surface of the moon. This paper mainly describes the data processing procedures and methods of deriving the elemental abundances by using the CE-1 GRS time series corrected spectra: first, to bin data into pixels for mapping; then, to perform a background deduction of the cumulative spectra and obtain a peak area of the elements; and finally, to use the elemental abundances inversion model to produce the elemental abundances. Based on these processing methods, the global abundance maps of U, K, and Th at a 5°×5° equal-area pixel are acquired by CE-1 GRS data. The paper gives a preliminary analysis of the uncertainties of the elemental abundances     

城市水环境承载能力研究

针对人类高强度活动区——城市水资源系统特点和存在的水环境问题,探讨城市水环境承载能力和水资源承载能力的概念及内涵;提出了计算城市水环境承载能力的"控制目标反推模型"(COIM模型),该模型主要包括:城市污染物排放量计算、控制断面径流量计算、控制断面水质指标计算、控制目标方程和城市水环境承载能力计算;以郑州市为应用范例,介绍城市水环境承载能力计算模型应用及水环境调控对策制定.     

利用偏光显微镜反射光系统观察黑色生油岩电子探针薄片中的生烃母质特征

鄂尔多斯盆地上三叠统延长组长7油层组的黑色泥岩、油页岩等黑色生油岩薄片中的生烃母质,因黑色石油、沥青等黑色有机质的覆盖或不透明,导致其在偏光显微镜透射光系统下观察常局部或整体呈现为黑色。因此,建立一种黑色生油岩薄片中生烃母质有效观察的方法,对致密油、页岩油的生烃研究具有重要的理论和实际意义。本文提出了一种利用电子探针薄片和偏光显微镜的反射光系统观察黑色生油岩中生烃母质特征的方法。该方法能够克服黑色生油岩薄片中生烃母质因被黑色有机质覆盖或不透明,而在偏光显微镜的透射光系统下局部或整体呈黑色的弊端,能够对生烃母质的大小、形态、结构、分布和物质成分等特征进行整体且清晰的观察。实践表明,本文提出的利用偏光显微镜反射光系统观察黑色生油岩电子探针薄片中生烃母质特征的方法,简单有效,易在致密油、页岩油的生烃研究领域推广使用。     

拉鸡山裂谷带特征及演化

拉鸡山构造带东西长逾 6 50km ,展布于由元古宇组成的结晶地块内部 ,是一条早古生代火山岩极为发育的构造带。通过作者在拉鸡山多年的野外调查工作和研究 ,认为该地区无论在区域地质学、岩石学、构造变形学还是大地构造演化方面 ,其早古生代构造演化史皆具典型的裂谷带特征。晚古生代以来 ,区内经历了陆内多阶段造山过程。新生代早更新世 ,拉鸡山巨型断裂带发生左旋走滑运动 ,导致断裂带弧形转折部位强烈崛起 ,形成雄伟高山。     

RELATIONSHIP BETWEEN SUMMER LOW-FREQUENCY RAINFALL OVER SOUTHERN CHINA AND PROPAGATION OF TROPICAL INTRASEASONAL OSCILLATION

This study investigates the relationship between summer low-frequency rainfall over southern China and tropical intraseasonal oscillation (ISO) in the atmosphere by examining systematically the propagation features of the tropical ISO in terms of focusing on five large-scale low-frequency rainfall regimes in summer over southern China. It is demonstrated that there is a close linkage between the five rainfall regimes over southern China and the northward propagation of the tropical ISO. The moist ISO signals, which influence the low-frequency rainfall events in different regions of southern China, mainly propagate northwestward from the tropical ocean to the southeast of China. The southeast China rainfall regime is intimately associated with the moist ISO signals propagating northwestward from the equatorial mid-western Pacific Ocean. For both the Yangtze River regime and South of Yangtze River regime, the moist ISO signals over the northern South China Sea show an evident northward propagation towards the Yangtze River region, and then propagate westward. It is further found that the interaction between the northward propagation of low-latitude ISO signals and the southward propagation of high-latitude ISO signals can also make a clear influence on the low-frequency rainfall in southern China. For the Southern China regime, the moist ISO signals show a significant northward propagation from the Philippines. Moreover, for the rainless regime, southern China is under dry ISO signals’ control, and the latter shows no clear propagation to southern China. This study may provide insights for the extended-range forecasting of summer rainfall in southern China.     

Identification of Convective and Stratiform Clouds Based on the Improved DBSCAN Clustering Algorithm

A convective and stratiform cloud classification method for weather radar is proposed based on the density-based spatial clustering of applications with noise (DBSCAN) algorithm. To identify convective and stratiform clouds in different developmental phases, two-dimensional (2D) and three-dimensional (3D) models are proposed by applying reflectivity factors at 0.5° and at 0.5°, 1.5°, and 2.4° elevation angles, respectively. According to the thresholds of the algorithm, which include echo intensity, the echo top height of 35 dBZ (ET), density threshold, and ε neighborhood, cloud clusters can be marked into four types: deep-convective cloud (DCC), shallow-convective cloud (SCC), hybrid convective-stratiform cloud (HCS), and stratiform cloud (SFC) types. Each cloud cluster type is further identified as a core area and boundary area, which can provide more abundant cloud structure information. The algorithm is verified using the volume scan data observed with new-generation S-band weather radars in Nanjing, Xuzhou, and Qingdao. The results show that cloud clusters can be intuitively identified as core and boundary points, which change in area continuously during the process of convective evolution, by the improved DBSCAN algorithm. Therefore, the occurrence and disappearance of convective weather can be estimated in advance by observing the changes of the classification. Because density thresholds are different and multiple elevations are utilized in the 3D model, the identified echo types and areas are dissimilar between the 2D and 3D models. The 3D model identifies larger convective and stratiform clouds than the 2D model. However, the developing convective clouds of small areas at lower heights cannot be identified with the 3D model because they are covered by thick stratiform clouds. In addition, the 3D model can avoid the influence of the melting layer and better suggest convective clouds in the developmental stage.     

辽宁中部城市群大气能见度变化趋势及影响因子分析

通过分析辽宁中部相对集中分布的5个城市群1987-2002年间的大气能见度、影响能见度的气象因子和污染物的变化特征及能见度与气象因子、污染物浓度之间的相关关系等,得到以下结论：（1）各城市能见度有明显的月、季和年际变化特征,能见度月变化呈双峰型,第一个峰值在5月份,第二个峰值在9,10月份;冬季能见度的值最低,春、秋季高;本溪市的能见度在逐年变好;沈阳的能见度从1987-1997年逐年变好,1997年以后又逐年变差;其它城市的能见度呈逐年变差的趋势。（2）各城市影响能见度的气象因子的年际变化特征基本是一致的;5个城市TSP,SO2污染浓度年均值均呈下降趋势,NOx的年际变化趋势不明显。（3）能见度与湿度、雾的相关关系都呈负相关且非常显著;与降雨量、风速及温度之间的关系比较复杂;与各种污染物的相关都呈负相关。     

LAS在西北干旱区荒漠均匀下垫面的观测研究

利用“古浪非均匀近地层观测试验”的仪器平行对比观测部分试验数据,首先分析荒漠均匀下垫面大孔径闪烁仪(Large Aperture Scintillometer,LAS)光径线上等间距架设的4台涡动相关仪(Eddy Covariance System,EC)观测的摩擦速度和感热通量的一致性.然后,基于4种不同下垫面建立稳定度普适函数分析,利用4台EC观测摩擦速度平均值,计算了LAS观测区域的感热通量,进而比较了LAS和EC两者观测值的差异.结果表明,4台EC观测的摩擦速度与感热通量一致性好,摩擦速度的差别＜10％,感热通量的差别在10％左右.4种稳定度普适函数计算的LAS区域感热通量在白天、夜晚与EC观测平均值变化趋势一致,但计算值偏大;TAG (Thiermann and Grassl)稳定度普适函数计算值与EC观测平均值较接近.其主要原因除不同下垫面试验所得稳定度普适函数的差异外,Kipp&Zonen LAS所测感热通量的系统性偏高不可忽视.     

大气环流的季节突变与季风的建立Ⅰ.基本理论方法和气候场分析

将曾庆存等提出的大气环流的季节划分和计算季风的理论方法作了改进,使之更便于研究季风的建立过程.该理论方法将环流突变和季风建立时段,其"变差度"和与其前和其后场的"相似度"等由空间场的泛函随时间的变化(即数学名词上的"流"[flow])一起求出来.研究Ⅰ先分析气候平均场,Ⅱ分析各个别年份的情况及年际变化.研究Ⅰ的结果表明:(1)该方法可以客观定量地定出"突变"时段的关键日期;与季风建立过程联系,即是季风建立的"预兆日期",它比人们用天气-气候学方法(甚至用别的气象要素)定出的可以明显感觉到的或有明显实用价值的"季风来临日期"要早2至4天.(2)在北半球亚澳季风系统区域,夏季风的来临在许多关键地区伴有明显的环流突变,建立和推进者很快,但也有许多区域不表现为当地环流的突变,推进速度也慢.(3)北半球亚澳季风系统低空的热带季风分支,在6月中以前可明确区分为3个子系统,(a)西太平洋暖池和邻近低纬区域,4月中下旬建立;(b)热带东北印度洋(北界与孟加拉湾相邻,但不包括其在内)及索马里东边海洋,4月末至5月初建立;和(c)南海区域,5月上旬从南到5月下旬到北部.南海夏季风向北推进最快,于5月末候即可达北回归线附近,然后与暖池西北区域风场的突变一起,于6月中旬影响到东亚30°N区域;印度洋季风于6月初到达印度半岛东南端,然后逐渐推向印-巴次大陆.7月中以后,热带季风才连成一片,由非洲东岸直至长江下游和菲律宾附近.副热带季风分支于6月中旬可以感到其影响,于7、8月盛行于东亚和西太平洋区域,且结构和演变都比较复杂;6～7月间只表现为在(5～20°N,120～150°E)区域有强的环流突变(与副高增强并北移对应),7月中至8月底,则在上述区域和沿30°N的长江下游和日本以南的洋面上有3个强的环流突变中心(对应于副高又一次增强北移和西伸).这里暂不讨论温寒带季风分支.(4)季风具有鲜明的三度空间斜压结构,尤其是在低空季风"爆发"之前,平流层早已有强的环流突变,季节调整完成,然后突变向下延伸(虽然强度大减),跟着就有当地的低空季风"爆发"(建立).平流层和对流层环流的相互作用及其与季风建立的关系很值得进一步研究.