大瑞铁路高黎贡山越岭段主要工程地质问题与地质选线

在野外地质调查、钻探、地应力测量和室内测试分析的基础上,对大瑞铁路高黎贡山越岭段规划设计中可能遇到的高地温、高地应力、活动断裂断错、岩爆、涌水突泥、软岩大变形和边坡稳定性等主要工程地质问题进行了论述,认为高地温和热害是制约高黎贡山深埋隧道段建设的关键因素。根据地热钻探、测试资料分析,该区的地热分布受断裂构造控制明显,黄草坝断裂具有阻水隔热的工程地质特性。对比分析认为,C12K方案(34.5 km越岭长隧道方案)位于黄草坝阻水隔热断层之南,通道内相对低温,且在隧道口处避让了古滑坡等不利工程地质问题,在众多比选方案中工程地质条件较好。调查研究结果对大瑞铁路全线贯通具有重要意义。     

元胞自动机和克隆选择算法的蓝藻水华预测模型

针对蓝藻水华频发影响水体质量和生态环境的问题,该文以太湖为例,探讨了元胞自动机和克隆选择算法在蓝藻水华预测方面的可行性。使用遥感经验算法计算水体叶绿素a浓度;将叶绿素a浓度分布数据作为预测模型的输入数据,将基于平衡方程的预报模型与元胞自动机进行耦合,对蓝藻水华时空变化过程进行了动态模拟;在预测方面实现了蓝藻水华空间分布情况的可视化,并采用克隆选择算法优化了预测模型中的重要参数。研究结果表明:利用克隆选择算法优化的元胞自动机模型能够在蓝藻水华预测中直观地显示蓝藻水华的时空变化特征;能够在短时间内重复性地预演蓝藻水华的变化过程,为决策者提供有用的参考。     

Household level influences on fragmentation in an African park landscape

The process of landscape fragmentation outside park borders occurs through the actions of people living near the boundaries. In the Kibale National Park landscape in western Uganda, human-landscape relationships are typified by small-scale subsistence agriculture, in which households rely on resources provided in forests and wetlands, whose use is in turn shaped by perceptions of resource availability. To understand and manage for fragmentation of resource pools, modeling and identifying the proximate drivers, and thus enacted resource extraction and utilization – is of fundamental importance. We combine landscape analysis at the household scale, using remotely sensed data, with household surveys, to understand the potential human drivers of local scale landscape change. We found strong evidence for a local household zone (LHZ) effect on fragmentation patterns with geographical and socioecological heterogeneities in LHZ impact. Differences were influenced by wealth, and in some cases, tribal identity. The perception of crop raiders – primarily baboons and small monkeys, but also elephants and other animals – may have largely shaped human-environment interactions, and were associated with fragmentation. Ninety-two percent of the best fit models included the attitude that the park should stay, but associated it with increased fragmentation, suggesting that the uncharacteristic non-hostile attitude about Kibale does not directly translate into conservation-friendly local human-environment interactions. This study provides insight into park–neighbor interactions and the influence of the LHZ on protected-area landscapes, and it points to important points in the system for collaborative opportunities to engage communities and conservation managers.     

A discrete spatial choice model of burglary target selection at the house-level

This article studies how burglars select a house to burglarize. We draw on the rational choice perspective to investigate how burglars select a target by relying on house-related attributes to optimize a combination of perceived rewards, efforts and risk. It extends current applications of the discrete spatial choice framework to burglary target selection by adopting the house as the spatial unit of analysis and studies burglars' target selection process in a larger and more diverse study area than that of earlier studies. Using data on 650 residential burglaries and on approximately 500,000 residential properties in the Belgian province East Flanders, we consider a discrete spatial choice model of burglary target selection to establish which house-related attributes influence burglars' target selection process. Our findings demonstrate that terraced houses, houses without a garage, houses that have not been outfitted with a central heating and/or air-conditioning system and houses nearby burglars' residences are more likely to be selected. Overall, our analysis suggests that burglars rely on effort-related attributes to distinguish between targets while higher perceived rewards actually decrease the odds of a house being burglarized. Risk-related attributes are unimportant for burglars' target choice.     

Clinoform geometry,geomorphology, facies character and stratigraphic architecture of a sand‐rich subaqueous delta: Jurassic Sognefjord Formation,offshore Norway

The integration of core sedimentology, seismic stratigraphy and seismic geomorphology has enabled interpretation of delta‐scale (i.e. tens of metres high) subaqueous clinoforms in the upper Jurassic Sognefjord Formation of the Troll Field. Mud‐prone subaqueous deltas characterized by a compound clinoform morphology and sandy delta‐scale subaqueous clinoforms are common in recent tide‐influenced, wave‐influenced and current‐influenced settings, but ancient examples are virtually unknown. The data presented help to fully comprehend the criteria for the recognition of other ancient delta‐scale subaqueous clinoforms, as well as refining the depositional model of the reservoir in the super‐giant Troll hydrocarbon field. Two 10 to 60 m thick, overall coarsening‐upward packages are distinguished in the lower Sognefjord Formation. Progressively higher energy, wave‐dominated or current‐dominated facies occur from the base to the top of each package. Each package corresponds to a set of seismically resolved, westerly dipping clinoforms, the bounding surfaces of which form the seismic ‘envelope’ of a clinoform set and the major marine flooding surfaces recognized in cores. The packages thicken westwards, until they reach a maximum where the clinoform ‘envelope’ rolls over to define a topset–foreset–toeset geometry. All clinoforms are consistently oriented sub‐parallel to the edge of the Horda Platform (N005–N030). In the eastern half of the field, individual foresets are relatively gently dipping (1° to 6°) and bound thin (10 to 30 m) clinothems. Core data indicate that these proximal clinothems are dominated by fine‐grained, hummocky cross‐stratified sandstones. Towards the west, clinoforms gradually become steeper (5° to 14°) and bound thicker (15 to 60 m) clinothems that comprise medium‐grained, cross‐bedded sandstones. Topsets are consistently well‐developed, except in the westernmost area. No seismic or sedimentological evidence of subaerial exposure is observed. Deposition created fully subaqueous, near‐linear clinoforms that prograded westwards across the Horda Platform. Subaqueous clinoforms were probably fed by a river outlet in the north‐east and sculpted by the action of currents sub‐parallel to the clinoform strike.     

新疆克拉玛依油田一中区克拉玛依组辫状河储层砂体类型及分布特征

通过露头实测、岩心观察及测录井资料分析等结果表明,克拉玛依油田一中区克拉玛依组S7、S5和S4砂层组沉积时期以发育辫状河为特征,可进一步划分为近源砾质辫状河、远源砾质辫状河和砂质辫状河沉积3种类型。上述3种类型的辫状河沉积在沉积特征、河道空间叠置样式及组合关系等方面存在明显的差异。近源砾质辫状河河道岩性以砾岩为主,为中孔低渗储层。单河道沉积厚度2~4.5m,宽度500~800m,表现为河道-河道直接接触的连片组合方式;远源砾质辫状河河道岩性仍以砾岩为主,含少量砂岩,物性较近源砾质辫状河略好,为中孔低渗储层。单河道沉积厚度为1.5~4m,河道砂体宽度400~750m,表现为河道-溢岸-河道的连片组合方式;砂质辫状河河道岩性以砂岩为主,为中孔低渗储层,物性优于砾质辫状河。单层厚度为0.5~2.5m,宽度为300~700m,但河道沉积分布范围有限,河道之间多为带状或交织带状组合方式。根据上述对比分析认为砾质辫状河河道砂体虽然物性相对较差、非均质性较强,但砂体厚度大、分布广泛、连通性好,目前为全区主要油气开发的目的层;砂质辫状河河道砂体尽管物性较好,但由于厚度较薄,分布局限,仅在东部地区其累计厚度较大,当与其它成藏条件匹配时,可形成具有开发潜力的目的层。     

深部细粒碎屑岩储层成岩作用研究——以苏北盆地张家垛油田阜三段为例

毗邻烃源岩的细粒储层,由于其岩石结构、组分及沉积环境的特殊性,成岩作用表现出一定差异。本文以张家垛油田阜三段细粒碎屑岩储层为例,通过铸体薄片、X射线衍射、扫描电镜等相关分析,研究其成岩作用的特殊性。研究结果表明:(1)细粒储层的成分成熟度和结构成熟度较高,常被泥岩包裹,在压实作用中若存在欠压实,粒间孔可以被很好地保留下来;(2)细粒储层形成时水动力较弱,杂基含量高导致微孔较多;(3)大量的粘土矿物使孔隙比表面增加,抑制了后期硅质和碳酸盐胶结物的析出;(4)比表面的增加减缓了孔隙流体的对流速率和扩散速率,不利于次生孔隙的形成,粒度越细,次生孔隙越不发育。细粒碎屑岩储层有别于常规储层,对其特殊的成岩作用进行研究具有重要的理论价值和实际意义。     

A Method for Determining Sedimentary Micro-Facies Belts Automatically

It is important to understand the distribution of sedimentary facies, especially the distribution of sand body that is the key for oil production and exploration. The secondary oil recovery requires analyzing a great deal of data accumulated within decades of oil field development. At many cases sedimentary micro-facies maps need to be reconstructed and redrawn frequently, which is time-consuming and heavy. This paper presents an integrated approach for determining the distribution of sedimentary micro-facies, tracing the micro-facies boundary, and drawing the map of sedimentary micro-facies belts automatically by computer technique. The approach is based on the division and correlation of strata of multiple wells as well as analysis of sedimentary facies. The approach includes transform, gridding, interpolation, superposing, searching boundary and drawing the map of sedimentary facies belts, and employs the spatial interpolation method and "worm" interpolation method to determine the distribution of sedimentary micro-facies including sand ribbon and/or sand blanket. The computer software developed on the basis of the above principle provides a tool for quick visualization and understanding the distribution of sedimentary micro-facies and reservoir. Satisfied results have been achieveed by applying the technique to the Putaohua Oil Field in Songliao Basin, China.     

MIXTURE ANGLYSIS USING FACTOR ANGLYSIS I: CALIBRATION AND QUANTITATION

One of the major application areas of factor analysis, multivariate calibration and quantitation, is coveredin this review. The algorithms, methodologies and applications covered include principal componentregression, target transformation factor analysis, singular value decomposition and rank annihilationfactor analysis. Many important areas of research having relevance to multivariate calibration andquantitation problems are also covered in this review, including background correction, measurementerror, rank determination, cross-validation, figures of merit, detection of invalid samples, experimentaldesign, sample selection, statistical inference and wavelength selection.     

Models of the formation of the solar nebula

Models of the collapse of a protostellar cloud and the formation of the solar nebula reveal that the size of the nebula produced will be the larger of $\text{R}{}_{\mathrm{<mtext>CF</mtext>}}\text{≡ J}{}^2\text{/k}{}^2\text{GM}{}^3\text{and}\text{R}{}_{\mathrm{<mtext>V</mtext>}}\text{≡ (GMv/2c}{}_{\mathrm{<mtext>c</mtext>}}{}^3\text{)}\text{1}\text{2}$ (where J, M, and c_s are the total angular momentum, total mass, and sound speed of the protosetellar material; G is the gravitational constant; k is a number of order unity; and v is the effective viscosity in the nebula). From this result it can be deduced that low-mass nebulas are produced if P ≡ (R_V/R_CF)² ? 1; “massive” nebulas result if P ? 1. Gravitational instabilities are expected to be important for the evolution of P ? 1 nebulas. The value of J distinguishes most current models of the solar nebula, since P ∝ J^?4. Analytic expressions for the surface density, nebular mass flux, and photospheric temperature distributions during the formation stage are presented for some simple models that illustrate the general properties of growing protostellar disks. It does not yet seem possible to rule out either P ? 1 or P < 1 for the solar nebula, but observed or possible heterogeneities in composition and angular-momentum orientation favor P < 1 models.