复杂储层识别的地震反演方法及其在塔木察格盆地的应用

随着油气藏勘探开发程度的加深,准确识别复杂储层变得愈发重要,地震反演已成为储层预测的核心技术.本文对蒙占国塔木察格盆地南部凹陷1 800 km²地震资料进行波阻抗反演研究,研究工作包括测井曲线的标准化校正、地质框架模型的准确建立及其它反演参数的正确选取.波阻抗反演结果为研究沉积相划分、砂体空问展布的认识提供了可靠依据,在一定程度上解决了该区主要日的层南屯组沉积物源多、相变快和在地震剖面上无法追踪的问题.     

海拉尔盆地上库力组重矿物组合特征

海拉尔盆地兴安岭群上库力组自下而上可分出5个重矿物组合：磁黄铁矿-锆石-白钛石-锐钛矿组合,黄铁矿高含量组合,黑云母-白钛石-锆石-钛铁矿组合,菱铁矿-白钛石-黑云母-电气石组合,白钛石-黑云母-菱铁矿-石榴子石组合.不稳定矿物含量高,不同层段呈现高低韵律性变化则与火山-沉积作用强弱交替变化的环境有关.较高的ATi指数反映母岩应为中-酸性火山岩.ZTR指数不高说明重矿物的成熟度较低.由下至上陆源重矿物变少,尤其是上库力组D段（凝灰岩段）,自生黄铁矿占很高的百分比.     

叶面积指数的快速测定方法——植被定量遥感的地面标定技术

本文论述了用“底视法”测量叶面积指数的基本原理,并在中国科学院禹城综合试验站遥感试验场以“冠层分析仪”对该方法进行了试验,提出了刺柏针叶叶面积指数的新估算方法。通过计算证明,测定值和估算值具有较好的一致性。这种以“底视法”为基础的冠层分析仪可以用于植被定量遥感的快速地面定标。     

空间决策支持系统及其支撑软件的设计与应用

本文讨论了SDSS的概念和基本理论,以决策支持为目标,面向半结构化和非结构化问题,用模型驱动的SDSS,是GIS未来的发展方向。在技术上用C语言实现了SDSS支撑软件的设计,并应用于国家科技攻关课题“三川河流域区域治理与开发信息系统”,取得了良好效果;同时对SDSS开发中存在问题作了讨论。     

Comparison of Line-of-Sight Magnetograms Taken by the Solar Dynamics Observatory/Helioseismic and Magnetic Imager and Solar and Heliospheric Observatory/Michelson Doppler Imager

We compare line-of-sight magnetograms from the Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics Observatory (SDO) and the Michelson Doppler Imager (MDI) onboard the Solar and Heliospheric Observatory (SOHO). The line-of-sight magnetic signal inferred from the calibrated MDI data is greater than that derived from the HMI data by a factor of 1.40. This factor varies somewhat with center-to-limb distance. An upper bound to the random noise for the 1′′ resolution HMI 720-second magnetograms is 6.3 Mx?cm^?2, and 10.2 Mx?cm^?2 for the 45-second magnetograms. Virtually no p-mode leakage is seen in the HMI magnetograms, but it is significant in the MDI magnetograms. 12-hour and 24-hour periodicities are detected in strong fields in the HMI magnetograms. The newly calibrated MDI full-disk magnetograms have been corrected for the zero-point offset and underestimation of the flux density. The noise is 26.4 Mx?cm^?2 for the MDI one-minute full-disk magnetograms and 16.2 Mx?cm^?2 for the five-minute full-disk magnetograms observed with four-arcsecond resolution. The variation of the noise over the Sun’s disk found in MDI magnetograms is likely due to the different optical distortions in the left- and right-circular analyzers, which allows the granulation and p-mode to leak in as noise. Saturation sometimes seen in sunspot umbrae in MDI magnetograms is caused by the low intensity and the limitation of the onboard computation. The noise in the HMI and MDI line-of-sight magnetic-field synoptic charts appears to be fairly uniform over the entire map. The noise is 2.3 Mx?cm^?2 for HMI charts and 5.0 Mx?cm^?2 for MDI charts. No evident periodicity is found in the HMI synoptic charts.     

Simulation of Lake-Groundwater Interaction under Steady-State Flow

MODFLOW is one of the most popular groundwater simulation tools available; however, the development of lake modules that can be coupled with MODFLOW is lacking apart from the LAK3 package. This study proposes a new approach for simulating lake - groundwater interaction under steady-state flow, referred to as the sloping lakebed method (SLM). In this new approach, discretization of the lakebed in the vertical direction is independent of the spatial discretization of the aquifer system, which can potentially solve the problem that the lake and groundwater are usually simulated at different scales. The lakebed is generalized by a slant at the bottom of each lake grid cell, which can be classified as fully submerged, dry, and partly submerged. The SLM method accounts for all lake sources and sinks, establishing a governing equation that can be solved using Newton's method. A benchmarking case study was conducted using a modified model setup in the LAK3 user manual. It was found that when there is a sufficient number of layers at the top of the groundwater model, SLM simulates an almost identical groundwater head as the LAK3-based model; when the number of layers decreases, SLM is unaffected while LAK3 may be at a risk of giving unrealistic results. Additionally, the SLM can reflect the relationship between the simulated lake surface area and lake water depth more accurately. Therefore, the SLM method is a promising alternative to the LAK3 package when simulating lake - groundwater interaction.     

Vertical concentration profile of nonuniform sediment

A new formula for the concentration profile of nonuniform sediment is derived using the diffusion differential equation with equilibrium bed concentration.The interaction coefficient for nonuniform sediment particles as a function of both relative diameter and geometric standard deviation of nonuniform sediment is taken into account in the settling velocity.The diffusion coefficient is obtained from the logarithmic velocity profile.This new formula possesses several advantages as follows:(1)avoids theoretical defect of the Rouse formula,which states that the sediment concentration is infinite at the bottom and zero at the water surface.(2)suitable for an arbitrary fraction of nonuniform sediment,and(3)easy to apply with a simple form.The formula yields less difference among concentration profiles for various particles than that for uniform sediment and reveals the lawfor fractional concentration distribution of nonuniform sediment.The calculated concentration agrees well with the measured data from the Yangtze River.     

Impacts of coastal reclamation on tidal and sediment dynamics in the Rui’an coast of China

Ocean Dynamics - Coastal reclamation projects have been extensively constructed along the coastline of the East China Sea over the past decades. To investigate the impact of reclamations on the...     

西安市地裂缝地震效应的理论分析

本文采用有限元方法对西安市地裂缝的地震效应进行了分析,其目的在于探索强震时地裂缝对地面运动的影响。所用方法的理论基础是在双向地震动的作用下求解多质点体系的强迫振动方程组。[M]{(?)}+[C](?)}+[K]{X}=[M]({A_x}(?)。(t)+{A_y}(?)。(t))。式中[M]、[C]、[K]分别为体系的质量、阻尼、刚度矩阵,{x}、{x}、{x}分别为体系自由度的加速度、速度、位移向量,{A_x}、{A_y}为水平和垂直方向的自由度向量,(?)。(t)、(?)。(t)为水平及垂直方向上的基岩强震加速度时程向量。分析时根据西安市地裂缝的具体情况,做了如下简化: 1.裂缝不作为发震构造,即强震时裂缝不是弹性波的发源地。强震是通过铰结支座输入进来的。2.裂缝带在模型上是一向下尖灭的楔体,楔体顶面宽10米,楔体深20米,中间有一宽1米、深2米的裂口。整个模型的土质是层状的,各层土的主要参数在现场测定。裂缝带楔体的参数不易取得,按经验强度取周围原土的一半左右。3.模型厚度为50米,输入地震为El Centro和文县强震记录,输入时将最大加速度值调整为150gal。计算结果表明,西安裂缝带在强震时对地面运动没有显著的影响,如地裂缝带内外的各种反映强震运动特征的指标几乎都没有什么差异。因为地裂缝带从区域上看毕竟是个很小的地质单元体,这样小的规模尚不足以对强震地面运动产生显著的影响。但是,地裂缝带在强震时的永久地形变却是值得注意的。从这一点上看,裂缝带内外地基失效程度必定有很大的差别,从而使裂缝上的震害加重。可见,在强震时,除地裂缝带本身因地基失效使震害加重而外,裂缝基本不对强震地面运动规律产生影响。所以在进行防震规划时,不必在常规的设防带之外再加宽防震地带。