首页> 外文会议>GCAGS 2012 >Geologic Evaluation of Regional Production Trends in the Upper Cretaceous Austin Chalk
【24h】

Geologic Evaluation of Regional Production Trends in the Upper Cretaceous Austin Chalk

机译:地白垩纪奥斯汀粉笔区域生产趋势的地质评价

获取原文

摘要

The Upper Cretaceous Austin Chalk, which extends across Texas and Louisiana, is characterized by reservoirs that produce oil,gas, and in some cases, anomalously large amounts of water. Reservoirs typically have low matrix permeability and contain natural fractures. Horizontal drilling has been used to enhance and connect these fracture systems to drain the reservoir more effectively. Although the formation contains continuous (unconventional) reservoirs, it behaves as a hybrid system, wherein varied geologic settings yield both continuous and conventional accumulations. Well data indicate that the primary Austin Chalk production trend is parallel to and just updip of the underlying Lower Cretaceous shelf edge. This trend includes Giddings and Pearsall fields, and smaller geologically similar fields. Recent drilling has expanded this belt eastward into Louisiana, as well as downdip of the paleoshelf edge; this new region of production has proved successful and includes significant fields such as Brookeland and Masters Creek. The Austin Chalk is classified as a biomicrite according to Folk (1959); it is comprised primarily of coccoliths (Dravis, 1979). This low-permeability, low-porosity rock requires large connected fracture systems to store and produce hydrocarbons. Most of the large-scale fractures are parallel to regional strike with few dip-oriented fractures (Haymond, 1991). This one-dimensional fracture network requires many smaller,localized fractures to maintain fluid flow in the reservoir. The clay component of the formation also affects fracture intensity and connectivity (Corbet et aL, 1987; Haymond, 1991). The Austin Chalk is a low-porosity, low-permeability carbonate with a dual pore system comprised of a microporous matrix and a moderately interconnected fracture system (Dawson et al., 1995). Micropores range in size from 5 to 7 μm and matrix porosity commonly ranges from 3 to 10% (Dawson et al., 1995), generally decreasing with depth (Dravis, 1979). Permeability also decreases with depth and typically ranges from 0.1 to 0.5 mD (Dawson et al., 1995). The Upper Cretaceous (Cenomanian to Turonian) Eagle Ford Formation (also termed the Eagle Ford Shale or Group) underlies the Austin Chalk and is the main source of Austin Chalk hydrocarbons. The Eagle Ford Shale possesses good to excellent source rock properties and probably generated large quantities of hydrocarbons (Liro et aL,1994). The most productive inteiyals are transgressive and condensed-interval marine shales that were deposited in oxygen-depleted environments (Dawson, 2000). Kerogen type is dominantly oil-prone, and source rock quality varies both laterally and vertically (Dawson, 2000). Total organic carbon (TOC) ranges from 1 to almost 10 wt.% (Robison, 1997). The Eagle Ford Shale entered the oil generation window sometime in the early Paleogene to early Neogene (J. Pitman, 2012,written communication), and is still generating oil in the updip part of the trend. This is critical, as this time frame postdates the creation of the fractured reservoirs in the historic trend, allowing for the emplacement of oil into these reservoirs immediately after generation. Salt movement likely began in the Late Jurassic, soon after deposition, and continued through the Late Cretaceous in the East Texas region (Pearson et al., 2010), creating salt-related structures and fractures in conventional reservoirs. Salt movement also predated Eagle Ford oil generation. Fracture density and connectivity in the Austin Chalk are highly variable,depending on proximity to faults, mineralogical variations (such as an increase in clay content), bed thickness, and the distribution of post-fracture cements (Dawson et al., 1995). Most fractures in the formation were created in response to the downwarping of the Gulf Coast basin,paired with associated faults and localized uplifts that tend to parallel regional strike of the strata (Haymond, 1991).
机译:上白垩统奥斯汀白垩,横跨得克萨斯州和路易斯安那延伸,其特征在于产生油,气,和在某些情况下,异常大量的水贮存器。储层通常具有低渗透性基质和包含天然裂缝。水平钻孔已被用于增强和连接这些裂缝系统更有效地排出贮存器。虽然形成包含连续的(常规的)的贮存器,它表现为一种混合系统,其特征在于,改变地质环境产生连续和常规积累。那么数据表明,初级奥斯汀白垩生产趋势是平行的,只是倾底层下白垩统陆架边缘的。这种趋势包括吉丁斯和皮尔索尔领域,而较小的地质类似领域。最近钻孔扩大此带向东进入路易斯安那州,以及所述paleoshelf边缘的下倾;生产这种新的区域已经证明是成功的,并且包括显著领域如Brookeland和大师小河。的奥斯汀白垩根据民歌(1959)分类为biomicrite;它主要包含coccoliths(Dravis,1979)。该低磁导率,低孔隙率的岩石需要大的连接断裂系统来存储和产生烃。大多数大型裂缝平行于少数面向浸骨折(Haymond,1991年),区域性走。这个一维断裂网络需要许多较小的,局部骨折保持在储存器的流体流动。形成的粘土组分也影响断裂强度和连接(科比特等人,1987; Haymond,1991)。的奥斯汀白垩是一种低孔隙率,低渗透率酯与由微孔基质的一个双重孔隙系统和适度互连断裂系统(Dawson等,1995)。微孔的尺寸范围从5至7微米,基质孔隙度通常为3〜10%(Dawson等,1995),通常与深度(Dravis,1979)降低。渗透性也随深度减小,并且典型地为0.1至0.5毫达西(Dawson等,1995)。上白垩统(森诺曼到土仑)鹰福特组(也称为鹰福特页岩或集团)伏于奥斯汀白垩和是奥斯汀白垩的烃的主要来源。鹰福特页岩具有良好至优异的源岩石性质,可能产生大量烃(里罗等人,1994)的。最有生产力inteiyals是沉积在贫氧环境(道森,2000),其侵和稠间隔海相页岩。干酪根类型是显性油多发,和源岩质量变化在横向和纵向(道森,2000)。总的有机碳(TOC)的范围从1至大约10重量%(罗宾逊,1997)。鹰福特页岩进入早期第三纪到第三纪初(J.皮特曼,2012年,书面通信)的油生成窗口的某个时候,和在趋势的上倾部分仍然产生油。这是至关重要的,因为这个时间段晚于在历史潮流的裂缝性储层的创建,允许石油进驻到这些水库发电之后。盐运动可能开始于晚侏罗世,沉积后不久,经过晚白垩世东德州地区(Pearson等人,2010)继续在常规储层创造盐相关结构和骨折。盐运动还早鹰福特生油。在奥斯汀白垩裂缝密度和连接是高度可变的,这取决于靠近故障,矿物学变化(例如在粘土含量的增加),床厚度和致裂后水泥的分布(道森等人,1995)。在形成最骨折应对墨西哥湾沿岸盆地的坳陷创建,以及相关的故障和局部隆起倾向于平行地层(Haymond,1991)的区域性走配对。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号