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Organic geochemistry and sequence biostratigraphy of the Upper Devonian-Lower Mississippian Exshaw and lower Banff formations, southern Alberta.

机译:阿尔伯塔省南部上泥盆统—下密西西比州Exshaw和下班夫组的有机地球化学和层序生物地层学。

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摘要

The integration of sequence stratigraphic, biostratigraphic, and organic geochemical techniques at both subsurface and outcrop locations provide new insights into the Upper Devonian-Lower Mississippian petroleum system. This system is represented by the upper Palliser, Exshaw, and lower Banff formations, and includes both reservoir and hydrocarbon source-rock units. Many oil families in southern Alberta have been linked to their source; an exception is oil Family M. Biomarker data for these oils indicate a source of Mississippian age capable of producing relatively large quantities of oil. One probable source for these oils is the lower Banff Formation, predominantly a Type II kerogen with total organic carbon (TOC) values from immature samples that commonly exceed10 wt.%.; At outcrop, the lower Banff Formation comprises overmature shales that vary in thickness from three to four metres in the eastern Front Range exposures (e.g. Inverted Ridge), to greater than 20 metres in westernmost exposures (e.g. near Fortress Mountain), and possesses TOC values up to 18.2 wt.%. In the subsurface, the shale members of the Exshaw and Banff formations vary dramatically in thickness from being not present to thicker than 7 metres. These changes in thickness may explain the existence of two distinct mid-late Paleozoic oil families.; Sequence stratigraphic techniques and conodont biostratigraphic data were combined to aid in the correlation of surfaces within this Upper Devonian to Lower Carboniferous interval. These data indicate that locally, the Exshaw Formation is missing; the absence of these strata is attributed to the development of a stratigraphic high after the deposition of the Big Valley Formation and prior to the deposition of the lower Exshaw Formation. In this area, oils generated from the lower Banff Formation could have migrated without mixing with Exshaw Formation sourced oils providing a possible explanation for the existence of Family M oils in Cretaceous reservoirs.
机译:地下和露头位置的层序地层学,生物地层学和有机地球化学技术的整合为上泥盆统—下密西西比石油系统提供了新的见识。该系统由上部的Palliser,Exshaw和下部的Banff地层代表,包括储层和烃源岩单元。艾伯塔省南部的许多石油家庭都与他们的来源有联系。油族M是一个例外。这些油的生物标记数据表明,密西西比年龄的来源能够产生相对大量的油。这些油的一个可能来源是较低的班夫地层,主要是II型干酪根,未成熟样品中的总有机碳(TOC)值通常超过10 wt。%。在露头,较低的班夫组包括过早的页岩,其厚度从东部锋范围暴露(例如倒立脊)的三米到四米不等,到最西部暴露区域(例如在堡垒山附近)的20米以上不等,并具有TOC值高达18.2重量%。在地下,Exshaw和Banff地层的页岩层厚度变化很大,从不存在到厚度超过7米。这些厚度的变化可以解释存在两个不同的中晚期古生代油族。层序地层学技术和牙形石生物地层学数据相结合,以帮助在上泥盆纪至石炭纪下层之间的地表相关性。这些数据表明,当地缺少Exshaw组。这些地层的缺乏归因于大谷地层沉积之后和下埃克肖地层沉积之前地层高的发展。在该地区,下班夫组产生的油可以在不与Exshaw组来源的油混合的情况下迁移,这为白垩纪储层中M族油的存在提供了可能的解释。

著录项

  • 作者

    Schmidt, Michael J.;

  • 作者单位

    University of Calgary (Canada).;

  • 授予单位 University of Calgary (Canada).;
  • 学科 Geology.
  • 学位 M.Sc.
  • 年度 2005
  • 页码 216 p.
  • 总页数 216
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 地质学;
  • 关键词

  • 入库时间 2022-08-17 11:41:22

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