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首页> 外文期刊>Facies >TEM study of Mg distribution in micrite crystals from the Mishrif reservoir Formation (Middle East, Cenomanian to Early Turonian)
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TEM study of Mg distribution in micrite crystals from the Mishrif reservoir Formation (Middle East, Cenomanian to Early Turonian)

机译:Mishrif储层组(中东,西诺曼尼亚至早期土伦期)的微晶晶体中Mg分布的TEM研究

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Microporous limestones composed of micrite crystals constitute sizeable hydrocarbon reservoirs throughout the world and especially in the Middle East. However, the crystallization history of micrites is poorly understood. Scanning electronic microscopy (SEM) with X-ray energy dispersive spectroscopy (EDS) studies give morphological and bulk composition information about micrites, but no information exists on the distribution of minor elements inside micrite grains. This study proposes Mg maps obtained with X-ray EDS combined with scanning transmission electron microscopy (STEM) of micrite crystals from the Mishrif reservoir Formation (Middle East, Cenomanian to Early Turonian). Three types of Mg distribution were observed through micrite crystals from five different samples: (1) homogenous Mg concentration, (2) small Mg-enriched areas close to the center of the crystal, and (3) geometric Mg impoverishments near crystal edges and parallel to present crystallographic faces. The homogenous Mg distribution is the most frequent and is found both in microporous and in tight micrites. The second type of distribution showing small Mg-enriched areas inside micrite crystals relatively close to their center comes from a microporous sample located below an emersive surface. These enriched areas may correspond to crystal seeds. The third type of distribution was observed in micrite crystals from another microporous sample situated just below an emersive surface. The Mg-poor zones probably represent overgrowths that precipitated in contact with less Mg-rich meteoric fluids.
机译:由微晶晶体组成的微孔石灰岩在世界范围内,尤其是在中东构成了可观的碳氢化合物储集层。但是,人们对微晶的结晶历史知之甚少。借助X射线能量色散光谱(EDS)研究的扫描电子显微镜(SEM)给出了有关微晶的形态学和整体组成信息,但没有信息表明微晶晶粒内部微量元素的分布。这项研究提出了利用X射线EDS结合Mishrif储层(中东,西诺曼尼亚至早期土伦)的微晶晶体的扫描透射电子显微镜(STEM)获得的Mg图。通过五个不同样品的微晶晶体观察到三种类型的Mg分布:(1)均匀的Mg浓度;(2)靠近晶体中心的富Mg的小区域;(3)晶体边缘附近和平行的Mg几何贫化呈现晶体学的面孔。均匀的Mg分布最常见,并且存在于微孔和致密的微晶中。第二种分布类型显示了在微晶晶体内部相对靠近其中心的Mg富集区域很小,该微结构来自位于发芽表面下方的微孔样品。这些富集区域可能对应于晶种。第三类分布是在刚好位于新兴表面下方的另一个微孔样品的微晶晶体中观察到的。镁含量低的区域可能代表了与较少的富含镁的陨石流体接触而沉淀的过度生长。

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