Magnetic susceptibility and natural gamma radioactivity as indirect proxies for characterization of sandstones and limestones of the Sabinas basin

IF 0.9 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Geofizika Pub Date : 2017-06-30 DOI:10.15233/GFZ.2017.34.6
J. A. B. Rodríguez, J. Fernández, A. Vega, Felipe de Jesús López Saucedo, Karla I. Cázares Carreón
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引用次数: 4

Abstract

An analysis of magnetic susceptibility and natural gamma radioactivity is presented as indirect proxies of the characteristics of sandstones and limestones of the Sabinas basin. These rocks are located in the sedimentary sequence ranging from the Upper Jurassic to the Cretaceous. The magnetic susceptibility indicates changes in the magnetic composition of these rocks and suggests changes in their weathering degree. Ranges of values of magnetic susceptibility in sandstones and limestones allow classifying them into different groups, suggesting variability regarding conditions of origin and evolution. High values of magnetic susceptibility in limestones can be linked to sedimentation in anoxic or reducing environment, as well as with its siliciclastic content. The natural gamma radioactivity expressed in the contents of Th and relationships U / K and Th / U also suggest the degree of weathering of these rocks, mainly in the sandstones. These relations also highlight others characteristics in the sandstones related the probable provenance of sediments, its distance, degree of weathering and transport dynamics. Using the values of U / K ratio in the sandstones, it is possible to suggest the probable quartz-feldspar relationships. These ratio values classified rocks as arkose or quartzarenite, indicating the maturity of the sandstones. According to the U / K ratio values, most of these rocks which show little maturity are called arkose. Using the values of the Th / U ratio, it is possible to suggest the textures of quartzarenites, classifying them as rocks with fabric that is clast-supported or matrix-supported.
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磁化率和自然伽马放射性作为Sabinas盆地砂岩和灰岩表征的间接指标
用磁化率分析和自然伽马放射性作为萨比纳斯盆地砂岩和灰岩特征的间接指标。这些岩石位于上侏罗统至白垩纪的沉积序列中。磁化率反映了岩石磁性成分的变化,反映了岩石风化程度的变化。砂岩和灰岩的磁化率值范围可以将它们分为不同的组,这表明它们在起源和演化条件方面存在差异。石灰石的高磁化率值可能与缺氧或还原性环境中的沉积有关,也与其硅塑性含量有关。天然γ放射性在Th含量中的表达以及U / K和Th / U的关系也反映了这些岩石的风化程度,主要表现在砂岩中。这些关系还突出了砂岩中与沉积物可能的物源、距离、风化程度和运输动力学有关的其他特征。利用砂岩中的U / K比值值,可以推测出石英与长石的可能关系。这些比值值将岩石划分为长石或石英岩,表明砂岩的成熟度。根据U / K比值值,这些成熟度较低的岩石大多被称为长石。利用Th / U比值值,可以推测石英砂岩的结构,将其划分为碎屑支撑型和基质支撑型。
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来源期刊
Geofizika
Geofizika 地学-地球化学与地球物理
CiteScore
1.60
自引率
0.00%
发文量
17
审稿时长
>12 weeks
期刊介绍: The Geofizika journal succeeds the Papers series (Radovi), which has been published since 1923 at the Geophysical Institute in Zagreb (current the Department of Geophysics, Faculty of Science, University of Zagreb). Geofizika publishes contributions dealing with physics of the atmosphere, the sea and the Earth''s interior.
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