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Development of a fracture network in crystalline rocks during weathering: Study of Bishop Creek chronosequence using X-ray computed tomography and C-14-PMMA impregnation method

机译:风化过程中晶体岩石中裂缝网络的发展:利用X射线计算机断层扫描和C-14-PMMA浸渍方法研究Bishop Creek时序序列

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The progressive development of porosity during subsoil weathering of granodiorite clasts was studied at the Bishop Creek moraine chronosequence in east-central California. Fractures and other pores were examined using two complementary imaging techniques, X-ray computed tomography (XRCT) and a C-14-PMMA (C-14-polymethylmethacrylate) method. The well-known XRCT method allows the investigation of three-dimensional (3-D) pore space. C-14-PMMA is a less-known method based on the complete impregnation of pore space with C-14-doped PMMA, and subsequent autoradiograph of a rock section. These imaging methods allow us to decipher the evolution of pore space in the granodiorite during the 120 k.y. weathering period. The C-14-PMMA imaging technique was found to be more suitable for following the evolution of the whole sequence, from "intact" bedrock to saprock, in terms of crack density, porosity, and aperture. Working with hand specimens, this method was adapted to detect both the low-aperture fractures (microcracks) and macrocracks. Only a slight and progressive increase in total fracture density was observed during the whole weathering period. However, this trend does not hold if macrocracks and microcracks are separated: Microcrack density slightly decreases, whereas macro-crack density increases due to a progressive expansion of microcracks. The total porosity of the rock increases during weathering and is correlated to the progressive aperture increase of all types of cracks. This evolution is accompanied by a change of crack morphology and connectivity, and an overall increase in intragranular porosity of biotite and plagioclase aggregates.
机译:在加利福尼亚州中东部的Bishop Creek冰ora年代序列中研究了花岗闪长岩岩层在土壤下风化过程中孔隙的逐步发展。使用两种互补的成像技术,X射线计算机断层扫描(XRCT)和C-14-PMMA(C-14-聚甲基丙烯酸甲酯)方法检查了裂缝和其他孔。众所周知的XRCT方法允许研究三维(3-D)孔隙空间。 C-14-PMMA是一种鲜为人知的方法,该方法基于用C-14掺杂的PMMA对孔空间进行完全浸渍,然后对岩石剖面进行放射自显影。这些成像方法使我们能够解读120 k.y期间花岗闪长岩中孔隙空间的演变。风化时期。发现C-14-PMMA成像技术在裂缝密度,孔隙率和孔径方面更适合跟踪从“完整”基岩到边材的整个序列的演化。通过处理手标本,该方法适用于检测低孔径裂缝(微裂纹)和大裂纹。在整个风化期间,仅观察到总裂缝密度略有增加。但是,如果将大裂纹和微裂纹分开,则这种趋势将不成立:微裂纹的密度会稍微降低,而由于微裂纹的逐步扩展,大裂纹的密度会增加。岩石的总孔隙度在风化过程中增加,并且与所有类型的裂缝的孔径逐渐增加相关。这种演化伴随着裂纹形态和连通性的变化,以及黑云母和斜长石聚集体的颗粒内孔隙度总体增加。

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