桑托斯盆地天秤座断裂带活动性及其对火成岩分布的影响——基于高分辨率三维地震数据的断裂带活动性半定量到定量评价

Jian Zhao, M. J. R. Oliveira, Junfeng Zhao, K. Ren, Leonardo Costa de Oliveira, I. O. Carmo, Cristiano Camelo Rancan, Qicai Deng
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引用次数: 4

摘要

Libra碳酸盐岩储层除非均质性强外,还存在火成岩,这对储层建模和生产动态预测提出了挑战。本文的研究目标有三个方面:1)更好地了解岩浆事件的成因及其与断层活动的关系;2)尽量减少地球物理和岩石物理方法结果的不确定性;3)提高火成岩预测的可靠性和准确性。已经尝试了几种半定量到定量的评价方法来评价断层活动性。断裂生长指数结果表明,ⅰ类断裂在整个裂谷期从PIC (PiÇarras Fm.)至BVE (Barra Velha Fm.)连续活动,但活动强度值最高的时间自西向东逐渐变晚。在天秤座的NW结构中,它们的强度最大出现在PIC沉积时期。在中央构造,它们主要在ITP (Itapema Fm)阶段表现出最高的活度值。即使在BVE沉积时期,SE构造的ⅰ类断裂也继续活跃。8条ii类断裂主要在PIC和ITP期活动,BVE期不再活动。NW构造的2条ii级断裂活动更活跃,活动强度在PIC期间最大,而中央和SE构造的同阶断裂持续时间更长,活动强度最高,出现在ITP沉积期。所有断层,包括ⅰ类断层和ⅱ类断层,其中部活动时间较长,强度较高,而两端活动时间较短,强度值较低(图3)。建立了火成岩成因地质模型。将阿普田火山解释为岩浆沿区域断裂分布的一种裂隙事件。二级断裂和部分一级断裂及其运动对阿普田陨石坑的形成起着重要作用,并控制了后期喷出岩的分布。ⅰ类断裂及其后期的再活化对三东系侵入火成岩的分布起着关键作用。在该模型的指导下,采用多尺度、多学科的方法进行火成岩预测,可以显著有效地降低地震资料的不确定性,提高火成岩预测的可靠性和准确性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Fault Activity and its Influences on Distribution of Igneous Rocks in Libra Block, Santos Basin: Semi-Quantitative to Quantitative Assessment of Fault Activity Based on High-Resolution 3D Seismic Data
Libra carbonate reservoirs, besides its great heterogeneity, are also characterized by occurrence of igneous rocks, as a challenge to reservoir modeling and production performance prediction. The objectives of this paper are three fields:1) To better understand the genetic cause of magma events and its relationship with fault activity;2) To minimize the uncertainties of the outcomes from geophysical and petrophysical methods;3) To enhance the reliability and accuracy of igneous rocks’ prediction. Several semi-quantitative to quantitative assessment methods have been attempted and employed to evaluate the fault activity. The result from fault growth index reveal that the Class-I faults are continuously active from PIC (PiÇarras Fm.) to BVE (Barra Velha Fm.), throughout the whole rift period, but the time when they have the highest activity intensity value is getting later from west to east. In NW structure of Libra, their most intensity appeared during the period of PIC deposition. In Central structure, they show their highest activity values mainly during ITP (Itapema Fm.) stage. And the Class-I faults in SE structure continue to be active even during the deposition time of BVE. The eight class-II faults show their movement mainly during the PIC and ITP period and they were no longer active during BVE stage. The two Class-II faults in NW structure were more active, with a largest value of activity intensity during PIC while the same order faults in Central and SE structure lasted for even longer time, and their highest intensity occurred in ITP deposition period. All the faults, including Class-I faults and Class-II faults, usually have a longer activity duration and a higher intensity in their middle part, and a relatively shorter activity time and a lower intensity value in their two endpoints (Figure.3). An igneous rocks genetic geological model is built up. The Aptian volcano was interpreted as a type of fissure event when the magma was distributed along the regional faults. The Class-II and some Class-I faults and their movement contribute to the formation of Aptian craters and then controlled the distribution of afterward extrusive rock. The Class-I faults and their later reactivation play a key role in the distribution of Santonian intrusive igneous rocks. Under the guidance of such model, methods of multi-scale and multi-disciplinary could be used to predict igneous rocks, which could significantly and effectively reduce the uncertainties of seismic data and enhance the reliability and accuracy of igneous rocks’ prediction.
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