首页> 外文期刊>Sedimentary geology >Palaeohydrogeological control of palaeokarst macro-porosity genesis during a major sea-level lowstand: Danian of the Urbasa-Andia plateau, Navarra, North Spain
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Palaeohydrogeological control of palaeokarst macro-porosity genesis during a major sea-level lowstand: Danian of the Urbasa-Andia plateau, Navarra, North Spain

机译:主要海平面低位期古喀斯特宏观孔隙成因的古水文地质控制:西班牙北部纳瓦拉的Urbasa-Andia高原的达尼安

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摘要

An extensive palaeokarst porosity system, developed during a pronounced mid-Paleocene third-order lowstand of sea level, is hosted in Danian limestones of the Urbasa-Andia plateau in north Spain. These limestones were deposited on a 40-50 km wide rimmed shelf with a margin characterised by coralgal buildups and coarse-grained bioclastic accumulations. The sea-level fall that caused karstification was of approximately 80-90 m magnitude and 2.5 Ma in duration. During the exposure, a 450 m wide belt of sub-vertical margin-parallel fractures developed a few hundred metres inboard of the shelf edge. Most fractures are 90-100 m deep, average 1 m in width, and are associated with large erosional features created by collapse of the reefal margin. Inland from the fracture belt, three superimposed laterally extensive cave systems were formed over a distance of 3.5 km perpendicular to shelf edge, at depths ranging from 8-31 m below the exposure surface. The palaeocaves range from 0.3 to 2 m in height, average 1.5 m high. They show no evidence of meteoric processes and are filled with Thanetian grainstones rich in reworked Microcodium, a lithology that also occurs infilling the fractures. The caves are interpreted as due to active corrosion at the saline water-fresh-water mixing zone. Caves are missing from the shelf edge zone probably because the fractures beheaded the meteoroic lens preventing mixing-zone cave development beyond the fracture zone. Towards the platform interior, each cave system passes into a prominent horizon, averaging 1 m in thickness, of spongy porosity with crystal silt infills and red Fe-oxide coatings. The spongy horizons can be traced for 5.5 km inboard from the cave zone and occur at 10.5 m, 25 m and 32 m below the exposure surface. In the inland zone, two additional horizons with the same spongy dissolution have been recognised at depths of 50 m and 95 m. All are analogous to Swiss-cheese mixing-zone corrosion in modern carbonate aquifers and probably owe their origins to microbially-mediated dissolution effects associated with a zone of reduced circulation in marine phreatic water. In the most landward sections a number of collapse breccia zones are identified, but their origin is unclear. The palaeokarst system as a whole formed during the pulsed rise that followed the initial sea-level drop, with the three main cave-spongy zones representing three successive sea-level stillstands, recorded by stacked parasequences infilling large erosional scallops along the shelf margin. The geometry of the palaeo-rnmixing zones indicates a low discharge system, and together with the lack of meteoric karstic features favours a semi-arid to arid climatic regime, which is further supported by extensive calcrete-bearing palaeosols occurring in coeval continental deposits.
机译:在西班牙北部Urbasa-Andia高原的达尼安石灰岩中,存在着一个明显的古岩溶孔隙系统,该系统是在一个明显的古新世中期三阶海平面开发的。这些石灰石沉积在一个40-50 km宽的有边缘的架子上,其边缘的特征是珊瑚堆积和粗粒生物碎屑堆积。引起岩溶作用的海平面下降幅度约为80-90 m,持续时间为2.5 Ma。在暴露过程中,一条450 m宽的亚垂直边缘平行裂缝带在货架边缘内侧发展了几百米。大多数裂缝的深度为90-100 m,平均宽度为1 m,并伴有因珊瑚礁边缘塌陷而形成的大型侵蚀特征。从断裂带向内陆,在垂直于陆架边缘的3.5 km距离上,在暴露面以下8-31 m的深度范围内,形成了三个叠加的横向扩展的洞穴系统。古土壤的高度为0.3至2 m,平均高度为1.5 m。它们没有流星过程的迹象,并充满了富含返工的微co的塔尼阶粒岩,这种岩性也充满了裂缝。这些洞穴被解释为是由于盐水-淡水-混合区的活跃腐蚀所致。架子边缘区域缺少洞穴,这可能是因为裂缝将流星透镜斩首,阻止了混合区洞穴在裂缝区域之外的发展。朝向平台内部,每个洞穴系统进入一个明显的地平线,平均厚度为1 m,海绵状孔隙中带有结晶粉砂填充物和红色的氧化铁涂层。海绵状地平线可以追溯到洞穴区域内侧5.5 km,发生在暴露面以下10.5 m,25 m和32 m处。在内陆地区,在50 m和95 m的深度处发现了两个海绵状溶蚀相同的附加层位。所有这些都类似于现代碳酸盐含水层中的瑞士-奶酪混合区腐蚀,并且可能归因于微生物介导的溶解作用,该溶解作用与海洋潜水水中循环减少的区域有关。在最陆路段,发现了多个塌陷角砾岩带,但其起源尚不清楚。整个古岩溶系统是在初始海平面下降之后的脉冲上升过程中形成的,三个主要的洞穴海绵状带代表了三个连续的海平面静止地带,由堆积的副层序记录了沿着陆架边缘的大侵蚀扇贝。古混交带的几何结构表明其排泄系统很低,加上缺乏陨石岩溶特征,有利于半干旱到干旱的气候体系,这进一步得到了近代大陆沉积物中大量含钙质古土壤的支持。

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