首页> 外文期刊>Basin research >Unravelling key controls on the rift climax to post-rift fillofmarine rift basins: insights from3Dseismic analysis of the Lower Cretaceous of the Hammerfest Basin,SWBarents Sea
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Unravelling key controls on the rift climax to post-rift fillofmarine rift basins: insights from3Dseismic analysis of the Lower Cretaceous of the Hammerfest Basin,SWBarents Sea

机译:解开裂谷高潮的关键控制到裂谷后腓汞裂谷盆地:哈默菲斯特盆地下白垩纪的3DS发射分析洞察瑞文人

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In this study, we investigate key factors controlling the rift climax to post-rift marine basin fill. We use two- and three-dimensional seismic data in combination with sedimentological core descriptions from the Hammerfest Basin, south-western Barents Sea to characterize and analyse the tectonostratigraphy and seismic facies of the Lower Cretaceous succession. Based on our biostratigraphic analyses, the investigated seismic facies are correlated to 5–10 million year duration sequences that make up the stratigraphic framework of the basin fill. The seismic facies suggest the basin fill was deposited in shallow to deep-marine conditions. During rift climax in Volgian/Berriasian to Barremian times, a fully linked fault array controlled the formation of slope systems consisting of gravity flow deposits along the southern margin of the basin. Renewed uplift of the Loppa High north of the basin provided coarse-grained sediments for fan deltas and shorelines that developed along the northern basin margin. During the early to middle late Aptian, the input of coarse-grained sediments occurred mainly in the NW and SW corners of the basin, reflecting renewed uplift-induced topography in the western flank of the Loppa High and along the western Finnmark Platform. The lower Albian part of the basin fill is interpreted as a post-rift succession, where the remnant topography associated with the Finnmark Platform continued to provide sediments to prograding fan deltas and adjacent shorelines. During the Albian, a series of faults were reactivated in the northern part of the basin, and footwall wedges comprising various gravity flow deposits occur along these faults. During the latest Albian to Cenomanian, the south-eastern part of the Loppa High was flooded by a rise in eustatic sea-level and differential subsidence. However, the western part of the high remained exposed and acted as a sediment source for a shelf-margin system prograding towards the SE. It is concluded that the r
机译:在这项研究中,我们调查将裂谷高潮的关键因素调查到裂谷后海洋盆地填充。我们将两维和三维地震数据与哈默菲斯特盆地,西南部的小海区的沉积物核心描述相结合,以表征和分析下白垩纪连续的构造数据和地震相。基于我们的生物数据分析,调查的地震相与5-10万年的持续时间序列相关,构成了盆地填充的地层框架。地震相表明盆地填充物沉积在浅层到深海疾病。在Volgian / Berriasian到Barremian时代的裂谷高潮期间,一个完全连接的故障阵列控制了沿盆地南部边缘的重力流沉积物组成的坡度系统的形成。盆地北部的Loppa高隆起提供了粗粒沉积物,适用于沿北部盆地边缘开发的风扇Deltas和海岸线。在早期到中间的安谦期,粗粒沉积物的输入主要发生在盆地的NW和SW角落,反映了罗帕皮的西部侧翼和沿着西菲诺克平台的再生隆起诱导的地形。盆地填充的下奥尔类部分被解释为裂车后连续,其中与FINNMARCH平台相关的残余地形继续为促进范多特和相邻的海岸线提供沉积物。在白葡萄舞期间,在盆地的北部重新激活一系列故障,并且沿着这些故障发生包括各种重力沉积物的脚壁楔。在最新的白尔米亚人到CENOMANIAN期间,Loppa高位的东南部被突然海平和微分沉降的增加。然而,高剩余的西部仍然暴露,并充当朝向SE的搁板边缘系统的沉积物来源。它得出结论,r

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