Late Oligocene - Early Miocene syntectonic fluvial sedimentation in the Aragonese Pyrenean domain of the Ebro Basin: facies models and structural controls.

G. P. Tirapu, C. Arenas
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引用次数: 7

Abstract

This contribution deals with a part of the northern margin of the Ebro Basin (Fig. 1). The Upper Oligocene-Lower Miocene molassic infilling in that part mainly corresponds to an extensive fluvial system: the Luna system, which drained the Gavamie unit area and emerged in the basin to the west of the Sierras Exteriores Aragonesas. Small, margina] alluvial fans originated along the Sierras combined in the Luna fluvial system, as well as in the eastern Huesca fluvial system, outside the study area. TIn-ce tectosedimentary units (T.S.U.> were differentiated in the Uncastilio Formation (Figs. 2, 3 and 4), the evolution of whichwas controlled by teetonies affecting the drainage basins. The study of the different lithofacies, their lateral relationsbips and their areal distribution through time (Fig. 5) led to establish sedimentary models for the marginal fans and Luna fluvial system (Hg. 6>. The Luna system resulted from coalescence of two fluvial fans (Figs. 6 and 7). Despite the fluvial network appears mainily as radial, it was controlled by the syndepositional development of the Fuencalderas and Uncastillo anticlines, within the Ebro Basin. Syndepositional folding is shown by important thickness variations in T.S.U., as wel] as by tibe formation of wedge systems within the basin. Progressive uplift of these structures channeled part of the diseharge parallel to tibe basin margin (Figs. 6 and 7), while another portion flowed basinward from the periclinal ends. Vertical aceretion in the synclinal areas north of the anticlines compensated tibe anticlinal uplift, making the siope more genfle and originating bench terraces within tibe general fan slope. In these arcas of gentle slope meandering sandy rivers developed in proximal scctors of tibe systcm, 5.5 lun fair from the margin at present. i
埃布罗盆地阿拉贡-比利牛斯山脉地区晚渐新世-早中新世同构造河流沉积:相模式与构造控制
这一贡献涉及埃布罗盆地北缘的一部分地区(图1)。该地区的上渐新世-下中新世molassic充填主要对应于一个广泛的河流系统:Luna系统,它排干了Gavamie单位面积,并出现在sierra Exteriores Aragonesas以西的盆地中。小型边缘冲积扇起源于沿山脉合并的月神河系统,以及研究区域外的韦斯卡河系统东部。在Uncastilio组中划分出TIn-ce构造沉积单元(t.s.u)(图2、3和4),其演化受影响流域的构造控制。通过对不同岩相及其横向关系和区域分布的研究(图5),建立了边缘扇和月神河系(Hg. 6)的沉积模型。Luna系统是由两个河流扇合并而成(图6和图7)。尽管河流网络主要呈放射状,但它受到埃布罗盆地内Fuencalderas和Uncastillo背斜同沉积发育的控制。同沉积褶皱表现在T.S.U的重要厚度变化,以及盆地内楔形体系的形成。这些构造的逐渐抬升使部分水流平行于胫骨盆地边缘(图6和图7),而另一部分则从斜周端向盆地内流动。背斜以北向斜地区的垂直沉降补偿了背斜隆升,使斜坡更为平缓,并在总体扇坡内形成阶地。在这些缓坡弧形地带,在系近段发育曲流沙质河流,目前距边缘约5.5公里。我
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