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Provenance of the upper Miocene Modelo Formation and subsidence analysis of the Los Angeles basin, southern California: Implications for paleotectonic and paleogeographic reconstructions

机译:加利福尼亚南部洛杉矶盆地上中新世Modelo的物源和沉陷分析:对古构造和古地理重建的启示

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摘要

The Los Angeles basin has undergone three stages of development related to complex plate interactions within the evolving San Andreas transform system: transrotation (16–12 Ma), transtension (12–6 Ma), and transpression (6–0 Ma). Timing of these stages correlates with microplate-capture events along the continental margin, and is expressed in changes in subsidence rates and provenance within the Los Angeles basin. The Modelo Formation and related units were deposited in the northern part of the Los Angeles basin at bathyal depths during late Miocene time. The northern Los Angeles basin was segmented into three subbasins, in each of which coarse sediment was deposited as submarine fans (Puente, Tarzana, and Simi). A fourth fan system (Piru) formed in the Ventura basin, just north of the Los Angeles basin. The Puente, Tarzana, and Piru fans were derived from the San Gabriel block, which consists primarily of crystalline basement and lesser volcanic and sedimentary components. Sandstone within the Puente fan reflects unroofing of the central and eastern San Gabriel block. The Tarzana fan was derived primarily from the central San Gabriel block, and the Piru fan was derived primarily from the western San Gabriel block, which is distinctly characterized by Ca-rich plagioclase derived from Proterozoic anorthosite and related bodies. The lack of Ca-rich plagioclase in the other fans eliminates the western San Gabriel block as a possible source area, and confirms differentiation of the Ventura basin from the Los Angeles basin by late Miocene time. The Simi fan was derived from locally uplifted Cretaceous and Paleogene strata; sandstone composition reflects the recycling of these sediments. Subsidence and provenance analyses are consistent with the following paleogeographic and paleotectonic reconstruction. Beginning at approximately 16 Ma, transrotation of the Western Transverse Ranges induced extension and thermal subsidence of the Los Angeles basin area. A second pulse of extension and thermal subsidence occurred when motion began along the San Gabriel fault at 12 Ma. Right slip of 60–70 km occurred along the San Gabriel fault, which produced transtension in the Los Angeles basin area and deposition of the Puente, Tarzana, Simi, and Piru fan systems. At 6 Ma, transform motion was transferred to the San Andreas fau transpression has dominated the Los Angeles basin since 6 Ma, including rapid uplift, flexural subsidence due to tectonic loading, and rapid sedimentary filling. The rapid subsidence and filling and the sudden switch between transtension and transpression in the Los Angeles basin are typical of strike-slip basins in general. However, initiation of the Los Angeles basin by transrotation reflects the uncommon process of microplate capture along the rapidly evolving California margin.
机译:洛杉矶盆地经历了与不断发展的San Andreas变换系统内复杂的板块相互作用有关的三个发展阶段:反转(16-12 Ma),转变 < / sup>(12–6 Ma)和压制(6–0 Ma)。这些阶段的时间与沿大陆边缘的微孔板捕获事件有关,并表示为洛杉矶内沉降速率和物源的变化。 在中新世末期,Modelo组和相关单元沉积在洛杉矶盆地的北部 深处。洛杉矶北部盆地被划分为三个子盆地,每个子盆地中都有深层沉积物作为海底扇沉积(普恩特,塔尔扎纳和西米)。第四个风扇 系统(Piru)在文图拉盆地中形成,就在 洛杉矶盆地的北部。 Puente,Tarzana和Piru扇是从San Gabriel区块衍生而来的,它主要由结晶性基底和较少的火山和沉积成分组成。 Puente扇内的砂岩 反映了圣加布里埃尔东部和东部东部sup> 的屋顶。 Tarzana风扇主要 来自中央圣加百利街区,而Piru风扇主要 来自西部圣加百利街区,这明显是 以富含钙的斜长石为特征,富含钙质的斜长石起源于原生钙长石和相关体。其他风扇中缺乏富含钙的斜长石 消除了西部圣盖博块,这可能是 的可能来源区域,并确认了 Ventura的分化 Simi扇是由白垩系和 Paleogene地层抬升而来的。砂岩组成反映了这些沉积物的循环利用。沉降和物源分析与以下古地理和古构造重建一致。 始于大约16 Ma,Western Transverse Ranges的逆转引起了洛杉矶 盆地地区的扩张和热沉降。当沿圣加布里埃尔断裂在12Ma处开始运动时,发生了第二个伸展和热沉降脉冲 。沿着圣加百利断裂发生了60–70 km的右滑,这在洛杉矶盆地 区域造成了高压变形,并形成了普恩特,塔尔扎纳,西米和皮鲁扇形沉积物。 系统。在6 Ma时,变换运动转移到San Andreas断层;自6 Ma以来,反压作用一直主导着洛杉矶盆地 ,包括快速隆升,构造载荷引起的弯曲沉降和快速沉积。总体上,走滑盆地通常具有快速的 下沉和充填,以及超高压 和超高压之间的突然转换。但是,通过逆转引发的洛杉矶盆地 反映了沿迅速发展的加利福尼亚边缘微孔板 捕获的罕见过程。

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  • 来源
    《GSA Bulletin》 |1997年第7期|885-899|共15页
  • 作者单位

    Department of Earth and Space Sciences, University of California, Los Angeles, California 90095-1567;

    Department of Earth and Space Sciences, University of California, Los Angeles, California 90095-1567;

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