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Geodynamic evolution of crust accretion at the axis of the Reykjanes Ridge, Atlantic Ocean

机译:大西洋雷克雅尼斯海脊轴线上地壳增生的地球动力学演化

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摘要

The results of analysis of the anomalous magnetic field of the Reykjanes Ridge and the adjacent basins are presented, including a new series of detailed reconstructions for magnetic anomalies 1-6 in combination with a summary of the previous geological and geophysical investigations. We furnish evidence for three stages of evolution of the Reykjanes Ridge, each characterized by a special regime of crustal accretion related to the effect of the Iceland hotspot. The time interval of each stage and the causes of the variation in the accretion regime are considered. During the first, Eocene stage (54-40 Ma) and the third, Miocene-Holocene stage (24 Ma-present time at the northern Reykjanes Ridge north of 59° N and 17-11 Ma-present time at the southern Reykjanes Ridge south of 59° N), the spreading axis of the Reykjanes Ridge resembled the present-day configuration, without segmentation, with oblique orientation relative to the direction of ocean floor opening (at the third stage), and directed toward the hotspot. These attributes are consistent with a model that assumes asthenospheric flow from the hotspot toward the ridge axis. Decompression beneath the spreading axis facilitates this flow. Thus, the crustal accretion during the first and the third stages was markedly affected by interaction of the spreading axis with the hotspot. During the second, late Eocene-Oligocene to early Miocene stage (40-24 Ma at the northern Reykjanes Ridge and 40 to 17-11 Ma at the southern Reykjanes Ridge), the ridge axis was broken by numerous transform fracture zones and nontransform offsets into segments 30-80 km long, which were oriented orthogonal to the direction of ocean floor opening, as is typical of many slow-spreading ridges. The plate-tectonic reconstructions of the oceanic floor accommodating magnetic anomalies of the second stage testify to recurrent rearrangements of the ridge axis geometry related to changing kinematics of the adjacent plates. The obvious contrast in the mode of crustal accretion during the second stage in comparison with the first and the third stages is interpreted as evidence for the decreasing effect of the Iceland hotspot on the Reykjanes Ridge, or the complete cessation of this effect. The detailed geochronology of magnetic anomalies 1-6 (from 20 Ma to present) has allowed us to depict with a high accuracy the isochrons of the oceanic bottom spaced at 1 Ma. The variable effect of the hotspot on the accretion of oceanic crust along the axes of the Reykjanes Ridge and the Kolbeinsey and Mid-Atlantic ridges adjoining the former in the north and the south was estimated from the changing obliquity of spreading. The spreading rate tends to increase with reinforcing of the effect of the Iceland hotspot on the Reykjanes Ridge. [PUBLICATION ABSTRACT]
机译:给出了雷克雅尼斯海岭和邻近盆地异常磁场的分析结果,包括一系列新的详细的磁异常1-6重建结果,并结合了以前的地质和地球物理调查的摘要。我们提供了雷克雅尼斯海岭演化的三个阶段的证据,每个阶段都具有与冰岛热点影响有关的特殊地壳增生机制。考虑每个阶段的时间间隔和吸积机制变化的原因。在第一个始新世阶段(54-40 Ma)和第三个中新世-全新世阶段(北雷克雅尼斯海脊,北纬59°,目前为24 Ma,现在为南雷克雅尼斯海脊,南为17-11 Ma,现在)雷克雅内斯山脊(59°N)的扩张轴类似于当今的构造,没有分段,相对于海床开口方向呈倾斜方向(在第三阶段),并指向热点。这些属性与假设从热点向脊轴的软流圈流动的模型一致。扩散轴下方的减压有助于这种流动。因此,第一和第三阶段的地壳增生受到扩展轴与热点相互作用的显着影响。在始新世的第二个晚期至中新世至中新世早期(雷克雅尼斯山脊的北部为40-24 Ma,雷克雅尼斯山脊的南部为40至17-11 Ma),脊轴被众多的转换断裂带破坏,并且非转换偏移为30-80公里长的线段,其方向垂直于海床开口方向,这是许多缓慢扩展的山脊的典型特征。适应第二阶段磁性异常的海床板块构造重建证明,与相邻板块运动学变化有关的脊轴几何形状的周期性重排。与第一阶段和第三阶段相比,第二阶段地壳增生模式的明显差异被解释为冰岛热点对雷克雅内斯岭的影响减小或这种影响完全停止的证据。磁性异常1-6(从20 Ma到现在)的详细地质年代学使我们能够高精度地描绘间隔为1 Ma的海底等时线。从分布倾斜的变化角度估计了热点对沿雷克雅内斯山脊以及与前者邻接的柯尔本西脊和中大西洋海脊轴线上的洋壳积聚的可变影响。随着冰岛热点对雷克雅尼斯海岭的影响的增强,扩散速度趋于增加。 [出版物摘要]

著录项

  • 来源
    《Geotectonics》 |2009年第3期|p.1-15|共15页
  • 作者单位
  • 收录信息 美国《科学引文索引》(SCI);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

  • 入库时间 2022-08-17 23:19:43

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