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首页> 外文期刊>Earth and Planetary Science Letters: A Letter Journal Devoted to the Development in Time of the Earth and Planetary System >Effect of the Galapagos hotspot on seafloor volcanism along the Galapagos Spreading Center (90.9-97.°W)
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Effect of the Galapagos hotspot on seafloor volcanism along the Galapagos Spreading Center (90.9-97.°W)

机译:加拉巴哥群岛热点对沿加拉巴哥群岛传播中心的海底火山活动的影响(90.9-97。°W)

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摘要

Studies along the Mid-Atlantic Ridge (MAR) and East Pacific Rise (EPR) show that seamount abundance is a strong function of spreading rate. At the MAR, small axial seamounts are a dominant morphologic feature of the inner valley floor, while at the EPR seamounts are rarely observed within the neovolcanic zone. The Galápagos Spreading Center (GSC) provides an excellent location to test the influence of hotspot-related magma supply variations on seamount formation at a relatively constant spreading rate. In this study, we use multibeam bathymetry data to examine the distribution of axial seamounts with distance from the hotspot along the GSC. A numerical algorithm is developed to identify isolated volcanic edifices by searching bathymetry for closed, concentric contours protruding above the surrounding seafloor. Seamount populations are fit with a maximum likelihood model to estimate the total number of seamounts per unit area and the characteristic seamount height. The number of seamounts in the axial zone decreases significantly as the Galápagos hotspot is approached, varying from MAR-like abundances west of 95.5°W to EPR-like abundances east of 92.7°W. The along-axis variation in seamount density corresponds to a change in lava flow morphology from dominantly pillow flows in the west to a combination of pillows and sheet/lobate flows in the east. These changes in volcanic style suggest a transition from point-source to fissure-fed eruptions as magma supply increases. We find no evidence for along-axis variations in lava viscosity and, therefore, interpret the differences in seamount abundance and flow morphology to indicate an increase in effusion rates approaching the hotspot. Comparing seamount abundance with axial morphology, crustal thickness, and the presence and depth of an axial magma chamber (AMC), we find that the transition from point-source to fissure-fed eruptions is most sensitive to the presence of a steady-state AMC. In summary, the correlation between seamount abundance, lava morphology, and magma supply at the GSC suggests that effusion rate is directly related to the presence of a steady-state crustal magma chamber.
机译:沿大西洋中脊(MAR)和东太平洋上升(EPR)进行的研究表明,海山丰度是扩散速率的强大函数。在MAR,小轴向海山是内谷底的主要形态特征,而在EPR,新火山带内很少观察到海山。加拉帕戈斯群岛传播中心(GSC)提供了一个极好的位置,以相对恒定的传播速率测试热点相关的岩浆供应变化对海山形成的影响。在这项研究中,我们使用多波束测深数据来检查轴向海山的分布以及沿GSC距热点的距离。开发了一种数值算法,通过搜索测深法寻找突出于周围海底的封闭同心轮廓,从而识别孤立的火山构造。海山人口符合最大似然模型,以估算每单位面积的海山总数和特征性海山高度。随着加拉帕戈斯群岛热点的临近,轴向带海山数量显着减少,从95.5°W以西的MAR类丰度到92.7°W以西的EPR类丰度变化。海山密度沿轴的变化与熔岩流形态的变化相对应,从西部的主要为枕形流向东部的为枕形和片状/叶状流的组合。火山样式的这些变化表明,随着岩浆供应的增加,从点源喷发向裂隙性喷发过渡。我们没有发现熔岩粘度沿轴向变化的证据,因此,解释了海山丰度和流动形态的差异,以表明临近热点的积水速率增加。将海山丰度与轴向形态,地壳厚度以及轴向岩浆室(AMC)的存在和深度进行比较,我们发现从点源到裂隙性喷发的过渡对稳态AMC的存在最敏感。综上所述,GSC的海山丰度,熔岩形态和岩浆供应之间的相关性表明,积水速率与稳态地壳岩浆室的存在直接相关。

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