Mid-Ocean Ridge (MOR) Ash Dispersal on Axial Seamount, Juan de Fuca Ridge

IF 3 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Ryan A. Portner, Guangyu Xu, Arran P. Murch, David A. Clague, Brian M. Dreyer, Jennifer B. Paduan
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Abstract

Rare eruption of primitive normal mid-ocean ridge basalt (N-MORB) magma (∼9.5 wt% MgO) on the summit of Axial Seamount generated abundant ash that was dispersed for several km. The unique geochemical signature of this ash deposit is distinct from otherwise typical MORB with more evolved compositions. As such, it is a key marker bed that can be used to track the dispersal of ash from an inferred source. The deposit rapidly fines over 1–4 km and becomes more chemically heterogeneous with distance. Toroidal bottom current circulation around Axial's summit caldera primarily constrained it to the southwest part of the summit with limited dispersal to the southeast and northern flanks. Computer simulations that best match the observed dispersal pattern suggest that ash was lofted to ∼250 masf by a moderate heat transfer rate (∼109 W) from a small hydrothermal megaplume and co-genetic lava flow. Models invoking lower heat transfer rates from just a cooling lava flow could only loft the finest material to <225 m above the seafloor, and could not recreate the observed dispersal pattern, even under a strong bottom current regime. Radiocarbon ages and lithostratigraphy imply that the marker bed formed ∼600 years BP, after caldera formation, which occurred sometime between 1400 and 1000 years BP. Chemostratigraphic trends show that eruptions tapped more primitive magmas (8.0–9.7 wt% MgO) for several hundreds of years after caldera formation. This observation is interpreted to reflect catastrophic changes in crustal permeability that reduced the volume and magma storage times in crustal reservoirs, which in turn allowed magmas to rapidly ascend to the surface.

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胡安德富卡海岭轴向海山的洋中脊(MOR)火山灰扩散
轴向海山峰顶罕见的原始正常海中脊玄武岩(N-MORB)岩浆(~ 9.5 wt% MgO)喷发产生了丰富的火山灰,并分散了数公里,该火山灰矿床具有独特的地球化学特征,与其他成分更进化的典型海中脊玄武岩不同。因此,它是一个关键的标记床,可以用来追踪从推断来源的灰烬的扩散。沉积物在1-4公里的范围内迅速变细,随着距离的增加,其化学性质变得更加不均匀。轴向山顶破火山口周围的环状底流环流主要将其限制在山顶的西南部分,东南和北部侧翼的扩散有限。与观测到的扩散模式最匹配的计算机模拟表明,火山灰是通过中等传热率(~ 109 W)从一个小的热液巨柱和共生熔岩流中被抛到~ 250质量的。采用较低的热传递率的模型,仅仅从冷却的熔岩流中,只能将最细的物质抛到海底上方225米的地方,即使在强烈的海底水流状态下,也无法重现观察到的扩散模式。放射性碳年龄和岩石地层学表明,标志层形成于约600年BP,在破火山口形成之后,发生在1400年至1000年BP之间。化学地层学趋势表明,在火山口形成后的几百年里,火山喷发释放出了更多的原始岩浆(8.0-9.7 wt% MgO)。这一观察结果被解释为反映了地壳渗透率的灾难性变化,这种变化减少了地壳储层的体积和岩浆储存时间,从而使岩浆迅速上升到地表。
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来源期刊
Geochemistry Geophysics Geosystems
Geochemistry Geophysics Geosystems 地学-地球化学与地球物理
CiteScore
5.90
自引率
11.40%
发文量
252
审稿时长
1 months
期刊介绍: Geochemistry, Geophysics, Geosystems (G3) publishes research papers on Earth and planetary processes with a focus on understanding the Earth as a system. Observational, experimental, and theoretical investigations of the solid Earth, hydrosphere, atmosphere, biosphere, and solar system at all spatial and temporal scales are welcome. Articles should be of broad interest, and interdisciplinary approaches are encouraged. Areas of interest for this peer-reviewed journal include, but are not limited to: The physics and chemistry of the Earth, including its structure, composition, physical properties, dynamics, and evolution Principles and applications of geochemical proxies to studies of Earth history The physical properties, composition, and temporal evolution of the Earth''s major reservoirs and the coupling between them The dynamics of geochemical and biogeochemical cycles at all spatial and temporal scales Physical and cosmochemical constraints on the composition, origin, and evolution of the Earth and other terrestrial planets The chemistry and physics of solar system materials that are relevant to the formation, evolution, and current state of the Earth and the planets Advances in modeling, observation, and experimentation that are of widespread interest in the geosciences.
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