Ryan A. Portner, Guangyu Xu, Arran P. Murch, David A. Clague, Brian M. Dreyer, Jennifer B. Paduan
{"title":"胡安德富卡海岭轴向海山的洋中脊(MOR)火山灰扩散","authors":"Ryan A. Portner, Guangyu Xu, Arran P. Murch, David A. Clague, Brian M. Dreyer, Jennifer B. Paduan","doi":"10.1029/2025GC012229","DOIUrl":null,"url":null,"abstract":"<p>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 (∼10<sup>9</sup> 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.</p>","PeriodicalId":50422,"journal":{"name":"Geochemistry Geophysics Geosystems","volume":"26 9","pages":""},"PeriodicalIF":3.0000,"publicationDate":"2025-09-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://agupubs.onlinelibrary.wiley.com/doi/epdf/10.1029/2025GC012229","citationCount":"0","resultStr":"{\"title\":\"Mid-Ocean Ridge (MOR) Ash Dispersal on Axial Seamount, Juan de Fuca Ridge\",\"authors\":\"Ryan A. Portner, Guangyu Xu, Arran P. Murch, David A. Clague, Brian M. Dreyer, Jennifer B. Paduan\",\"doi\":\"10.1029/2025GC012229\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>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 (∼10<sup>9</sup> 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.</p>\",\"PeriodicalId\":50422,\"journal\":{\"name\":\"Geochemistry Geophysics Geosystems\",\"volume\":\"26 9\",\"pages\":\"\"},\"PeriodicalIF\":3.0000,\"publicationDate\":\"2025-09-16\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://agupubs.onlinelibrary.wiley.com/doi/epdf/10.1029/2025GC012229\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Geochemistry Geophysics Geosystems\",\"FirstCategoryId\":\"89\",\"ListUrlMain\":\"https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2025GC012229\",\"RegionNum\":2,\"RegionCategory\":\"地球科学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"GEOCHEMISTRY & GEOPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Geochemistry Geophysics Geosystems","FirstCategoryId":"89","ListUrlMain":"https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2025GC012229","RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
Mid-Ocean Ridge (MOR) Ash Dispersal on Axial Seamount, Juan de Fuca Ridge
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.
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.