Volcanic arcs fed by rapid pulsed fluid flow through subducting slabs
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00025798%3A_____%2F12%3A00000022" target="_blank" >RIV/00025798:_____/12:00000022 - isvavai.cz</a>
Výsledek na webu
<a href="http://www.nature.com/ngeo/archive/index.html" target="_blank" >http://www.nature.com/ngeo/archive/index.html</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1038/ngeo1482" target="_blank" >10.1038/ngeo1482</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Volcanic arcs fed by rapid pulsed fluid flow through subducting slabs
Popis výsledku v původním jazyce
At subduction zones, oceanic lithosphere that has interacted with sea water is returned to the mantle, heats up during descent and releases fluids by devolatilization of hydrous minerals. Models for the formation of magmas feeding volcanoes above subduction zones require largescale transport of these fluids into overlying mantle wedges. Fluid flow also seems to be linked to seismicity in subducting slabs. However, the spatial and temporal scales of this fluid flow remain largely unknown, with suggestedtimescales ranging from tens to tens of thousands of years. Here we use the Li?Ca?Sr isotope systems to consider fluid sources and quantitatively constrain the duration of subduction-zone fluid release at ~70 km depth within subducting oceanic lithosphere, now exhumed in the Chinese Tianshan Mountains. Using lithiumdiffusion modelling, we find that the wall-rock porosity adjacent to the flowpath of the fluids increased ten times above the background level. We show that fluids released by
Název v anglickém jazyce
Volcanic arcs fed by rapid pulsed fluid flow through subducting slabs
Popis výsledku anglicky
At subduction zones, oceanic lithosphere that has interacted with sea water is returned to the mantle, heats up during descent and releases fluids by devolatilization of hydrous minerals. Models for the formation of magmas feeding volcanoes above subduction zones require largescale transport of these fluids into overlying mantle wedges. Fluid flow also seems to be linked to seismicity in subducting slabs. However, the spatial and temporal scales of this fluid flow remain largely unknown, with suggestedtimescales ranging from tens to tens of thousands of years. Here we use the Li?Ca?Sr isotope systems to consider fluid sources and quantitatively constrain the duration of subduction-zone fluid release at ~70 km depth within subducting oceanic lithosphere, now exhumed in the Chinese Tianshan Mountains. Using lithiumdiffusion modelling, we find that the wall-rock porosity adjacent to the flowpath of the fluids increased ten times above the background level. We show that fluids released by
Klasifikace
Druh
J<sub>x</sub> - Nezařazeno - Článek v odborném periodiku (Jimp, Jsc a Jost)
CEP obor
DD - Geochemie
OECD FORD obor
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Návaznosti výsledku
Projekt
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Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2012
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Nature Geoscience
ISSN
1752-0894
e-ISSN
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Svazek periodika
5
Číslo periodika v rámci svazku
7
Stát vydavatele periodika
GB - Spojené království Velké Británie a Severního Irska
Počet stran výsledku
4
Strana od-do
489-492
Kód UT WoS článku
000307098400019
EID výsledku v databázi Scopus
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