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Cited by 465

The DOI matches its Crossref record; 91 of the 91 references it cites were found in a registry or an index.

Fluids in accretionary prisms

Langseth, M. G., Casey Moore, J.·1990·Eos, Transactions American Geophysical Union

Abstract

Subduction zones are the most dynamic tectonic environments on the face of Earth. Most subduction zones are submarine and at many, large accretionary prisms are formed of sediments scraped from the subducting oceanic lithosphere. These prisms grow in a water‐saturated environment; consequently, their tectonic, thermal and chemical evolution is strongly influenced by fluids, and the role of the aqueous phase must be considered in any study in this realm. In view of widespread and growing interest, the North Atlantic Treaty Organization and National Science Foundation sponsored the workshop “The Role of Fluids in Sediment Accretion, Deformation, Diagenesis and Metamorphism at Subduction Zones,” which convened September 19–23, 1988, at Il Ciocco, Tuscany, Italy. This meeting assembled 60 geologists, geochemists and geophysicists representing eight countries whose interests spanned both marine and continental environments.

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Metadata

Authors
Langseth, M. G., & Casey Moore, J.
Venue
Eos, Transactions American Geophysical Union
Published
1990-01-30
Volume
71
Issue
5
Pages
245-246
ISSN
  • 0096-3941 (ISSN-L)
  • 2324-9250
OpenAlex
W1971534802
Cited by
465
References
91
FWCI
5.98
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Fluids in accretionary prisms. https://app.cochat.ai/papers/10.1029/90eo00031
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Langseth, M. G., & Casey Moore, J. (1990). Fluids in accretionary prisms. Eos, Transactions American Geophysical Union. https://doi.org/10.1029/90eo00031

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