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Heat flow, tectonics, and fluid circulation at the toe of the Barbados ridge accretionary prism

Journal Article · · Journal of Geophysical Research; (United States)
 [1]; ; ;  [2]; ;  [3];  [4];  [5]
  1. Inst. Francais de Recherche pour l'Exploitation de la Mer, Plouzane (France)
  2. Ecole Normale Superieure, Paris (France)
  3. Lamont-Doherty Geological Observatory, Palisades, NY (United States)
  4. Univ. Pierre et Marie Curie, Paris (France)
  5. Univ. of Birmingham (England)
Detailed patterns of near surface tectonics and heat flow were investigated at two locations at the toe of the Barbados Ridge accretionary prism. At the two locations, in the thickly sedimented southern portion of the prism near 12{degree}20{prime}N and in the northern area drilled during Ocean Drilling Program (ODP) leg 110 near 15{degree}32{prime}N, relative highs of heat flow were associated with zones of thrusting. The authors attribute them to upward advection of water rising from the decollement along faults through sediments. In the ODP area, a significant heating plate effect from warm fluids flowing along the decollement and thrusts is required to account for the high regional heat flow. This effect implies high rates of fluid flow at the decollement, which can only be non-steady state or would require massive lateral transport of fluids along strike.
OSTI ID:
5009494
Journal Information:
Journal of Geophysical Research; (United States), Journal Name: Journal of Geophysical Research; (United States) Vol. 95:B6; ISSN 0148-0227; ISSN JGREA
Country of Publication:
United States
Language:
English