1990
DOI: 10.1111/j.1365-246x.1990.tb04586.x
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Heat flow maintained in ocean basins of great age: investigations in the north-equatorial West Pacific

Abstract: S U M M A R YMultipenetration heat flow measurements have been made at four sites in deep basins of the west-central Pacific Ocean: the West Mariana Basin, Central Mariana Basin, Nauru Basin and Central Pacific Basin. The final heat flows are, respectively, 46.6 f 0.5, 49.4 f 0.2, 44.2 f 0.9 and 49.5 f 1.1 mW m-*. Each site was surveyed bysingle-channel seismic reflection profiling, and provided a gravity core. The instrument measured thermal conductivity in situ over the entire depth intervals used for determ… Show more

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Cited by 62 publications
(62 citation statements)
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“…This suboceanic heat flow varies from several hundreds of milliwatts per square meter at mid-oceanic ridges to about 50 mW m −2 over oceanic lithosphere older than 80 Myr (Lister et al, 1990). When thermal effects of hydrothermal circulation are removed, this variation is well explained by the cooling plate model.…”
Section: Mantle Heat Flow Variationsmentioning
confidence: 62%
“…This suboceanic heat flow varies from several hundreds of milliwatts per square meter at mid-oceanic ridges to about 50 mW m −2 over oceanic lithosphere older than 80 Myr (Lister et al, 1990). When thermal effects of hydrothermal circulation are removed, this variation is well explained by the cooling plate model.…”
Section: Mantle Heat Flow Variationsmentioning
confidence: 62%
“…Considering the thermal evolution of terrestrial planets is beyond the scope of this study, and we use the Earth's oceanic lithosphere as a reference point and take the interior temperature T i as $1700 K and surface heat flux in the old oceanic lithosphere as 40 mW/m 2 (Parsons and Sclater, 1977;Lister et al, 1990;Stein and Stein, 1992). Since the scaling laws used in this paper are derived from calculations using Newtonian rheology, we use the activation energy of diffusion for olivine which is about 375 kJ/mol (Hirth and Kohlstedt, 2003).…”
Section: Physical Parameters For Terrestrial Planetsmentioning
confidence: 99%
“…Dans les océans, le flux est élevé près de la ride médio-océanique (une moyenne globale de 110 mW-m" 2 , Jessop, 1990), et diminue systématiquement vers les bassins et fossés océaniques (48 mW-m~2, Lister et al, 1990). L'explication généralement acceptée est que la lithosphère océanique se refroidit en s'éloignant de la ride.…”
Section: Résuméunclassified