Over het archief
Het OWA, het open archief van het Waterbouwkundig Laboratorium heeft tot doel alle vrij toegankelijke onderzoeksresultaten van dit instituut in digitale vorm aan te bieden. Op die manier wil het de zichtbaarheid, verspreiding en gebruik van deze onderzoeksresultaten, alsook de wetenschappelijke communicatie maximaal bevorderen.
Dit archief wordt uitgebouwd en beheerd volgens de principes van de Open Access Movement, en het daaruit ontstane Open Archives Initiative.
Basisinformatie over ‘Open Access to scholarly information'.
one publication added to basket [381148] |
Direct observations of general geothermal convection in deep Mediterranean waters
In: Ocean Dynamics. Springer-Verlag: Berlin; Heidelberg; New York. ISSN 1616-7341; e-ISSN 1616-7228, meer
| |
Author keywords |
Deep Western Mediterranean; High-resolution moored temperature observations; Geothermal heating outside volcanic vents; Convection turbulence directly observed |
Abstract |
Like elsewhere in the deep sea, life in the deep Mediterranean depends on turbulent exchange across the stable vertical density stratification for supply of nutrients and oxygen. Commonly modelled, turbulent exchange is inversely proportional to the stratification rate. However, this proportionality depends on the particular turbulence type, whether it is driven by vertical current differences (shear) or by buoyancy (convection). While shear turbulence is well observed in stratified seas, direct observations of convection turbulence are limited. In this paper, high-resolution moored temperature observations show that Mediterranean Sea waters are not stagnant in the lower 109 m above the seafloor at 2480 m, although variations are in the range of only 0.0001–0.001 °C. In winter, convection turbulence is regularly observed. Fortnightly averaged spectra show a collapse to the inertial-subrange scaling of dominant shear turbulence for data from about 100 m above the seafloor, and to the buoyancy-subrange scaling of dominant convection turbulence at about 10 m above the seafloor. Time-depth images reveal details of convection turbulence driven from below, which is considered primarily due to general geothermal heating through the Earth crust not related to volcanic vents. When its observation is not masked by (sub-)mesoscale eddies that advect warmer, stratified waters from above, the geothermal heat flux matches the deep-sea turbulence dissipation rate, if in the calculations a mixing efficiency of 0.5 is taken typical for natural convection, integration is over 250 m above the seafloor as confirmed from shipborne CTD, and if maximum 2-m-scale buoyancy frequency replaces its 100-m-scale mean equivalent. |
IMIS is ontwikkeld en wordt gehost door het VLIZ.