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Titel Internal tides and energy fluxes over Great Meteor Seamount
VerfasserIn T. Gerkema, H. Haren
Medientyp Artikel
Sprache Englisch
ISSN 1812-0784
Digitales Dokument URL
Erschienen In: Ocean Science ; 3, no. 3 ; Nr. 3, no. 3 (2007-10-01), S.441-449
Datensatznummer 250001102
Publikation (Nr.) Volltext-Dokument vorhandencopernicus.org/os-3-441-2007.pdf
 
Zusammenfassung
Internal-tide energy fluxes are determined halfway over the southern slope of Great Meteor Seamount (Canary Basin), using data from combined CTD/LADCP yoyoing, covering the whole water column. The strongest signal is semi-diurnal and is concentrated in the upper few hundred meters of the water column. An indeterminacy in energy flux profiles is discussed; it is argued that a commonly applied condition used to determine these profiles is in fact invalid over sloping bottoms. However, the vertically integrated flux can be established unambiguously; the observed results are compared with the outcome of a numerical internal-tide generation model. For the semi-diurnal internal tide, the vertically integrated flux found in the model corresponds well to the observed one. The observed diurnal signal appears to be largely of non-tidal origin.
 
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