2013
DOI: 10.3390/rs5073239
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Surface Imprints of Water-Column Turbulence: A Case Study of Tidal Flow over an Estuarine Sill

Abstract: Turbulent mixing in the ocean can, in some cases, be so intense as to leave surface imprints, or "boils", that are detectable from space. Examples include turbulent flow over a submerged obstacle and instability of large-amplitude internal waves. In this paper we examine the particular case of tidal flow over a ~60-m-deep sill, which forms a barrier for the flow of dense water from the Pacific Ocean into the Strait of Georgia. The flow response during flood tide is illustrated using visible and thermal-band sa… Show more

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Cited by 7 publications
(6 citation statements)
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References 31 publications
(47 reference statements)
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“…(a) Observed sea surface temperature of a cyclonic eddy in the Southern California Countercurrent. The image was taken on 1 February 2013 at 20:34 in the framework of SubEx (Marmorino et al, 2018). (b) Modelled salinity and (c) potential temperature of the cyclone C3 on 26 June at 15 m of depth (see Figs.…”
Section: Discussionmentioning
confidence: 99%
“…(a) Observed sea surface temperature of a cyclonic eddy in the Southern California Countercurrent. The image was taken on 1 February 2013 at 20:34 in the framework of SubEx (Marmorino et al, 2018). (b) Modelled salinity and (c) potential temperature of the cyclone C3 on 26 June at 15 m of depth (see Figs.…”
Section: Discussionmentioning
confidence: 99%
“…A growing number of airborne studies [10][11][12][13][14][15][16] demonstrated the power of this remote sensing modality to detect and image a wide variety of dynamical processes taking place at or below the air-sea interface. A mid-or long-wave infrared camera is capturing passive radiation emitted by the water no deeper than the skin layer, i.e., tens of microns.…”
Section: Infrared Methodsmentioning
confidence: 99%
“…16) near its tail with diameters of about 10 m and mean distances of 20 m. From a video, it appears that the spots are accompanied by breaking surface waves. Potentially, the spots are created by intense turbulent mixing (Marmorino et al, 2013). Because of the small scales it is certainly not possible to model the spots with R100, but it is weird that the model on the one hand reproduces filaments with width of 2 times the model resolution (200 m), and contrariwise, the smallest eddy sizes in R100 are around 1 km, i.e.…”
Section: Comparison Of Features With Observationsmentioning
confidence: 99%