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The burst-sweep dynamics study <strong>of</strong> Utami & Ueno (1987) , used flow<br />

visualisations taken by two still cameras for picture processing<br />

<strong>of</strong> horizontal cross-sections taken just above each other at 0.2s<br />

intervals. They proposed a detailed mechanism for the flow<br />

structure as shown in figure 1. From their visualisations they<br />

concluded that a perturbation in the high shear and vorticity<br />

layer very close to the wall (ie the viscous sublayer) produced<br />

vortex filaments in this sublayer which were lifted and elongated<br />

by the mean shear flow. Such vortices interacted with each other<br />

forming a horseshoe vortex as in figure la.<br />

Utami and Ueno then proposed that the horseshoe vortices rolled<br />

around each other and were stretched further to give the large<br />

scale spiral and slightly inclined vortex shown in figures lb,c.<br />

The fluid between the legs <strong>of</strong> the main spiral would thus be<br />

driven in the upstream-upward direction consistent with an<br />

ejection and the outer fluid would be driven in the downstreamdownward<br />

direction, consistent with a sweep.<br />

Whether this work presents an accurate picture is still open to<br />

debate, but it is given some credence by the work <strong>of</strong> Acarlar &<br />

Smith (1987a,b), who studied hairpin vortices shed firstly from<br />

a hemispherical protuberance and secondly by fluid injection in<br />

a developing laminar boundary layer. Their visualisations (shown<br />

in figure 2) and hot-film-anemometry studies have shown that such<br />

boundary layers develop remarkably similar velocity pr<strong>of</strong>iles to<br />

those found in a turbulent boundary layer, and that the hairpins<br />

interacted in the exact same way as described by Utami and Ueno.<br />

Al-5

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