Stereoscopic and velocimetric reconstructions of the free surface topography of antidune flows

Intro Experiments Particle imaging Stereo Velocimetry Results Conclusions / references

2. Experimental set-up and imaging configuration

Experiments are conducted in a hydraulic flume having the following dimensions: length = 6 m; width = 50 cm; side wall height = 40 cm. The flume is tilted to obtain a bottom slope of 1 %. A 5 cm deep layer of loose sediment covers the flume bottom and is replenished during the flow by an upstream silo. Sand of nearly uniform size distribution is used as sediment material, and has the following characteristics: mean grain diameter = 1.65 mm; density = 2615 kg/m3. For the proof-of-concept experiments presented hereafter, the water inflow was not tightly controlled but rather loosely operated in order to produce a variety of patterns. Water discharges in the flume ranged from 15 to 35 l /s, yielding flow depths of 3 to 6 cm and Froude numbers in the range Fr = 1.4 to 2. For such high Froude numbers, the water free surface responds strongly to the underlying oscillatory topography of the bedforms, up to the point of breaking at the wave crests when antidunes are fully developed. The experimental parameters of the three runs selected for analysis are listed in Table 1.

Starting from a plane bed, the antidunes emerge as longitudinal trains of crests and troughs initiating from downstream but stationary in phase. The antidunes are observed to respond to transient changes in the flow rate (both increase and decrease) by temporarily growing in amplitude. Amplitude responses and gradual shifts in pattern occur on a time scale of tens of seconds. By contrast, on the shorter time scale corresponding to the image acquisition (of the order of 2 s), the hydrodynamics can be assumed to be quasi-steady and this is exploited hereafter to derive a single surface from each measurement sequence. The flow is however observed to exhibit small unsteady pulses, and this physical source of noise may slightly affect the results concurrently with measurement errors.

The short wavelength features of the water surface itself are not suitable for either matching or tracking. Specular reflection changes the appearance of these features when viewed from different angles. They also continuously evolve in time under the action of capillarity and gravity. Floating particles dispersed on the water free surface are used instead as tracers. The tracer particles are white wooden pearls 9 mm in diameter. The measurement section is placed some 2 m upstream of the flume outlet. Further upstream and moments before image acquisition, a uniform dispersion of floats is dropped onto the mean surface by means of staggered metal meshes.

Image sequences are obtained using digital cameras placed above the flow. The velocimetric and stereoscopic methods require rather different image acquisition systems, hence some care is necessary in order to operate them simultaneously and observe the same scene. Two commercial digital cameras (miniDV, PAL, 25 frames per second) are used for the stereoscopic measurements. These cameras offer good image resolution (768 by 576 pixels) but cannot be synchronised with each other during the acquisition. To avoid motion-stereo ambiguity, it will thus be necessary to synchronise them a posteriori using an interpolation procedure (see below). The stereo cameras are placed above the flow with oblique optical axes contained in a vertical plane parallel to the direction of flow (see Fig. 2). For the velocimetric measurements, on the other hand, a high frame rate camera (250 frames per second; resolution of 239 by 192 pixels) is placed directly over the flow with a nearly vertical optical axis. Due to the high frame rate, this camera requires strong lighting, obtained with four 2 kW light sources. Such powerful lighting saturates the commercial cameras even at maximum shutter speed, and these have to be fitted with dimming filters.

Imaging configuration for the antidune experiments

Figure 2. Imaging configuration for the antidune experiments.

After positioning, the viewpoints of all three cameras are determined by placing a calibration target in their shared viewing volume. This is essential for stereo reconstruction and allows the results of the two methods to be obtained in the same three-dimensional referential. For ease of reference in the next sections, we adopt labels V = L, R, and T to identify the three viewpoints. Labels L and R designate the left and right oblique cameras used for stereoscopic reconstruction, while label T refers to the top camera used for velocimetric reconstruction. The camera configuration shown on Fig. 2b is reconstructed based on actual calibrated viewpoints.