The results displayed in the following are based on the vector field maps assessed from pairs of PIV particle images by means of the adaptive correlation method, as implemented in data processing.
3.1. Analytical Characterization of the Experimental Waves
The models described in
Section 2.2 were taken into account and their reliability in reproducing the experimental waves generated was tested. To allow a consistent comparison between theoretical and experimental waves, we specifically referred to the streamwise velocity component
u, suitably treated. Considering a fixed position (in our case
), we computed
u(
t) through all the aforementioned analytical models. We used the following procedure for both cases W1 and W2 to extract the velocity measurements for the wave cycle from the experimental time series. We examined the streamwise velocity measured in a large number of points distant and undisturbed by the cylinders, both in the vertical plane upstream (
Figure 2a) and in the horizontal plane (
Figure 2b). For each measurement, the phase averaging technique was used to process the
u(
t) signal, so that it was decomposed in a time-averaged value
U, a phase-averaged value
up(
t) and a turbulent fluctuation
u’(
t) [
17]. The ensemble-averaged value
<u(
t)
> was also taken into account with the sum
. This phase averaging operation was applied to the eight waves measured, even if the assumption made of a solitary wave actually implies a non-periodical wave. We decided to follow this procedure because in this way (i) we could account for more robust and consistent measurements, not referring to a single episodic wave event, (ii) and we could operate statistics and extract turbulent components from the signal. Consequently, we were able to compare the trends of the theoretical
u varying in the wave cycle with the corresponding phase-averaged experimental values
up. As an example, for a selected point representative of the undisturbed hydrodynamic condition (far from the cylinder C2 and having coordinates
X = 10.95 m,
Y = 0.07 m and
Z = 0.035 m),
Figure 3 shows the comparison among the computed values of
u and the measured
up (normalized by the time-averaged velocity
U). The time-averaged velocity in the two experiments is
U = 0.28 m/s for W1 and
U = 0.40 m/s for W2, respectively.
In qualitative terms, for both waves W1 and W2, the WH method seems to show the best matching with the experimental data, while the linear model provides the largest overestimations in absolute terms. To evaluate the agreement also in quantitative terms, the Wilmott index
was considered [
23]:
where
and
are, respectively, the computed and the experimental values; the overbar stands for the corresponding average value; and
N is the total number of data in a wave cycle. The
index takes a value of 1 when a perfect agreement is obtained. If calculated for the whole wave cycle, it provides the highest values for the WH method for both W1 and W2 waves, resulting
= 0.99 and
= 0.97, respectively.
In any case, at a closer inspection, a worse agreement can be observed between the measured data and the WH data during the wave crest transit. Thus, we also computed
for partial data intervals, namely for the positive velocity values (typical of the wave crest transit) and for the negative velocity values (typical of the wave trough transit). The resulting indexes are shown in
Table 2.
It is evident that for wave W1, the WH method is the best suited one along the whole wave cycle. For wave W2, it remains the best referring to the wave trough; while for the wave crest case, the PER model better reproduces the velocities
up. It is worth noting that we obtain analogous results (within ±2%, i.e., comparable to PIV accuracy) even when experimental velocities are examined at other undisturbed points. Finally, these results are also consistent with Iwagaki’s abacus [
15].
3.2. Upstream Vertical Profiles of the Streamwise Velocity
For both W1 and W2 waves, we analyzed the FoVs in the vertical plane, upstream the cylinder (
Figure 2a). The flow field was observed both in stationary condition (i.e., base flow) and in wave condition, during the transit of the long wave. The vertical profiles of the ensemble-averaged velocity display a quite flat and uniform trend along most
Z, during each phase of the wave. Apart from the typical values of the ratio
h/L and the indications of Iwagaki’s abacus already written in
Section 2.2, it was this observation that led us to address theoretically shallow water waves characterized by a condition of homogeneous flow along
Z. The rapid release of the added mass into the laboratory flume head tank produced a long flooding wave that promptly affected the entire water depth from the most superficial layer towards the channel bottom. The effect of the bottom on the flow is most visible during the descending wave phase when a reduction in velocity is generally assessed over the entire depth, but is even faster in the range
Z/
h < 0.4. In this range, for both waves, the logarithmic trend typical of uniform flow in open channels is identifiable.
Figure 4 displays, as an example, the vertical distribution of <
u> normalized by
U at four different wave phases, in the profile at
X = 10.842 m (i.e., at 0.058 m upstream of the cylinder) and
Y = 0.10 m, for both W1 and W2. For wave W1 the phases addressed are (
Figure 4a):
t/
T = 0.05, i.e., the wave trough;
t/
T = 0.3, i.e., the ascending wave phase;
t/
T = 0.65, i.e., the wave crest; and
t/
T = 0.8, i.e., the descending wave phase. Analogously, for wave W2, we have (
Figure 4b):
t/
T = 0,
t/
T= 0.3,
t/
T = 0.55, and
t/
T= 0.7, respectively.
The vertical profiles were obtained by stitching the instantaneous velocity maps of the two FoVs upstream of the cylinder. In fact, we originally acquired a top FoV and a bottom FoV, which overlapped 0.005 m along their common edge, as plotted in
Figure 2a. In particular, for the W1 wave the lower edge of the bottom FoV was positioned at
Z = 0.01 m, while W2 was at
Z = 0.03 m, in order to ensure the measurement by the PIV in the upper region during wave crest transit. This transit is evident from the increasing relative heights
Z/
h where velocities were measured. In fact, in the trough condition the highest point investigated is close to
Z/
h ≅ 1 in both waves, while in the crest condition, it is close to
Z/
h ≅ 1.2 for W1 and
Z/
h ≅ 1.4 for W2 consistently with the wave heights. We observed increasing values of <
u> due to the wave transit, as expected, reaching maxima values under the wave crest, with <
u> = 1.24
U for W1 and <
u> = 1.4
U for W2. Recalling that <
u> is the sum of the time-averaged component and the phase-averaged velocity, we can equally write that the initial current flow at most increases by about 24% and 40%, respectively, for W1 and W2 due to the wave crest transit. In addition, approaching from the trough to the crest condition, the <
u> values double for W1, while increasing 3.5 times for W2, meaning that a more pronounced effect of the wave on the underlying current is evident in the W2 case rather than in the W1 case.
Plotting the same vertical profiles of <
u> normalized by the maximum value of <
u> detected at each profile (named
max<
u>), we obtain
Figure 4c, where all profiles tend to collapse and clearly show a flat trend for
Z/
h > 0.4. For
Z/
h < 0.4 the logarithmic trend of <
u> is easily recognizable, especially in the W1 case, having measured points closer to the bottom. However, for both cases a bottom boundary layer with a thickness
δ ≅ 0.4
h is clearly detected, regardless of the wave phase.
3.3. Downstream Horizontal Maps of Streamwise Velocity and Vorticity
The horizontal maps of
<u>/U measured at
Z = 0.03 m are displayed in
Figure 5. For the sake of brevity, only the maps corresponding to the trough and crest phases already selected and shown in
Figure 4 are depicted. For greater convenience, a new local reference system (
x,
y) was chosen in the FoV, with the origin in the center of the cylinder.
Some spurious results close to the left edge of the frame are present, due to some technical limitations in the lighting system during PIV acquisition. They do not affect the signal downstream of the cylinder in the area of greatest interest, but we decided to mask them to avoid misinterpretations. For both tests, a shaded area downstream of the cylinder is always present, as expected, showing negative <
u> values in the near wake. Due to a less intense base flow and a lower wave height in W1, the absolute values of <
u> are lower than those in W2, both in the trough (
Figure 5a) and in the crest (
Figure 5b). Further, the higher
U value for W2 determines a more extended shaded area (
Figure 5c,d). In fact we observe negative values of <
u> for
x/
d = 0 ÷ 3 in the W1 case and up to
x/d ≅ 4 in the W2 case. Instead, the transversal spreading of such negative velocities is of order O(
d) for both tests. The inversion of the sign of <
u> delimits the shaded area, with values close to zero along its edge. As a result, a recirculation arises, with eddies detaching from the cylinder and antisymmetric with respect to the local
X axis, as already observed in uniform flows. However, the transit of the solitary wave, and thus the presence of a trough and a crest condition, induces a variation in the vorticity distribution and in the characteristics of coherent turbulent eddies, as explained below.
The vorticity <
Wz> in the horizontal plane at
Z = 0.03 m was computed starting from the ensemble-averaged streamwise <
u> and spanwise <
v> velocity components measured by the PIV.
Figure 6 displays the corresponding horizontal maps for trough and crest phases, for W1 and W2, respectively.
Even in these plots the areas with rough data are masked, showing unreliable results. Opposite values of vorticity are observed downstream of the cylinder, mainly clockwise (negative) for
y/d > 0 and anticlockwise (positive) for
y/d < 0 consistently with the stationary case of a flow investing a cylinder. During the wave cycle, from trough to crest condition, the cylinder Reynolds number
increases, due to the increase in <
u>, from 3400 to 6800 for W1 and from 3600 to 11,200 for W2. Thus, a more intense fully turbulent vortex street appears, as evident by comparing
Figure 6a,b as well as by comparing
Figure 6c,d. The antisymmetry of vorticity along the
X axis is generally kept, with the highest values of
Wz located at the trailing edge of the shaded area, while a spreading of vorticity with lower intensity is noted outside. In crest conditions, the values of
Wz increase, especially for the W2 case where they are in the range (−0.8 ÷ 0.8) Hz, while for the W1 case they remain in the range (−0.6 ÷ 0.6) Hz.
3.4. Turbulent Coherent Structures
Methods based on vorticity magnitude were used fairly extensively to identify vortices in the flow. Nevertheless, it should be considered that shear layers also exhibit high vorticity magnitudes. Turbulence structures essentially evolve from the interactions between vorticity and strain rate, so in the present study, to better characterize coherent turbulent vortices in the flow, we applied the continuous wavelet transform (CWT), a power tool capable of pinpointing regions with different spatial and temporal scales in turbulent flows [
24], thus providing continuous time-frequency identification of eddy structures.
Classical methods to decompose the velocity signal into frequency bands have invariably been based on the Fourier transform [
25]. That is, the underlying assumption is that the same spectral components are always present in a signal. However, this approach is not particularly suited for the treatment of non-stationary signals, such as in the present case, where we distinguish and establish the length and time scales of the coherent structures residing downstream of the cylinder.
The CWT approximates a complex function as a weighted sum of simpler functions, which themselves are obtained from one simple prototype function Ψ, called the mother wavelet. Several functions can be used as the mother wavelet and we assumed the Morlet one [
24,
26]. In CWT, the temporal distribution of the frequency components of the signal is found by successively passing stretched and compressed versions of the function Ψ, throughout the signal. By decomposing a time series into time-frequency space, one is able to determine both the dominant modes of variability and how those modes vary in time [
22].
For both waves we operated in the same way, but for convenience, we firstly focused on the results of the W2 wave. We selected six reference points in the horizontal plane (at
Z = 0.03 m), along two different transversal sections at relative distances
x/d = 2.5 and
x/d = 3.5, and specifically: O1(
x/d = 2.5,
y/d = 1.5), O2(
x/d = 3.5,
y/d = 1.5), E1(
x/d = 2.5,
y/d = 1), E2(
x/d = 3.5,
y/d = 1) I1(
x/d = 2.5,
y/d = 0.5), and I2(
x/d = 3.5,
y/d = 0.5). Points O1 and O2 are outside the cylinder wake; points E1 and E2 are located at the trailing edge; points I1 and I2 are inside the wake (refer to
Figure 6 for points location). For each point, the time series of the turbulent streamwise velocity
u’(
t) to be processed by CWT was obtained by stitching the
u’(
t) signals of the eight consecutive waves generated in the channel and cutting out the time interval between two succeeding waves. For the six target points,
Figure 7a–f display the
u’(
t) time series, the corresponding scalogram obtained with CWT, and the global wavelet spectrum. The scalogram is the wavelet power spectrum where the highest values in the contour plot correspond to the most energetic frequencies of the signal. The black line represents the cone of influence for the wavelet, meaning that values external to such cone are untrusted because they are too close to the extremes of the time series. The global wavelet spectrum is obtained for each frequency scale from the integral of the wavelet power calculated over the period of investigation.
Considering points O1 and O2 (
Figure 7a,d) in the wavelet power spectrum low intensities are generally observed, except than in the range of frequencies (0.0625 ÷ 0.25 s
−1) where more energetic spots are evident during most of the examined time interval. They are related to the presence of large coherent structures which retain the maximum turbulent power, as can easily be seen by observing the global wavelet spectrum. According to [
24,
25], we can rely on the well-known Taylor’s approximation to convert the time scale
1/f into the length scale
λ. That is
, where
is a proper velocity scale, greater than the turbulent velocity. In the present case, following [
26], we assumed the local ensemble-averaged velocity <
u> as
, resting on the assumption that it conveys downstream of the coherent structures. As a result, the above written large coherent structures outside the wake have corresponding length scales with an order of magnitude in the range O(10
0 ÷ 10
−1 m), in particular varying between one-tenth of the wavelength
L/10 and the flume width
B, thus controlled by the flume geometry.
The results of the wavelet power spectrum for points E1 and E2 along the edge (
Figure 7b,e) are also remarkable. Moreover, in this case, high intensities in the wavelet spectrum occur at frequencies (0.0625 ÷ 0.25 s
−1), manifesting again the presence of large coherent structures similar to what was already noted for O1 and O2 points, even if characterized by lower power values. More interestingly, in E1 and E2, high power spots are visible even at higher frequencies (2 ÷ 3.5 s
−1), thus, we would expect them to represent small eddies. Considering that they appear only during the peak phase of the wave (as evident by moving on the time axis in
Figure 7b,e), in the computation of the associated length scales we used the <
u> velocity assessed at the wave crest; therefore, their length scales result in the range (10
−2 ÷ 10
−1 m). More precisely, the spectrograms of
Figure 7b,e show that, when the wave crest is approaching, coherent structures with the size of order of the cylinder diameter O(
d) are present along the edge; during the transit of the crest, such structures become larger and are affected by the wave height with
λ values around O(4
H).
Figure 7c,f display the CWT results for points I1 and I2 inside the wake but close to the edge, where a behavior analogous to what was already observed for points E1 and E2 is detected. In this case, the structures at frequencies (0.0625 ÷ 1 s
−1), present during most of the recorded time period, show again a higher turbulent power, comparable to O1 (
Figure 7a) and O2 (
Figure 7d) cases. The power intensity of the smaller coherent structures arising at higher frequencies (2 ÷ 3.5 s
−1) is quite the same as for points E1 (
Figure 7b) and E2 (
Figure 7e).
Referring to the coherent structures detected in the W1 case, when investigated with CWT, the turbulent power values in the spectrograms are generally halved compared with the W2 case. Nevertheless, results are similar to the W2 case in terms of frequency of occurrence of the detected coherent structures. Moreover, the order of magnitude of the length scales of the eddies is generally kept, even if their size is reduced compared with the W2 case. The reduced size of vortices behind the cylinder in the case of lower wave amplitudes was also observed by [
27] for harmonic waves. For brevity, only one result for the W1 case is shown in
Figure 8, referring to a representative point along the trailing edge, namely E3, at
x/d = 3, and
y/d = 1.
We can also consider the dimensionless Strouhal number St to compute the frequency of vortex shedding from the cylinder fs. Using the local <u> as the reference velocity scale and the diameter d as the characteristic length of the obstacle in St and posing St = 0.2, we obtain a shedding frequency varying from fs~2 s−1 in absence of the wave (for both W2 and W1 cases) and fs~3 s−1 for the W1 wave crest transit or fs~4 s−1 for the W2 wave crest transit. Thus, such values are consistent with those of the eddies detected with the CWT method along the edge and inside the wake of the cylinder.
The global reading of the analysis conducted with the CWT reveals that the most energetic turbulent eddies in the horizontal plane, downstream of the cylinder, are large and have size varying in the range O(10−1 ÷ 100 m), regardless of the position considered in the FoV. Along the edge and inside the wake other coherent structures appear at higher frequencies, consistent with the Strouhal frequency. In absence of the wave, they have the size of order of the cylinder diameter, while during the transit of the wave crest their size are of order O(4H), i.e., they depend on the wave height. This event, occurring during the transit of the long wave crest, is in fact due to the augmented <u> velocity produced by the wave itself.