U Journal Logos (RGB) Open Access Natural Hazards and Earth System Sciences Nonlinear Processes in Geophysics Open Access Open Access tural Hazards Earth System Sciences Open Access Open Access Nonlin. Processes Geophys., 20, 179–188, 2013 Advances in Annales www.nonlin-processes-geophys.net/20/179/2013/ doi:10.5194/npg-20-179-2013 Geosciences Geophysicae © Author(s) 2013. CC Attribution 3.0 License. Chemistry I. Didenkulova1,2 and A. Rodin1,2 and Physics 1 Laboratory Chemistry and Physics Open Access Open Access Discussions A typical wave wake from high-speed vessels: its group structure Atmospheric Atmospheric and run-up Measurement Measurement Correspondence to: I. Didenkulova ([email protected]) Techniques Techniques Open Access Open Access of Wave Engineering, Institute of Cybernetics at Tallinn University of Technology, Akadeemia tee 21, Discussions 12618 Tallinn, Estonia 2 Nizhny Novgorod State Technical University,Atmospheric Atmospheric Nizhny Novgorod, Russia Received: 2 September 2012 – Revised: 4 February 2013 – Accepted: 4 February 2013 – Published: 26 February 2013 Discussions Open Access Open Access 1 Introduction Abstract. High-amplitude water wavesBiogeosciences induced by highare regularly observed in Tallinn Bay, the Discussions Baltic Sea, causing intense beach erosion and disturbing maWaves induced by high-speed vessels, the depth Froude numrine habitants in the coastal zone. Such a strong impact on ber (the ratio of the ship’s speed and the maximum phase the coast may be a result of a certain group structure of of linear water waves for the given depth) of which the wave wake. In order to understand it, here we present Climatespeed during the regular sailing regime exceeds 0.6, have become Climate an experimental study of the group structure of these wakes of the Pasta subject of intensive study in the last ten years after the Pikakari beach, Tallinn Bay. The most energetic vessel of theatPast new generation of large and powerful ships operating at waves at this location (100 m from the coast at the Discussions water cruise speeds up to 30 knots has been introduced (Parnell and depth 2.7 m) have amplitudes of about 1 m and periods of Kofoed-Hansen, 2001; Parnell et al., 2007, 2008; Soomere, 8–10 s and cause maximum run-up heights on a beach up to Kurennoy et al., 2009, 2011; Torsvik et al., 2009; Ra1.4 m. These waves represent frequency modulated packets Earth System2007; paglia et al., 2011). It has been demostrated that these waves Earth System where the largest and longest waves propagate ahead of other Dynamics can be a major contributor of energy to sections of coasts smaller amplitude and period waves. Sometimes the groups Dynamics Discussionsthat are exposed to significant natural hydrodynamic loads of different heights and periods can be separated even within (Soomere, 2005a). The actual effect depends upon the feaone wave wake event. The wave heights within a wake are tures of the coastal environment and the existing hydrodywell described by the Weibull distribution, which has differGeoscientific namic loads. In this context, specific types of disturbances, ent parameters for wakes from different vessels.Geoscientific Wave run-up such as high leading waves, monochromatic packets of relanstrumentation Instrumentation heights can also be described by Weibull distribution and its parameters of the distri-andtively short waves, solitary and cnoidal wave trains ahead of Methods and can be connected to the parametersMethods the vessel and associated depression areas, all qualitatively bution of wave heights 100 m from the coast. Finally, the runData Systems Data Systems different from the usual wind waves or constituents of the up of individual waves within a packet is studied. It is shown Discussions linear Kelvin wake, are extremely important (Brown et al., that the specific structure of frequency modulated wave pack1989; Neuman et al., 2001; Garel et al., 2008). These specific ets, induced by high-speed vessels, leads to Geoscientific a sequence of wave disturbances have been observed, for example, in the Geoscientific high wave run-ups at the coast, even when the original wave Venice Lagoon, Italy (Rapaglia et al., 2011), Savannah River, Model heights are rather moderate. This feature canDevelopment be a key to unDevelopment Georgia (Houser, 2011), New Zealand and Denmark (Parnell derstanding the significant impact on coasts caused by fast Discussions and Kofoed-Hansen, 2001) and Tallinn Bay, Estonia (Parnell vessels. et al., 2008). Hydrology and All of these cases are characterized by the seriHydrology and ous damage of coastal environment. In the Marlborough Earth SystemSounds, New Zealand, the introduction of high-speed ferEarth System Sciencesries was accompanied by rapid and significant accretion Sciences ogeosciences speed vessels Open Access Open Access Open Access Open Access Open Access Open Access Open Access Open Access Open Access Open Access Discussions Ocean Science Discussions Open Acces cean Science Open Acces Published by Copernicus Publications on behalf of the European Geosciences Union & the American Geophysical Union. level oscillations were recorded. 180 I. Didenkulova and A. Rodin: A typical wave wake from high-speed vessels Fig. 1. Location scheme of the Baltic Sea and the study site. Fig. 1. Location scheme of the Baltic Sea and the study site. 4 Fig. 2. High-speed vessel wakes at the Pikakari beach, Tallinn Bay, Baltic Sea. Fig. 2. High-speed vessel wakes at the Pikakari beach, Tallinn Bay, Baltic Sea. The time of video-recording was synchronized with the time of the echosounder, so it (Parnell and Kofoed-Hansen, 2001). In contrast, in Tallinn cific shape of the coast, which allows anomalous “nonreflectwasand possible to linkgroups the wave height measured the echosounder and(Didenkulova run-up at theetcoast for Bay, Estonia, long energetic of vessel waves ating” wave behavior al., 2009b). resulted in dramatic beach at 86 wakes Even though the significant effect“Star”, of waves from higheacherosion wave in of theinitially wake. Inaccreting total, run-ups from were measured: 36 of them from Aegna Island (Parnell et al., 2008; Soomere et al., 2009). speed vessels on low-energy coasts has been demonstrated 31 from “SuperStar” and 19 from “Viking XPRS”. These groups could easily smooth out the emerging berm and for different basins and environments, the reason of its such sometimes exert very large run-up events (Didenkulova et al., strong impact still remains unclear. It can be partially con2009a; Soomere et al., 2009). The highest and longest ship nected to the net transport of water, excited by ships sailStatistics of waves and corresponding run‐ups in the wake waves from the first 3. group reached over 1 m above still waing at transcritical speeds, which may produce water level ter level with several examples going over 1.5 m above still set-up under groups of high vessel waves and result in a water level (DidenkulovaThe et al., 2009a; Torsvik et al., 2009). of thestudy coastof(Soomere et al., data set at Pikakari beach, Tallinn Bayrapid allowsreaction for a detailed the statistics of 2011). This efHowever, on a few days there was evidence of overwash defect may also be reinforced by the specific group structure vessel-induced waves and corresponding run-ups. The most energetic vessel waves at this posits at heights about 2 m above water level (Soomere et of vessel-induced waves, when the largest, the longest and location have amplitudes of one aboutvessel 1 m and periods the of 8-10 with maximum up more symmetric al., 2009). The loss of sediments caused by wake mostsec asymmetric wavesrun-up comeheights first and was up to 1 m3 per meter of the coastline (Soomere et al., waves of smaller amplitude and period come after. The charto 1.4 m. 2009). At Pikakari beach in Tallinn Bay, wake-induced sedacteristic properties of these groups are experimentally studAll measured wave wakes have a specific structure of frequency modulated packets, iment transport produced a stable convex nearshore beach ied in this paper for Pikakari beach in Tallinn Bay, the Baltic whereand theSoomere, largest and2011) longest wavestocome first andSea. waves of smaller amplitude and period after profile (Didenkulova similar a spe(Fig. 3). Sometimes the groups of different heights and periods can be separated even within one wake, as it is shown in Fig. 3a, where three groups of waves can be clearly identified. The Nonlin. Processes Geophys., 20, 179–188, 2013 www.nonlin-processes-geophys.net/20/179/2013/ highest waves (with a height of up to 1 m) usually belong to the first group and occur after the passage of several long, high-amplitude waves. I. Didenkulova and A. Rodin: A typical wave wake from high-speed vessels Water displacement, m 0.4 a 181 b 0.4 0.2 0.2 0 0 -0.2 -0.4 0 -0.2 2 4 6 8 10 12 -0.4 0 2 4 6 8 10 12 Time, min Time, min Fig.wakes 3. Vessel wakes from(18a)June “SuperStar” (18(20 June Fig. 3. Vessel from (a) SuperStar 2009), (b) Star June2009, 2009).16:15), b) “Star” (20 June 2009, 12:10). from Star, 23 fromwake SuperStar and 14by from ExperimentalThe set-up averaged distributions of wave heights29within the vessel computed theViking up- XPRS. Maximum wave heights (up to 1 m) occurred exclusively for crossing method are demonstrated in Figs. 4 andthe 5. longest The averaging was performed over alltypical 66 wind waves with periods ∼ 10 s whereas Tallinn Bay is a semi-sheltered bay in the almost tideless wave periods were 2–3 s. events (Fig.by 4)the and for each has crossed the bay several times Baltic Sea,recorded which is characterized relatively mildspecific wind shipInwhich addition, maximum run-ups of all wake waves were wave climate. Thethe peak periods wind waves are usually measureddistribution at the coastgathering manually,the by data following during time of theofobservations (Fig. 5). The average from the all inundawell below 3 s, reaching 4–6 s in strong storms and only in tion of each wake wave and using video recording from 12 ships might be reasonable, since all studied vessels aretill characterized similar lengths,between widths,the echo exceptional cases exceeding 7–8 s (Soomere, 2005b). The June 1 July 2009. by Since the distance significant wave height in the bay exceeds 0.5 m with a probsounder wave and coastal measurements was rather draughts and operational speeds and induce similar wakes, and, therefore, canshort be(slightly ability of 10 % (Soomere, 2005b). more than 2 wavelengths), it was easy to follow the propagaIn contrast to this low wave activity, Tallinn Bayheight reg- distribution. considered aswind an averaged wake wave It can bewave seenupthat waveshoaling tion of each particular to themost coast.ofA wake ularly hosts fast vessel traffic, with fairways located close on the beach at the experiment site is shown in Fig. 2. On the heightsand arevessels distributed within the interval and the number of particularly high waves in to the shoreline operating at cruise speeds up<30 to cmcoast, one can see a pole for the run-up measurements and 30 knots (Parnell et al., et al.,example, 2009; Soomere et farther heights offshore are a tripod, levelconstitute oscillations were the wake is 2008; ratherTorsvik low. For the waves whose largerwhere than sea 40 cm al., 2011). Fast vessel generated waves considerably exceed recorded. just 2% the wave heights one wake. fromofdifferent vessels itwas varies from 1%with the typical periods andof heights of wind waveswithin (Soomere, 2005a; For wakes The time video-recording synchronized Parnell et al., 2008). The periods of the highest waves are of time of the echo sounder, so it was possible to link the wave for “Viking XPRS”, 2% for “Star” and 3% for “SuperStar”. 8–15 s and their heights are up to 2 m depending on location height measured at the echo sounder and run-up at the coast (Parnell et al., 2008; Kurennoy et al., 2009, 2011). for each wave in the wake. In total, run-ups from 86 wakes An experiment focusing on the properties of vessel wakes were measured: 36 of them from Star, 31 from SuperStar and 6 and their impact on coasts was performed at the Pikakari 19 from Viking XPRS. beach, Tallinn Bay (Fig. 1) during the high traffic period 5 from 12 June till 1 July 2009. The environmental conditions in the period of the experiment were 4 rather low, with the 3 Statistics of waves and corresponding run-ups in wind wave background mostly of about 10 cm and reaching 3 the wake 40 cm during three days. The vessels of our interest were the high-speed ferries Star, SuperStar and Viking XPRS, follow2 The data set at Pikakari beach, Tallinn Bay, allows for a deing routes Helsinki–Tallinn. All three vessels are large contailed study of the statistics of vessel-induced waves and corventional ships with lengths of about1200 m and operational speeds of 30 knots, which are capable to generate largeresponding run-ups. The most energetic vessel waves at this 0 in Tallinn bay. Howhave of about 1 m and periods of 8–10 s amplitude, long and long-crested waves 0 0.1 0.2 0.3 location 0.4 0.5 amplitudes 0.6 0.7 with maximum run-up heights up to 1.4 m. ever, due to the variability in ship track and its speed along Wave height, m the track, the parameters of ship generated waves may vary, All measured wave wakes have a specific structure of freFig. values 4. Averaged distribution of wave the wave wake;packets, red dashed linethecorresponds quency modulated where largest and longest their averaged are described in Kurennoy et al.heights (2009). within Vessel generated waves were recorded using a downwardwaves come first and waves of smaller amplitude and period to the Rayleigh distribution ( =0.12 m), black solid line corresponds to the Weibull distribution after (Fig. 3). Sometimes the groups of different heights and looking ultrasonic echo sounder (LOG aLevel®) with a sam( =0.16onm, q =1.53) fitted using the maximum estimate. pling frequency of 5 Hz, mounted a stable tripod approxperiods can belikelihood separated even within one wake, as it is shown in Fig. 3a, where three groups of waves can be clearly idenimately 100 m from the shoreline, 2.4 km from the sailing tified. The highest waves (with a height of up to 1 m) usually line at a water depth of about 2.7 m from 17 June till 1 July belong to the first group and occur after the passage of sev2009, and were studied overall and with respect to the type of 6 the vessel. The record contains 66 clearly identifiable wakes: eral long, high-amplitude waves. pdf, m-1 2 www.nonlin-processes-geophys.net/20/179/2013/ Nonlin. Processes Geophys., 20, 179–188, 2013 f the wave heights within one wake. For wakes from different vessels it varies from 1% ng XPRS”, 2% for “Star” and 3% for “SuperStar”. 182 I. Didenkulova and A. Rodin: A typical wave wake from high-speed vessels wave fields, a generalization of Rayleigh distribution – twoparametric Weibull distribution is used. Since Rayleigh dis5 tribution fails to describe ship-generated waves, we follow the same scheme as for wind waves and apply two4 parametric Weibull distribution for a better fit. Both approximated distributions are plotted in Figs. 4 and 5. It can be 3 seen that Rayleigh pdf does not work well for description 2 of the waves in the vessel wake. The best observed fit is for the Viking XPRS. However, Weibull pdf seems to be a fairly 1 good model describing distribution of wave heights within a single vessel wake. Even though it underestimates the height 0 0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 of the distribution for waves of small (∼ 10 cm) amplitude, Wave height, m it describes well the distribution of all larger wave heights veraged distribution of wave heights within wavewithin wake;theredwave dashed>line corresponds Fig. 4. Averaged distribution of wavethe heights 15 cm. The mentioned discrepancy for small amplitude wake; red dashed line corresponds to the Rayleigh distribution waves can be related to the existence of wind wave backyleigh distribution =0.12 m), black solid lineto corresponds to the Weibull distribution (σ = 0.12(m), black solid line corresponds the Weibull distribuground, whose amplitudes were < 15 cm during most of the tion m, (σ =q0.16 m, qfitted = 1.53) fittedthe using the maximum likelihood time of the experiment except a few days. ( =0.16 =1.53) using maximum likelihood estimate. estimate. Approximated scale parameter σ remains the same for overall wave distribution (Fig. 4) and for distributions found for particular vessel types (Fig. 5) and is of the same order The averaged distributions6of wave heights within the for both Rayleigh and Weibull pdfs. It changes from 0.1 m till vessel wake, computed by the up-crossing method, are 0.13 m for Rayleigh distribution and from 0.15 m to 0.16 m demonstrated in Figs. 4 and 5. The averaging was performed for Weibull distribution. over all 66 recorded events (Fig. 4) and for each specific The shape parameter q in Weibull distribution varies more ship that crossed the bay several times during the time of significantly. It is equal to 1.53 for overall distribution and the observations (Fig. 5). The average distribution gatherreaches the value of 1.45 for Star, 1.52 for SuperStar and ing the data from all ships might be reasonable, since all 1.71 for Viking XPRS vessels. This variety can be explained studied vessels are characterized by similar lengths, widths, if we consider a physical meaning of the parameter q comdraughts and operational speeds and induce similar wave paring Weibull distribution with Glukhovsky distribution obwakes, and, therefore, can be considered as an averaged wake tained for description of sea wave statistics at intermediwave height distribution. It can be seen that most of wave ate water depth (Glukhovsky, 1966). Glukhovsky distribuheights are distributed within the interval < 30 cm and the tion has been obtained semi-empirically for wind waves in number of particularly high waves in the wake is rather low. the coastal zone of the Caspian Sea by including an addiFor example, the waves whose heights are larger than 40 cm tional parameter, the water depth. Since both Weibull and constitute just 2 % of the wave heights within one wake. For Glukhovsky distributions represent a generalization of the wakes from different vessels it varies from 1 % for Viking Rayleigh distribution, we use this analogy and apply it to XPRS, 2 % for Star and 3 % for SuperStar. ship-generated waves in shallow water. For this purpose it The obtained distributions of wave heights H within a is more convenient to consider cumulative distribution funcwave wake are approximated by the mostly used probability tions (cdf). For Weibull distributions it has the following density functions (pdf) in wave statistics: the one-parametric form Rayleigh pdf q " # H H H2 . (3) FW (H, σ, q) = 1 − exp − fR (H, σ ) = 2 exp − 2 , (1) σ σ 2σ The Glukhovsky cdf is described by the following expression described by the only one scale parameter σ , measured in m, (Glukhovsky, 1966) and two-parametric Weibull pdf q 2 1−H̄ / h q H q−1 H H π , fW (H, σ, q) = exp − , (2) FG H, H̄, h = 1 − exp − σ σ σ H̄ 4 1 + √H̄ pdf, m-1 6 2π h described by a scale parameter σ and a shape parameter q, using a nonlinear least squares method. Rayleigh distribution describes amplitudes of narrow-band Gaussian processes. However, sea wave measurements often deviate from Rayleigh. This is why, in oceanology, e.g. for wind Nonlin. Processes Geophys., 20, 179–188, 2013 (4) where H̄ is the mean wave height and h is the water depth. Comparing Eqs. (3) and (4) we find a connection between parameter σ and q in Eq. (3) and characteristics of wave field: www.nonlin-processes-geophys.net/20/179/2013/ I. Didenkulova and A. Rodin: A typical wave wake from high-speed vessels 6 183 a pdf, m-1 5 4 3 2 1 0 0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 Wave height, m pdf, m-1 6 6 b 5 5 4 4 3 3 2 2 1 1 0 0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0 0 c 0.1 0.2 0.3 0.4 0.5 Wave height, m Wave height, m Fig. 5. Averaged distribution of wave heights within the wave wake of a) “Star”, b) “SuperStar” Fig. 5. Averaged distribution of wave heights within the wave wake of (a) Star, (b) SuperStar and (c) Viking XPRS; red dashed line corresponds to the fitted Rayleigh distribution with corresponding parameter σ (a)to 0.12 (b) 0.13 m, (c) distribution 0.11 m; blackwith solid line corresponds to and c) “Viking XPRS”; red dashed line corresponds them, fitted Rayleigh the fitted Weibull distribution with corresponding parameters (σ , q) (a) (0.15 m, 1.45), (b) (0.16 m, 1.52), (c) (0.15 m, 1.71) fitted using the corresponding parameter a) 0.12 m, b) 0.13 m, c) 0.11 m; black solid line corresponds to the maximum likelihood estimate. fitted Weibull distribution with corresponding parameters ( , q ) a) (0.15 m, 1.45), b) (0.16 m, 1.52), c) (0.15 m, 1.71) fitted using the maximum likelihood estimate. 2.5 pdf, m-1 2 3/2 ! 1−H̄2 / h H̄ 4 2 distributions 2 The obtained of wave heights H within a wave wake are approximated by , σ = H̄ + . (5) q= π h density functions (pdf) 1.5 1 − H̄ / h the mostly πused probability in wave statistics: the one-parametric pdf, m-1 Rayleigh pdf 1 Taking into account the water depth at the location of conducted measurements (h = 2.7 m) and applying the mean 0.5 wave height (H̄ = 0.14 m), parameters of the Weibull dis-H H2 H ,which (1) 2 exp 2 , tribution can be estimated as σ ≈ 0.16 m and q ≈f R2.1, 200 0.2 0.4 0.6 0.8 1 1.2 1.4 are close to the values calculated from the original data. Runup height, m The averaged distributions of corresponding run-up heights on a beach, caused by a single wave wake are shown Fig. 6. Averaged distribution ofWeibull run-up heights within the wave by the only one scale parameter , measured in m, and two-parametric pdf the Averaged heights wave wake; red dashed in Figs. 6 and 7described for overall run-up distribution andFig. with6.rewake;distribution red dashed of linerun-up corresponds to within the Rayleigh distribution spect to vessels of different types. Similar to wave heights, (σ = 0.38 m), black solid (line corresponds to thesolid Weibull distribucorresponds to the Rayleigh distribution =0.38 m), black line corresponds to th these distributions can also be approximated by Rayleigh and q tion (σ = 0.56q m, q = 2.77) fitted using the maximum likelihood 1 q H estimate. H Weibull pdfs, which are marked by the corresponding ( =0.56 maximum likelihood estimat lines m, , q =2.77) fitted using the(2) fW H , , q distribution exp in Figs. 6 and 7, and it can be seen that the Weibull distribu tion works quite well even for description of run-up heights. 2.5 all distribution, 2.75 for Star, 2.93 for SuperStar and 2.70 a for However, the shape parameters are more diversed for run-up 7 Viking XPRS vessels. heights. For the Rayleigh distribution, σ = 0.38 m for over2 Knowing parameters of distributions, we can calculate the all distribution and for Star, 0.40 m for SuperStar and 0.33 m corresponding mean wave and run-up heights straight from 1.5 for Viking XPRS vessels. Similar to wave heights, scale pathe distribution: rameter in Weibull distribution for run-ups is slightly larger 1 Z∞ than the one for the Rayleigh pdf: σ = 0.56 m for overall distribution and for Star, 0.59 m for SuperStar and 0.49 m for H̄ = Hf (H ) dH , (6) 0.5 Viking XPRS vessels. The shape parameter q = 2.77 for over0 0 0 www.nonlin-processes-geophys.net/20/179/2013/ 2.5 0.2 0.4 0.6 0.8 1 1.2 1.4 RunupGeophys., height, m 20, 179–188, 2013 Nonlin. Processes b 3 Fig. 6. Averaged distribution of run-up heights within the wave wake; red dashed line corresponds to the Rayleigh distribution ( =0.38 m), black solid line corresponds to the Weibull 184 I. Didenkulova and A. Rodin: A typical wave wake from high-speed vessels distribution ( =0.56 m, q =2.77) fitted using the maximum likelihood estimate. 2.5 a pdf, m-1 2 1.5 1 0.5 0 0 0.2 0.4 0.6 0.8 1 1.2 1.4 Runup height, m 2.5 3 2 2.5 Knowing parameters of distributions, we can calculate the correspondingbmean wave and pdf, m-1 up heights straight from the distribution: c 2 1.5 1.5 1 H Hf H dH , 0.5 0 0 1 0.2 0.4 (6) 0.5 0 0.6 0.8 1 1.2 1.4 0 0 0.2 0.4 0.6 0.8 1 Runup height, m Runup height, m consider an average wave amplification on a beach. The calculated values of mean wave and Fig. 7. Averaged distribution of run-up heights within the wave wake of a) “Star”, b) Fig. 7. Averaged distribution run-up within the wave of (a)Rayleigh Star, (b) SuperStar and (c) Viking XPRS; red dashed line up heights, calculated from the originalofdata andheights reconstructed from thewake obtained “SuperStar” and c) “Viking XPRS”; redparameters dashed line corresponds to 0.40 the Rayleigh distribution corresponds to the Rayleigh distribution with corresponding σ (a) 0.38 m, (b) m, (c) 0.33 m; black solid line corresponds Weibull distributions for distribution overall statistics and for each vessel separately in (0.59 m, 2.93), (c) (0.49 m, 2.70) fitted using the to the Weibull with corresponding parameters (σ , q) (a) are (0.56presented m, 2.75), (b) with corresponding parameters a) 0.38 m, b) 0.40 m, c) 0.33 m; black solid line corresponds maximum likelihood estimate. 8. to the Weibull distribution with corresponding parameters ( , q ) a) (0.56 m, 2.75), b) (0.59 m, 2.93), c) (0.49 m, 2.70) fitted using thebution maximum likelihood are so close toestimate. each other that they practically coinRunup height, m 0.55 0.5 0.45 0.4 0.13 0.14 0.15 Wave height, m 0.16 0.17 cide, which strongly indicates that Weibull distribution is an 10 appropriate model for description of waves within a vessel wake. The heights reconstructed from Rayleigh distributions underestimate run-up observations by 10–20 %. Based on the calculated data, the corresponding regression curves of wave amplification at the coast can be plotted (Fig. 8). Though regression lines, based on four points only, are not satisfactory, they can still indicate some trend. In the case of the Rayleigh and Weibull distributions they can be described by the following expressions = 3.1 H̄, 8. Mean run-up and wave height in the wake, calculated from the original dataR̄(red squares) (7) Fig. 8. Mean run-up and wave height in the wake, calculated from the from original data (red squares) and reconstructed fromtriangles) Rayleigh distributions; blue d reconstructed Rayleigh (blue circles) and Weibull (black R̄ = 3.5H̄. (8) (blue circles) and Weibull (black triangles) distributions; blue solid olid and black dashed lines corresponds to the regression curve fitted the heights calculated and black dashed lines correspond to the regression curve fitted heights calculated from the Weibull distributions, reAs it has been noticed before, the Rayleigh approximation from the Rayleigh andRayleigh Weibulland distributions respectively. spectively. gives smaller amplification at the coast and underestimates run-up heights. It is remarkable that original values of mean wave and run-up heightsFor andcomparison, those we estimate the amplification of nonbreaking sinusoidal waves with a period T = 10 s, which corand consider an average wave amplification on a beach. The nstructed from the Weibull distribution are so close to each other that practically coinside, responds to the period of the largest vessel waves, by the calculated values of mean wave and run-up heights, calcuch strongly indicates that Weibull distribution is an appropriate model for shallow description offormula for long wave run-up on a plane beach water lated from the original data and reconstructed from the obes within tained a vessel wake.andThe heights reconstructed fromstatisRayleigh(Didenkulova distributionset al., 2007) Rayleigh Weibull distributions for overall s tics and for each vessel separately are presented in Fig. 8. erestimate run-up observations by 10-20%. Based on the calculated data, the corresponding R 2L It is remarkable that original values of mean wave and run=π √ ≈ 6. (9) ession curves wave amplification at the coastfrom can be 8). Though upofheights and those reconstructed theplotted Weibull(Fig. distriH regression ghT s based on four points only are not satisfactory, still they can indicate some trend. In the case Nonlin. Processes Geophys., 20, 179–188, 2013 he Rayleigh and Weibull distributions they can be described by the following expressionswww.nonlin-processes-geophys.net/20/179/2013/ wave height. This is clearly seen in Figs. 9b and 9c, where the absolute maximum wave heights are not so pronounced as in Fig. 9a and are just slightly larger than for other waves. I. Didenkulova and A. Rodin: A typical wave wake from high-speed vessels 185 Wave/runup heights, m 1 a 0.8 0.6 0.4 0.2 0 0 2 4 6 8 10 12 14 16 18 Time, min Wave/runup heights, m 0.8 1.2 c b 1 0.6 0.8 0.4 0.6 0.4 0.2 0.2 0 0 2 4 6 8 10 12 0 0 1 2 Time, min 3 4 5 6 7 8 9 Time, min Fig. 9. Wave heights (blue circles) and corresponding run-up heights (red triangles) within the Fig. 9. Wave heights (blue circles) and corresponding run-up heights (red triangles) within the wake from (a) SuperStar (19 June 2009), (b) Star (20 June 2009) (c)a)Viking XPRS (21 2009). wake and from “SuperStar” (19June June 2009, 19:15), b) “Star” (20 June 2009, 12:10) and c) “Viking XPRS” (21 June 2009, 13:50). 4 Run-up of individual waves in the vessel wake At the same time Fig. 9a with an outstanding peak for the highest wave demonstrates In order to better understand the details of individual wave numerous waves of much smaller height, whichrun-up result within in an the almost thewesame (justthe slightly wake, consider run-up of three packetsdifferent corresponding three different smaller) run-up. This can be partially explained by periodstoof wake waves,types whichofisvessels. As it has been mentioned before, the time at the echo sounder and at reflected in the time-frequency spectrum in Fig. 10.video recording was synchronized, making possible to identifydifferent the run-up of most of waves in in theFig. wake, The approach of three different groups with periods is clearly seen 10.except waves of very small amplitude (< 10 cm at the echo sounder record). The first group of waves with peak period at 8 sec appears at the time moment of 1 min. Then, 3 For this analysis we select a wave wake from SuperStar, minutes after the second group with peak period which 5 sec approaches. finally, afterat 319:15; more from Star, ococcurred onAnd 19 June 2009 minutes the third group of waves with 4 sec periodscurred comes.on 20 June 2009 at 12:10; and from Viking XPRS, occurred on 21 June 2009 at 13:50. Corresponding wave and So, the structure of the wave packet is such that waves of longer period come first. At the run-up heights for all of them are shown in Fig. 9. same time the run-up height increases with decreaseItincan thebewave period from [see Eq. andthere this is a fairly good concluded Fig.(9)] 9 that correlation between wave run-up waves data. Increase in the may explain, why waves of the second group, which have smaller periods thanand the largest wave height generally corresponds to the increase in the runof the first group, produce the same run-up (see, time min in the Fig.maximum 9a). up interval height. 4-8 However, run-up in the wake does not always correspond to the maximum wave height. This is 13 clearly seen in Fig. 9b and c, where the absolute maximum Fig. 10. Time-frequency spectrum for SuperStar (19 June 2009). wave heights are not so pronounced as in Fig. 9a and are just slightly larger than for other waves. At the same time Fig. 9a, with an outstanding peak for Here L is the distance to the shore (in our case L = 100 m), the highest wave, demonstrates numerous waves of much g is the gravity acceleration and h is the water depth (h = smaller height, which result in almost the same (just slightly 2.7 m). smaller) run-up. This can be partially explained by different Thus, averaged amplification of vessel waves is almost periods of wake waves, which is reflected in the timetwice as smaller than the one predicted by Eq. (9). This can frequency spectrum in Fig. 10. be explained by strong dissipation during wave breaking, as The approach of three different groups with different perivery often vessel wakes break before reaching the coast (see ods is clearly seen in Fig. 10. The first group of waves, with Fig. 2). peak period at 8 s, appears at the time moment of 1 min. www.nonlin-processes-geophys.net/20/179/2013/ Nonlin. Processes Geophys., 20, 179–188, 2013 closer to the “breaking” curve, while smaller-amplitude waves are closer to the “non-breaking” line, what corresponds to our expectations. 186 I. Didenkulova and A. Rodin: A typical wave wake from high-speed vessels a Amplification 8 6 4 2 0 0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 Wave height, m 8 Amplification Amplification 6 4 6 4 2 2 0 0 c b 8 0.1 0.2 0.3 0.4 0.5 Wave height, m 0.6 0.7 0 0 0.1 0.2 0.3 0.4 Wave height, m Fig. 11.onWave amplification on the wave beachheight plotted wave height forSuperStar wake waves Fig. 11. Wave amplification the beach plotted against foragainst wake waves from (a) (19from June a) 2009), (b) Star (20 June 2009) and (c) Viking XPRS (21 June 2009). Dashed lines correspond to Eq. (9) and dotted lines correspond to calculation of breaking run-up “SuperStar” (19 June 2009), b) “Star” (20 June 2009) and c) “Viking XPRS” (21 June 2009). with the characteristic period of 6 (blue) and 14 s (black). Black solid line corresponds to the power approximation described by Eq. (10). Dashed lines correspond to Eq. (9) and dotted lines correspond to calculation of breaking run-up with the characteristic period of 6 (blue) and 14 (black) sec. Black solid line corresponds to the Then, 3 min after, the second group with peak period 5s up on(10). a plane beach (Eq. 9), calculated for waves with peripoweratapproximation approaches. And finally, after 3 more minutes, the third group ods of 6 and 14 s. It can be seen that some smaller (probably, of waves with 4 s periods comes. non-breaking) waves with wave heights < 20 cm may have So, the structure of the wave packet is such that waves of the same amplification, but the majority of wake waves lie longer period come first. At the same time the run-up height below threshold. The data from all three vessels on Fig. 11 can be very wellthis described using the power regression increases with decrease in the wave period (see Eq. 9) and The dotted lines in Fig. 11 represent the result of nucurve (see, solid line in Figs. 11) merical simulation of wave amplification along a Pikakari this may explain why waves of the second group, which have beach profile. The numerical simulation is performed ussmaller periods than the largest waves of the first group, proing the CLAWPACK (Conservation Laws Package) packduce the same run-up (see, time interval 4–8 min in Fig. 9a). This effect may also be a key to the understanding of rapid 15 age (LeVeque, 2004), which models shallow water equations in the form of laws of conservation and allows formation beach erosion caused by fast-vessel wakes. The group struc ture of the wake works so that waves with the largest run-up and propagation of breaking waves parameterized by the heights come one after another resulting in the anomalous shock waves. The propagation of such waves along a flat bottom is described in Pelinovsky and Rodin (2011); and Diimpact on the coast. denkulova et al. (2011). The calculated amplification curve Another factor, which influences run-up height, is wave decreases with an increase in the wave height, which is in a breaking, which affects waves of large amplitudes reducing good agreement with the behavior of the experimental data. their run-up. Observations show that very often the largest Waves of larger amplitude, which are more subject of wave vessel induced waves break before they reach the coast (see, breaking, are closer to the “breaking” curve, while smallerFig. 2). Waves of larger amplitude break farther from the amplitude waves are closer to the “non-breaking” line, what coast and dissipate stronger than smaller amplitude waves. corresponds to our expectations. This can be seen in Fig. 11 for wave amplification at the The data from all three vessels in Fig. 11 can be very well coast (R/H ), where waves of smaller amplitude amplify described using the power regression curve (see, solid line in stronger than the larger ones. For comparison, blue and black dashed horizontal lines correspond to the non-breaking runNonlin. Processes Geophys., 20, 179–188, 2013 www.nonlin-processes-geophys.net/20/179/2013/ I. Didenkulova and A. Rodin: A typical wave wake from high-speed vessels Figs. 11) R = aH −b , (10) H where the power coefficient varies within 0.75 ≤ b ≤ 0.95 depending on the type of the vessel and dimensional coefficient changes within the range 0.4 ≤ a ≤ 1.0. Obtained experimentally, Eq. (10) can be used for estimates of run-up heights from vessel generated waves. 5 Conclusions The anomalous impact of waves from high-speed vessels on coasts is considered with respect to their specific group structure. The intensive vessel-induced waves and their run-ups are studied experimentally at the Pikakari beach in Tallinn Bay, the Baltic Sea, in summer 2009. In total, 66 wave wakes were recorded and 86 run-ups were measured from three different high-speed vessels: Star, SuperStar and Viking XPRS. It is shown that Weibull distribution can be a good model describing the distribution of wave heights in a single wake and corresponding run-up heights. This works for the overall distribution, as for wakes from different vessels. Both parameters of the Weibull distribution for wave heights can also be estimated from the Glukhovsky distribution for wind waves in shallow or intermediate water (Glukhovsky, 1966) and these estimates are in a good agreement with measured data. The mean wave and run-up heights, reconstructed from the Weibull distributions, demonstrate a great coincidence with the measurements. There is also a correspondence between mean wave and run-up heights showing that increase in one results in the increases in the other. It is found that, on average, vessel wave heights are amplified 3.5 times during 100 m of propagation to the coast. The run-up of three particular wake waves, which correspond to three different vessels, is studied in detail. It is demonstrated that group structure of the wake, where the largest and the longest waves come first and waves of smaller amplitude and period come after, works so that waves with largest run-up heights come one after another resulting in the anomalous impact on the coast. This effect may be a key to understanding of the rapid beach erosion caused by fast vessel wakes. Wave amplification varies significantly within a wake. Waves of large amplitude have very little amplification, which is explained by the influence of the wave breaking. At the same time small amplitude (< 20 cm) waves amplify significantly at the coast and can be described by the run-up of long non-breaking waves on a plane beach in the shallow water framework. Waves of moderate amplitude represent an intermediate case where wave breaking effects are still important, but they are influenced by wave dispersion and dissipation in the near bottom layer. For the description of these waves an empirical formula based on experimental data is provided. www.nonlin-processes-geophys.net/20/179/2013/ 187 Acknowledgements. This research was partially supported by the Federal Targeted Program “Research and educational personnel of innovation Russia” for 2009-2013, targeted financing by the Estonian Ministry of Education and Research (grant SF0140007s11), Estonian Science Foundation (Grant 8870), grants MK-1440.2012.5 and RFBR-12-05-33087. 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