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HAL Id: hal-00302256 https://hal.archives-ouvertes.fr/hal-00302256 Submitted on 1 Jan 2003 HAL is a multi-disciplinary open access archive for the deposit and dissemination of sci- entific research documents, whether they are pub- lished or not. The documents may come from teaching and research institutions in France or abroad, or from public or private research centers. L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des établissements d’enseignement et de recherche français ou étrangers, des laboratoires publics ou privés. Soliton interaction as a possible model for extreme waves in shallow water P. Peterson, T. Soomere, J. Engelbrecht, E. van Groesen To cite this version: P. Peterson, T. Soomere, J. Engelbrecht, E. van Groesen. Soliton interaction as a possible model for extreme waves in shallow water. Nonlinear Processes in Geophysics, European Geosciences Union (EGU), 2003, 10 (6), pp.503-510. hal-00302256

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Page 1: Soliton interaction as a possible model for extreme waves

HAL Id: hal-00302256https://hal.archives-ouvertes.fr/hal-00302256

Submitted on 1 Jan 2003

HAL is a multi-disciplinary open accessarchive for the deposit and dissemination of sci-entific research documents, whether they are pub-lished or not. The documents may come fromteaching and research institutions in France orabroad, or from public or private research centers.

L’archive ouverte pluridisciplinaire HAL, estdestinée au dépôt et à la diffusion de documentsscientifiques de niveau recherche, publiés ou non,émanant des établissements d’enseignement et derecherche français ou étrangers, des laboratoirespublics ou privés.

Soliton interaction as a possible model for extremewaves in shallow water

P. Peterson, T. Soomere, J. Engelbrecht, E. van Groesen

To cite this version:P. Peterson, T. Soomere, J. Engelbrecht, E. van Groesen. Soliton interaction as a possible modelfor extreme waves in shallow water. Nonlinear Processes in Geophysics, European Geosciences Union(EGU), 2003, 10 (6), pp.503-510. �hal-00302256�

Page 2: Soliton interaction as a possible model for extreme waves

Nonlinear Processes in Geophysics (2003) 10: 503–510Nonlinear Processesin Geophysics© European Geosciences Union 2003

Soliton interaction as a possible model for extreme waves inshallow water

P. Peterson1, T. Soomere2, J. Engelbrecht1, and E. van Groesen3

1Institute of Cybernetics, Tallinn Technical University, Akadeemia tee 21, 12618 Tallinn, Estonia2Marine Systems Institute, Tallinn Technical University, Akadeemia tee 21, 12618 Tallinn, Estonia3Faculty of Mathematical Sciences, University of Twente, P.O. Box 217, 7500 AE Enschede, The Netherlands

Received: 16 January 2003 – Revised: 27 March 2003 – Accepted: 2 April 2003

Abstract. Interaction of two long-crested shallow waterwaves is analysed in the framework of the two-soliton solu-tion of the Kadomtsev-Petviashvili equation. The wave sys-tem is decomposed into the incoming waves and the interac-tion soliton that represents the particularly high wave humpin the crossing area of the waves. Shown is that extremesurface elevations up to four times exceeding the amplitudeof the incoming waves typically cover a very small area butin the near-resonance case they may have considerable ex-tension. An application of the proposed mechanism to fastferries wash is discussed.

1 Introduction

The phenomenon of particularly high and steep (freak orrogue) waves is one of the most dangerous events that a trav-eller at sea may encounter. At the early stage of freak wavestudies, their existence and appearance were explained by ba-sically linear models like interaction of waves with oppos-ing currents (see Peregrine, 1976; Jonsson, 1990 and bib-liography therein) or with uncharted seamounts (see Whiteand Fornberg, 1998 and bibliography therein), blockage ofshort waves by longer waves and currents (Shyu and Phillips,1990), interaction of surface waves with internal waves (Do-nato et al., 1999) or linear superposition of long waves withpreceding shorter waves (e.g. Sand et al., 1990; Stansberg,1990). Later on, a number of deeply interesting results wereobtained based on the wave ray theory (e.g. Shyu and Tung,1999; White and Fornberg, 1998) and on the assumption ofthe presence of either specific bathymetry or structure of cur-rents.

Freak waves became a subject of significant interest forscientists in 1990s when it was established that they occurmuch more frequently than predicted by surface wave statis-tics. They are too high, too asymmetric and too steep, andnot necessarily related with other dynamical processes in the

Correspondence to:T. Soomere ([email protected])

ocean (Sand et al, 1990). During the last decade, many ef-forts were concentrated in order to find an appropriate mech-anism that can cause considerable changes in the wave am-plitudes exclusively resulting from (possibly nonlinear) su-perposition of long-crested waves and leading to spatially lo-calised extreme surface elevations. For water waves, prob-ably the first mechanism of this type has been first used toexplain the origin of freak waves in (Dean, 1990). Modu-lation instability of wave trains with respect to longitudinaland transversal perturbations (Trulsen and Dysthe, 1997, Os-borne et al., 2000) was one of the possibilities in order tounderstand the nature of freak waves or to establish the areawhere they are expected.

The most promising has been the approach of nonlin-ear wave focusing occurring in situations resembling roughseas in natural conditions and claiming that a large numberof waves with different frequencies and propagation direc-tions may produce a large long-living transient wave groupat a particular point. This phenomenon has been theoret-ically validated in several simple but realistic models, e.g.in the framework of the simplest one-dimensional (1-D)Korteweg-de Vries equation (Pelinovsky et al., 2000) andfor the two-dimensional wave field in the framework of theDavey-Stewartson equation (Slunyaev et al., 2002). Numer-ically, it has been demonstrated to work in irregular or ran-dom sea even for extreme wave design purposes (Smith andSwan, 2002) and also in the framework of generalized 2-DSchrodinger equation (Onorato et al., 2002). There exist bril-liant experiments showing that this effect indeed occurs inlaboratory conditions (e.g. Baldock and Swan, 1996; Johan-nessen and Swan, 2001).

A detailed description of another source for considerablechanges in the wave amplitudes that can be related to the non-linear superposition of long-crested waves and that also leadsto spatially localised extreme surface elevations is the aim ofthe present paper. As different from the effect of wave focus-ing that generally presumes the existence of a number of dif-ferent wave components that partially may be short-crested,the proposed mechanism is effective for a small number but

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504 P. Peterson et al.: Soliton interaction as a possible model for extreme waves in shallow water

definitely long-crested and soliton-like waves. This situa-tion apparently is uncommon for storm waves or swell butmay frequently occur in relatively shallow areas with heavyfast ferry traffic (Soomere et al., 2003, Parnell and Kofoed-Hansen, 2001). A simple way to describe the interaction ofsoliton-like waves in water of a finite depth is to consider twolong-crested solitary waves travelling in different directionson a surface of water under gravity (Hammack et al., 1989,1995). This is the simplest setup for multi-directional wavephenomena that can occur on sea. In this paper the extremewave hump is described resulting from the crossing of thesewaves. This wave hump resembles Mach stem that ariseswhen waves propagate in a semi-bounded area (also calledMach reflection, see, e.g. Funakoshi, 1980; Peregrine, 1983;Tanaka, 1993). Contrary to the case of a linear superpositionwhen the resulting wave height does not exceed the sum ofthe heights of the counterparts, this hump can be up to fourtimes higher than the incoming wave(s).

A suitable mathematical model for the description ofnonlinear shallow water gravity waves is the Kadomtsev-Petviashvili (KP) equation (Kadomtsev and Petviashvili,1970). Exact solutions for the KP equation can be foundby using Hirota bilinear formalism (Hirota, 1971). The 2-Dtwo-soliton interaction has been analysed, among others, in(Satsuma, 1976; Miles, 1977a, 1977b; Freeman, 1980), withmain attention to the phase shifts and resonance phenomena.The resonance in this context is related to two interactingsolitons (Miles, 1977a, b) resulting in a single soliton thatwas resonant with both interacting waves. In this framework,many authors have demonstrated that the amplitude of thewater elevation at the intersection point of two solitons mayexceed that of the sum of incoming solitons (see, for exam-ple, Segur and Finkel, 1985; Haragus-Courcelle and Pego,2000; Tsuji and Oikawa, 2001; Chow, 2002) but neither thelimits of the elevation nor the spatial occupancy of the highelevation have been analysed in detail. This model allowsto consider the solitons with arbitrary amplitudes whereas inthe case of the Mach reflection the amplitudes of the coun-terparts generally are related to each other.

Recently, Peterson and van Groesen have explicitly stud-ied the two-soliton interaction (Peterson and van Groesen,2000, 2001) with a special decomposition distinguishing thesingle solitons and the interaction soliton that connects thesingle solitons and mostly is concentrated in the intersectionarea of the single solitons. The decomposition permits tostudy the properties of an interaction soliton in detail andclarify the mechanism of its emergence. Shown is that un-der certain conditions the amplitude of the interaction solitonmay exceed considerably the amplitudes of the interactingsingle solitons.

The general idea elaborated below is the following. As in(Peterson and van Groesen, 2001), we associate waves withsolitons by assuming the KP equation to be a valid modelfor such waves in shallow water, that is, waves are relativelylong and small but finite when comparing to the water depth.Oblique interaction of two solitons (below called incomingsolitons) propagating in slightly different directions involves

the so-called interaction soliton that connects two solitonswith their shifted counterparts (Peterson and van Groesen,2001) and can be associated with the wave hump resultingfrom their crossing (cf. experimental evidence in Hammacket al., 1989, 1995).

We aim to clarify the regions in the parameter space of atwo-soliton solution where the height of the interaction soli-ton exceeds the value predicted by the linear theory and toevaluate its maximum height and length and the conditionswhen they are achieved. When two waves of amplitudesa1anda2 meet, the maximum amplitudeM of their (linear ornonlinear) superposition can be written asM = m(a1 + a2),where “amplification factor”m may depend on botha1 anda2 and their intersection angleγ12. Linear theory givesm = 1. We show that, at least, for specific combinationsof a1, a2 and γ12, the maximum “amplification factor” ismmax = 2 as in the case of the Mach reflection.

The paper is organized as follows. In Sect. 2 the solutionof the KP equation is given decomposed into a sum of twosoliton terms and interaction soliton term. The analysis of thespatial occupancy and the height of the interaction solitonis presented in Sect. 3. Section 4 includes the estimates ofthe the critical angle between incoming solitons, leading toextreme elevations, and occurrence and spatial structure ofextreme elevations. In Sect. 5 physical evidence of extremewaves, possible modelling of such entities using the notionof interaction solitons and further prospects of modelling arediscussed.

2 Two-soliton solution

The KP equation in normalized variables reads (Segur andFinkel, 1985)

(ηt + 6ηηx + ηxxx)x + 3ηyy = 0 , (1)

where normalised variables(x, y, t, η) are related to physicalvariables(x, y, t , η) in a coordinate frame moving in thex-direction as follows:

x =ε1/2

h

(x − t

√gh

), y =

ε

hy ,

t =ε3/2√gh

6ht , η =

3

2εhη + O(ε) , (2)

whereη is the elevation of the water surface (η = 0 cor-responds to the undisturbed surface),ε = |η|max/h � 1is maximal wave amplitude normalized against the depth ofthe fluidh andg is gravity acceleration. In this framework,the phase speed of a disturbance always exceeds the max-imum linear wave phase speed

√gh. Since the interaction

pattern of a two-soliton solution is stationary in the mov-ing coordinate frame, in the following we taket = 0 with-out loss of generality. Below we mean that a gravity wavewith amplitudeη0 and wave lengthL propagating in waterof depthh, is a shallow-water wave if its Ursell number isU = η0L

2h−3≈ 1. The KP equation itself is valid pro-

vided l/k = O(κh) = O(ε), where(k, l) is a wave vector

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P. Peterson et al.: Soliton interaction as a possible model for extreme waves in shallow water 505

Fig. 1. The shape of surface in thevicinity of the intersection of solitonss1, s2 (upper left panel) and surface el-evation caused by the interaction soli-ton s12 (upper right) and incoming soli-tons (lower panels) in normalised coor-dinates(x, y), cf. Fig. 3. Area|x| ≤

30, |y| ≤ 30, 0 ≤ z ≤ 4a1 is shown ateach panel.

for the waves in question,κ = |(k, l)|, andx-direction is theprincipal direction of wave propagation.

A two-soliton solution of the KP Eq. (1) reads (Segur andFinkel, 1985)

η(x, y, t) = 2∂2

∂x2ln θ ,

where

θ = 1 + eϕ1 + eϕ2 + A12eϕ1+ϕ2 ,

ϕ1,2 = k1,2 x + l1,2 y + ω1,2 t are phase variables,κ1 = (k1, l1), κ2 = (k2, l2) are the wave vectors of theincoming solitons, the “frequencies”ω1,2 can be foundfrom the dispersion relation of the linearized KP equationP(k1,2, l1,2, ω1,2) = k1,2 ω1,2 + k4

1,2 + 3l21,2 = 0 andA12 isthe phase shift parameter

A12 = −P(k1 − k2, l1 − l2, ω1 − ω2)

P (k1 + k2, l1 + l2, ω1 + ω2)

=λ2

− (k1 − k2)2

λ2 − (k1 + k2)2, (3)

whereλ = l1/k1 − l2/k2 (Peterson and van Groesen, 2001).The two-soliton solution can be decomposed into a sum of

two incoming solitonss1, s2 and the interaction solitons12(Peterson and van Groesen, 2000)

η = s1 + s2 + s12 , (4)

where the counterpartss1, s2 ands12 (Fig. 1) are defined as:

s1,2 =

A1/212 k2

1,2 cosh(ϕ2,1 + ln A

1/212

)22

,

s12 =

(k1 − k2

)2+ A12

(k1 + k2

)2

222,

2 = cosh[(

ϕ1 − ϕ2)/2

]+A

1/212 cosh

[(ϕ1 + ϕ2 + ln A12

)/2

]. (5)

The heigth and orientation of the interaction soliton onlydepend on the amplitudes of the incoming solitons and theangle (interaction angle) between their crests. Within restric-tions of the KP model, interaction may result in either thepositive or the negative phase shift112 = − ln A12 of thecounterparts. The positive phase shift (when the interactionsoliton generally does not exceed the larger incoming one)typically occurs for interactions between solitons with fairlydifferent amplitudes. The negative phase shift is typical ininteractions of solitons with comparable amplitudes and re-sults generally in an interaction soliton which height exceedsthat of the sum of the two incoming solitons. This observa-tion agrees with the fact that the total mass and energy of allthree solitons (as well as other integrals of motion) in a spe-cific direction (called the principal propagation direction) areconstant in the transversal direction.

3 The height and length of the interaction soliton

Since we are basically interested in extreme amplitudes, inwhat follows we concentrate on the region in the parame-ter space that corresponds to the negative phase shift case,equivalently, to the region whereA12 > 1 (Fig. 2). In this re-gion, the maximum height of the interaction soliton exceedsthat of the counterparts (except in the limiting caseA12 → 1with no phase shift when the height of the interaction solitontends to

(k2

1 + k22

)/4, that is the mean height of the incoming

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506 P. Peterson et al.: Soliton interaction as a possible model for extreme waves in shallow water

Fig. 2. “Map” of negative and positive phase shift areas for the two-soliton solution of the KP equation for fixedl1,2. The phase shiftparameter has a discontinuity along the linek1 + k2 = λ where|A12| = ∞.

Fig. 3. Idealised patterns of crests of incoming solitons (solid lines)and the interaction soliton (bold line) corresponding to the negativephase shift case. Notice that the crest of the interaction soliton is notnecessarily parallel to they-axis except in the case of equal heights(equivalently, equal lengths of the wave vectors) of incoming soli-tons.

solitons). Further, in the case of considerably different am-plitudes of incoming solitons (A12 < 1), the amplitude of theinteraction soliton is smaller than the mean height of incom-ing solitons. However, in the case of equal amplitude incom-ing solitons, the surface elevation in the interaction regionmay up to four times exceed the amplitudea1,2 = k2

1,2/2of the incoming solitons (see below; cf. Tsuji and Oikawa,2001).

It is convenient to take thex-axis to bisect the interaction

angleα12 between the wave vectorsκ1, κ2 (Fig. 3) that yieldsλ = 2l1/k1 = 2 tan

(12α12

), l1/k1 = −l2/k2 and

A12 =4l21 − k2

1

(k1 − k2

)2

4l21 − k21

(k1 + k2

)2. (6)

In (Peterson and van Groesen, 2000) it is shown that thephase shiftsδ1, δ2 of the incoming solitons satisfy the rela-tion |δ1,2κ1,2| = |112|. It is natural to interpret the interval[b, c] on Fig. 3 (where the crests of the incoming solitonspractically coincide) as the crest of the interaction soliton.From Fig. 3 it follows that the (geometrical) length of the in-teraction solitonL12 equals to the longer diagonal of the par-allelogram with the sidesδ1,2/ sinα12 (that are perpendicularto wave vectorsκ2,1, respectively) and the acute angleα12.This consideration immediately gives

L12 =|κ1 + κ2|

|κ1 × κ2||112| =

|112| · |κ1 + κ2|

κ1κ2 sinα12. (7)

From Eq. (7) it follows that, formally,L12 may vary from0 to infinity. Since the first factor in Eq. (7) has a minimum

value√

κ−21 + κ−2

2 > 0 if κ1 ⊥ κ2 (this value indeed cannotbe achieved, because in this case the KP equation becomesinvalid) and since in physically meaningful cases at least onewave vectorκ1,2 has finite length,L12 may approach zeroif and only if A12 → 1. This is possible only ifk1k2 =

0, i.e. in the trivial case when one of the incoming solitonshas zero amplitude. Further,L12 approaches infinity either ifA12 → ∞ or in the trivial subcaseκ1 ‖ κ2. The first case isequivalent to the limiting processl1 →

12k1(k1 + k2) which

gives a nontrivial solution.For a given nonzero angleα12 between the incoming soli-

tons and fixedk1 + k2, the interaction soliton lengthL12 hasa maximum value if the vectorsκ1, κ2 have an equal length.In the particular case of equal height solitonsk1 = k2 = k,l1 = −l2 = l, A12 = l2/

(l2 − k4

)and we have

L12 =

√(k1 + k2

)2+

(l1 + l2

)2

|k1l2 − k2l1|ln A12

=ln A12

l, A12 > 1 . (8)

In the case of equal amplitude solitons, the direction ofx-axis (the principal propagation direction) coincides withthat of vectorκ1 + κ2. With the use of Eqs. (3) and (5) it canbe shown that the maximum heights of the the counterpartss1, s2, ands12 read (Peterson and van Groesen, 2001):

a1,2 =1

2k2

1,2, a12 =

(k1 − k2

)2+ A12

(k1 + k2

)2

2(1 + A

1/212

)2. (9)

Notice that the maximum heights of the incoming solitonsare achieved atϕ1 = 0, ϕ2 → −∞ or ϕ2 = 0, ϕ1 → −∞.From the definition of the interaction soliton in Eq. (5) itfollows that its height is always nonzero and has a max-imum value at the center of the interaction region definedby (ϕ1, ϕ2) =

12(112, 112). Figure 4 shows dependence of

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P. Peterson et al.: Soliton interaction as a possible model for extreme waves in shallow water 507

Fig. 4. The dependence of the phase shift parameterA12, lengthof the interaction solitonL12 and amplitudes of the incominga1and the interaction solitona12 on the wave vector componentk

along the linek1 = k2 = k in Fig. 2 for l1 = −l2 = 0.3. Thecasek = kres = λ/

√2 corresponds to the intersection of the line

k1 = k2 with the border of the areaA12>1, i.e. with the line where|A12| = ∞. Notice that for small values ofk/kres the assumption|l| � |k| is violated.

quantitiesA12, L12, a1, a2, a12 on the wave vector lengthin the case of equal amplitude incoming solitons. For fixedl1,2 and equal height solitons, from Eqs. (6), (8) and (9) itfollows thatA12 monotonously increases from 1 to infinitywhen parameterk of incoming solitions increases from 0 tok = λ/

√2. Further,L12 increases from 0 to infinity and the

amplitude of an interaction soliton monotonously increasesfrom 0 to 2k2

= λ2.

In terms of the decomposition (Eq. 4), the componentss1, s2 and s12 are shown in Fig. 5, whereζ = y/L12 andvalues correspond to crests approximately following the lineabcd (s2), a′bcd ′ (s1) or bc (s12) in Fig. 3. The origin ofζis taken in the centre of the interaction soliton. It is seen thatalthough the visible part of interaction crest has the lengthL12 (Fig. 3), the changes in components occur beyond thislimit. Namely, the length of the area where the height ofthe interaction soliton exceeds the double amplitude of theincoming solitons (or, equivalently, where nonlinear effectscreate higher elevation than simple superposition of heightsof two waves) may considerably exceedL12. The reason isthat the above definition of the interaction soliton lengthL12in Eq. (7) is based on the geometrical image of crest patternsof the interacting solitons.

Fig. 5. The maximum surface elevation maxy=const (s1 + s2 + s12)

and the height of the incoming solitons maxy=const (s1, s2) andthe interaction soliton maxy=const (s12) along their crests fork1 =

k2 = 0.5; l1 = −l2 = 0.3. The origin coincides with the centre ofthe interaction soliton.

4 The critical angle, occurrence and spatial structure ofextreme elevations

Equation (2) shows that the normalized co-ordinate axes havedifferent scaling factorsx ∼ ε1/2x, y ∼ εy that must betaken into account when interpreting the results in physicalco-ordinates. Letα12 be the angle between soliton crests inthe physical space. If we defineλ = 2 tan

(12α12

), then it is

easy to show thatλ = λε1/2. The physical lengthL12 of theinteraction soliton crest is

L12 =h

εL12 =

2h|112|

ε1/2kλ,

where

112 = − lnλ2

λ2 − 4εk21

.

The above has shown that the highest surface elevation oc-curs in the center of the interaction area when two solitons ofcomparable height interact. In the particular case of equal inheight solitonsk1 = k2 = k, l1 = −l2 = l and Eqs. (3) and(9) are simplified as follows:

A12 =l2

l2 − k4, a12 =

2A12k2(

1 + A1/212

)2.

The interaction soliton has maximum amplitude2k2 if A12 = ∞. In this case we havel = k2 that isconsistent with the assumption of the KP equation that|l| � |k| provided|k| < 1.

For given wave depthh and incoming soliton amplitudesη, the resonance takes place and the extent of extreme water

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508 P. Peterson et al.: Soliton interaction as a possible model for extreme waves in shallow water

Fig. 6. Surface elevation in the vicin-ity of the interaction area, correspond-ing to incoming solitons with equalamplitudesa1 = a2, l = −l1 =

0.3, kres =√

0.3 and k = 0.8kres(upper left panel),k = 0.9kres (up-per right), k = 0.99kres (lower left),k = 0.9999kres (lower right) in nor-malised coordinates(x, y), cf. Fig. 3.Area |x| ≤ 30, |y| ≤ 30, 0 ≤ z ≤ 4a1is shown at each panel.

level elevation described byL12 may increase dramaticallyif the solitons intersect under a physical angle

α12 = 2 arctan√

3η/h .

The critical angle (at which the interaction soliton heightand length are extreme) for two solitary waves in realis-tic conditions is reasonable. For example, for waves withheightsη = 1.8 m meeting each other in an area with typicaldepthh = 50 m, the critical angle is about 36◦.

From Fig. 4 it follows that the maximum relative ampli-tude of the interaction soliton mostly remains modest al-though it always exceeds that of incoming solitons. Eleva-tions exceeding two times the incoming soliton height occurrelatively seldom, only if

(kres− k

)/kres ≈< 0.05.

The analysis until now has concerned only the occurrenceof extreme elevations. We studied numerically the appear-ance of the interaction soliton depending on the wave vectorlength along the linek1 = k2 for a fixed pair of wavenum-bersl1 = −l2 (Fig. 6). If the wavenumberk1 differs fromkres =

√l1 more than 10%, the length of the interaction soli-

ton (the extent of the extreme elevation) remains modest (cf.Fig. 4). Whenk1 → kres (equivalently, the wave vectors ofthe incoming solitons approach the border of the areaA12>1in Fig. 2), the area of extreme elevation widens. However,the length of the interaction soliton considerably exceedsk−1

1only if the difference betweenk1 andkres (equivalently, thedifference between the interaction angle and the critical an-gle) is less than 1% (Fig. 6).

5 Discussion

The fact that the total energy density of all three solitons,integrated in the principal propagation direction, is constant

in the transversal direction confirms that the described am-plitude amplification is not accompanied by energy pumpinginto the interaction region. Further on, the central part ofthe interaction region with extreme water surface elevation,if “cut” out from the interaction picture and let to evolve onits own in a channel of suitable width, apparently will nothave the properties of a KP (KdV) soliton. The reason is thatgenerally (except in the limiting case|A12| → ∞) it does notcorrespond to a one-soliton solution of the KP equation, be-cause its profile is wider compared to that of the one-solitonsolution with the same fixed height.

Since there occurs no energy concentration in the extremesurface elevation region, one might say that the described ef-fect is interesting only theoretically. This is true to some ex-tent. But in natural conditions the sea bottom is never perfect,and the moving interaction soliton, generally, after a whilemeets conditions where KP equation itself might be invalidor the negative phase shift is impossible. The transition fromthe regionk1 < kres to the casek1 > kres needs a furtheranalysis. In this situation, the interaction soliton may breakas any other water wave does. This particular moment con-tains acute danger, because, as it is generally believed, “nonon-breaking wave is dangerous”, e.g. for offshore yachts(Kirkman and McCurdy, 1987).

The discussed model of extreme water elevations or freakwaves assumes the existence of more or less regular long-crested 2-D wave trains. This assumption suggests that afreak wave caused by the soliton interaction mechanism isa rare phenomenon at open sea in natural conditions. In-deed, the influence of the most important source of surfacewaves – wind fields during storms – generally results in anextremely irregular sea surface and the appearance of long-living solitary waves is unlikely. The presented mechanism

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P. Peterson et al.: Soliton interaction as a possible model for extreme waves in shallow water 509

may be far more important in relatively shallow coastal areaswith high ship traffic density. It is well known that long-crested soliton-like surface waves are frequently excited bycontemporary high speed ships if they sail with critical or su-percritical speeds (e.g. Chen and Sharma, 1997; navigationalspeeds are distinguished according to the depth Froude num-berFd = νship/

√gh, that is the ratio of the ship speed and

the maximum phase speed of gravity waves. Operating atspeeds resultingFd = 1 is defined as critical andFd > 1 assupercritical).

Groups of soliton-like ship waves intersecting at a smallangle may appear if two high speed ships meet each other orif a ship changes its course. The first opportunity frequentlyhappens in areas with heavy high speed traffic like the TallinnBay, Baltic Sea, where up to 70 bay crossings take place dailywhereas at specific times three fast ferries depart simultane-ously (Soomere et al., 2003).

The length of interactions solitons (equivalently, the extentof the area where considerable amplification of wave heightsmay take place) generally is moderate, thus these structuresare short-crested three-dimensional (3-D) stationary waves.This property should be particularly emphasized, because theincoming solitons are virtually one-dimensional and their in-teraction pattern is a two-dimensional structure. In terms ofdimensions, this situation is principally different from thatarising in studies of focusing of transient and directionallyspread waves. In these experiments (both numerical and lab-oratory) a number waves with different frequencies and prop-agation directions are focused at one point at a specific timeinstant to produce a time-varying transient wave group (e.g.Johannessen and Swan, 2001). In this context, the forming ofan interaction soliton resembles the 3-D freak wave appear-ance in numerical simulations based on the generalized 2-DSchrodinger equation (Onorato et al., 2002).

Substantial areas of extreme surface elevation may occuronly if the heights of the incoming waves, their intersectionangle and the local water depth are specifically balanced.Thus, the fraction of sea surface occupied by the interac-tion solitons corresponding to extreme elevations apparentlyis very small as compared with the area covered by intensewash. By that reason, detecting of an interaction soliton inone-point in situ measurements is unlikely. Yet the nonlinearamplification of wave heights in the crossing points of wavecrests (that happens always when negative phase shift takesplace) may be one of the reasons why superposition of crit-ical wash generated before and after turns is mentioned asparticularly dangerous (Kirk McClure Morton, 1998).

In populated or industrial areas, a possible hit of the cen-tral part of a near-resonant long-crested interaction solitonon an entrance of a channel (harbour entrance, river mouthetc.) may cause serious consequences. The reason is that thisstructure is basically different from a superposition of twolinear wave trains at the same place. Linear waves continueto move in their original directions, and result in a system ofinterfering waves in the channel. If a near-resonant interac-tion soliton enters a channel, it concentrates energy of bothincoming solitons in one structure, the further behaviour and

stability of which is yet unclear. In a highly idealised caseof interactions of five solitons surface elevations may exceedthe amplitudes of the incoming solitons more than an order(Peterson, 2001).

Acknowledgements.This work has been supported by the EstonianScience Foundation, grant 4025 (TS). Part of the work has beensupported by STW technology foundation on the project “ExtremeWaves” TWI.5374 at Twente University.

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