1 Introduction
The global oceanic circulation is believed to be maintained by the occurrence of enhanced diapycnal mixing events over some regions of the oceans (Munk & Wunsch Reference Munk and Wunsch1998). The enhancement is expected to result from strong internal-wave activity, which, in the open ocean, has been found by field observations to be most significant over underwater topographical features (e.g. continental shelves, mid-oceanic ridges; cf. Polzin et al. Reference Polzin, Toole, Ledwell and Schmitt1997; Ledwell et al. Reference Ledwell, Montgomery, Polzin, St Laurent, Schmitt and Toole2000; Nash et al. Reference Nash, Alford, Kunze, Martini and Kelly2007; Waterhouse et al. Reference Waterhouse, MacKinnon, Nash, Alford, Kunze, Simmons, Polzin, St Laurent, Sun and Pinkel2014). Energy injection into the internal-wave field (Wunsch & Ferrari Reference Wunsch and Ferrari2004) and the contribution of internal waves to turbulent mixing through nonlinear processes (Staquet & Sommeria Reference Staquet and Sommeria2002) are thus important aspects of the ocean dynamics that are being gradually incorporated into global ocean models (Exarchou, Von Storch & Jungclaus Reference Exarchou, Von Storch and Jungclaus2012; Lefauve, Muller & Melet Reference Lefauve, Muller and Melet2015; Timko et al. Reference Timko, Arbic, Goff, Ansong, Smith, Melet and Wallcraft2017).
The final processes by which internal waves lead to turbulent diapycnal mixing are fundamentally nonlinear (Staquet & Sommeria Reference Staquet and Sommeria2002). However, a significant fraction of energy injection in the internal-wave field first occurs via bottom scattering (Garrett & Kunze Reference Garrett and Kunze2007), which can be considered as a linear process when the bottom slope is subcritical (see e.g. Legg Reference Legg2014, for a case with critical slope). As a result, the linear generation of internal waves over variable seabed is of significant interest, and, for small-amplitude topography, some of the mechanisms that can be and have been studied using regular perturbation methods include the topographic scattering of existing low-wavenumber internal waves toward higher wavenumbers (Müller & Xu Reference Müller and Xu1992), the generation of topographic lee waves (Bell Reference Bell1975a ) and the conversion of barotropic tidal energy into internal waves over rough topography (Balmforth, Ierley & Young Reference Balmforth, Ierley and Young2002; Garrett & Kunze Reference Garrett and Kunze2007). The generation of internal waves by large-amplitude subcritical topography has, on the other hand, been investigated using the semi-analytical Green function approach (Bühler & Muller Reference Bühler and Muller2007; Mathur, Carter & Peacock Reference Mathur, Carter and Peacock2014) and ray tracing (Bühler & Holmes-Cerfon Reference Bühler and Holmes-Cerfon2011; Guo & Holmes-Cerfon Reference Guo and Holmes-Cerfon2016).
The generation of high-wavenumber internal waves by topographic scattering is of significant interest because nonlinear processes leading to turbulent mixing are more efficient when internal waves have short wavelengths (Sarkar & Scotti Reference Sarkar and Scotti2017). Thus, a natural question is: what topographical features of the seafloor can most efficiently generate high-wavenumber waves? In the case of small-amplitude topography, previous studies have usually considered a continuous topographic spectrum and have shown that the amplitude of the generated waves is proportional to the height of topographical features (Bell Reference Bell1975b ; Müller & Xu Reference Müller and Xu1992; St Laurent & Garrett Reference St Laurent and Garrett2002; Llewellyn Smith & Young Reference Llewellyn Smith and Young2002; Khatiwala Reference Khatiwala2003). This means that the bottom forcing by small seabed features is in general expected to result in a weak perturbation of the incident wave field, such that only a small fraction of the available energy can be transferred to high-wavenumber internal waves.
Because previous studies have focused on the overall effect of a continuous seabed spectrum, the possibility that some seabed wavenumbers (out of the complete spectrum) can resonantly generate high-wavenumber internal waves has been seldom discussed (here we use the term resonant to qualify the generation of internal waves whose amplitudes are comparable to the amplitude of the incident wave). In a relatively recent investigation of wave focusing in a one-horizontal-dimension finite-depth ocean, and in agreement with earlier analyses of tidal conversion (Garrett & Kunze Reference Garrett and Kunze2007), Bühler & Holmes-Cerfon (Reference Bühler and Holmes-Cerfon2011) briefly discussed that the interaction of an incident internal tide (wavenumber
$k_{1}$
) with a single bottom harmonic (wavenumber
$k_{b}$
) can generate a series of shorter internal waves resonantly provided that
$k_{b}/k_{1}$
is an integer. For instance, when
$k_{b}=k_{1}$
, all internal-wave wavenumbers are indeed integer multiples of
$k_{1}$
such that each successively resonated wave
$k_{j}$
, starting with
$k_{2}=k_{1}+k_{b}=2k_{1}$
, can resonate other new higher-wavenumber internal waves
$k_{j+1}=k_{j}+k_{b}$
. Thus, the incident-wave energy is transferred to the shorter waves through perfect wave–bottom resonances occurring in series, but the mechanism requires a two-dimensional linearly stratified fluid and a top rigid lid.
(a) Top view schematic of incident internal waves with dimensionless wavenumber
$\unicode[STIX]{x1D705}_{in}$
and arbitrary incidence angle
$\unicode[STIX]{x1D703}_{in}$
, propagating toward a finite number of monochromatic seabed bars with which they can resonate new waves of varying wavelengths and directions of propagation. (b) The chain resonance diagram in dimensionless wavenumber space obtained when
$\unicode[STIX]{x1D703}_{in}\sim \unicode[STIX]{x03C0}/4$
. The light coloured concentric circles in the background show the natural dimensionless wavenumbers of the system, i.e. solutions of the dispersion relation
$\unicode[STIX]{x1D705}_{j}=j\unicode[STIX]{x03C0}$
(
$j$
an integer). Upon interacting resonantly with the seabed bars, the incident
$\unicode[STIX]{x1D705}_{in}$
waves generate the transmitted
$\unicode[STIX]{x1D705}_{r_{+1}}$
and reflected
$\unicode[STIX]{x1D705}_{r_{-1}}$
waves, which themselves resonate the new waves
$\unicode[STIX]{x1D705}_{r_{\pm 2}}$
. The process repeats itself with subsequent waves possibly infinitely. The successive resonances cannot all be perfect, however, which we clearly show in (c) by zooming in on the circle highlighting
$\unicode[STIX]{x1D705}_{r_{+2}}$
in (b); the resonant natural wavenumber
$\unicode[STIX]{x1D73F}_{r_{+2}}$
can be seen to be the result of the interaction wavenumber
$\unicode[STIX]{x1D73F}_{r_{+1}}+\unicode[STIX]{x1D73F}_{b}$
, plus a small detuning term
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D739}_{+2}$
.

In this paper, we demonstrate that the strong resonant transfer of energy from a low-mode internal wave to shorter waves by bottom scattering is not limited to the special two-dimensional case discussed in Bühler & Holmes-Cerfon (Reference Bühler and Holmes-Cerfon2011), and that it can occur in three dimensions with oblique incidence of the low-mode wave at and away from perfect resonance (cf. figure 1). By focusing our analysis on monochromatic corrugations rather than bathymetric spectra, we can explore in detail the resonance mechanism and the energy transfers from the incident low-mode internal waves to the shorter waves. The monochromatic corrugations considered in this paper may be seen as idealizations of ridges and valleys with length scales 10–100 km running perpendicular to the prominent mid-ocean ridges, since a dominant bottom wavenumber vector can be extracted for these topographical features (see e.g. Thurnherr et al. (Reference Thurnherr, St Laurent, Speer, Toole and Ledwell2005), in which significant mixing is observed above crest-parallel bathymetric sills on a mid-ocean ridge flank). (See also available seafloor maps at http://topex.ucsd.edu/marine_topo.) Monochromatic corrugations cannot be considered representative of abyssal hills, however, because the topographic spectra of abyssal hills are assumed to have random phase distributions, and hence cannot be accurately approximated by a single bottom mode (we refer the reader to Goff & Jordan (Reference Goff and Jordan1988), Smith & Sandwell (Reference Smith and Sandwell1997), Becker et al. (Reference Becker, Sandwell, Smith, Braud, Binder, Depner, Fabre, Factor, Ingalls and Kim2009), Goff & Arbic (Reference Goff and Arbic2010), for additional information on seafloor topography).
We solve the resonant three-dimensional boundary-value problem of internal-wave scattering at the steady state by deriving an evolution equation for the spatial variations of envelope amplitudes using the method of multiple scales in the weak topography limit. The method has been successfully applied for many investigations of wave–bottom resonance in homogeneous water (known as Bragg resonance), including shore protection (Yu & Mei Reference Yu and Mei2000a ; Couston, Jalali & Alam Reference Couston, Jalali and Alam2017), sandbar formation (Yu & Mei Reference Yu and Mei2000b ), wave lensing (Elandt, Shakeri & Alam Reference Elandt, Shakeri and Alam2014) and in two-layer density stratified fluids (Alam, Liu & Yue Reference Alam, Liu and Yue2009) with applications in the attenuation of long interfacial waves by random bathymetry (Alam & Mei Reference Alam and Mei2007) and broadband cloaking (Alam Reference Alam2012). Multiple-scale methods have also been employed in studies of wave dynamics in stratified fluids, including weakly nonlinear wave–mean flow interactions at topography (Nikurashin & Ferrari Reference Nikurashin and Ferrari2010) and the scattering of internal tides by irregular bathymetry (Li & Mei Reference Li and Mei2014). Because of the obliquity of the incident waves, but also because we allow the first interaction between the incident waves and the corrugations to be detuned, it should be noted that the chain resonances include mostly near-resonance waves. Near-resonance interactions (also known as detuned resonance) are of increasing interest in nonlinear wave science (Tobisch Reference Tobisch2016), and will be shown to play a major role in the present analysis.
The outline of the paper is as follows. In § 2, we present the governing equations and the different waves involved in chain resonance for arbitrary incidence angle, and we introduce a detuning parameter for each of the near-resonance interactions. In § 3, we provide the derivation details for the multiple-scale equation and give the solution method for the boundary-value problem. In § 4, we consider physical parameters representative of idealized oceanic conditions, and we discuss the chain resonance results obtained for a wide range of incidence angles and detunings. Finally, in § 5, we provide concluding remarks.
2 Problem formulation
2.1 Governing equations
Consider the propagation of small-amplitude waves in a stably stratified rotating fluid with constant buoyancy frequency
$N$
and under
$f$
-plane approximation with
$f$
the Coriolis frequency. In the Boussinesq approximation and neglecting viscosity, the linearized wave equation and boundary conditions for the vertical velocity
$w$
in a Cartesian domain
$(x,y,z)$
can be written as (e.g. Sutherland Reference Sutherland2010)
following a straightforward manipulation of the continuity and linearized momentum equations, with (2.2) known as the polarization relations for linear internal waves (cf. e.g. Sutherland Reference Sutherland2010).
Our goal is to investigate the effect of a finite patch of monochromatic seabed corrugations on incident internal waves coming from
$x=-\infty$
at the steady state. Thus we consider a seabed topography superimposed on the mean water depth of the form
$$\begin{eqnarray}b(x,y)=\left\{\begin{array}{@{}cc@{}}\displaystyle \frac{d}{2}(\text{e}^{\text{i}\unicode[STIX]{x1D711}}\text{e}^{\text{i}\boldsymbol{k}_{b}\boldsymbol{\cdot }\boldsymbol{x}_{h}}+\text{c.c.}), & 0\leqslant x\leqslant \ell ,-\infty \leqslant y\leqslant +\infty ,\\ 0, & \text{otherwise},\end{array}\right.\end{eqnarray}$$
with
$\boldsymbol{k}_{b}$
the corrugation wavenumber vector,
$\unicode[STIX]{x1D711}$
an arbitrary phase,
$d$
the corrugation amplitude,
$\ell$
the length of the patch,
$\text{c.c.}$
denotes the complex conjugate and
$\boldsymbol{x}_{h}=(x,y)$
. We look for a steady-state time-periodic solution of the form
$(u,v,w)=Re[(\hat{u} ,\hat{v},{\hat{w}})\text{e}^{-\text{i}\unicode[STIX]{x1D714}t}]$
(
$Re$
denoting the real part) with
$\unicode[STIX]{x1D714}$
the angular frequency of the incident waves. Therefore,
$\unicode[STIX]{x2202}_{t}$
can be substituted with
$-\text{i}\unicode[STIX]{x1D714}$
and
$(u,v,w)$
with
$Re[(\hat{u} ,\hat{v},{\hat{w}})\text{e}^{-\text{i}\unicode[STIX]{x1D714}t}]$
in (2.1)–(2.2), leading to (dropping the hat symbol)
with
$\boldsymbol{u}(x,y,z)=(u,v,w)$
the time-independent complex-valued velocity field to be found and
$\unicode[STIX]{x1D707}(\unicode[STIX]{x1D714})=\sqrt{(\unicode[STIX]{x1D714}^{2}-f^{2})/(N^{2}-\unicode[STIX]{x1D714}^{2})}$
the so-called internal-waves slope (cf. e.g. Bühler & Holmes-Cerfon Reference Bühler and Holmes-Cerfon2011).
Upstream (
$x\leqslant 0$
) and downstream (
$x\geqslant \ell$
) of the corrugated patch, the bottom is flat (
$b=0$
) and the solution of (2.1) can be written as a sum
$w=\sum _{j}w_{j}$
of internal-wave modes of the form
provided that
$f<\unicode[STIX]{x1D714}<N$
, with
$\unicode[STIX]{x1D6FE}_{j}=j\unicode[STIX]{x03C0}/H$
the vertical wavenumber and
$A_{j}$
the complex wave-mode amplitude. For each wave mode (2.6), the magnitude of the horizontal wavenumber
$k_{j}=|\boldsymbol{k}_{j}|$
can be related to the vertical wavenumber through the dispersion relation
While the wave modes (2.6) propagate independently from each other over the flat bottom, they become coupled over the corrugations (i.e. when
$b\neq 0$
) through the bottom boundary condition (2.4c
). We will demonstrate that energy transfers at the steady state between the wave modes can become significant under resonance conditions.
2.2 Regular perturbation
We consider the case of bottom corrugations that are small compared to the mean water depth, i.e. we let
$\unicode[STIX]{x1D716}=d/H\ll 1$
, such that the problem can be solved via asymptotic analysis. To ease the derivation, we use primed dimensionless variables given by
$(u,v)=(Uu^{\prime },Uv^{\prime })$
,
$w=\unicode[STIX]{x1D707}Uw^{\prime }$
,
$b=db^{\prime }$
,
$\boldsymbol{x}_{h}=(H/\unicode[STIX]{x1D707})\boldsymbol{x}_{h}^{\prime }$
,
$z=Hz^{\prime }$
, with
$U$
the magnitude of the characteristic horizontal velocity of the incident waves. The proposed scaling is suggested by the dimensional form of the wave modes over the flat bottom, i.e. (2.6). With the proposed scaling, the dimensionless form of the flat-bottom modes reads
where
$\unicode[STIX]{x1D73F}_{j}=\boldsymbol{k}_{j}H/\unicode[STIX]{x1D707}$
is the dimensionless wavenumber (
$\unicode[STIX]{x1D705}_{j}=|\unicode[STIX]{x1D73F}_{j}|$
),
$w_{j}^{\prime }\sim \sqrt{(u_{j}^{\prime })^{2}+(v_{j}^{\prime })^{2}}\sim O(1)$
, and the bottom topography becomes
with
$\unicode[STIX]{x1D73F}_{b}=\boldsymbol{k}_{b}H/\unicode[STIX]{x1D707}$
.
Using dimensionless variables the steady-state equations are now written as (dropping the primes from here onward)
Let us approximate the solution by a perturbation series of the form
with
$\boldsymbol{u}^{(j)}\sim O(1)$
for
$j=1,2$
. Substituting (2.12) into (2.10c
) yields
which, using a first-order Taylor series approximation about
$z=-1$
, can be further expanded as
$$\begin{eqnarray}\displaystyle & & \displaystyle w^{(0)}+\unicode[STIX]{x1D716}b\unicode[STIX]{x2202}_{z}w^{(0)}+\unicode[STIX]{x1D716}w^{(1)}+\unicode[STIX]{x1D716}^{2}b\unicode[STIX]{x2202}_{z}w^{(1)}+\cdots \nonumber\\ \displaystyle & & \displaystyle \quad =\unicode[STIX]{x1D716}[u^{(0)}+\unicode[STIX]{x1D716}b\unicode[STIX]{x2202}_{z}u^{(0)}+\unicode[STIX]{x1D716}u^{(1)}+\unicode[STIX]{x1D716}^{2}b\unicode[STIX]{x2202}_{z}u^{(1)}+\cdots \,]\unicode[STIX]{x2202}_{x}b\nonumber\\ \displaystyle & & \displaystyle \qquad +\,\unicode[STIX]{x1D716}[v^{(0)}+\unicode[STIX]{x1D716}b\unicode[STIX]{x2202}_{z}v^{(0)}+\unicode[STIX]{x1D716}v^{(1)}+\unicode[STIX]{x1D716}^{2}b\unicode[STIX]{x2202}_{z}v^{(1)}+\cdots \,]\unicode[STIX]{x2202}_{y}b,\quad z=-1.\end{eqnarray}$$
The zero- and first-order equations obtained from (2.14) become, respectively,
The asymptotic expansion resulting in (2.15) for the bottom boundary condition is valid provided that
$\unicode[STIX]{x1D716}=d/H\ll 1$
and the right-hand side of (2.15b
) remains of order one. For monochromatic bottom corrugations given by (2.9), this means that we require (i)
$\unicode[STIX]{x1D73F}_{b}\sim O(1)$
(from the terms
$u^{(0)}\unicode[STIX]{x2202}_{x}b$
and
$v^{(0)}\unicode[STIX]{x2202}_{y}b$
on the right-hand side of (2.15b
)) and (ii)
$\unicode[STIX]{x1D705}\sim O(1)$
where
$\unicode[STIX]{x1D705}$
is the dimensionless vertical wavenumber of internal waves (from the term
$b\unicode[STIX]{x2202}_{z}w^{(0)}$
on the right-hand side of (2.15b
)). The first condition (i) implies in terms of dimensional variables
$k_{b}d/\unicode[STIX]{x1D707}\sim O(\unicode[STIX]{x1D716})\ll 1$
, i.e. the bottom slope
$k_{b}d$
must be much smaller than the internal-wave slope
$\unicode[STIX]{x1D707}$
, such that (i) is a stronger requirement than the typical subcritical-slope assumption
$k_{b}d\leqslant \unicode[STIX]{x1D707}$
(cf. Bühler & Holmes-Cerfon Reference Bühler and Holmes-Cerfon2011). The second condition (ii) implies in terms of dimensional variables
$\unicode[STIX]{x1D6FE}d\sim O(\unicode[STIX]{x1D716})\ll 1$
, i.e. the corrugation height much be much smaller than the vertical wavelength (
$2\unicode[STIX]{x03C0}/\unicode[STIX]{x1D6FE}$
) of internal waves. Note that (ii) is always verified for the incident mode-one wave since the vertical wavelength is half the water depth.
It can be noted that in considering the linear form (2.1) of the wave equations, we have neglected the advection of bottom-generated waves by the incident flow. When the incident flow corresponds to semi-diurnal internal tides, which is the case of our interest, this simplification is acceptable because velocities of the internal tides are in general of order
$U\sim O(1~\text{cm}~\text{s}^{-1})$
or smaller (e.g. Zhao et al.
Reference Zhao, Alford, Girton, Rainville and Simmons2016) such that the advective term is much smaller than the acceleration term, i.e. in dimensional form
$(U\unicode[STIX]{x2202}_{x}/\unicode[STIX]{x2202}_{t})\sim (Uk/\unicode[STIX]{x1D714})\ll 1$
, for wavelengths down to a few kilometres or smaller.
2.3 Chain resonance conditions
As expected, the zero-order solution is not affected by bottom corrugations, such that it can be written as a superposition of wave modes given by (2.8). Using the dimensionless polarization relations (2.11), the forcing term on the right-hand side of (2.15b ) due to the interaction of a leading-order wave mode (2.8) with bottom corrugations can thus be written as
where
$\unicode[STIX]{x1D703}$
denotes the direction of propagation of the internal waves, i.e. we note
$\unicode[STIX]{x1D73F}_{j}=(\unicode[STIX]{x1D705}_{j}\cos \unicode[STIX]{x1D703},\unicode[STIX]{x1D705}_{j}\sin \unicode[STIX]{x1D703})$
.
For incident waves with wavenumber
$\unicode[STIX]{x1D73F}_{j}=\unicode[STIX]{x1D73F}_{in}$
and
$b$
given by (2.9), it can be seen from (2.16) that the forcing of
$w^{(1)}$
is by wave-like terms with wavenumber
$\unicode[STIX]{x1D73F}_{in}\pm \unicode[STIX]{x1D73F}_{b}$
. Because
$w^{(0)}$
and
$w^{(1)}$
satisfy the same governing equations (except for the bottom boundary condition), we thus know from the theory of wave–bottom resonance that
$w^{(1)}$
can grow unbounded over the corrugated patch and potentially become much larger than
$O(1)$
when
$\unicode[STIX]{x1D73F}_{in}\pm \unicode[STIX]{x1D73F}_{b}$
is a natural wavenumber of the zero-order problem, i.e. when there exists an integer
$m>0$
such that
$|\unicode[STIX]{x1D73F}_{in}\pm \unicode[STIX]{x1D73F}_{b}|=m\unicode[STIX]{x03C0}$
(see e.g. Liu & Yue Reference Liu and Yue1998, for the case of surface waves). Regular perturbation fails to capture an accurate solution at resonance (the unbounded growth of
$w^{(1)}$
is unphysical) because the wave–bottom interaction are so strong that the incident wave loses significant energy and new waves become strongly and coherently generated by the many small seabed undulations. This resonant scattering can be dealt with by the method of multiple scales, i.e. including all possibly blowing-up modes at leading order and allowing them to slowly evolve over the corrugations, as done in § 3. It is important to note here that the wave–bottom resonance is a resonance condition on the horizontal wavenumbers only because the interaction happens at a boundary between a freely propagating wave and a frozen bottom wave (i.e. of zero frequency). This is a situation different from nonlinear wave–wave interactions for which the resonance condition requires a frequency match and a wavenumber match in all spatial dimensions.
When a resonance is obtained between the incident wave and the bottom corrugations, the newly (resonantly) generated wave is added to the set of zero-order wave modes and we note the corresponding wavenumber
$\unicode[STIX]{x1D73F}_{r_{\pm 1}}=\unicode[STIX]{x1D73F}_{in}\pm \unicode[STIX]{x1D73F}_{b}$
(cf. figure 1
a). In a homogeneous fluid, the interaction of an incident wave with monochromatic corrugations can resonate at most one wave (i.e. the reflected wave
$\unicode[STIX]{x1D73F}_{r_{-1}}$
). In a continuously stratified fluid, however, the initial interaction can resonate both
$\unicode[STIX]{x1D73F}_{r_{+}1}$
and
$\unicode[STIX]{x1D73F}_{r_{-1}}$
, and each one of these two waves can then resonate other new waves. Such a chain resonance is shown in figure 1(b), which includes the incident mode-one internal wave (
$\unicode[STIX]{x1D73F}_{in}$
) interacting with monochromatic corrugations (
$\unicode[STIX]{x1D73F}_{b}$
), the resulting forcing (resonant) wavenumbers (noted
$\unicode[STIX]{x1D73F}_{r_{\pm 1}}$
), as well as the forcing (again resonant) wavenumbers
$\unicode[STIX]{x1D73F}_{r_{+2}}=\unicode[STIX]{x1D73F}_{r_{+1}}+\unicode[STIX]{x1D73F}_{b}$
due to the interaction of
$\unicode[STIX]{x1D73F}_{r_{+1}}$
with the same monochromatic corrugations. Other forcing resonant higher-mode wavenumbers (
$\unicode[STIX]{x1D73F}_{r_{-1}},\unicode[STIX]{x1D73F}_{r_{-2}},\ldots$
,
$\unicode[STIX]{x1D73F}_{r_{+2}},\unicode[STIX]{x1D73F}_{r_{+3}},\ldots$
) also participate in the chain resonance, with the sequence being potentially infinite.
As can be expected from a purely geometric argument, the successive forcing wavenumbers cannot all be perfectly resonant unless the incident wave comes at normal incidence (i.e.
$\unicode[STIX]{x1D703}_{in}=0$
), since in this case the spacing between the successively resonated wavenumbers is always
$\unicode[STIX]{x1D705}_{1}=\unicode[STIX]{x03C0}$
in a linearly stratified fluid (Bühler & Holmes-Cerfon Reference Bühler and Holmes-Cerfon2011). In figure 1(c), we illustrate the effect of detuning due to oblique incidence by showing that the
$\unicode[STIX]{x1D73F}_{r_{+1}}$
wave is in fact only near resonance with the corrugations
$\unicode[STIX]{x1D73F}_{b}$
, such that the forcing and resonant wavenumbers,
$\unicode[STIX]{x1D73F}_{r_{+1}}+\unicode[STIX]{x1D73F}_{b}$
and
$\unicode[STIX]{x1D73F}_{r_{+2}}$
respectively, are separated by a (small) detuning wavenumber, which we note
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D739}_{+2}$
.
In the general case, we write the positive and negative branches of the successively resonated wavenumbers as
3 Derivation of the envelope equations
In order to obtain a uniformly valid solution of energy exchanges between the incident and bottom-generated waves at resonance, we now introduce the slow variable
$\overline{\boldsymbol{x}}_{h}=\unicode[STIX]{x1D716}\boldsymbol{x}_{h}$
and look for a solution
$\boldsymbol{u}(\boldsymbol{x}_{h},\overline{\boldsymbol{x}}_{h};\unicode[STIX]{x1D716})$
that depends on both
$\boldsymbol{x}_{h}$
and
$\overline{\boldsymbol{x}}_{h}$
.
Inserting the multiple-scale ansatz
$\boldsymbol{u}=\boldsymbol{u}^{(0)}(\boldsymbol{x}_{h},\overline{\boldsymbol{x}}_{h};\unicode[STIX]{x1D716})+\unicode[STIX]{x1D716}^{1}\boldsymbol{u}^{(1)}(\boldsymbol{x}_{h},\overline{\boldsymbol{x}}_{h};\unicode[STIX]{x1D716})+\cdots \,$
into equations (2.10) yields at zero order
$$\begin{eqnarray}\displaystyle w^{(0)} & = & \displaystyle A_{in}(\overline{\boldsymbol{x}}_{h})S_{in}(z)E_{in}(\boldsymbol{x}_{h})+\mathop{\sum }_{m=1}^{\infty }A_{+m}(\overline{\boldsymbol{x}}_{h})S_{+m}(z)E_{+m}(\boldsymbol{x}_{h})\nonumber\\ \displaystyle & & \displaystyle +\mathop{\sum }_{m=1}^{\infty }A_{-m}(\overline{\boldsymbol{x}}_{h})S_{-m}(z)E_{-m}(\boldsymbol{x}_{h}),\end{eqnarray}$$
where
$A_{in}(\overline{\boldsymbol{x}}_{h})$
and
$A_{\pm m}(\overline{\boldsymbol{x}}_{h})$
are the slowly varying amplitudes of the incident and resonated waves to be found,
$\unicode[STIX]{x1D73F}_{r_{\pm m}}$
are the resonated wavenumbers given by the chain resonance equations (2.17),
$S_{\pm m}=\sin [\unicode[STIX]{x1D705}_{r_{\pm m}}(z+1)]$
is the zero-order sine vertical structure function (recall
$\unicode[STIX]{x1D705}_{r_{\pm m}}=\unicode[STIX]{x03C0}r_{\pm m}$
with
$r_{\pm m}$
the wave-mode number) and
$E_{\pm m}=\exp (\text{i}\unicode[STIX]{x1D73F}_{r_{\pm m}}\boldsymbol{\cdot }\boldsymbol{x}_{h})$
. From the dimensionless steady-state polarization relations (2.11) we find at zero order (using a compact expression in which the sum includes both the positive and negative branches)
Inserting the multiple-scale ansatz
$\boldsymbol{u}=\boldsymbol{u}^{(0)}(\boldsymbol{x}_{h},\overline{\boldsymbol{x}}_{h};\unicode[STIX]{x1D716})+\unicode[STIX]{x1D716}^{1}\boldsymbol{u}^{(1)}(\boldsymbol{x}_{h},\overline{\boldsymbol{x}}_{h};\unicode[STIX]{x1D716})$
into equations (2.10) yields at first order
The solvability condition ensures that
$w^{(1)}$
remains bounded by requiring the resonant forcing due to the slow variations of the wave amplitudes (represented by the right-hand side of (3.4a
)) to counterbalance the resonant forcing due to the wave–bottom interactions (3.4c
). Mathematically the solvability condition is obtained as the condition that the direct integration of the forcing (3.4a
) projected onto the eigenmodes
$S_{\pm m}E_{\pm m}^{\ast }$
of the linear operator (e.g. Mei Reference Mei1985), i.e.
$$\begin{eqnarray}\displaystyle & & \displaystyle \int \text{d}x\,\text{d}y\int _{z=-1}^{0}\text{d}z[S_{\pm m}E_{\pm m}^{\ast }(\unicode[STIX]{x2202}_{z}^{2}-\unicode[STIX]{x1D6FB}_{h}^{2})w^{(1)}]\nonumber\\ \displaystyle & & \displaystyle \quad =\int \text{d}x\,\text{d}yE_{\pm m}^{\ast }2\overline{\unicode[STIX]{x1D735}}_{h}\boldsymbol{\cdot }\unicode[STIX]{x1D735}_{h}\int _{z=-1}^{0}\text{d}zS_{\pm m}w^{(0)},\nonumber\\ \displaystyle & & \displaystyle \quad =\int \text{d}x\,\text{d}yE_{\pm m}^{\ast }\overline{\unicode[STIX]{x1D735}}_{h}\boldsymbol{\cdot }\unicode[STIX]{x1D735}_{h}\left(\mathop{\sum }_{\ell =0}^{\infty }A_{\pm \ell }E_{\pm \ell }\right),\end{eqnarray}$$
derived with the help of (3.4a
) (
$^{\ast }$
denotes the complex conjugate), is equal to the integral value projected on the boundaries (obtained following Green’s method), i.e.
$$\begin{eqnarray}\displaystyle & & \displaystyle \int \text{d}x\,\text{d}y\int _{z=-1}^{0}\text{d}z[S_{\pm m}E_{\pm m}^{\ast }(\unicode[STIX]{x2202}_{z}^{2}-\unicode[STIX]{x1D6FB}_{h}^{2})w^{(1)}]\nonumber\\ \displaystyle & & \displaystyle \quad =\int \text{d}x\,\text{d}y\int _{z=-1}^{0}\text{d}z[S_{\pm m}E_{\pm m}^{\ast }(\unicode[STIX]{x2202}_{z}^{2}-\unicode[STIX]{x1D6FB}_{h}^{2})w^{(1)}-w^{(1)}(\unicode[STIX]{x2202}_{z}^{2}-\unicode[STIX]{x1D6FB}_{h}^{2})S_{\pm m}E_{\pm m}^{\ast }],\nonumber\\ \displaystyle & & \displaystyle \quad =\int \text{d}x\,\text{d}y\{[S_{\pm m}\unicode[STIX]{x2202}_{z}w^{(1)}]_{z=-1}^{0}E_{\pm m}^{\ast }-[w^{(1)}\unicode[STIX]{x2202}_{z}S_{\pm m}]_{z=-1}^{0}E_{\pm m}^{\ast }\},\nonumber\\ \displaystyle & & \displaystyle \quad =\int \text{d}x\,\text{d}y\unicode[STIX]{x1D705}_{r_{\pm m}}\left\{\underbrace{\unicode[STIX]{x2202}_{x}[u^{(0)}(z=-1)b]}_{{\mathcal{X}}}+\underbrace{\unicode[STIX]{x2202}_{y}[v^{(0)}(z=-1)b]}_{{\mathcal{Y}}}\right\}E_{\pm m}^{\ast },\end{eqnarray}$$
where, using the chain resonance equations for the resonated wavenumbers (2.17),
$$\begin{eqnarray}\displaystyle {\mathcal{X}} & = & \displaystyle \unicode[STIX]{x2202}_{x}\left\{\frac{1}{2}(\text{e}^{\text{i}\unicode[STIX]{x1D711}}\text{e}^{\text{i}\unicode[STIX]{x1D73F}_{b}\boldsymbol{\cdot }\boldsymbol{x}_{h}}+\text{e}^{-\text{i}\unicode[STIX]{x1D711}}\text{e}^{-\text{i}\unicode[STIX]{x1D73F}_{b}\boldsymbol{\cdot }\boldsymbol{x}_{h}})\mathop{\sum }_{n=0}^{\infty }\text{i}A_{\pm n}\left[\cos (\unicode[STIX]{x1D703}_{\pm n})+\frac{\text{i}f}{\unicode[STIX]{x1D714}}\sin (\unicode[STIX]{x1D703}_{\pm n})\right]E_{\pm n}\right\}\nonumber\\ \displaystyle & = & \displaystyle \unicode[STIX]{x2202}_{x}\left\{\frac{1}{2}\mathop{\sum }_{n=0}^{\infty }\text{i}A_{\pm n}\left[\cos (\unicode[STIX]{x1D703}_{\pm n})+\frac{\text{i}f}{\unicode[STIX]{x1D714}}\sin (\unicode[STIX]{x1D703}_{\pm n})\right](\text{e}^{\text{i}\unicode[STIX]{x1D711}}\text{e}^{\text{i}(\unicode[STIX]{x1D73F}_{r_{\pm n}}+\unicode[STIX]{x1D73F}_{b})\boldsymbol{\cdot }\boldsymbol{x}_{h}}+\text{e}^{-\text{i}\unicode[STIX]{x1D711}}\text{e}^{\text{i}(\unicode[STIX]{x1D73F}_{r_{\pm n}}-\unicode[STIX]{x1D73F}_{b})\boldsymbol{\cdot }\boldsymbol{x}_{h}})\right\}\nonumber\\ \displaystyle & = & \displaystyle \unicode[STIX]{x2202}_{x}\left\{\frac{1}{2}\mathop{\sum }_{n=0}^{\infty }\text{i}A_{+n}\left[\cos (\unicode[STIX]{x1D703}_{+n})+\frac{\text{i}f}{\unicode[STIX]{x1D714}}\sin (\unicode[STIX]{x1D703}_{+n})\right](\!\text{e}^{\text{i}\unicode[STIX]{x1D711}}\text{e}^{\text{i}\unicode[STIX]{x1D73F}_{r_{+(n+1)}}\boldsymbol{\cdot }\boldsymbol{x}_{h}}\text{e}^{-\text{i}\unicode[STIX]{x1D739}_{+(n+1)}\boldsymbol{\cdot }\overline{\boldsymbol{x}}_{h}}\right.\nonumber\\ \displaystyle & & \displaystyle +\,\text{e}^{-\text{i}\unicode[STIX]{x1D711}}\text{e}^{\text{i}\unicode[STIX]{x1D73F}_{r_{+(n-1)}}\boldsymbol{\cdot }\boldsymbol{ x}_{h}}\text{e}^{\text{i}\unicode[STIX]{x1D739}_{+n}\boldsymbol{\cdot }\overline{\boldsymbol{x}}_{h}}\! )+\frac{1}{2}\mathop{\sum }_{n=0}^{\infty }\text{i}A_{-n}\left[\cos (\unicode[STIX]{x1D703}_{-n})+\frac{\text{i}f}{\unicode[STIX]{x1D714}}\sin (\unicode[STIX]{x1D703}_{-n})\right]\nonumber\\ \displaystyle & & \displaystyle \left.\times \,(\text{e}^{\text{i}\unicode[STIX]{x1D711}}\text{e}^{\text{i}\unicode[STIX]{x1D73F}_{r_{-(n-1)}}\boldsymbol{\cdot }\boldsymbol{ x}_{h}}\text{e}^{\text{i}\unicode[STIX]{x1D739}_{-n}\boldsymbol{\cdot }\overline{\boldsymbol{x}}_{h}}+\text{e}^{-\text{i}\unicode[STIX]{x1D711}}\text{e}^{\text{i}\unicode[STIX]{x1D73F}_{r_{-(n+1)}}\boldsymbol{\cdot }\boldsymbol{ x}_{h}}\text{e}^{-\text{i}\unicode[STIX]{x1D739}_{-(n+1)}\boldsymbol{\cdot }\overline{\boldsymbol{x}}_{h}})\vphantom{\frac{1}{2}\mathop{\sum }_{n=0}^{\infty }\left[\frac{\text{i}f}{\unicode[STIX]{x1D714}}\right]}\right\},\end{eqnarray}$$
and where the expression for
${\mathcal{Y}}$
is the same as
${\mathcal{X}}$
provided that we make the changes
$\unicode[STIX]{x2202}_{x}\rightarrow \unicode[STIX]{x2202}_{y}$
and
$f\rightarrow -f$
.
The equation for each wave amplitude
$A_{\pm m}(\overline{\boldsymbol{x}}_{h})$
is obtained by equating non-zero terms in (3.5) with those in (3.6) for all
$m$
(
$\int \text{d}x\text{d}y\equiv 0$
unless the integrand is non-oscillatory). In (3.5), non-zero terms are trivially given by
$\text{i}\unicode[STIX]{x1D73F}_{r_{\pm m}}\boldsymbol{\cdot }\overline{\unicode[STIX]{x1D735}}_{h}A_{\pm m}$
. In (3.6), non-zero terms are obtained by selecting the wave modes
$A_{\pm (m-1)}$
and
$A_{\pm (m+1)}$
within the sums in
${\mathcal{X}}$
and
${\mathcal{Y}}$
. Equating the non-zero terms, the equation for
$A_{\pm m}$
is finally obtained as
$$\begin{eqnarray}\displaystyle & & \displaystyle \left[\left(\frac{\unicode[STIX]{x1D73F}_{r_{\pm m}}}{\unicode[STIX]{x1D705}_{r_{\pm m}}}\right)\boldsymbol{\cdot }\overline{\unicode[STIX]{x1D735}}_{h}\right]A_{\pm m}=\frac{\text{i}\unicode[STIX]{x1D705}_{r_{\pm m}}}{2}\left[\left(\frac{\unicode[STIX]{x1D73F}_{r_{\pm m}}}{\unicode[STIX]{x1D705}_{r_{\pm m}}}\right)\cdot +\frac{\text{i}f}{\unicode[STIX]{x1D714}}\left(\frac{\unicode[STIX]{x1D73F}_{r_{\pm m}}}{\unicode[STIX]{x1D705}_{r_{\pm m}}}\right)\times \right]\nonumber\\ \displaystyle & & \displaystyle \quad \left\{\left(\frac{\unicode[STIX]{x1D73F}_{r_{\pm (m-1)}}}{\unicode[STIX]{x1D705}_{r_{\pm (m-1)}}}\right)A_{\pm (m-1)}\text{e}^{-\text{i}\unicode[STIX]{x1D739}_{\pm m}\boldsymbol{\cdot }\overline{\boldsymbol{x}}_{h}}\text{e}^{\pm \text{i}\unicode[STIX]{x1D711}}+\left(\frac{\unicode[STIX]{x1D73F}_{r_{\pm (m+1)}}}{\unicode[STIX]{x1D705}_{r_{\pm (m+1)}}}\right)A_{\pm (m+1)}\text{e}^{\text{i}\unicode[STIX]{x1D739}_{\pm (m+1)}\boldsymbol{\cdot }\overline{\boldsymbol{x}}_{h}}\text{e}^{\mp \text{i}\unicode[STIX]{x1D711}}\right\},\end{eqnarray}$$
where we recall that
$\unicode[STIX]{x1D6FF}_{\pm m}$
is the detuning wavenumber (cf. (2.17)) which must be of order
$O(1)$
for the multiple-scale derivation to be valid, and ‘
$\cdot$
’ and ‘
$\times$
’ (inside the brackets on the right-hand side of (3.8)) are the dot and cross-product operators acting on the (vector) terms inside the curly brackets. The left-hand side of (3.8) represents the slow variations of
$A_{\pm m}$
, while the right-hand side represents the effect of the interactions between the corrugations and its resonant neighbours, i.e.
$A_{\pm (m-1)}$
and
$A_{\pm (m+1)}$
. The strength of energy exchanges between the two coupled pairs of waves is, for the case of colinear waves, given by
$\unicode[STIX]{x1D705}_{r_{\pm m}}$
. Thus, energy exchanges occur over a shorter length scale if the waves’ wavenumber
$\unicode[STIX]{x1D705}_{r_{\pm m}}$
is larger. Provided that there is no detuning (i.e.
$\unicode[STIX]{x1D6FF}_{\pm m}=0$
), energy exchanges also occur over a shorter length scale if the waves propagate in the same direction (from the
$\unicode[STIX]{x1D73F}_{r_{\pm m}}\boldsymbol{\cdot }\unicode[STIX]{x1D73F}_{r_{\pm (m\pm 1)}}$
terms), since in this case the imaginary (weakening) Coriolis term is zero. With non-zero detuning, however, the effect of Coriolis becomes more complex and no general conclusion can be drawn. It is interesting to note that the exchange of energy through wave–bottom interactions between waves that are perpendicular (
$\unicode[STIX]{x1D73F}_{r_{\pm m}}\boldsymbol{\cdot }\unicode[STIX]{x1D73F}_{r_{\pm (m\pm 1)}}=0$
), which is impossible in a non-rotating system (a phenomenon known as Bragg degenerate resonance in the case of surface waves, see e.g. Couston et al. (Reference Couston, Jalali and Alam2017)), becomes possible with the addition of the Coriolis effect. A straightforward manipulation and combination of (3.8) (i.e. multiplying by
$A_{\pm m}^{\ast }/\unicode[STIX]{x1D705}_{r_{\pm m}}$
with
$^{\ast }$
denoting the complex conjugate, adding the complex conjugate counterpart and summing all equations over
$\pm m$
) can be shown to result in an equation for the conservation of total energy flux, i.e.
which is expected since the system is conservative and at steady state (recall
$A_{0}=A_{in}$
). Note that since the dimensional horizontal group velocity is
$\boldsymbol{C}_{g}=(\unicode[STIX]{x1D714}^{2}-f^{2})\boldsymbol{k}/[\unicode[STIX]{x1D714}(1+\unicode[STIX]{x1D707}^{2})k^{2}]$
and
$\unicode[STIX]{x1D714}$
,
$\unicode[STIX]{x1D707}$
are the same for all waves, the expression to the right of the gradient in (3.9) is indeed the total horizontal energy flux.
The envelope equation can be rewritten in a more convenient form, i.e. with constant coefficients, provided that we consider the modulated version of the envelope amplitude
where
Substituting (3.10) in (3.8) yields, dropping the tilde symbol,
$$\begin{eqnarray}\displaystyle & & \displaystyle \left[\left(\frac{\unicode[STIX]{x1D73F}_{r_{\pm m}}}{\unicode[STIX]{x1D705}_{r_{\pm m}}}\right)\boldsymbol{\cdot }\overline{\unicode[STIX]{x1D735}}_{h}\right]A_{\pm m}=\frac{\text{i}\unicode[STIX]{x1D705}_{r_{\pm m}}}{2}\left[\left(\frac{\unicode[STIX]{x1D73F}_{r_{\pm m}}}{\unicode[STIX]{x1D705}_{r_{\pm m}}}\right)\cdot +\frac{\text{i}f}{\unicode[STIX]{x1D714}}\left(\frac{\unicode[STIX]{x1D73F}_{r_{\pm m}}}{\unicode[STIX]{x1D705}_{r_{\pm m}}}\right)\times \right]\nonumber\\ \displaystyle & & \displaystyle \quad \,\left\{\left(\frac{\unicode[STIX]{x1D73F}_{r_{\pm (m-1)}}}{\unicode[STIX]{x1D705}_{r_{\pm (m-1)}}}\right)A_{\pm (m-1)}\text{e}^{\pm \text{i}\unicode[STIX]{x1D711}}+\left(\frac{\unicode[STIX]{x1D73F}_{r_{\pm (m+1)}}}{\unicode[STIX]{x1D705}_{r_{\pm (m+1)}}}\right)A_{\pm (m+1)}\text{e}^{\mp \text{i}\unicode[STIX]{x1D711}}\right\}+\text{i}\frac{(\unicode[STIX]{x1D73F}_{r_{\pm m}}\boldsymbol{\cdot }\unicode[STIX]{x1D71F}_{\pm m})}{\unicode[STIX]{x1D705}_{r_{\pm m}}\cos \unicode[STIX]{x1D703}_{\pm m}}A_{\pm m},\nonumber\\ \displaystyle & & \displaystyle\end{eqnarray}$$
which is a system of ordinary differential equations with constant coefficients easily amenable to numerical treatment. Physically, the energy exchanges between
$A_{\pm m}$
and its resonant neighbours occur after the successive (detuned) transfers of energy from the incident to the
$A_{\pm m}$
wave, such that energy exchanges are subject to the cumulative detuning of the chain resonance rather than the individual pair detunings. This explains the presence of the cumulative detuning term
$\unicode[STIX]{x1D71F}_{\pm m}$
on the right-hand side of (3.12). Note that for the positive (respectively negative) branch of the chain resonance, we take in (3.12) the upper
$+$
(respectively lower
$-$
) sign of the subscript indices.
In the results section § 4 we restrict our attention to sinusoidal corrugations that are long-crested and parallel to the
$y$
axis, i.e. we set
$\unicode[STIX]{x1D711}=-\unicode[STIX]{x03C0}/2$
and assume
$\unicode[STIX]{x1D73F}_{b}=\unicode[STIX]{x1D705}_{b}\hat{\boldsymbol{x}}$
(
$\hat{\boldsymbol{x}}$
denoting the unit vector in
$x$
direction), such that
$\unicode[STIX]{x2202}_{y}A_{\pm m}\equiv 0$
. The envelope equation (3.12) thus becomes one dimensional and is simplified as (substituting the slow variable
$\bar{x}$
with
$\unicode[STIX]{x1D716}x=(d/H)x$
)
$$\begin{eqnarray}\displaystyle & & \displaystyle \frac{\text{d}A_{\pm m}}{\text{d}x}=\pm \frac{d\unicode[STIX]{x1D705}_{r_{\pm m}}}{2H}\left[A_{\pm (m-1)}\frac{\displaystyle \cos (\unicode[STIX]{x1D703}_{\pm m}-\unicode[STIX]{x1D703}_{\pm (m-1)})+\frac{\text{i}f}{\unicode[STIX]{x1D714}}\sin (\unicode[STIX]{x1D703}_{\pm m}-\unicode[STIX]{x1D703}_{\pm (m-1)})}{\cos \unicode[STIX]{x1D703}_{\pm m}}\right.\nonumber\\ \displaystyle & & \displaystyle \quad \left.-\,A_{\pm (m+1)}\frac{\displaystyle \cos (\unicode[STIX]{x1D703}_{\pm m}-\unicode[STIX]{x1D703}_{\pm (m+1)})+\frac{\text{i}f}{\unicode[STIX]{x1D714}}\sin (\unicode[STIX]{x1D703}_{\pm m}-\unicode[STIX]{x1D703}_{\pm (m+1)})}{\cos \unicode[STIX]{x1D703}_{\pm m}}\right]+\text{i}\frac{\displaystyle \left(\unicode[STIX]{x1D73F}_{r_{\pm m}}\boldsymbol{\cdot }\frac{d}{H}\unicode[STIX]{x1D71F}_{\pm m}\right)}{\unicode[STIX]{x1D705}_{r_{\pm m}}\cos \unicode[STIX]{x1D703}_{\pm m}}A_{\pm m},\nonumber\\ \displaystyle & & \displaystyle\end{eqnarray}$$
for the resonated waves
$m\geqslant 1$
(note that the waves still propagate in both
$x$
and
$y$
even though slow variations only occur in
$x$
, as shown in figure 1), and
$$\begin{eqnarray}\displaystyle \frac{\text{d}A_{in}}{\text{d}x} & = & \displaystyle \frac{\text{d}\unicode[STIX]{x1D705}_{in}}{2H}\left[A_{-1}\frac{\displaystyle \cos (\unicode[STIX]{x1D703}_{in}-\unicode[STIX]{x1D703}_{-1})+\frac{\text{i}f}{\unicode[STIX]{x1D714}}\sin (\unicode[STIX]{x1D703}_{in}-\unicode[STIX]{x1D703}_{-1})}{\cos \unicode[STIX]{x1D703}_{in}}\right.\nonumber\\ \displaystyle & & \displaystyle \left.-\,A_{+1}\frac{\displaystyle \cos (\unicode[STIX]{x1D703}_{in}-\unicode[STIX]{x1D703}_{+1})+\frac{\text{i}f}{\unicode[STIX]{x1D714}}\sin (\unicode[STIX]{x1D703}_{in}-\unicode[STIX]{x1D703}_{+1})}{\cos \unicode[STIX]{x1D703}_{in}}\right],\end{eqnarray}$$
for the incident wave (
$m=0$
). We solve (3.13)–(3.14) as an eigenvalue problem over the domain
$x\in [0,{\mathcal{N}}\unicode[STIX]{x1D706}_{b}]$
(
${\mathcal{N}}$
the number of corrugations and
$\unicode[STIX]{x1D706}_{b}=2\unicode[STIX]{x03C0}/\unicode[STIX]{x1D705}_{b}$
the dimensionless corrugation wavelength) with
$x=0$
(respectively
$x={\mathcal{N}}\unicode[STIX]{x1D706}_{b}$
) the beginning (end) of the corrugated patch. The boundary conditions are
$A_{in}=1$
at
$x=0$
, i.e. the incident wave has a constant unitary amplitude upstream of the bars,
$A_{+m}=0$
at
$x=0$
, i.e. waves propagating in
$+x$
direction grow in amplitude from
$x=0$
onward, and
$A_{-m}=0$
at
$x={\mathcal{N}}\unicode[STIX]{x1D706}_{b}$
, i.e. waves propagating in
$-x$
direction can only exist upstream of the last seabed bar. As we solve (3.13)–(3.14), we consider a solution of the form
i.e. we consider a finite number
$M^{+}$
and
$M^{-}$
of resonated waves on both the positive and negative resonance branch (cf. (2.17)). We choose
$M^{+}$
and
$M^{-}$
such that increasing them (i.e. adding more modes to the solution) does not change the solution amplitudes of the lower-wavenumber modes significantly, i.e. the amplitudes do not change more than
${\sim}10\,\%$
. The convergence of the truncated series (3.15) with
$M^{\pm }$
toward the infinite series solution (3.2) is expected because high-mode-number waves grow more slowly, i.e. they require a longer corrugated patch, than low-mode-number waves (which besides carry most of the energy). It should be remarked that waves with relatively large detuning are not accurately predicted by multiple-scale analysis (since the derivation requires
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D6FF}_{\pm m}\ll \unicode[STIX]{x1D705}_{1}=\unicode[STIX]{x03C0}$
), but at the same time are not expected to carry a significant amount of energy as they result from wave–bottom interactions far from resonance. Therefore, here we check that waves with large detuning (i.e. specifically,
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D6FF}_{\pm m}/\unicode[STIX]{x1D705}_{1}\geqslant 0.1$
) included in (3.15) have small amplitudes (i.e. we check that the combined amplitude of detuned waves is always less than
${<}0.1$
), such that their effect on the multiple-scale solution can be neglected.
4 Results for idealized oceanic conditions
Here we demonstrate through different case studies that the interaction of an incident internal wave with long-crested bottom corrugations can lead to the resonant generation of many new high-wavenumber internal waves, thus potentially contributing to enhanced mixing events in the oceans. The variations of the incident and resonated wave amplitudes are obtained from (3.13)–(3.14) and the sequence of resonated wavenumber vectors is given by (2.17). The solution is fully determined by specifying the incident-wave parameters
$\{\unicode[STIX]{x1D705}_{in},\unicode[STIX]{x1D703}_{in},f/\unicode[STIX]{x1D714}\}$
, the number of corrugations
${\mathcal{N}}$
and their amplitude
$d/H$
and the corrugation wavenumber
$\unicode[STIX]{x1D73F}_{b}$
or alternatively the initial detuning
$\unicode[STIX]{x1D6FF}_{+1}$
or
$\unicode[STIX]{x1D6FF}_{-1}$
.
We consider incident waves that are mode-one internal waves (i.e.
$\unicode[STIX]{x1D705}_{in}=\unicode[STIX]{x1D705}_{1}=\unicode[STIX]{x03C0}$
) because such waves are known to carry significant amount of energy, to propagate long distances and to interact with seabed topographies in the oceans (Zhao et al.
Reference Zhao, Alford, MacKinnon and Pinkel2010). Mode-one internal waves are most often generated by surface tides or geostrophic flows over seabed topographies, and thus typically have low frequency, i.e. close to the tidal or inertial frequency. This implies that the internal-wave slope considered are relatively small, i.e. e.g.
$\unicode[STIX]{x1D707}\sim 0.07{-}0.18$
for
$N/f\sim 10{-}15$
and
$\unicode[STIX]{x1D714}/f\sim 1.5{-}2$
, and that the mode-one internal wavelength is in the 33–114 km range for a mean water depth
$H\sim 3{-}4~\text{km}$
. More specifically, here we consider incident waves at semi-diurnal tidal frequency
$\unicode[STIX]{x1D714}=1.4\times 10^{-4}~\text{rad}~\text{s}^{-1}$
and Coriolis frequency
$f=8.3\times 10^{-5}~\text{rad}~\text{s}^{-1}$
(obtained at
$35^{\circ }$
latitude), such that
$f/\unicode[STIX]{x1D714}=0.6$
. It can be noted that for the case of long-crested corrugations parallel to the
$y$
axis (as in figure 1), the chain resonance tends to resonate waves going primarily in the
$x$
direction, such that the Coriolis effect is in general weak. The efficiency of energy transfers becomes independent of the incident-wave frequency or slope, and hence of all wave parameters, when the incident wavenumber and corrugation wavenumber are colinear and/or
$f=0$
(Bühler & Holmes-Cerfon Reference Bühler and Holmes-Cerfon2011).
Variations of the incident and resonated envelope amplitudes (
$A_{in}$
and
$A_{+1},A_{+2},\ldots$
) over 25 seabed bars for normal incidence (
$\unicode[STIX]{x1D703}_{in}=0$
, cf. figure 1), as obtained from (3.13)–(3.14) (
$\unicode[STIX]{x1D706}_{b}=2\unicode[STIX]{x03C0}/\unicode[STIX]{x1D705}_{b}$
). With
$\unicode[STIX]{x1D705}_{b}\sim \unicode[STIX]{x1D705}_{in}=\unicode[STIX]{x03C0}$
, the first resonated wave
$A_{+1}$
is a mode-two wave in all cases and there can be no back-scattered (
$A_{-m}$
) wave. The detuning of the incident wave
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D6FF}_{+1}/\unicode[STIX]{x1D705}_{in}$
is (a) 0, (b) 2 %, (c) 4 %. Increasing detuning results in fewer resonated waves and a recapture of the available energy by the incident wave before the end of the patch (cf. (c)). The corrugation amplitude is
$d/H=0.008$
. Note that Coriolis has no effect on the variations of envelope amplitudes in this case of colinear waves.

Topographical features in the real ocean that are prominent and appear almost monochromatic are canyons and crests of fracture zones in the deep ocean. Such submarine features can be observed worldwide and in particular along the mid-oceanic ridges in regions of the East Pacific Rise and Mid-Atlantic Ridge (St Laurent & Garrett Reference St Laurent and Garrett2002), the Drake passage region in the Southern Ocean (Nikurashin & Ferrari Reference Nikurashin and Ferrari2010) and in the northeast Pacific (Bell Reference Bell1975b
). The wavelength of submarine canyons and crests is generally in the 50–120 km range, hence is similar to the wavelength of mode-one internal waves. As a result, here we will consider corrugation wavenumbers of the same order as the wavenumber of the incident waves, i.e.
$\unicode[STIX]{x1D705}_{b}\sim \unicode[STIX]{x1D705}_{in}=\unicode[STIX]{x1D705}_{1}=\unicode[STIX]{x03C0}$
, which implies that the first resonated waves will be low-mode internal waves (i.e. 1 or 2).
Because the multiple-scale theory requires
$\unicode[STIX]{x1D705}(d/H)\ll 1$
(cf. (2.15)), the normalized corrugation amplitude
$d/H$
must be small compared to the inverse of the largest mode number obtained in the chain resonance. For chain resonance including up to 10 modes, for instance, the theory thus requires
$d/H\sim O(0.01)$
. With such small corrugation amplitudes, a relatively large number of corrugations is required to obtain substantial energy transfers from the incident to the resonated waves. Therefore, here we will fix the number of corrugations to
${\mathcal{N}}=25$
and consider corrugation amplitudes
$d/H\sim O(0.01)$
for all our results. Much fewer seabed bars would be necessary if they were of a larger amplitude. However, satisfying the assumption
$\unicode[STIX]{x1D705}(d/H)\ll 1$
shall prevail, so we restrict our analysis to small seabed bars. Note that we made sure that the right-hand side of (2.10c
) is
$O(0.1)$
and always smaller than
$1/3$
for all our results.
4.1 Chain resonance at normal incidence
In this section we describe the chain resonance obtained at normal incidence and for long corrugations (i.e.
$\unicode[STIX]{x1D705}_{b}\sim \unicode[STIX]{x1D705}_{in}=\unicode[STIX]{x03C0}$
and
$\unicode[STIX]{x1D703}_{in}=0$
). The incident wave can be either perfectly tuned or detuned, i.e. such that
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D6FF}_{+1}=0$
or
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D6FF}_{+1}\neq 0$
(cf. (2.17)). We consider
${\mathcal{N}}=25$
seabed bars and the corrugation amplitude is
$\unicode[STIX]{x1D716}=d/H=0.008$
.
The perfectly tuned one-dimensional case was briefly discussed in Bühler & Holmes-Cerfon (Reference Bühler and Holmes-Cerfon2011), following a prior derivation by Chen (Reference Chen2009) who obtained a closed-form solution for the amplitude variations. Solving (3.13)–(3.14) with
$\unicode[STIX]{x1D705}_{b}=\unicode[STIX]{x1D705}_{1}$
, we find the variations of the incident (
$A_{in}$
) and resonated (
$A_{+m}$
) wave amplitudes as shown in figure 2(a); there are no back-scattered
$A_{-m}$
waves because the spacing between the corrugations is large and the detuning of the
$\unicode[STIX]{x1D705}_{r_{-1}}$
wave is also large. Note that our results agree perfectly with the solution of Chen (Reference Chen2009), which is expected since we solve (3.13)–(3.14) with a sufficiently large number of waves (i.e.
$M^{\pm }$
in (3.15) is sufficiently large that the truncated solution is close to the infinite series solution). The chain resonance for perfectly tuned normally incident waves only includes perfect resonances, such that we observe a cascade of the incident wave energy from the longest to the smallest scales. The initial amplitude decays monotonically over the bars while newly resonated waves successively capture the incident-wave energy.
Same as figure 2, except that this time we have backward-going resonated (
$A_{-m}$
) waves in addition to the forward-going (
$A_{+m}$
) waves as we consider shorter corrugations, i.e. for which
$\unicode[STIX]{x1D705}_{b}\sim 2\unicode[STIX]{x1D705}_{in}$
. The first resonated wave
$A_{+1}$
is a mode-three wave, and
$A_{-1}$
is a mode-one wave. The detuning
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D6FF}_{+1}/\unicode[STIX]{x1D705}_{in}$
is again (a) 0, (b) 2 % and (c) 4 %.

When the first wave–bottom interaction is not perfectly resonant, we obtain the amplitude variations shown in figure 2(b–c). For
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D6FF}_{+1}/\unicode[STIX]{x1D705}_{in}=0.02$
, figure 2(b) shows that the energy cascade still takes place, albeit at a slower rate over the seabed bars compared to the perfectly tuned case. With increased detuning
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D6FF}_{+1}/\unicode[STIX]{x1D705}_{in}=0.04$
, we can see in figure 2(c) that the chain resonance is stopped at approximately the second or third resonated wave. We also observe that the incident wave even gains energy back from the resonated waves, such that downstream of the patch the incident mode-one internal wave is again close to 1. With half the number of seabed bars, the incident wave amplitude would on the contrary be at its minimum, as can be seen at
$x/\unicode[STIX]{x1D706}_{b}\sim 12.5$
in figure 2(c). Indeed, the solution obtained for forward-scattered waves only is independent of the number of seabed bars, such that the results shown in figure 2 also apply for smaller patches. As the detuning is further increased (not shown), energy exchanges become even less strong and oscillate more rapidly. With
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D6FF}_{+1}/\unicode[STIX]{x1D705}_{in}=0.1$
, the decrease of the incident wave is negligible. It should be remarked, however, that detuning effects depend upon the interaction strength, measured as
$d/H$
. From (3.13), it can be seen that the ratio of the detuning term to the interaction term is proportional to
$(\unicode[STIX]{x1D716}\unicode[STIX]{x1D6E5}_{\pm m}/\unicode[STIX]{x1D705}_{r_{\pm m}})/(d/H)$
, such that detuning effects become less important as
$d/H$
is increased.
Variations of the incident and resonated wave envelopes for incidence angles (a)
$\unicode[STIX]{x1D703}_{in}=\unicode[STIX]{x03C0}/6$
, (b)
$\unicode[STIX]{x1D703}_{in}=\unicode[STIX]{x03C0}/4$
, (c)
$\unicode[STIX]{x1D703}_{in}=\unicode[STIX]{x03C0}/3$
. The first resonance resulting in the mode-two wave
$A_{+1}$
is perfect (
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D6FF}_{+1}=0$
). Back-resonated (
$A_{-m}$
) waves have negligible amplitude in all three cases due to large detuning that damp energy exchanges, and therefore are not shown. As in figure 2,
${\mathcal{N}}=25$
,
$f/\unicode[STIX]{x1D714}=0.6$
,
$\unicode[STIX]{x1D705}_{in}=\unicode[STIX]{x03C0}$
, but the corrugation height is this time increased to
$d/H=0.015$
.

We show in figure 3 the chain resonance when the normally incident waves and the corrugations first resonate a back-scattered mode-one wave
$A_{-1}$
, propagating in the
$-x$
direction, in addition to the forward-going mode-three wave
$A_{+1}$
(which is the situation that corresponds to corrugations approximately half the size of those considered in figure 2, i.e.
$\unicode[STIX]{x1D705}_{b}\sim 2\unicode[STIX]{x1D705}_{in}$
). The first resonance condition is perfectly satisfied with
$\unicode[STIX]{x1D705}_{b}=2\unicode[STIX]{x1D705}_{in}$
, hence so are the successive resonances (cf. figure 3
a). A cascade of energy is again obtained from the longest to the smallest scales. Back-scattered waves have zero amplitude at the end of the patch, but grow monotonically to the upstream. With detuning, as in figure 2, we see that fewer waves are resonated, but overall the effect of detuning up to 4 % is relatively small such that many new waves can be resonated. Note that the effect of detuning is smaller for the case with back-scattered waves compared to the case of figure 2(b–c) partly because
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D6FF}_{\pm 1}/\unicode[STIX]{x1D705}_{b}$
is smaller in figure 3(b–c) due to the larger
$\unicode[STIX]{x1D705}_{b}$
.
4.2 Chain resonance at oblique incidence
An oblique incidence of the mode-one waves results in non-zero detuning wavenumbers for most resonated waves, even when the incident wave is perfectly tuned (see figure 1
b): we call this the angular detuning. To isolate the effect of the angular detuning from the incident detuning (between the incident waves and the corrugations), here we first assume that the first forward-going forced wave is perfectly resonated, i.e.
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D6FF}_{+1}=0$
.
For a relatively broad range of incidence angles, i.e.
$\unicode[STIX]{x1D703}_{in}<\unicode[STIX]{x03C0}/8$
, we find that the chain resonance results are very similar to the normal-incidence case with no detuning. For
$\unicode[STIX]{x1D703}_{in}=\unicode[STIX]{x03C0}/6$
, figure 4(a) shows a number of new waves attaining large amplitude over the patch, suggesting that the chain resonance still takes place despite an individual detuning
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D6FF}_{+m}/\unicode[STIX]{x1D705}_{in}$
and cumulative detuning
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D6E5}_{+m}/\unicode[STIX]{x1D705}_{r_{+m}}$
increasing up to approximately 2 % for the first 10 waves. The detuning for the back-scattered waves is quite large (up to 50 % for
$A_{-1}$
), but even when we consider them, their predicted amplitude is negligible (less than 0.01), such that the results at leading order do not violate multiple scales.
For larger incidence angle
$\unicode[STIX]{x1D703}_{in}=\unicode[STIX]{x03C0}/4$
, figure 4(b) shows that the chain resonance is effectively stopped at just 2 or 3 resonated waves. In this case, individual
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D6FF}_{+m}/\unicode[STIX]{x1D705}_{in}$
and cumulative
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D6E5}_{+m}/\unicode[STIX]{x1D705}_{r_{+m}}$
detuning wavenumbers go up to 15 % and 4 % for the first 4 resonated waves, and are higher for further resonances. As for the previous case (figure 4
a), the detuning of the back-scattered waves is large such that no back-scattered waves are resonated. Figure 4(c) shows that the two resonated forward-going waves (
$A_{+1}$
and
$A_{+2}$
) are of even smaller amplitudes when the incidence angle is increased to
$\unicode[STIX]{x1D703}_{in}=\unicode[STIX]{x03C0}/3$
compared to
$\unicode[STIX]{x1D703}_{in}=\unicode[STIX]{x03C0}/4$
.
In figure 5(a–c) we show the same case of figure 4(b), i.e. with incidence angle
$\unicode[STIX]{x1D703}_{in}=\unicode[STIX]{x03C0}/4$
, but this time we consider a detuned incident wave. In figure 5(a) we show the results obtained for
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D739}_{+1}=-0.025\unicode[STIX]{x1D73F}_{r_{+1}}$
(i.e.
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D6FF}_{+1}=0.05\unicode[STIX]{x1D705}_{in}$
), corresponding to incident waves that are too short to perfectly resonate the
$\unicode[STIX]{x1D73F}_{r_{+1}}$
waves. Fewer waves are resonated and have smaller maximum amplitude than in figure 4(b). The effect of the incident-wave detuning can thus be seen to be added to that due to the oblique incidence. The oblique angular detuning is indeed opposite to the direction of the
$\unicode[STIX]{x1D73F}_{r_{+m}}$
waves (as is the case of the incident detuning), which makes the wave-bottom interactions always result in a wavenumber larger than the next closest natural resonated wavenumber
$\unicode[STIX]{x1D73F}_{r_{+(m+1)}}$
. When the incident-wave detuning is
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D739}_{+1}=0.025\unicode[STIX]{x1D73F}_{r_{+1}}$
(cf. figure 5
b), however, it counteracts the angular detuning such that more waves with relatively large amplitudes are resonated and a chain resonance is again obtained. With a larger positive detuning of
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D739}_{+1}=0.05\unicode[STIX]{x1D73F}_{r_{+1}}$
, even more waves are resonated but the maximum amplitudes of the low-mode waves over the patch are smaller (figure 5
c). The trend continues as the detuning is increased, until no resonances remain.
Same case as figure 4(b), except that this time the incident-wave detuning
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D6FF}_{+1}/\unicode[STIX]{x1D705}_{in}$
is 5 % for (a,b) and 10 % for (c). Unlike in other cases, in (a) the detuning is negative, i.e.
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D739}_{+1}\boldsymbol{\cdot }\unicode[STIX]{x1D73F}_{r_{+1}}<0$
(cf. (2.17)). In (a) the effects of the incident detuning and the angular detuning are added, such that fewer waves of smaller amplitudes are obtained compared to the perfectly tuned incident-wave case of figure 4(b). In (b,c), the two effects are opposite such that more waves are obtained resulting in an oblique chain resonance of many waves with different angles of propagation.

4.3 Discussion of results
From the various results shown in figures 2–5 it is found that the resonant generation of multiple internal waves over seabed corrugations is not limited to the special case of perfectly tuned normally incident waves, although the efficiency of energy transfers does change with changing incidence angle and detuning. The sensitivity of the resonance to the incident detuning can be partly assessed from the variations with
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D6FF}_{+1}/\unicode[STIX]{x1D705}_{in}$
of
which is the maximum energy flux of the resonated waves in
$x$
direction over the patch (normalized by the incident energy flux; see (3.9)). For normal incidence (
$\unicode[STIX]{x1D703}_{in}=0$
), figure 6(a) shows that the resonated waves capture more than 50 % of the incident energy flux with zero detuning and more than 40 % for a broad range of detuning wavenumber. The peak as well as the half-width of this curve would be increased provided that the corrugation amplitude increases too; the peak would also increase with the number of corrugations. While figure 6(a) implies that strong energy exchanges occur with or without detuning, it does not yet allow us to assess whether high-wavenumber waves are generated for relatively large detuning. In fact, as shown in figure 4(c), the incident wave can cede a significant fraction of its energy to just two resonated waves.
Effect of detuning on (a) the maximum of energy flux of the resonated waves
$\tilde{F}$
(4.1) and (b) the minimum Richardson number
$\tilde{Ri}$
(see (4.2)). The results are shown as a function of the normalized detuning wavenumber
$\unicode[STIX]{x1D716}\unicode[STIX]{x1D6FF}_{+1}/\unicode[STIX]{x1D705}_{in}$
for the case of normal incidence (
$\unicode[STIX]{x1D703}_{in}=0$
). As in figure 2,
$\unicode[STIX]{x1D705}_{in}=\unicode[STIX]{x03C0}$
,
${\mathcal{N}}=25$
,
$f/\unicode[STIX]{x1D714}=0.6$
and
$d/H=0.008$
.

Same as figure 6 but for incidence angle
$\unicode[STIX]{x1D703}_{in}=\unicode[STIX]{x03C0}/6$
(——, blue),
$\unicode[STIX]{x03C0}/4$
(——, red),
$\unicode[STIX]{x03C0}/3$
(——, yellow) and
$d/H=0.015$
. The energy flux ceded to the resonated waves is close to unity in all three cases when
$\unicode[STIX]{x1D6FF}_{+1}\sim 0$
.
$\tilde{Ri}$
decreases significantly for
$\unicode[STIX]{x1D703}_{in}=\unicode[STIX]{x03C0}/6,\unicode[STIX]{x03C0}/4$
, although the location of the global minimum is obtained for non-zero detuning; this implies that the effect of oblique incidence and incident detuning can cancel each other, resulting in the generation of multiple higher-wavenumber resonated modes. Parts of the curves shown as dotted lines correspond to cases for which the theory is relatively stretched, and therefore may not be quantitatively accurate.

Because generating high-wavenumber waves is expected to increase the vertical shear, here we make a parallel between the efficiency of chain resonance at generating high-wavenumber waves and the decrease of the Richardson number
$Ri=(HN/U)^{2}/(\unicode[STIX]{x2202}V/\unicode[STIX]{x2202}z)^{2}$
over the patch, where
$V$
is the dimensionless horizontal velocity and
$z$
the dimensionless vertical coordinate. The Richardson number is of great interest to the oceanographic community as it is often used as a proxy to predict the likelihood of overturning events and enhanced mixing in a stratified fluid, due to shear instability acting against the stable buoyancy field. Though the existence of a universal critical Richardson number
$Ri_{c}$
at which turbulent mixing can start is still debated, the lower bound
$Ri<Ri_{c}=1/4$
, originally derived for horizontal shear flows, of the order of unity is often assumed (Mack & Schoeberlein Reference Mack and Schoeberlein2004; Galperin, Sukoriansky & Anderson Reference Galperin, Sukoriansky and Anderson2007). The Richardson number for mode-one internal waves at tidal frequency can be roughly estimated from field measurements in the open ocean. Velocities of mode-one semi-diurnal internal waves have been reported to be of order
$U\sim O(0.01~\text{m}~\text{s}^{-1}{-}0.1~\text{m}~\text{s}^{-1})$
and higher close to large topographic features (Alford & Zhao Reference Alford and Zhao2007; Alford et al.
Reference Alford, MacKinnon, Zhao, Pinkel, Klymak and Peacock2007; Garrett & Kunze Reference Garrett and Kunze2007), such that for a depth of
$H=4000~\text{m}$
and constant buoyancy of
$N=2\times 10^{-4}~\text{s}^{-1}$
(which is within the range reported in some parts of the deep ocean, see e.g. St Laurent & Garrett Reference St Laurent and Garrett2002), the minimum Richardson number is of order
$Ri=(NH/U)^{2}/\unicode[STIX]{x03C0}^{2}\sim O(10)-O(10^{3})\gg 1$
. Low-mode internal tides at the semi-diurnal frequency are thus unlikely to overturn because of shear instability, which explains why it is generally assumed that a nonlinear mechanism or modal transformation must take place in order to destabilize the flow and induce mixing (Staquet & Sommeria Reference Staquet and Sommeria2002).
Here with simple monochromatic corrugations we showed that an efficient modal transformation can occur for a wide range of incidence angles and detuning. The efficiency of the energy transfer from low-mode to high-mode internal waves is now related to the drop of Richardson number
$\tilde{Ri}$
, i.e.
$$\begin{eqnarray}\tilde{Ri}=\frac{\displaystyle \left(1+\frac{f^{2}}{\unicode[STIX]{x1D714}^{2}}\right)\unicode[STIX]{x1D705}_{in}^{2}}{\max _{x,z}\left[\unicode[STIX]{x2202}_{z}\sqrt{|u^{(0)}|^{2}+|v^{(0)}|^{2}}\right]^{2}},\end{eqnarray}$$
which gives the minimum of the Richardson number over the corrugations normalized by the Richardson number of the incident wave. For the case of normal incidence (see figure 6
b), we find that
$\tilde{Ri}$
is close to
$10^{-2}$
, with no detuning. This is a relatively large decrease of the Richardson number. However, whether it is a sufficient decrease for the waves to overturn depends on the Richardson number of the initial wave (say
$Ri_{0}$
), since the actual Richardson number is
$Ri_{0}\times \tilde{Ri}$
. Interestingly, the decrease of Richardson number can be used to obtain a lower bound on the number of short internal waves generated by the chain resonance. Assuming that all of the incident energy flux is sent to the
$\unicode[STIX]{x1D705}_{r_{+m}}$
wave only, the wave amplitude becomes
$\unicode[STIX]{x1D705}_{r_{+m}}^{1/2}$
such that
$\tilde{Ri}\sim (2\unicode[STIX]{x1D705}_{in})^{2}/(4\unicode[STIX]{x1D705}_{r_{+m}}^{5/2})$
or
$\tilde{Ri}\sim 1/(m+1)^{5/2}$
if
$\unicode[STIX]{x1D705}_{r_{+m}}=(m+1)\unicode[STIX]{x1D705}_{in}$
(as is the case for figure 6). Therefore, a drop of
$10^{-2}$
implies the lower bound
$m=5$
for the number of resonated waves; it can be checked from figure 2(a) that at least 5 waves are resonated with non-negligible amplitude.
We show in figure 7(a) the maximum energy flux of the resonated waves and in figure 7(b) the minimum Richardson number for oblique incident waves (
$\unicode[STIX]{x1D703}_{in}=\unicode[STIX]{x03C0}/6,\unicode[STIX]{x03C0}/4,\unicode[STIX]{x03C0}/3$
). The maximum energy flux of the resonated waves is large (even higher than in the case of normal incidence, see figure 6
a), partly because the corrugation amplitude is larger, but also because the energy transfer from the incident to the resonated waves can occur more rapidly with only one wave resonated. In figure 7(b) we observe that there exists an incident detuning for which the minimum Richardson number drops by several orders of magnitude for
$\unicode[STIX]{x1D703}_{in}=\unicode[STIX]{x03C0}/6,\unicode[STIX]{x03C0}/4$
, as was the case for normal incidence. Again, the occurrence of chain resonance for non-zero detuning at oblique incidence comes from the fact that the angular detuning is negative, hence can be counter-balanced with a positive detuning of the first resonance. Because the first interaction that feeds all subsequent resonances is weakened with non-zero incident detuning, the resonated waves have relatively smaller amplitudes in chain resonance at oblique incidence (for which we require a non-zero incident detuning) than in chain resonance at normal incidence (obtained with zero incident detuning). At oblique incidence, however, the projected patch length onto the internal waves’ path is longer than at normal incidence, hence resulting in the generation of more waves (this is the effect of the
$\cos \unicode[STIX]{x1D703}_{\pm m}$
terms in (3.13)). These two effects compete with each other, allowing for significant decrease of the Richardson number at oblique incidence (cf. figure 7
b). The fact that the minimum Richardson number is obtained for increasing detuning as the incidence angle is increased is simply the effect of the increased angular detuning that must be counter-balanced.
4.4 Extension to polychromatic seabed
In this section we briefly discuss the extension of the present theory to the case of a polychromatic seabed, i.e. with corrugations given by (in dimensionless form)
In (4.3) the bottom wavenumbers
$\unicode[STIX]{x1D705}_{bn}$
are ordered from smallest to largest,
$d_{n}$
is real (
$d_{n}/H\ll 1$
) and
$\unicode[STIX]{x1D711}_{n}$
is the mode phase. For simplicity we restrict the analysis to one horizontal dimension, no rotation and we consider the discretized bathymetric spectrum to be narrow-banded, such that all seabed modes resonate the same sequence of internal waves
$\{\unicode[STIX]{x1D705}_{r_{\pm m}}\}$
for a given incident wavenumber
$\unicode[STIX]{x1D705}_{in}$
. In other words we assume that all wavenumbers in
$[\unicode[STIX]{x1D705}_{b1},\unicode[STIX]{x1D705}_{bN}]$
are closest to the same perfectly resonant bottom wavenumber
$\unicode[STIX]{x1D705}_{b}^{\ast }$
.
Histograms of (a)
$\tilde{F}$
(4.1) and (b)
$\tilde{Ri}$
(4.2) obtained for
$10^{6}$
distinct uniform random bottom phase distributions
$\unicode[STIX]{x1D711}_{n}\in [\!0,2\unicode[STIX]{x03C0}\![$
(see (4.3)). Three bottom modes are considered with amplitudes
$d_{n}/H=[0.0025,0.005,0.0025]$
and detuning
$\unicode[STIX]{x1D6FC}_{n}/\unicode[STIX]{x1D705}_{in}=[-0.02,0,0.02]$
. The incident wave is normal to the
${\mathcal{N}}=25$
corrugations considered. The vertical dashed lines show the solutions when the two detuned bottom modes are discarded, and the light green solid line shows the unfilled histogram obtained when two bottom modes of amplitudes
$0.0025$
and detuning
$\pm 0.08$
are added to the three modes used in constructing the filled histogram.
$f/\unicode[STIX]{x1D714}=0$
.

Equation (4.3) can be recast advantageously as
with
$\unicode[STIX]{x1D6FC}_{n}$
a bottom detuning representing the deviation of each bottom wavenumber from
$\unicode[STIX]{x1D705}_{b}^{\ast }$
. For a narrow-banded topographic spectrum we have
$|\unicode[STIX]{x1D6FC}_{n}|\ll \unicode[STIX]{x1D705}_{b}^{\ast }\sim 1$
, such that the sum term in (4.4) is a slowly varying function of
$x$
. Therefore, considering a narrow-banded polychromatic seabed is the same as considering a slowly varying and oscillating bottom corrugation amplitude
$d\equiv D(x)$
, such that the envelope equation (3.8) can be readily modified as
with the slowly varying interaction term
for bottom corrugations of the form (4.3). It should be noted that (4.5)–(4.6) can be derived formally as in § 3 provided that a superposition of
$N_{c}$
interactions is considered on the right-hand side of the bottom boundary condition (3.4c
); while necessary for broadband spectra, this procedure is, however, not justified for the present case.
Equations (4.5)–(4.6) demonstrate that the resonance mechanism due to multiple seabed components can be described as a superposition of resonances (from the sum term). The interference effects resulting from the superposition can be destructive or constructive depending on the bottom phases
$\unicode[STIX]{x1D711}_{n}$
, detuning
$\unicode[STIX]{x1D6FC}_{n}$
, and location
$x$
over the corrugations. Some results on the sensitivity of the chain resonance to arbitrary bottom phase distributions are provided in figure 8. We consider 3 bottom modes and solve (4.5) for
$10^{6}$
different cases of uniform random phase distributions
$\unicode[STIX]{x1D711}_{n}\in [\!0,2\unicode[STIX]{x03C0}\![$
. Figure 8(a,b) shows the histograms of the maximum energy flux ceded by the incident wave to the resonated waves (
$\tilde{F}$
), and of the minimum normalized Richardson number (
$\tilde{Ri}$
) for the
$10^{6}$
random phase distributions (cf. (4.1)–(4.2)). The most probable values of the histograms of
$\tilde{F}$
and
$\tilde{Ri}$
are approximately equal to what is obtained when only the perfectly tuned bottom mode is considered (shown by the dashed vertical lines). The histograms are skewed toward higher/smaller values of
$\tilde{F}/\tilde{Ri}$
, such that adding bottom modes with random phases is found to lead to constructive interference (higher
$\tilde{F}$
, lower
$\tilde{Ri}$
) with slightly higher probabilities than destructive interference. This suggests that the chain resonance mechanism can be expected to occur in most cases of topographic spectra even though the intensity is as expected sensitive to the phase distribution. The minimum/maximum values of
$\tilde{F}$
and maximum/minimum values of
$\tilde{Ri}$
are obtained when the interference lead to the minimum/maximum possible transfer of energy to the shorter waves. With two bottom modes of relatively large detuning added (light green solid lines), it is seen that the histograms do not change significantly. This is expected since the higher the detuning the lesser the contribution to the generation of new resonated waves.
5 Concluding remarks
In this work we have derived the envelope equation (3.12) describing energy transfers from an incident low-mode internal wave to shorter waves in space over resonant seabed topography. We considered the case of a linearly stratified rotating Boussinesq fluid with a top rigid lid, and we focused on monochromatic small-amplitude seabed corrugations as the resonant bathymetry. Interference effects obtained when considering a polychromatic seabed with arbitrary phase distributions were briefly discussed in § 4.4.
For a broad range of incidence angles of the mode-one internal wave, we demonstrated that a large number of other freely propagating waves become generated as a result of wave–bottom resonances occurring in series. The successively resonated waves are of increasing wavenumber, and, for oblique incidence of the incident mode-one wave, they propagate in many different directions. The resonated waves naturally experience some detuning when (i) the incident wave is oblique with respect to the corrugations (because then the resonant wavenumbers are not uniformly spaced, this is called angular detuning) and (ii) when the first interaction between the incident mode-one wave and the corrugations is detuned (which we called incident detuning). The spatial variations of the envelope amplitudes are a priori arbitrary, but turn out to be periodic when the number of resonated waves is finite (note, however, that the periodicity is only clearly seen for a long enough corrugated patch, cf. e.g. figure 5 a).
Because near-resonance waves are as important as perfectly resonant waves, the effect of the incident detuning must be thoroughly considered. Unlike the classical Bragg resonance of surface waves in the homogeneous ocean, we showed that the effect of the incident detuning can be complex and potentially lead to enhanced wave generation when it balances off the angular detuning at oblique incidence.
An important limitation of the model comes from the asymptotic expansion of the bottom boundary condition, which requires large internal-wave wavelengths in the vertical direction compared to the corrugation amplitude. This implies that one must consider corrugations with quite small amplitudes, and therefore in large number, to obtain and correctly predict the envelope variations of high-wavenumber waves in a chain resonance. Fully linear models that do not rely on an asymptotic expansion of the bottom boundary condition are not subject to this limitation, but become significantly computationally expensive in three dimensions. This is why the present leading-order multiple scales model is expected to advance our understanding of resonant scattering events in the oceans for many different physical conditions.
We expect the extension of our results to the case of arbitrary stratification to be relatively straightforward. The number of resonated waves as well as the intensity of energy exchanges in the chain resonances will differ from one stratification profile to another, but the solution method stays the same. The effect of a free surface, which we investigated but did not report here, has in general very little effect on the chain resonance obtained. The wave mode solutions of the linear problem are the same as with a rigid lid, and only the wavenumbers become slightly shifted. The possibility to resonate back-scattered waves via the surface-wave mode for long corrugations (i.e.
$\unicode[STIX]{x1D705}_{b}\sim \unicode[STIX]{x1D705}_{in}$
), however, is unique to stratified fluids with a free top boundary.
Even though most of our results were presented for monochromatic long-crested corrugations (
$\unicode[STIX]{x1D73F}_{b}=\unicode[STIX]{x1D705}_{b}\hat{\boldsymbol{x}}$
), the theory can be easily extended to multiple corrugation wavenumbers with arbitrary orientations in
$(x,y)$
space, in which case one can expect a ramification of the chain resonance across the two-dimensional wavenumber space. The number of resonant branches may in fact become infinite with just two seabed harmonics and may exhibit interesting different chain resonance dynamics. In order to extend the range of applicability of the theory to more general cases, finite-amplitude bottom corrugations should be considered and are worth independent investigation. However, large seabed variations require higher-order or exact linear wave theories, such as Green functions approach or Floquet theory, making the problem much less tractable analytically (see e.g. in homogeneous water Yu & Howard Reference Yu and Howard2012).
The redistribution of energy across the internal-wave spectrum near topography is of significant importance when it leads to the occurrence of enhanced mixing events and wave breaking. Therefore, it will be essential to include the effect of finite-amplitude internal waves in future studies. Laboratory experiments and numerical simulations will be particularly helpful in extending the present predictions to fully nonlinear wave regimes, and in considering relatively large seabed corrugations over which the chain resonance of internal waves should occur rapidly.
Acknowledgements
The authors would like to thank the support from the American Bureau of Shipping. L.-A.C. was supported by a Frank and Margaret Lucas Scholarship while at the University of California, Berkeley. We would also like to thank the anonymous reviewers for their constructive suggestions and comments, which greatly improved the paper.








