1 Introduction
Fine-scale vertical profiles of density in the ocean and atmosphere sometimes take the appearance of a series of step-like layers of nearly uniform density separated by strongly stratified interfaces. Several explanations for the formation of these layers have been proposed, including double diffusion (Schmitt Reference Schmitt1994; Radko Reference Radko2016), localized breaking of internal gravity waves (Garrett & Munk Reference Garrett and Munk1971), shear instabilities (Pelegrí & Sangrà Reference Pelegrí and Sangrà1998) and amplification of small disturbances to a linear density profile (Phillips Reference Phillips1972).
Phillips (Reference Phillips1972) proposed a simple thought experiment to illustrate how layers could develop from small perturbations to a uniformly stratified fluid. He showed that if the magnitude of the buoyancy flux is a decreasing function of the local gradient Richardson number,
$J\equiv N^{2}/S^{2}$
, where
$N\equiv \sqrt{\unicode[STIX]{x2202}b/\unicode[STIX]{x2202}z}$
is the buoyancy frequency and
$S\equiv \unicode[STIX]{x2202}u/\unicode[STIX]{x2202}z$
is the vertical derivative of the horizontal velocity, small disturbances to the initial stratification profile can grow in time. Using a parameterized form of the buoyancy flux, Posmentier (Reference Posmentier1977) showed that this mechanism can lead to the formation of distinct step-like layers.
In subsequent years, laboratory experiments were conducted which appeared to support the idea of the emergence of layers in forced stratified turbulence. These experiments have recently been revisited by Thorpe (Reference Thorpe2016). Linden (Reference Linden1979, Reference Linden1980) found evidence in various experimental configurations that the flux Richardson number,
$R_{f}$
, defined as the fraction of the available kinetic energy that induces a change in the potential energy by mixing the density profile, can be a non-monotonic function of the overall (or bulk) Richardson number,
$J_{o}$
. At small values,
$R_{f}$
increases with increasing
$J_{o}$
, while for values of the overall Richardson number larger than a critical value,
$J_{c}$
, the flux Richardson number decreases with increasing values of
$J_{o}$
. For a constant rate of work on the fluid,
$R_{f}$
is proportional to the buoyancy flux. Therefore, decreasing
$R_{f}$
with increasing
$J_{o}$
for
$J_{o}>J_{c}$
is consistent with the layering mechanism discussed by Phillips (Reference Phillips1972) and Posmentier (Reference Posmentier1977).
Park, Whitehead & Gnanadeskian (Reference Park, Whitehead and Gnanadeskian1994) conducted laboratory experiments where a salt-stratified fluid with an initially linear buoyancy profile was stirred with an oscillating vertical rod. They found that the buoyancy profile develops a series of step-like layers when the overall Richardson number is sufficiently large and the Reynolds number is sufficiently small. They found that the critical Richardson number separating the layering and non-layering regimes was
$J_{c}\approx \exp (Re/900)$
. The dependence of the flux Richardson number was generally consistent with the Phillips (Reference Phillips1972) and Posmentier (Reference Posmentier1977) mechanism for layer formation.
Accumulating evidence from numerical simulations and laboratory experiments indicates that stratified turbulence depends on at least one more non-dimensional parameter,
$G\equiv \unicode[STIX]{x1D700}/(\unicode[STIX]{x1D708}N^{2})$
, where
$\unicode[STIX]{x1D700}$
is the dissipation rate of turbulent kinetic energy and
$\unicode[STIX]{x1D708}$
is the kinematic viscosity (Shih et al.
Reference Shih, Koseff, Ivey and Ferziger2005; Brethouwer et al.
Reference Brethouwer, Billant, Lindborg and Chomaz2007; Bartello & Tobias Reference Bartello and Tobias2013; Bouffard & Boegman Reference Bouffard and Boegman2013; Lozovatsky & Fernando Reference Lozovatsky and Fernando2013; Mater & Venayagamoorthy Reference Mater and Venayagamoorthy2014a
,Reference Mater and Venayagamoorthy
b
; Portwood et al.
Reference Portwood, de Bruyn Kops, Taylor, Salehipour and Caulfield2016). This non-dimensional number is sometimes called the buoyancy Reynolds number since it can be formed using the velocity scale,
$U=\unicode[STIX]{x1D700}^{1/3}L_{O}^{1/3}$
, and the Ozmidov scale,
$L_{O}\equiv \unicode[STIX]{x1D700}^{1/2}N^{-3/2}$
(Dillon & Caldwell Reference Dillon and Caldwell1980). By definition,
$G\equiv (L_{O}/L_{K})^{4/3}$
, where
$L_{K}\equiv \unicode[STIX]{x1D708}^{3/4}\unicode[STIX]{x1D700}^{-1/4}$
is the Kolmogorov scale and
$G$
can be interpreted as an indication of the scale separation between the largest turbulent overturns (proportional to the Ozmidov scale) and the smallest motions allowed by viscosity (proportional to the Kolmogorov scale) (Gargett, Osborn & Nasmyth Reference Gargett, Osborn and Nasmyth1984). For reference, a collection of observations indicates that the buoyancy Reynolds number is typically
$O(1{-}1000)$
in the ocean (Salehipour et al.
Reference Salehipour, Peltier, Whalen and MacKinnon2016).
Here, we focus on layer formation in shear-driven stratified turbulence. Motivated by this and the recent parameterization developed by Salehipour et al. (Reference Salehipour, Peltier, Whalen and MacKinnon2016), we will emphasize the role of the gradient Richardson, buoyancy Reynolds and Prandtl numbers on the condition for layer formation. As noted by Mater & Venayagamoorthy (Reference Mater and Venayagamoorthy2014a ,Reference Mater and Venayagamoorthy b ), other non-dimensional parameters, such as the turbulent Froude number, might also be important. The relationship between the various non-dimensional parameters characterizing stratified turbulence is still the topic of active research. As will be discussed in § 5, the analysis carried out here could also be extended to examine the roles of other non-dimensional parameters on layer formation. Additionally, the non-dimensional parameters are generally defined in terms of averaged quantities, and there is some ambiguity in how the average is defined. The particular choice used here will be defined explicitly in § 2.
Below, in § 2, we extend the work of Phillips (Reference Phillips1972) and Posmentier (Reference Posmentier1977) by invoking the tracer coordinates introduced by Nakamura (Reference Nakamura1996) and Winters & D’Asaro (Reference Winters and D’Asaro1996). This has the advantage of eliminating the reversible component of the buoyancy flux and generalizing the condition for layer formation into a simple expression. We also extend the analysis to explicitly include the buoyancy Reynolds and Prandtl numbers. In § 3, we apply the new framework to direct numerical simulations (DNS) of stratified shear flow. In § 4, we consider various functional forms for the effective diffusivity, including a recent parameterization introduced by Salehipour et al. (Reference Salehipour, Peltier, Whalen and MacKinnon2016), and examine when layer formation might occur.
2 Formulation
Winters & D’Asaro (Reference Winters and D’Asaro1996) and Nakamura (Reference Nakamura1996) derived an evolution equation for a tracer in sorted buoyancy coordinates. Written here in terms of buoyancy,
$b$
, and sorted height,
$z_{\ast }$
, they showed that the buoyancy conservation equation in a closed system can be written as
where
$\unicode[STIX]{x1D705}$
is the constant molecular diffusivity,
$\unicode[STIX]{x1D735}$
denotes the gradient vector in physical coordinates and
$\langle \cdot \rangle _{z_{\ast }}$
indicates an average over all points with the same value of
$z_{\ast }$
. The effective diffusivity can also be written as
$\unicode[STIX]{x1D705}_{e}=\unicode[STIX]{x1D705}(A_{S}/A)^{2}$
, where
$A_{S}$
is an area associated with distorted buoyancy surfaces and
$A$
is the area of an undisturbed (flat) buoyancy surface (Winters & D’Asaro Reference Winters and D’Asaro1996). A simple interpretation is then that the effective diffusivity is larger for more highly distorted buoyancy surfaces with larger surface area, and is equal to the molecular diffusivity for undisturbed buoyancy surfaces (i.e. when the sorted profile is the same as the profile in physical coordinates).
Taking a derivative of (2.1) with respect to
$z_{\ast }$
gives an equation for the stratification in sorted height coordinates,
where
$N_{\ast }^{2}\equiv \unicode[STIX]{x2202}b/\unicode[STIX]{x2202}z_{\ast }$
is the buoyancy gradient in sorted height coordinates. Equation (2.3) was recently used by Zhou et al. (Reference Zhou, Taylor, Caulfield and Linden2017) to analyse the evolution of a density interface in DNS of stratified plane Couette flow. We will show below that, for a nearly uniform stratification, the second term on the right-hand side of (2.3) is expected to be small. In this case, the last term on the right-hand side of (2.3) represents diffusion of the sorted buoyancy profile through combined molecular and turbulent diffusivity. Since
$\unicode[STIX]{x1D705}_{e}\geqslant \unicode[STIX]{x1D705}>0$
, the corresponding diffusivity is always positive. Therefore, variations in
$N_{\ast }^{2}$
will grow in time when
$\unicode[STIX]{x2202}^{2}\unicode[STIX]{x1D705}_{e}/\unicode[STIX]{x2202}z_{\ast }^{2}>0$
and when the first term on the right-hand side of (2.3) is large enough to overcome the effects of diffusion.
We will assume that changes in
$\unicode[STIX]{x1D705}_{e}$
with respect to the sorted height,
$z_{\ast }$
, and time,
$t$
, can be parameterized in terms of the gradient Richardson number,
$J_{\ast }$
, and buoyancy Reynolds number,
$G_{\ast }$
, defined in sorted height coordinates. Specifically,
where
$S_{\ast }\equiv \langle \unicode[STIX]{x2202}u/\unicode[STIX]{x2202}z\rangle _{z_{\ast }}$
, the kinetic energy dissipation rate is
$\unicode[STIX]{x1D700}_{\ast }\equiv 2\unicode[STIX]{x1D708}\langle \unicode[STIX]{x1D634}_{ij}\unicode[STIX]{x1D634}_{ij}\rangle _{z_{\ast }}$
and
$\unicode[STIX]{x1D634}_{ij}$
is the rate of strain tensor. In this definition,
$\unicode[STIX]{x1D634}_{ij}$
is based on velocity gradients in physical space and the tensor product
$\unicode[STIX]{x1D634}_{ij}\unicode[STIX]{x1D634}_{ij}$
is averaged along levels of constant sorted height. It should be noted that the average operator used here is different from the more conventional choice of averaging over constant unsorted height. We can also include dependence of
$\unicode[STIX]{x1D705}_{e}$
on the Prandtl number,
$Pr\equiv \unicode[STIX]{x1D708}/\unicode[STIX]{x1D705}$
, or any other constant parameter, i.e.
Since
$Pr$
is constant, derivatives of
$\unicode[STIX]{x1D705}_{e}$
with respect to
$z_{\ast }$
involve variations with respect to
$J_{\ast }$
and
$G_{\ast }$
, but not
$Pr$
directly.
Following the thought experiment proposed by Phillips (Reference Phillips1972), we consider the evolution of a stratified flow with a nearly uniform stratification and shear. Phillips (Reference Phillips1972) further defined a turbulent velocity scale,
$u_{\ast }=\sqrt{\unicode[STIX]{x1D70F}/\unicode[STIX]{x1D70C}_{0}}$
, where
$\unicode[STIX]{x1D70F}$
is a constant stress and
$\unicode[STIX]{x1D70C}_{0}$
is the reference density. Here, we will instead assume that the turbulent kinetic energy dissipation rate,
$\unicode[STIX]{x1D700}_{\ast }$
, is nearly constant. Let
$N_{0}$
,
$S_{0}$
and
$\unicode[STIX]{x1D700}_{0}$
denote the constant background buoyancy frequency, shear and dissipation rate. The buoyancy gradient, shear and dissipation rate can be written in terms of small departures from the background values,
where
$\unicode[STIX]{x1D716}$
is a small expansion parameter. Here, all quantities are defined in sorted buoyancy coordinates, but the
$\ast$
subscript has been omitted from
$N_{0}$
,
$N_{1}$
,
$S_{0}$
, etc. to simplify the notation.
To leading order in
$\unicode[STIX]{x1D716}$
, the derivatives of the gradient Richardson number and buoyancy Reynolds number are
and
while the derivative of
$\unicode[STIX]{x1D705}_{e}$
can be written as
Using the expansions introduced above, the
$O(\unicode[STIX]{x1D716})$
contributions to (2.3) are
or, using (2.9) and (2.10) and their derivatives,
The term in brackets on the right-hand side of (2.13) can be interpreted as a diffusivity acting on the sorted buoyancy gradient. When the undisturbed state has
the diffusivity is negative, providing a mechanism for small disturbances to the density gradient to intensify. Since
$J_{\ast }$
and
$G_{\ast }$
are both positive for a stable stratification, conditions are favourable for this mechanism when
$\unicode[STIX]{x2202}\unicode[STIX]{x1D705}_{e}/\unicode[STIX]{x2202}J_{\ast }<0$
and
$\unicode[STIX]{x2202}\unicode[STIX]{x1D705}_{e}/\unicode[STIX]{x2202}G_{\ast }>0$
. The last two terms in (2.13) can also influence the evolution of
$N_{1}^{2}$
. These terms will be relatively small when variations in
$J_{\ast }$
and
$G_{\ast }$
are dominated by changes in
$N_{\ast }^{2}$
.
Equations (2.3) and (2.14) both contain terms proportional to
$\unicode[STIX]{x1D705}_{e}$
which act against layer formation. Flows with larger values of
$\unicode[STIX]{x1D705}_{e}$
will be less susceptible to layer formation. Molecular diffusion implicitly enters through these terms. It should be recalled that
$\unicode[STIX]{x1D705}_{e}$
cannot be smaller than the molecular diffusivity,
$\unicode[STIX]{x1D705}_{e}\geqslant \unicode[STIX]{x1D705}$
. Therefore, when the molecular diffusivity is large (e.g. when the Prandtl or Schmidt number is small), layer formation will be inhibited.
The dependence of the criterion in (2.14) on molecular diffusion and the Prandtl number can be made more explicit by recasting the criterion in terms of the irreversible mixing efficiency defined in Peltier & Caulfield (Reference Peltier and Caulfield2003). Salehipour & Peltier (Reference Salehipour and Peltier2015) recently showed that
where
$\unicode[STIX]{x1D6E4}=E/(1-E)$
is a flux coefficient and
$E$
is the irreversible mixing efficiency. We have added laminar diffusion to (2.15) through the second term on the right-hand side. This term was neglected by Salehipour & Peltier (Reference Salehipour and Peltier2015), but is not negligible unless
$\unicode[STIX]{x1D6E4}Pr\,G_{\ast }\gg 1$
. If we assume that the irreversible mixing efficiency,
$E$
, is a function of
$J_{\ast }$
and
$G_{\ast }$
, then the condition in (2.14) can be written as
When
$Pr\,G_{\ast }=\unicode[STIX]{x1D700}_{\ast }/(\unicode[STIX]{x1D705}N_{\ast }^{2})$
is small, the last term on the left-hand side of (2.16) will be large and positive, and will make the condition in (2.14) more difficult to meet.
We can recover criteria analogous to those obtained by Phillips (Reference Phillips1972) and Posmentier (Reference Posmentier1977) by assuming that
$\unicode[STIX]{x1D705}_{e}$
is independent of
$G_{\ast }$
, so that
$\unicode[STIX]{x2202}\unicode[STIX]{x1D705}_{e}/\unicode[STIX]{x2202}G_{\ast }=0$
. The last term in (2.13) is then identically zero. Further neglecting the second to last term in (2.13), under the assumption that variations in
$J_{\ast }$
are dominated by changes in
$N_{\ast }^{2}$
, gives
When
$\unicode[STIX]{x2202}(J_{\ast }\unicode[STIX]{x1D705}_{e})/\unicode[STIX]{x2202}J_{\ast }<0$
, equation (2.17) becomes a diffusion equation with a negative diffusion coefficient, and, as pointed out by Phillips (Reference Phillips1972), small disturbances in the density gradient will grow in time. If the shear rate,
$S$
, is constant, this condition is also equivalent to
$\unicode[STIX]{x2202}B_{\ast }/\unicode[STIX]{x2202}N_{\ast }^{2}<0$
, where
$B_{\ast }=N_{\ast }^{2}\unicode[STIX]{x1D705}_{e}$
is the buoyancy flux in sorted buoyancy coordinates. This is the same expression as obtained by Posmentier (Reference Posmentier1977) except that the buoyancy flux is defined in sorted buoyancy coordinates.
Linden (Reference Linden1979) showed that the layer formation condition proposed by Posmentier (Reference Posmentier1977) can be written as
$\unicode[STIX]{x2202}R_{f}/\unicode[STIX]{x2202}J_{o}<0$
, where
$R_{f}=B/(B+\unicode[STIX]{x1D700})$
is the flux Richardson number characterizing turbulent mixing and
$J_{o}$
is an overall Richardson number characterizing the strength of stratification. A similar condition can be obtained as a special case of (2.16). For
$Pr\,G_{\ast }\gg 1$
, the third term on the left-hand side of (2.16) might be negligible. If we can also neglect the second term on the left-hand side (e.g. if
$E$
is independent of
$G_{\ast }$
), equation (2.16) becomes
$\unicode[STIX]{x2202}E/\unicode[STIX]{x2202}J_{\ast }<0$
, which is analogous to the condition in Posmentier (Reference Posmentier1977) and Linden (Reference Linden1979), but now written in terms of the irreversible mixing efficiency,
$E$
, and the gradient Richardson number defined using sorted buoyancy coordinates,
$J_{\ast }$
.
3 Simulations
In this section, we apply the framework described above to DNS of a stratified shear flow. The flow is not intended to be typical of the ocean or atmosphere, but rather to demonstrate the possibility of layer formation in a simple configuration. The initial conditions consist of linear velocity and density profiles with sinusoidal disturbances,
where
$u$
is the velocity in the
$x$
direction and
$\unicode[STIX]{x1D6FF}$
and
$\unicode[STIX]{x1D6FE}$
are non-dimensional constants that control the relative size of the disturbances to the shear and stratification. The flow is bounded from above and below by rigid horizontal surfaces with boundary conditions
$u=\pm u_{0}/2$
and
$b=\pm b_{0}/2$
at
$z=\pm h/2$
, where
$u_{0}=S_{0}h$
and
$b_{0}=N_{0}^{2}h$
. The flow is periodic in the horizontal (
$x,y$
) directions and the domain size is
$LX=3h$
,
$LY=0.25h$
. The non-dimensional parameters are
$Re\equiv u_{0}h/\unicode[STIX]{x1D708}=14\,000$
,
$J_{0}=N_{0}^{2}/S_{0}^{2}=0.3$
,
$\unicode[STIX]{x1D6FF}=0.8$
and
$\unicode[STIX]{x1D6FE}=0.4$
. Two Prandtl numbers are considered,
$Pr=0.7$
and
$Pr=7$
, corresponding to typical values for the diffusion of heat in air and water respectively.
The incompressible Boussinesq Navier–Stokes equations are solved using the solver developed by Taylor (Reference Taylor2008) and used previously in Deusebio, Caulfield & Taylor (Reference Deusebio, Caulfield and Taylor2015) and Taylor et al. (Reference Taylor, Deusebio, Caulfield and Kerswell2016) to study stratified shear flow. A pseudo-spectral method is applied in the horizontal directions and a second-order finite difference method is used for vertical derivatives. The equations are time stepped with a mixed implicit/explicit scheme using a third-order accurate Runge–Kutta algorithm and Crank–Nicolson. Further details of the numerical method can be found in Taylor (Reference Taylor2008). Both simulations use
$384\times 32\times 193$
grid points, which ensures that the grid spacing is no larger than 2.5 times the Batchelor scale, as in the DNS of Smyth & Moum (Reference Smyth and Moum2000). To speed up the transition to turbulence, the velocity field is seeded with uniform random noise with an amplitude of
$0.2u_{0}$
. The PDF method introduced by Tseng & Ferziger (Reference Tseng and Ferziger2001) is used to calculate the sorted buoyancy profile.
The initial mean profiles of buoyancy and velocity used in the DNS (a) and the corresponding gradient Richardson number (b). Vertical (
$x$
–
$z$
) slices of the buoyancy at time
$t\simeq 52h/u_{0}$
show developing K–H billows and smaller-scale structures in the density field in the case with
$Pr=7$
(d) compared with
$Pr=0.7$
(c).
Initial profiles of velocity and buoyancy are shown in figure 1, along with the corresponding gradient Richardson number. Based on the Miles–Howard theorem, the flow has the capacity to support growing linear normal mode perturbations since
$J<1/4$
in regions above and below the centreline. Overall, the disturbances to the linear velocity and buoyancy profile (and variations in the gradient Richardson number) are large. The framework described above, where small disturbances are considered, can be viewed as an analysis of a narrow range of
$z_{\ast }$
. Kelvin–Helmholtz (K–H) billows develop in the weakly stratified regions, which distort the buoyancy contours (figure 1), with stronger distortion and smaller features in the
$Pr=7$
simulation.
Interestingly, the initial disturbances to the stratification grow over time in the strongly stratified region near the centreline (
$z=0$
) for
$Pr=7$
but not when
$Pr=0.7$
. Figure 2(a) shows profiles of
$N_{\ast }^{2}$
for both simulations at
$t\simeq 14h/u_{0}$
after decay of the initial random noise and at
$t\simeq 105h/u_{0}$
, corresponding to a time after the first K–H mixing event. In the simulation with
$Pr=7$
(blue), the stratification decreases in the regions that have
$J<0.25$
at the start of the simulation, while the stratification intensifies near the centreline. In contrast,
$N_{\ast }^{2}$
evolves towards a constant value in the simulation with
$Pr=0.7$
(red).
Vertical profiles in sorted buoyancy coordinates (
$z_{\ast }$
) for simulations with
$Pr=0.7$
(red) and
$Pr=7$
(blue). (a) Normalized
$N_{\ast }^{2}$
at
$t\simeq 14h/u_{0}$
(dashed) and
$t=105h/u_{0}$
(solid). (b) Normalized effective diffusivity,
$\unicode[STIX]{x1D705}_{e}/\unicode[STIX]{x1D705}$
. (c) Gradient Richardson number,
$J_{\ast }$
. (d) Buoyancy Reynolds number,
$G_{\ast }$
. (e) Terms in (2.14), each normalized by
$\unicode[STIX]{x1D705}$
.
The amplification of the perturbations to the
$N_{\ast }^{2}$
profile can be analysed using the theoretical framework introduced above. Profiles of
$\unicode[STIX]{x1D705}_{e}$
,
$J_{\ast }$
and
$G_{\ast }$
at individual times are relatively noisy and intense mixing occurs in intermittent bursts. However, the general trends in each simulation can be seen by examining the time-averaged profiles. Figure 2(b) shows profiles of
$\unicode[STIX]{x1D705}_{e}$
, normalized by the molecular value and averaged in the time interval bounded by the profiles shown in figure 2(a). The normalized effective diffusivity is larger in the case with
$Pr=7$
. In both cases,
$\unicode[STIX]{x2202}^{2}\unicode[STIX]{x1D705}_{e}/\unicode[STIX]{x2202}z_{\ast }^{2}<0$
in regions with relatively weak stratification and
$\unicode[STIX]{x2202}^{2}\unicode[STIX]{x1D705}_{e}/\unicode[STIX]{x2202}z_{\ast }^{2}>0$
in regions with relatively strong stratification. This implies that the first term on the right-hand side of (2.3) will tend to reinforce perturbations to the
$N_{\ast }^{2}$
profile. Time-averaged profiles of
$J_{\ast }$
and
$G_{\ast }$
are shown in figure 2(c,d). Regions with large
$\unicode[STIX]{x1D705}_{e}$
are associated with small
$J_{\ast }$
and large
$G_{\ast }$
. Here, the profiles of
$J_{\ast }(z_{\ast })$
and
$G_{\ast }(z_{\ast })$
are very close to the profiles of the more conventional definitions in terms of unsorted height,
$J(z)$
and
$G(z)$
(not shown).
The terms in (2.14) are shown in figure 2(e), where each term is evaluated based on the time-averaged profiles of
$\unicode[STIX]{x1D705}_{e}$
,
$J_{\ast }$
and
$G_{\ast }$
. Since the initial perturbations in the mean
$J_{\ast }$
and
$G_{\ast }$
profiles are not small, as assumed in obtaining (2.13), we have used the local values of
$J_{\ast }$
and
$G_{\ast }$
in evaluating (2.14), consistent with the interpretation that the framework applies to a small range of
$z_{\ast }$
. The first two terms in (2.14) are generally negative and hence encourage negative diffusion and layer formation. On the other hand, as noted above,
$\unicode[STIX]{x1D705}_{e}>0$
. When
$Pr=0.7$
(red),
$\unicode[STIX]{x1D705}_{e}$
is generally larger than the other terms, resulting in a positive diffusivity in (2.13). Although
$\unicode[STIX]{x1D705}_{e}/\unicode[STIX]{x1D705}$
is larger for
$Pr=7$
, the other terms more than compensate, and the condition in (2.14) is met at most locations. These results are consistent with the observation that changes in stratification intensify when
$Pr=7$
, but not when
$Pr=0.7$
.
Figure 2(e) includes the terms inside the bracket in (2.13) and hence determines whether the diffusion acting on
$N_{1}$
is positive or negative. However, in this particular case, the last two terms in (2.13) are not negligible. Based on our initial conditions,
$\unicode[STIX]{x2202}^{2}S_{\ast }/\unicode[STIX]{x2202}z_{\ast }^{2}$
has the opposite sign to
$\unicode[STIX]{x2202}^{2}N_{\ast }^{2}/\unicode[STIX]{x2202}z_{\ast }^{2}$
. Similarly, as the simulation evolves,
$\unicode[STIX]{x1D700}_{\ast }$
is large where
$N_{\ast }^{2}$
is small and, although there are large fluctuations
$\unicode[STIX]{x2202}^{2}\unicode[STIX]{x1D700}_{\ast }/\unicode[STIX]{x2202}z_{\ast }^{2}$
, generally has the opposite sign to
$\unicode[STIX]{x2202}^{2}N_{\ast }^{2}/\unicode[STIX]{x2202}z_{\ast }^{2}$
. As a result, both terms encourage layer formation in our simulations.
The irreversible mixing efficiency,
$E(J_{\ast },G_{\ast })$
, as parameterized by Salehipour et al. (Reference Salehipour, Peltier, Whalen and MacKinnon2016) (colour shading). Solid contours separate regions where the bracketed term in (2.13) is sharpening and diffusive for four different values of the Prandtl (or Schmidt) number,
$Pr=\unicode[STIX]{x1D708}/\unicode[STIX]{x1D705}$
. The dashed line delineates the region where
$\unicode[STIX]{x2202}E/\unicode[STIX]{x2202}J_{\ast }=0$
. Mean profiles of
$J_{\ast }$
and
$G_{\ast }$
from the DNS (as plotted in figure 2) are shown using white dots for
$Pr=7$
and black dots for
$Pr=0.7$
.
4 Parameterizations
The previous section demonstrates that the framework developed in § 2 is useful for diagnosing the sharpening of a density profile though stratified turbulence. The framework can be applied more broadly by assuming a particular functional form for
$\unicode[STIX]{x1D705}_{e}(J_{\ast },G_{\ast })$
. A simple expression follows if we assume that
$\unicode[STIX]{x1D705}_{e}$
depends on
$J_{\ast }$
and
$G_{\ast }$
through a power law,
where
$f(Pr,\ldots )$
includes the explicit dependence of
$\unicode[STIX]{x1D705}_{e}$
on the Prandtl number and any other constant parameters. This form is unlikely to hold over a wide range of
$J_{\ast }$
and
$G_{\ast }$
for fixed values of
$\unicode[STIX]{x1D6FC}$
and
$\unicode[STIX]{x1D6FD}$
, but it might provide a reasonable approximation to
$\unicode[STIX]{x1D705}_{e}$
for a limited range of
$J_{\ast }$
and
$G_{\ast }$
. The condition for a negative diffusivity in (2.14) then becomes simply
Based on DNS of homogeneous sheared stratified turbulence, Shih et al. (Reference Shih, Koseff, Ivey and Ferziger2005) found that the turbulent diffusivity increases with increasing
$G$
with an exponent of
$\unicode[STIX]{x1D6FD}\simeq 1$
for
$7<G<100$
and
$\unicode[STIX]{x1D6FD}\simeq 0.5$
for
$G>100$
. (It should be noted that the turbulent diffusivity in Shih et al. (Reference Shih, Koseff, Ivey and Ferziger2005) is defined in terms of the buoyancy flux and buoyancy gradient in the vertical (
$z$
) direction, while all quantities here are defined in terms of derivatives in sorted buoyancy coordinates,
$z_{\ast }$
.) Without additional dependence on the gradient Richardson number, this value of
$\unicode[STIX]{x1D6FD}$
would not be sufficient for (2.14) to hold.
Recently, Salehipour et al. (Reference Salehipour, Peltier, Whalen and MacKinnon2016) collected data from DNS and developed a parameterization for the irreversible mixing efficiency,
$E$
, as a function of the gradient Richardson and buoyancy Reynolds numbers in sorted buoyancy coordinates,
$J_{\ast }$
and
$G_{\ast }$
. Details of this parameterization can be found in Salehipour et al. (Reference Salehipour, Peltier, Whalen and MacKinnon2016). The colour shading in figure 3 shows the parameterized form of
$E(G_{\ast },J_{\ast })$
, which notably has non-monotonic behaviour in both parameters. Solid contours separate regions where the condition in (2.16) holds for three different values of the Prandtl (or Schmidt) number,
$Pr=0.7$
, 7, 700, corresponding approximately to the diffusion of heat in air, heat in water and salt in water. For reference, a line showing
$Pr=\infty$
is also shown. There is non-trivial Prandtl and buoyancy Reynolds dependence on the condition in (2.16) with the parameterized form of
$E(G_{\ast },J_{\ast })$
. The Prandtl number has a strong effect on the boundary for the range
$J_{\ast }\gtrsim 0.25$
and
$G_{\ast }\lesssim 100$
. Salehipour et al. (Reference Salehipour, Peltier, Whalen and MacKinnon2016) note that
$E$
might depend explicitly on the Prandtl number, although they did not include this dependence in their parameterization.
The dashed line in figure 3 indicates where
$\unicode[STIX]{x2202}E/\unicode[STIX]{x2202}J_{\ast }=0$
, and the region above this line satisfies
$\unicode[STIX]{x2202}E/\unicode[STIX]{x2202}J_{\ast }<0$
. This gives a very good approximation to the full condition in (2.16) for
$G_{\ast }>100$
. It should be noted, however, that the parameterized form of
$E$
and the location where
$\unicode[STIX]{x2202}E/\unicode[STIX]{x2202}J_{\ast }=0$
depend strongly on
$G_{\ast }$
in this range.
The DNS results described in § 3 are qualitatively consistent with the sharpening criteria derived from the Salehipour et al. (Reference Salehipour, Peltier, Whalen and MacKinnon2016) parameterization. Black and white dots in figure 3 show individual points along the mean
$J_{\ast }$
and
$G_{\ast }$
profiles for
$Pr=0.7$
(black) and
$Pr=7$
(white). When
$Pr=0.7$
, the values of
$J_{\ast }$
and
$G_{\ast }$
are always in the diffusing regime, while when
$Pr=7$
, the profiles pass into the sharpening regime.
5 Discussion
In this paper, we revisited the thought experiment proposed by Phillips (Reference Phillips1972) and the possibility that small perturbations to a uniform stable density stratification can grow in time, possibly leading to the formation of step-like layers. This extended previous work in two ways. First, the evolution equation for the stratification was written in isoscalar coordinates using the framework introduced by Winters & D’Asaro (Reference Winters and D’Asaro1996) and Nakamura (Reference Nakamura1996). This has the advantage of removing reversible contributions to the buoyancy flux and provides a useful diagnostic framework for identifying sharpening of stratified interfaces. There is a possibility for an increase in stratification when the curvature of the effective diffusivity in sorted buoyancy coordinates is positive (
$\unicode[STIX]{x2202}^{2}\unicode[STIX]{x1D705}_{e}/\unicode[STIX]{x2202}z_{\ast }^{2}>0$
) and sufficiently large to overcome diffusion by
$\unicode[STIX]{x1D705}_{e}$
.
We then assumed that the effective diffusivity could be written as a function of the gradient Richardson number,
$J_{\ast }$
, and buoyancy Reynolds number,
$G_{\ast }$
, defined in terms of quantities averaged in sorted buoyancy coordinates. Using this framework, small departures from a constant stratification can be written in the form of a diffusion equation with two additional terms that depend on variations in the background shear and turbulent dissipation rate. The coefficient of diffusion is negative when the effective diffusivity decreases with increasing gradient Richardson number and/or increases with increasing buoyancy Reynolds number, such that these changes overcome the stabilizing influence of diffusion through
$\unicode[STIX]{x1D705}_{e}$
. This criterion was also rewritten in terms of the irreversible mixing efficiency in (2.16) using a relation recently derived by Salehipour & Peltier (Reference Salehipour and Peltier2015).
Direct numerical simulations of a stratified shear flow demonstrated that existing disturbances to an otherwise linear density profile can grow following a mixing event. This occurred when the molecular Prandtl number was 7 (appropriate for the diffusion of heat in water), but not when the Prandtl number was 0.7 (appropriate for the diffusion of heat in air). Since the simulations used a linear equation of state, the simulations exclude the possible role of double diffusion. Instead, the tendency for the density profile to sharpen is a direct result of stratified turbulence.
The sharpening of the buoyancy profile seen in the DNS with
$Pr=7$
is small and transient. It is possible that a more dramatic sharpening would be seen for
$Pr=700$
, although this is presently beyond the reach of DNS. Further sharpening could develop in response to a series of mixing events, each similar to the one described in § 3. For example, if a train of low-frequency internal gravity waves propagated through a pre-existing shear layer, the oscillating shear associated with the internal waves could trigger repeated K–H mixing events similar to the one simulated here, and the net result might be the development of a step-like density profile.
Although (2.14) does not depend explicitly on the Prandtl number (or any other constant non-dimensional parameters), the Prandtl number can influence this condition in two ways. First, since
$\unicode[STIX]{x1D705}_{e}$
is bounded from below by
$\unicode[STIX]{x1D705}$
, more diffusive substances with small Prandtl numbers could lead to larger values of
$\unicode[STIX]{x1D705}_{e}$
, making it more difficult for (2.14) to be met. Second, the DNS results show that the Prandtl number can also change the dependence of
$\unicode[STIX]{x1D705}_{e}$
on
$J_{\ast }$
and
$G_{\ast }$
. The first two terms in (2.14) are more negative for
$Pr=7$
than for
$Pr=0.7$
, and this is true even when the size of the terms is not scaled with
$\unicode[STIX]{x1D705}$
(not shown).
In order to evaluate the condition for sharpening through negative diffusion in (2.14), the functional dependence of
$\unicode[STIX]{x1D705}_{e}$
on
$J_{\ast }$
,
$G_{\ast }$
and
$Pr$
(and possibly other parameters) must be specified. Using a parameterization recently developed by Salehipour et al. (Reference Salehipour, Peltier, Whalen and MacKinnon2016), equation (2.16) yields a criterion that depends non-trivially on
$J_{\ast }$
,
$G_{\ast }$
and
$Pr$
, but sharpening through negative diffusion generally occurs when
$J_{\ast }$
and
$G_{\ast }$
are large, and positive diffusion occurs more readily when the Prandtl number is small. It should be noted that the simulations used by Salehipour et al. (Reference Salehipour, Peltier, Whalen and MacKinnon2016) as a basis for their parameterization did not cover the full range of
$J_{\ast }$
and
$G_{\ast }$
shown in figure 3, and the details of the criterion should be viewed with caution. The criterion for sharpening through negative diffusion shown in figure 3 is specific to the parameterization developed by Salehipour et al. (Reference Salehipour, Peltier, Whalen and MacKinnon2016), although the framework developed here could be applied more generally.
The formation of a step-like density profile has been seen in several laboratory experiments where grids or bars have been towed through a fluid with an initially linear density profile (Ruddick, McDougall & Turner Reference Ruddick, McDougall and Turner1989; Park et al.
Reference Park, Whitehead and Gnanadeskian1994; Holford & Linden Reference Holford and Linden1999). As recently reviewed by Thorpe (Reference Thorpe2016), regimes with and without layer formation are separated by a boundary that depends on the Reynolds and Froude numbers associated with the towed grid. Different studies have proposed different functional forms for this boundary, and the estimates are not always consistent. Generally, layers are not seen when the Froude number is too large, and layer formation appears to be favoured for moderate Reynolds numbers. The framework presented here could be used to analyse layer formation in these experiments. For example, the analysis in § 2 could be repeated to include dependence of
$\unicode[STIX]{x1D705}_{e}$
on a turbulent Froude number associated with an oscillating grid.
In the thought experiment presented by Phillips (Reference Phillips1972), a vertical buoyancy flux was maintained by turbulence which was modulated by changes to the stratification. The derivation above raises the possibility that internal waves might be capable of inducing layer development without requiring turbulence or density overturns. This does not contradict the formulation in tracer coordinates which excludes reversible buoyancy fluxes. Instead, if the displacement of isopycnals is persistently large in regions of weak stratification, an increase in the tracer area and the effective diffusivity in the region of weak stratification could lead to layer formation. Perhaps consistent with this hypothesis, figure 3 suggests that when
$Pr=700$
, layer formation might be supported for
$G_{\ast }<1$
, in a part of parameter space where stratification effects are felt down to the viscous scale.
Acknowledgements
The EPSRC Programme Grant EP/K034529/1 entitled ‘Mathematical Underpinnings of Stratified Turbulence’ (MUST) is gratefully acknowledged for supporting the research presented here. We are grateful to the MUST team for many helpful discussions and suggestions, and to two anonymous referees whose comments helped to improve the paper. Supporting data in the form of source code and input files for the DNS can be obtained from https://doi.org/10.17863/CAM.9631.