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© Miles A. Sundermeyer (msundermeyer@umassd.edu)
Last modified: May 15, 2002
 
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Numerical Simulations of Vortical Mode Stirring

PIs: M.A. Sundermeyer, J.R. Ledwell, M.P. Lelong
Grant Title: Numerical Simulations of Episodic Mixing and Lateral Dispersion by Vortical Modes
Funding Agency: Office of Naval Research
Performance Period: 6/15/01-6/14/03
Award: $251,805

Objectives

We perform numerical studies of lateral dispersion due to the relaxation of diapycnal mixing events. The purpose of the simulations is to understand how diapycnal mixing associated with breaking internal waves effects lateral mixing through the formation and relaxation of vortical modes.

Background

Motivation for the numerical studies comes from observations collected during two recent ONR-funded field studies, the North Atlantic Tracer Release Experiment (NATRE), and the Coastal Mixing and Optics (CMO) program. As part of these programs, dye-release experiments were conducted by J. Ledwell and collaborators in order to measure diapycnal and isopycnal dispersion in the open ocean and over the continental shelf. A significant finding of both of these studies was that existing models of lateral dispersion could not account for the observed dispersion on scales of 1-10 km (Ledwell et al, 1998; Sundermeyer and Price, 1998; Sundermeyer, 1998; Sundermeyer and Ledwell, 2000).
      As discussed by Sundermeyer (1998) in relation to CMO, and by Polzin, et al.(2000) in relation to the NATRE, the observed lateral dispersion on scales of 1-10 km may be explained by vortical modes. In the coastal ocean, we hypothesize that a random vortical mode field can cause sufficient stirring on these scales to efficiently disperse the dye patch. In the open ocean we believe that vertical shear dispersion associated with the vertical structure of the vortical mode may also be important.
      While extensive observational evidence exists linking lateral dispersion on scales of 1-10 km to the vortical mode, our understanding of the details of the generation, adjustment, and ultimate decay of these small-scale geostrophic vorticies is limited. Even less is known about how these vorticies interact with an ambient internal wave field, or with large-scale shearing and straining which are typically found in the ocean. The present work attempts to address these issues through a series of direct numerical simulations of the effects of vortical mode stirring on a passive tracer.

A Stage-wise Modeling Approach

The numerical experiments use a three-dimensional model to solve the Navier-Stokes equations (e.g., Lelong and Riley, 1991; Riley and Lelong, 1999), along with a simple advection/diffusion equation to solve for the evolution of a passive tracer. The experiments will proceed in two phases, with only the simplest dynamics associated with vortical mode stirring being implemented in the first phase, and dynamics of increasing complexity being used in successive phases.
      The first phase of experiments will simulate the adjustment and relaxation phases of the vortical mode dynamics. Simulations will be initialized with density anomalies which are presumed to be generated by the internal wave field. The relaxation of these anomalies and their contribution to lateral dispersion of a passive tracer will be examined, first for a single vortical mode, and then for a random distribution of density anomalies. Appropriate scales for the vortical mode field will be obtained through a retrospective analysis of microstructure and dye observations collected during the CMO dye/microstructure studies (Ledwell, et al. 2000; Oakey 2000). Simulated tracer fields will be compared to observed dye distributions in terms of vertical and horizontal scales of the dye, and the rate of growth of the second moment of tracer, i.e., the effective horizontal diffusivity.
      The second phase of the numerical experiments will examine the effect of a background internal wave field on lateral stirring by vortical modes. Dispersion of a model tracer will be compared to the case without internal waves in order to assess the efficiency of dispersion by vortical modes in a typical oceanic environment.

Anticipated Results

The proposed simulations will provide a theoretical and numerical basis for examining current hypotheses on lateral dispersion by vortical modes. They will also provide a means of evaluating potential sampling strategies in the field during possible future dye-release experiments.

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Preliminary Results

Model Details

We use the fully optimized and paralellized code developed by Dr. Kraig Winters at the University of Seattle, Washington. The model solves the three-dimensional f-plane Boussinesq equations, coupled with an advection-diffusion equation for the density using a semi-/pseudo-spectral approach. Preliminary runs are conducted using either 64x64 or 128x128 gridpoints in the horizontal, and 64 gridpoints in the vertical, and a dimensionful domain size of Lx=Ly=500m, and Lz=50 m. In order to keep computations logistically tractable, we artificially elevate the value of the Coriolis term, f, by a factor of 10. This serves to reduce the ratio of the buoyancy frequency to the Coriolis frequency, N/f, and thus allows us to capture the dynamics associated with each of these time scales without having to perform prohibitively long numerical integrations. The artificially low ratio of N/f (order 10 vs. typical values of order 100) does not alter the inherent dynamics of the system.

Spinup

The model is spun up to a statistically steady state by injecting stratification anomalies periodically but at random locations in the domain, and allowing the system to adjust dynamically. The effect of this is to provide a quasi-steady source of potential energy (PE) to the system, which is then converted to kinetic energy (KE) through a combination of cyclostrophic, geostrophic, and/or frictional adjustment. A statisctically steady state is reached when the rate of energy input is balance by energy dissipation at the smallest scales. The anomalies are generated by imposing a spatially varying diapycnal diffusivity which is localized in both the horizontal and vertical according to a pre-determined Gaussian profile,

Kz(z)   =  

1
Dt

A zo2 e
( -  x2
2xo2
 -  y2
2yo2
 -  z2 )
2zo2

.

When applied to a linear density profile, this creates a gaussian density anomaly of the form,

ranomaly (z)   =  

A z e

dr
dz
( -  z2 )
2zo2

,

where x- and y-dependence in the latter expression are implied. Typical stratification anomaly and diffusivity profiles are shown in Figure 1. An example of the evolution of PE and KE during spinup is shown in Figure 2.

density and diffusivity profiles
Figure 1. Gaussian density anomaly and diffusivity profiles used in numerical simulations.

Figure 2. Time series of potential and kinetic energy showing model spinup and equilibration.
density & diffusivity profiles

Once the model reaches a statistically stationary state, we release a passive tracer into the flow. Subsequently, as additional density anomalies are introduced into the system, the diffusivity profile applied to density is also applied simultaneously to the Lagrangian tracer field.

Results

Figure 3 shows the results of a simulation in which a single density anomaly was released at the center of the domain. At the same time as the anomaly was introduced, a streak of tracer of the same width and vertical scale was also introduced. The result shows the effect of a single anomaly displacing the tracer. The initial radial displacement of tracer combined with the anti-cyclonic rotational displacement of the patch are evident in the animation. Corresponding density and velocity fields are also shown. Total simulation time was approximately 6 inertial periods.

model simulation
(Click on image to view mpeg animation - 7.7 Mbyte.)
Figure 3. Model run using a single density anomaly at the center of the domain. Top panels are plan views of dye, potential density anomaly, and horizontal velocity. Bottom panels are vertical cross sections of the same variables.

Figure 4 shows the results for a simulation in the case of a fully spun field of random stratification anomalies. Again the tracer was injected as a single streak of the same width and vertical scale as the density anomalies. The result shows the stirring effects of a random field of anomalies on the tracer. Corresponding density and velocity fields are also shown. Total simulation time in this case was approximately 37 inertial periods.

model simulation
(Click on image to view mpeg animation - 9.7 Mbyte.)
Figure 4. Model run using a field of random density anomalies distributed throughout the domain. Top panels are plan views of dye, potential density anomaly, and horizontal velocity. Bottom panels are vertical cross sections of the same variables.

The above simulations provide a means of evaluating the effective lateral dispersion caused by the relaxation of diapycnal mixing events. Theoretical predictions based on scaling of the horizontal momentum equations (Sundermeyer, 1998) suggest that the horizontal diffusivity due to such stirring should scale approximately as,

Kh   =  

1
2

h4 DN4
f4

1
L2

n   =  

1
2

U2
f2

n   =  

3
2

N2
f2

R2
L2

Kz ,

where DN, h, and L are the change in buoyancy frequency, the half-height, and the horizontal scale of the anomaly, respectively; U is a velocity scale associated with the adjustment, and R is the deformation radius associated with the anomaly, and n is the frequency at which anomalies occur.

Preliminary results using a relatively modest model resolution of 643 gridpoints indicate that the above parameter dependence is approximately valid to lowest order. Specifically, we have found that compared to a base run, increasing the buoyancy frequency N2 by a factor of 2 increases the effective horizontal diffusivity Kh by a factor of 3. Similarly, increasing the rate of anomaly input by a factor of 2 increases Kh by a factor of 1.5. Finally, increasing the height of the anomalies, h by a factor of 2 increeases Kh by a factor of 20. (Note that the expected dependence of Kh on the above parameters is best seen in the first equality of the above expression.) Horizontal diffusivity estimates based on the time rate of change of the horizontal second moment of tracer for the above described simulations are shown in Figure 5.

Increasing N2 by a factor of 2 increases Kh by a factor of 3. Model Kh
Doubling the rate of anomaly input increases Kh by a factor of 1.5. Model Kh
Doubling the height of anomalies increases Kh by a factor of 20. Model Kh
Figure 5. Time series of the second moment of tracer used to test theoretical parameter dependence. Horizontal diffusivities are estimated based on the slope of the curves during the linear growth phase of the tracer moments.

(... More results coming soon - as time permits!)