Instability of a coastal jet in a two-layer model ; application to the Ushant front

Similar documents
Vortices in the ocean. Lecture 4 : Baroclinic vortex processes

Ageostrophic instabilities of a front in a stratified rotating fluid

Baroclinic Rossby waves in the ocean: normal modes, phase speeds and instability

2. Baroclinic Instability and Midlatitude Dynamics

Stability of meridionally-flowing grounded abyssal currents in the ocean

A Truncated Model for Finite Amplitude Baroclinic Waves in a Channel

Contents. Parti Fundamentals. 1. Introduction. 2. The Coriolis Force. Preface Preface of the First Edition

Decay of Agulhas rings due to cross-frontal secondary circulations

Nonlinear Balance on an Equatorial Beta Plane

Chapter 3. Stability theory for zonal flows :formulation

Jet Formation in the Equatorial Oceans Through Barotropic and Inertial Instabilities. Mark Fruman

Chapter 13 Instability on non-parallel flow Introduction and formulation

Gravity Waves. Lecture 5: Waves in Atmosphere. Waves in the Atmosphere and Oceans. Internal Gravity (Buoyancy) Waves 2/9/2017

Lecture #2 Planetary Wave Models. Charles McLandress (Banff Summer School 7-13 May 2005)

Island Wakes in Shallow Water

Goals of this Chapter

3. Midlatitude Storm Tracks and the North Atlantic Oscillation

Eddy PV Fluxes in a One Dimensional Model of Quasi-Geostrophic Turbulence

The Eady problem of baroclinic instability described in section 19a was shown to

2013 Annual Report for Project on Isopycnal Transport and Mixing of Tracers by Submesoscale Flows Formed at Wind-Driven Ocean Fronts

Diagnosis of a Quasi-Geostrophic 2-Layer Model Aaron Adams, David Zermeño, Eunsil Jung, Hosmay Lopez, Ronald Gordon, Ting-Chi Wu

primitive equation simulation results from a 1/48th degree resolution tell us about geostrophic currents? What would high-resolution altimetry

Internal boundary layers in the ocean circulation

Do altimeter wavenumber spectra agree with interior or surface. quasi-geostrophic theory?

Transformed Eulerian Mean

Spherical Shallow Water Turbulence: Cyclone-Anticyclone Asymmetry, Potential Vorticity Homogenisation and Jet Formation

Shelf Impact on Buoyant Coastal Current Instabilities

Islands in Zonal Flow*

Modeling and Parameterizing Mixed Layer Eddies

NOTES AND CORRESPONDENCE. Effect of Sea Surface Temperature Wind Stress Coupling on Baroclinic Instability in the Ocean

Submesoscale Routes to Lateral Mixing in the Ocean

Superparameterization of Oceanic Boundary Layer Transport

Measurement of Rotation. Circulation. Example. Lecture 4: Circulation and Vorticity 1/31/2017

u g z = g T y (1) f T Margules Equation for Frontal Slope

Buoyancy-forced circulations in shallow marginal seas

Processes Coupling the Upper and Deep Ocean on the Continental Slope

weak mean flow R. M. Samelson

Influence Of Bottom Topography On An Upwelling Current: Generation Of Long Trapped Filaments

Model equations for planetary and synoptic scale atmospheric motions associated with different background stratification

The general circulation: midlatitude storms

Local generation of internal solitary waves in an oceanic pycnocline

Radiating Instability of a Meridional Boundary Current

Laboratory Modeling of Internal Wave Generation in Straits

Mean Flow Evolution of a Baroclinically Unstable Potential Vorticity Front

OCN660 - Ocean Waves. Course Purpose & Outline. Doug Luther. OCN660 - Syllabus. Instructor: x65875

PAPER 333 FLUID DYNAMICS OF CLIMATE

Traveling planetary-scale Rossby waves in the winter stratosphere: The role of tropospheric baroclinic instability

BALANCED FLOW: EXAMPLES (PHH lecture 3) Potential Vorticity in the real atmosphere. Potential temperature θ. Rossby Ertel potential vorticity

Nonlinear baroclinic dynamics of surface cyclones crossing a zonal jet

Meanders and eddy formation by a buoyant coastal current flowing over a sloping topography

Traveling planetary-scale Rossby waves in the winter stratosphere: The role of tropospheric baroclinic instability

Frictional Damping of Baroclinic Waves

Can a Simple Two-Layer Model Capture the Structure of Easterly Waves?

Global Variability of the Wavenumber Spectrum of Oceanic Mesoscale Turbulence

Internal Wave Generation and Scattering from Rough Topography

Influence of forced near-inertial motion on the kinetic energy of a nearly-geostrophic flow

Asymmetric inertial instability

Observation and modeling of eddies and dipoles in the Southern Indian Ocean

Quasigeostrophic Dynamics of the Western Boundary Current

Modeling the atmosphere of Jupiter

The Planetary Circulation System

Propagation of wind and buoyancy forced density anomalies in the North Pacific: Dependence on ocean model resolution

ESCI 343 Atmospheric Dynamics II Lesson 11 - Rossby Waves

6 Two-layer shallow water theory.

ROSSBY WAVE PROPAGATION

Eliassen-Palm Cross Sections Edmon et al. (1980)

Understanding inertial instability on the f-plane with complete Coriolis force

Chapter 9. Barotropic Instability. 9.1 Linearized governing equations

The Effect of Koshu Seamount on the Formation of the Kuroshio Large Meander South of Japan

Lecture 8. Lecture 1. Wind-driven gyres. Ekman transport and Ekman pumping in a typical ocean basin. VEk

Dynamics of the Extratropical Response to Tropical Heating

Boundary Conditions, Data Assimilation and Predictability in Coastal Ocean Models

The General Circulation of the Atmosphere: A Numerical Experiment

Generation and Separation of Mesoscale Eddies from Surface Ocean Fronts

Tide-Topography Interactions: Asymmetries in Internal Wave Generation due to Surface Trapped Currents

Dynamics and Kinematics

Wind Gyres. curl[τ s τ b ]. (1) We choose the simple, linear bottom stress law derived by linear Ekman theory with constant κ v, viz.

Mean Stream-Coordinate Structure of the Kuroshio Extension First Meander Trough

Geophysics Fluid Dynamics (ESS228)

Generation of strong mesoscale eddies by weak ocean gyres

Basin-Scale Topographic Waves in the Gulf of Riga*

Dissipative Selection of Low-Frequency Modes in a Reduced-Gravity Basin

Dynamics Rotating Tank

Atmosphere, Ocean, Climate Dynamics: the Ocean Circulation EESS 146B/246B

Modeling of Coastal Ocean Flow Fields

SIO 210: Dynamics VI (Potential vorticity) L. Talley Fall, 2014 (Section 2: including some derivations) (this lecture was not given in 2015)

LFV in a mid-latitude coupled model:

Eddy-resolving Simulation of the World Ocean Circulation by using MOM3-based OGCM Code (OFES) Optimized for the Earth Simulator

On Frontal Dynamics in Two Model Oceans

Generation and Evolution of Internal Waves in Luzon Strait

1/27/2010. With this method, all filed variables are separated into. from the basic state: Assumptions 1: : the basic state variables must

General Comment on Lab Reports: v. good + corresponds to a lab report that: has structure (Intro., Method, Results, Discussion, an Abstract would be

Non-linear patterns of eddy kinetic energy in the Japan/East Sea

Lecture 2 ENSO toy models

In two-dimensional barotropic flow, there is an exact relationship between mass

AFRICAN EASTERLY WAVES IN CURRENT AND FUTURE CLIMATES

Note that Rossby waves are tranverse waves, that is the particles move perpendicular to the direction of propagation. f up, down (clockwise)

Water mass transport associated with the oceanic fronts in the northwestern Pacific Ocean HIDEYUKI NAKANO (METEOROLOGICAL RESEARCH INSTITUTE)

GFD II: Balance Dynamics ATM S 542

Atmospheric dynamics and meteorology

Transcription:

Instability of a coastal jet in a two-layer model ; application to the Ushant front Marc Pavec (1,2), Xavier Carton (1), Steven Herbette (1), Guillaume Roullet (1), Vincent Mariette (2) (1) UBO/LPO, 6 av. Le Gorgeu, 29200 Brest, France ; (2) Actimar, 24 quai de la Douane, 29200 Brest, France ; xcarton@univ-brest.fr Abstract : The instability of a shelf front, with the characteristics of the Ushant front (steep density gradient and narrow jet), is investigated on the f-plane within the framework of a two-layer shallow-water model. Linear stability analysis and nonlinear numerical simulations show that baroclinic waves, with 20 and 40 km wavelengths, are the most unstable ones, with growth rates on the order of (1day) 1, which is comparable to what is observed on SST images. The analysis of growing perturbations in a two-layer primitive equation model (MICOM) shows that the latter are vertically shifted, which corroborates that the governing mechanism for the generation asymmetric meanders and eddies in our simulations, is baroclinic instability. Then, in order to take into account tidal effects, we add a time-periodic barotropic mean flow. Although we succeed observing some characteristics of parametric resonance (frequency selection, stepwise growth), baroclinic instability remains the main mechanism to explain the growth of meanders. Key-words : Frontal jet, baroclinic and parametric instability 1 Introduction The baroclinic instability of coastal jets, and in particular of frontal currents (defined here as currents associated with density fronts), has been the subject of recent studies (e.g. Boss et al. (1996)). This instability leads to the growth of waves with length comparable to 2π times the internal radius of deformation. If the lower layer outcrops at the front, instability also occurs on a separate band of shorter waves ; this mechanism was related to the interaction of Rossby and Kelvin modes (Sakai (1989)). If the mean velocity of the jet varies periodically with time (due to a variation of transport, for instance), parametric instability can also occur ; several studies in a idealized framework evidenced its predominance near the curve of marginal baroclinic instability (Pavec and Carton (2004), Pavec et al. (2005), Pavec et al. (2006)). An interesting example of coastal jet which can a priori develop both baroclinic and parametric instability is the Ushant front. This density front separates thermally stratified water masses west of 5 o 20 W from tidally-mixed, homogeneous water masses east of this longitude. Observations, both from satellite and in-situ, provide information on this flow : the temperature difference at the surface is 2 3 o C over 5km distance (the frontal jet width), the associated currents are on average 0.2-0.3m/s, the internal deformation radius near in the stratified zone is close to 6km, and this front undergoes a semi-diurnal tidal forcing with velocities that can reach 2m/s. Meanders with about 40km wavelength and filaments with about 20km cross-section are observed on this front (see figure 1 (left)). The objective of the present work is to determine if a simple two-layer shallow-water model, initialized with a slightly perturbed narrow jet, can reproduce the observed characteristics of the instability and if the interaction of the perturbation with a periodic barotropic mean flow (mimicking the tidal forcing) can lead to parametric resonance. 1

Figure 1: (left) SST in the Irish Sea on July 24, 2006 ; (right) average density structure of the front 2 Baroclinic instability of the frontal flow A two-layer shallow-water model is chosen to allow strong isopycnal deviations (see figure 1 (right)). For this preliminary study, a f-plane hypothesis is chosen in reason of the small latitudinal extent of the flow. The dynamical equations are t u j + ( u j u j ) f 0 v j = x P j (1) t v j + ( u j v j ) + f 0 u j = y P j (2) t h j + u j h j + h j uj = 0 (3) with j = 1, 2 the upper, lower layer index. A consequence of these equations is the conservation of potential vorticity q j = ( x v j y u j + f 0 )/h j. The mean flow is purely baroclinic U 1 (y) = U 2 (y), zonal (rotated by 90 degrees with respect to the ocean) and in geostrophic balance. U 2 = 1 f U 1 = 1 dp 1 f dy = g d f dy (h 1 + h 2 ) (4) ( dp 2 dy = g d h 1 + h 2 + ρ ) f dy ρ h 2 (5) leading to upper and lower layer thicknesses h 1 and h 2, in the steady state, defined by ( ) 1 h y h 1 = H 1 1 ρ/2ρ 2 tanh (6) σ h 2 = H 2 + 1 ( ) y 2 h tanh (7) σ To be consistent with the characteristics of the Ushant front, we choose H 1 = 50m,H 2 = 50m, h = 80m. Furthermore, ρ = αρ T, with α = 1.79 10 4 K 1. In the reference case, ρ/ρ = 7 10 4 and σ = 5km. The domain is a zonally periodic square basin 2

of 100km 100km. In the linear analysis, equations (1-2-3) are linearized around the mean flow (4-5) with a normal mode perturbation of the form (u j,v j,p j,h j) = (u j0,v j0,p j0,h j0)(y)e ik(x ct) and boundaries conditions for the perturbation are no normal flow at the northern and southern boundaries. The resulting matrix problem is solved with a generalized eigenvalue-eigenvector method. The nonlinear equations are solved numerically with the MICOM model (Bleck and Boudra (1981), Bleck and Boudra (1986), Herbette et al. (2004)) ; the horizontal grid size is 1km and we set the Smagorinski coefficient of the biharmonic horizontal dissipation operator to 0.1. 2.1 Reference case The values of the parameters given here-above lead to a baroclinic velocity on the order of 0.275m/s, quite compatible with measurements performed across the Ushant front (Mariette (1983)), and fall in the range of baroclinic instability as suggested by linear stability analysis. Numerical simulations, in which we initially add a small amplitude white-noise disturbance to the mean flow, show growing meanders and formation of eddies (See lower layer potential vorticity maps from day 11 to day 14 in figure 2). The growth of meanders and the wrapping Figure 2: Potential vorticity maps in the lower layer from day 11 to day 14 up of their tip leads to eddy formation. Though initially, a wavelength close to 30km seems to dominate, the front becomes irregular after a few days, indicating the presence of other wavelengths. Indeed, a spectral analysis of the perturbation in zonal modes indicates that mode 2 grows nearly as fast as mode 3, but to a smaller amplitude, and that mode 1 becomes large once the vortices have formed (see figure 3). The baroclinic nature of the instability is confirmed 3

by the vertical phase shift between the layer perturbations of potential vorticity (shown in Pavec (2007)). Figure 3: Spectral analysis of potential vorticity (PV) in the reference case : the log of the meridionally averaged PV of each mode is plotted with respect to time (in days) 2.2 Sensitivity study This part shows how sensitive are the growth rates of modes 1-2-3 to both the width of the front σ and the density jump ρ. If ρ is kept constant and σ increases, growth rates decrease (figures shown in Pavec (2007)). Conversely, growth rates increase ; in both cases, the baroclinic velocity varies. Now if the baroclinic velocity is kept constant and equal to about 0.275 m/s), σ is proportional to ρ in a good approximation. Figure 4 shows that the growth rates decrease with increasing σ in this case, and thus the width of the front is the dominant parameter in this evolution. A series of nonlinear simulations (for a front width varying between 2 and 20km) shows that too narrow a front leads to a very regular spacing of meanders (with a dominant mode 3 of perturbation) while too wide a front leads to too slow a growth of these meanders. A front width of 5km leads to results closer to observations, in particular two dominant modes with 30 and 50km wavelengths, comparable to the observed 20 and 40km spacing of meanders and filaments. Our simulations also indicate that, as the front is less marked, the wavelength increases, a feature indeed observed on the Ushant front in spring. 3 Parametric resonance Since tidal flow influences the Ushant front, we study here the influence of an oscillatory, barotropic mean flow on the stability of our idealized baroclinic current. Three different amplitudes, 0.02, 0.2 and 2m/s, and seven periods, ranging from 6 to 12 hours, are tested for this oscillating barotropic mean flow. Theory (e.g. Pavec et al. (2005), Pavec et al. (2006)) indicates that parametric instability of coastal currents is most effective near the curve of marginal baroclinic instability. The resonant period is then given by the pulsation of the marginal baroclinic wave. 4

Figure 4: Growth rates (in seconds 1 ) with respect to the width of the front for a baroclinic mean velocity set equal to 0.275 m/s Here, for a realistic choice of flow parameters, nonlinear simulations lead to the following results : whatever the choice of oscillatory flow amplitude, the growth rates previously obtained for baroclinic instability are not considerably altered. Nevertheless, for a finite range of periods of oscillatory flow, the growth of the perturbation has a steplike evolution with time (see modes k = 1, 3, 4 on figure 5) ; this effect is most marked for the 9h period whereas linear calculations suggest a peak of resonance at the 7h period. Frequency selection and steplike growth are characteristic of parametric resonance. But the influence of parametric resonance remains moderate here because for realistic flow conditions, baroclinic instability is dominant. 4 Conclusions The objective of this study was to analyze possible mechanisms leading to the growth of short waves on a shelf front in an idealized model, with application to the Ushant front. In fact, for the latter, satellite observations of SST, show meanders and filaments at 20 to 40 km spacing. Numerical simulations, with a two-layer shallow-water model, of the evolution of a narrow shelf jet in geostrophic balance, was able to reproduce the growth of meanders and eddies with similar sizes as those that are observed for the Ushant front. The width of the front appears to be the key parameter that governs its evolution. The analysis of the vertical phase shift of the growing perturbations confirmed that the governing mechanism was baroclinic and frontal instability. Within the range of realistic parameters values, the presence of an oscillatory barotropic mean flow was not able to trigger another type of instability, and baroclinic instability always remained the dominant process. Nevertheless, we could observe some signs of parametric resonance: frequency selection and step like growth. A first step towards more realism after this study should consider a meridional mean flow on the beta-plane; indeed, the beta-effect would then favor the zonal growth of perturbations. In a second step, realistic stratification, bathymetry and forcing should also be included. References Bleck, R., Boudra, B. 1981 Initial testing of a numerical ocean circulation model using a hybrid 5

Figure 5: Growth of the first four modes (k=1,2,3,4) with respect to time (in days) for a barotropic oscillatory flow of 2m/s with periods of 6, 7, 9 and 12 hours ; as in figure 3, the modal amplitude is the logarithm of meridionally averaged PV. 6

(quasi-isopycnic) vertical coordinate J. Phys. Oceanogr. 11 755-770. Bleck, R., Boudra, B.1986 Wind-driven spin-up eddy resolving ocean models formulated in isopycnic and isobaric coordinates. J. Geophys. Res. 91 (C6), 7611-7621. Boss, E., Paldor, N., Thompson L. 1996 Stability of a potential geostrophic front: from quasigeostrophy to shallow-water, J. Fluid Mech. 315 65-84 Herbette, S., Morel, Y., Arhan, M. 2004 Subduction of a surface vortex under an outcropping front J. Phys. Oceanogr. 34 1610-1627. Mariette, V. 1983 Effets des échanges atmosphériques sur la structure thermique marine; application à des zones du large et à une zone côtière Thèse de Doctorat, Université de Bretagne Occidentale Pavec, M., Carton, X. 2004 Parametric instability of a two-layer wall jet Reg. Chaot. Dyn. 9 499-508 Pavec, M., Carton, X., Swaters, G. 2005 Baroclinic instability of frontal geostrophic currents over a slope J. Phys. Oceanogr. 35 911-918 Pavec, M., Carton, X., Poulin, F. 2006 Parametric instability of boundary currents in a two-layer QG model Dyn. Atmos. Ocean submitted Pavec, M. 2007 Instabilités barocline et paramétrique des courants de bord ; application au front d Ouessant Manuscrit soumis à thèse de Doctorat, Université de Bretagne Occidentale Sakai, S. 1989 Rossby-Kelvin instability : a new type of ageostrophic instability J. Fluid Mech. 202 149-176 7