Internal wave simulation for different angles and shapes of continental shelf Himansu K. Pradhan*, A.D. Rao, K.K.G. Reddy and S. Mohanty Centre for Atmospheric Sciences, Indian Institute of Technology Delhi, New Delhi, India [email protected] Abstract- The average slope of the continental shelf in the world ocean is 0.5o and its width varies considerably. This paper illustrates experimental studies describing the internal wave run-up on different gradients of continental shelf varying from 0.2o to 0.5o. MIT general circulation model is configured with a variable grid, tidal information in the momentum equations and background stratification of density as initial fields to simulate internal waves. The model simulated density and temperature time-series is subjected to Fast Fourier Transform to compute the energy spectra of internal waves. The results reveal that the peak of internal wave activity varies spatially for different angles of the continental shelf. The experiments are further continued for concave coastline geometry to look at the internal wave energy distribution over the shelf. The results show that in a concave coastline the energy is large compared to a straight coastline inferring convergence of internal wave energy. Keywords—Continental Shelf, Internal Waves; MITgcm; Energy spectra. I. INTRODUCTION Internal waves (IWs) are common phenomena over the continental shelves and internal tides are IWs at a tidal frequency that are generated when barotropic tides/surface tides interact with shallow topographic features [1]. Occurring beneath the free surface of a density stratified water body; they have utmost importance in submarine acoustics, underwater navigation, offshore structures, ocean mixing, biogeochemical processes, etc. over the shelf-slope region. The geometry of the shelf-slope region and local hydrographic conditions determine the effect of this interaction. Wave trains formed after the interaction propagate both inward over the continental shelf and outward into the open ocean [2]. The conversion of barotropic tidal energy into baroclinic energy in the form of internal tides takes place at topographic boundaries. Earlier studies of Legg and Adcroft [3] examined mixing generated by internal wave reflection from variable topographic slopes of convex and concave shapes. The upper part of the continental slope plays an important role in non-linear effects and mixing as found by Lien and Gregg [4] in their in-situ observations. 978-1-4799-4918-2/14/$31.00 ©2014 IEEE Wallace and Wilkinson [5] described the internal wave run up and its dissipative phase on uniform slopes of 0.030 and 0.054 radian from a series of laboratory experiments. Periodic wave trains propagate onto the slope, steepens forms solitary wave as they travel shoreward into the continental shelf. Numerical study conducted by Gerkema et al [6] focused on the non-linear evolution of the internal tide and showed that the main region of generation of IWs in upper part of the slope using two- dimensional MITgcm. Studies by Munroe and Lamb [7] and Holloway and Merrifield [8] have shown that there are changes in conversion rates in threedimensional studies as compared to two-dimensional. Earlier studies considered simulation of IWs over Gaussian topography, laboratory experiments, etc. with two-layered and multi-layered stratifications. Present numerical study considers the real aspect ratio of the shelf-slope topography found in the world ocean with a stratified water column of a typical tropical ocean. The continental shelf across world ocean varies and the average gradient of the continental shelf is 0.5o . Similarly the average gradient of continental slope is 3-4o. Here, we at first reproduce the generation of IWs on different gradients of continental shelf and compute the spectral energy distribution. Secondly, a comparison is made for two different stratification of May and February. Finally, we demonstrate the crucial role of the coastal geometry. For this a comparison of spectral energy distribution is made between a straight and a concave coastline in a particular stratification. II. NUMERICAL MODEL CONFIGURATION MITgcm [9],[10] is an open source code available to the community, (see http://mitgcm.org/) designed to study both oceanic and atmospheric phenomena. This finite volume, z-coordinate model solves the incompressible Navier-Stroke equations with Boussineq approximation on an Arakawa-C grid. The lopped cell representing the topography [11] is essential for accurate representation of the interaction of barotropic tide with topography. For the current study the model uses polynomial equation of state [12] for the computation of density field. The main physical parameters governing the tidal flow are shelf break o 0.2 - RED 0.3o - GREEN 0.4o - PINK 0.5o - BLUE -1000 -1200 -1400 0 5 10 15 20 continental slope ( avg. angle ~ 3 o ) 25 30 35 distance ( km ) 40 45 50 55 60 Fig. 1: Schematic representation of bottom topography at a particular cross-section. The monthly climatological temperature and salinity fields are derived from World Ocean Atlas (2009) of National Oceanographic Data Centre that are taken as initial density fields representing the background density [16],[17]. The profiles are taken for the month of May and February bearing different stratifications found in the tropical waters of the Bay of Bengal in the North Indian Ocean. The simulation is carried out for 18 days of which the first 10 days are considered for spin-up and the next 8 days for analysis. A 3.5days time span is chosen containing a spring tide for computing the spectral estimates. This is obtained by direct method using the Fast Fourier Transform algorithm of Cooley and Tukey [18]. Spectral estimates of IWs is computed from the time > < > > < pycnocline depth ( m ) -200 < thermocline 0 -400 -600 (a) -800 4 (b) 8 12 16 20 24 28 33 temperature ( oC ) (c) 34 35 36 1020 salinity ( psu ) 1023 1026 density ( kg/m3 ) Fig. 2: Vertical profile for May (a) Temperature (b) Salinity (c) Density. The experiment details are tabulated below: open ocean -400 (angle varies between 0.2o to 0.5o ) -600 -800 The first set of experiments are carried out for different continental shelf angles 0.2o, 0.3o, 0.4o and 0.5o for a shelf width of 17km. Correspondingly, the shelf break falls at a water depth of 70m, 110m, 145m and 175m respectively. The cross-section at 90th grid point that falls at the centre of the domain along the y-axis is taken into account for study. The area averaged temperature and salinity for the month of May were given as initial conditions as shown in the Fig. 2a,b,c. This shows that the water is stratified continuously from the surface bearing a small mixed layer of depth 20-25m. The Coriolis frequency is fixed at 4.3E-5 and the beta plane approximation is at 2.18E-11. (a) (b) (c) (d) spectral estimate ( oC )2 depth ( m ) -200 III. RESULTS AND DISCUSSION Shelf angle Shelf width Depth at shelf break Slope angle Stratification 0.20 0.30 0.40 0.50 17km 17km 17km 17km 70m 110m 145m 175m 30 30 30 30 May May May May 300 0.2 o - RED 0.3o - GREEN 0.4o - PINK 0.5o - BLUE 250 200 150 100 50 0 (a) 10 15 20 0 25 30 35 40 distance ( km ) 45 open ocean continental shelf -200 50 55 70 m 110 m 145 m 175 m -50 -100 -150 -200 -250 continental slope -300 -300 impact points at shelf break -350 for different angles of -400 continental shelf -400 -500 60 0 shelf break -100 depth ( m ) coast continental shelf > 0 series of density and temperature that describes the distribution of signal power over wave frequencies. halocline (a)frequency of the barotropic tide, ωo (b) amplitude of the barotropic tide, Uo (c) coriolis frequency fo. The model is forced with real-time tides by adding tidal components in the momentum equations [13],[14] of the model. An oscillating barotropic flow is imposed uniformly throughout the domain as a surface forcing. Four tidal components M2, S2, K1 and O1 were considered for tidal forcing. The respective time periods are 12.4hr, 12hr, 23.93hr and 25.82hr and corresponding velocity amplitudes are 28.98cm/s, 30cm/s, 15.041cm/s and 13.943 cm/sec for the components. At open boundaries, Orlanski radiation boundary conditions [15] are prescribed which allow any disturbance generated in the domain to pass through without any significant distortion. No-slip boundary condition is applied at the bottom and a free-slip at the lateral boundary. It uses implicit free surface and no rigid lid for surface pressure. Four experiments with gradients of continental shelf varying from 0.2o to 0.5o and gradient of continental slope is 3o as shown in Fig. 1. The shelf break/shelf edge point is smoothened to avoid abrupt fall from continental shelf to continental slope. An orthogonal curvilinear grid bearing 390*180*23 grid points in x, y and z direction respectively. From the 23 vertical levels, the first 12 levels are from the sea surface with 10m interval each and next 4 levels are kept at 20m interval. However, the maximum depth at this cross-section of the domain is 2500m (not shown in figure). (b) -450 -500 10 15 20 25 30 35 40 distance ( km ) 45 50 10 15 55 20 25 60 30 o temperature ( C ) Fig. 3: (a) Spectral estimate of temperature for all continental shelf angles. (b) Bottom topography normal to the shelf for all angles (left) and vertical temperature profile (right). 0.2 o - RED 0.3o - GREEN 0.4o - PINK 0.5o - BLUE 40 30 10 > pycnocline < > < > 6 10 14 18 22 26 30 33 o (c) 34 35 salinity ( psu ) 36 1020 1023 1026 density ( kg/m3 ) Fig. 5: Vertical profile for February (a) Temperature (b) Salinity (c) Density. The detail of the experiments are tabulated below: Shelf angle Shelf width Depth at shelf break Slope angle Stratificatio n 0.20 0.30 0.40 0.50 17km 17km 17km 17km 70m 110m 145m 175m 30 30 30 30 Feb Feb Feb Feb (a) 10 15 20 25 30 35 40 distance ( km ) 45 50 shelf break open ocean continental shelf -200 (b) 15 20 25 30 35 40 distance ( km ) 70 m 110 m 145 m 175 m impact points at shelf break for different angles of continental shelf -400 10 60 -50 -100 -150 -200 -250 continental slope -300 55 0 -100 -500 (b) temperature ( C ) 45 50 1022 55 -300 -350 -400 -450 spectral estimate ( oC )2 0 < (a) -800 (a) (b) (c) (d) 20 thermocline depth ( m ) -400 -600 -500 102560 1028 3 density (kg/m ) Fig. 4: (a) Spectral estimate of density across all cross-sections. (b) Bottom topography normal to the shelf for all angles (left) and vertical density profile (right). The spectral estimate of density representing spectral energy distribution is also shown in Fig. 4. On comparison of Fig. 3 and 4, the behaviour of the profile for spectral estimate of both temperature and density is similar except its magnitude. Since the variables are different, it is expected the magnitudes of the spectral estimate to be different. The above simulations are compared with an experiment using a different stratification for February using February temperature while retaining May salinity to see the effect of temperature alone. The vertical profile of temperature, salinity and density calculated from both temperature and salinity are shown in Fig. 5. 300 0.2 o - RED 0.3o - GREEN 0.4o - PINK 0.5o - BLUE 250 200 150 100 50 0 (a) 10 15 20 0 25 30 35 40 distance ( km ) 45 50 open ocean continental shelf -200 55 70 m 110 m 145 m 175 m -50 -100 -150 -200 -250 continental slope -300 -300 impact points at shelf break -350 for different angles of -400 continental shelf -400 -500 60 0 shelf break -100 depth ( m ) spectral estimate ( d )2 -200 50 0 depth ( m ) 0 halocline Fig. 3a shows the computed spectral estimate of model simulated temperature for different angles (0.2o, 0.3o, 0.4o and 0.5o in Fig. 3b) of the shelf represented in different colours. The activity is predominant over the shelf-slope region as the wave excitement tends to increase with the height and the steepness of the shelf-slope. As the angle increases, the internal wave activity is seen more towards inner shelf. Particularly for 0.2o shelf, the activity is just over the shelf break and the estimate is less since the water column is limited to the upper part of the thermocline at the shelf break, whereas depth at the shelf break increases for all other angles [see Fig. 3b ]. In general, the spectral estimate in the open ocean is less due to less or no interaction with the bottom topography. (b) -450 -500 10 15 20 25 30 35 40 distance ( km ) 45 50 10 15 55 20 25 60 30 o temperature ( C ) Fig. 6: (a) Spectral estimate of temperature across all crosssections. (b) Bottom topography normal to the shelf (left) for all angles and vertical temperature profile (right). 20 (a) 40 45 50 open ocean -100 continental shelf impact points at shelf break for different angles of continental shelf -400 -500 (b) 10 15 20 25 30 35 40 distance ( km ) 70 m 110 m 145 m 175 m -50 30 17 -100 -150 39 16 0 -200 po -250 continental slope -300 60 0 shelf break -200 55 45 50 1022 55 -300 15 82 -350 -400 -450 -500 102560 1028 3 density (kg/m ) Fig. 7: (a) Spectral estimate of density across all cross-sections. (b) Bottom topography normal to the shelf (left) for all angles and vertical density profile (right). in (a) ts 83 84 85 longitude 200 b(i) 150 30 100 50 0 0 80 100 120 140 160 180 > shelf break ( 145 m ) -400 -600 0 80 90 50 60 0 80 100 120 140 160 180 0 0 -200 -200 -400 -400 -600 40 60 80 100 120 140 160 -600 -800 -1000 80 & 100 -1200 c(ii) -1400 60 80 100 120 140 160 180 b(iii) 100 -800 c(i) 80 100 120 140 160 180 150 -1000 -1400 60 200 -800 -1200 100 50 -1000 30 & 150 b(iv) 100 50 0 80 100 120 140 160 180 150 b(ii) 100 50 150 100 150 -200 depth ( m ) 200 b(v) 150 87 200 0 90 -1200 80 100 120 140 160 180 40 grid points grid points c(iii) -1400 60 80 100 120 140 160 grid points Fig. 8: (a) The domain of the concave coastline. b(i-v) The spectral energy distribution at different cross sections. c(i-iii) The bottom topography at the respective cross sections. 150 > 20 depth (m) 0 -10 -50 -100 -150 -200 -300 -400 -500 -600 -800 -1000 -1500 -2000 -2500 -3000 100 90 80 latitude 19 18 30 spectral estimate ( d ) 2 15 82 po po 0 0 in 18 39 16 in ts 17 (a) ts 83 84 200 b(i) 150 100 30 depth ( m ) -400 -600 87 200 100 b(ii) 80 100 120 140 160 180 shelf break ( 145 m ) 0 200 200 50 0 0 80 90 50 80 100 120 140 160 180 0 0 0 -200 -400 -400 -600 80 100 120 140 160 180 -600 -800 grid points b(iii) 100 -1000 80 100 120 140 160 180 80 100 120 140 160 180 200 -200 -1200 100 50 -800 c(i) b(iv) 100 -1000 -1400 80 100 120 140 160 180 150 -800 -1200 150 100 -1000 30 & 150 b(v) 150 150 50 0 -200 86 150 50 0 85 longitude > Fig. 6 shows spectral estimate of temperature for all continental shelf angles for February stratification. It also shows the propagation of IWs towards the coast enhances with the larger gradient of continental shelf as in the case of May. However, the overall spectral estimate are less compared to that of simulated for May. This fact is attributed to prevailing deeper mixed layer (extending up to 60m) in Feb. The peak spectral estimate at 0.2o lies outside the continental shelf region as observed in May due to small portion of stratified water column interacts at the shelf break (the depth of the shelf break is 70m as shown in figure). The spectral estimate of energies for May and Feb at 0.5o is approximately the same, which may be attributed to less effect of the mixed layer at higher depth (175m) of shelf break. In both the months, the shelf break at 175m interacts with lower portion of the pycnocline. Also in these cases, the extent of spectral estimate of energy propagation over the shelf is nearly the same however their peak varies. In all other continental shelf angles (0.2o, 0.3o and 0.4o ) the spectral estimate in Feb is less than May, as a deep mixed layer doesn't support growth of IWs propagation/generation. As discussed previously, the spectral estimate of density shown in Fig.7 describes the energy spectra have the same behaviour as spectral estimate of temperature. The experiments are further continued to see the effect of the geometry of the coastline. For this, an experiment with May stratification is carried out with concave coastline for a continental shelf angle of 0.4o and continental slope angle of 3o [see Fig. 8a] . Spectral energy distribution at the cross-section of interest i.e. at 30, 80, 90, 100 and 150 in solid lines shown in Fig. 8b(iv) is analysed. The 80th, 90th and 100th grid point falls in the concave portion with the 90th point falling at the 86 200 spectral estimate ( d )2 35 ts 30 distance ( km ) in 25 po 20 0 15 18 18 10 latitude 0 0 -10 -50 -100 -150 -200 -300 -400 -500 -600 -800 -1000 -1500 -2000 -2500 -3000 100 90 80 19 10 depth (m) spectral estimate ( d ) 2 150 spectral estimate ( d )2 20 spectral estimate ( d ) 2 30 > 40 spectral estimate ( d ) 2 spectral estimate ( d )2 0.2 o - RED 0.3o - GREEN 0.4o - PINK 0.5o - BLUE 0 depth ( m ) centre of curvature. In this experiment, rotation is not taken into account i.e. coriolis force is kept as zero. 50 80 & 100 -1400 c(ii) -1200 90 -1400 c(iii) 80 100 120 140 160 180 80 100 120 140 160 180 grid points grid points Fig. 9: (a) The domain of a straight coastline. b(i-v) The spectral energy distribution at different cross sections. c(i-iii) The bottom topography at the respective cross sections. The energy is maximum at the 90th cross-section and decreases on either side indicating the convergence of energy due to the concave shape of the coastline. To understand further this energy accumulation due to the concave shape of the coastline, an experiment with straight coastline is carried out keeping the same congfiguration (continental shelf angle of 0.4o and continental slope angle of 3o) shown in Fig. 9. The energy distribution shows no change at all the crosssections [see Fig. 9b(i-v)]. The spectral energy in the concave coastline is almost double at 90th cross-section as compared to the straight coastline. Thus, the energy maximum at the curved portion is the due to the geometry of the coastline. [8] [9] [10] [11] [12] [13] IV. CONCLUSION The shelf edge remains the region of maximum internal wave activity. With the increasing depth of the shelf break the stratified water column allows more IW activity over the continental shelf. 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