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The Atmospheric Response to Changes in Tropical Sea Surface Temperatures. An overview of Gill, A.E., 1980, Some simple solutions for heat-induced tropical circulation and
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The Atmospheric Response to Changes in Tropical Sea Surface Temperatures An overview of Gill, A.E., 1980, Some simple solutions for heat-induced tropical circulation and Lindzen, R.S. and S. Nigam, 1987, On the Role of Sea Surface Temperature Gradients in Forcing Low-level Winds and Convergence in the Tropics Ann Gravier AT 750 19 Nov 2002
Outline • Gill’s model: Response of tropical atmosphere to focused diabatic heating • Response to symmetric and asymmetric forcing • Other solutions • Conclusions • Lindzen and Nigam’s model: Response of the tropical atmosphere to SST gradients • Observations • Model assumptions/the back-pressure effect • Solutions • Conclusions
Gill’s Model • Forcing: Heating of a limited area at or near the Equator such as over the Indonesian region • Responses: • Eastward propagating Kelvin waves, creating easterly tradewinds, and producing a Walker-type circulation, with rising over the source and sinking to the east • Slower (1/3) westward propagating planetary wave, of lesser extent producing a region of surface westerlies such as observed over the Indian Ocean
Gill’s model formulation and assumptions • Linear for small perturbations on a resting atmosphere • Non-dimensional forced shallow water equations on equatorial b-plane where f =by • Dissipative processes for friction and cooling = e~small • Forcing ~O(1) • Rigid lid at Z=D
Response to symmetric forcing about the Equator (and x=0) • Kelvin wave response travels eastward at unit speed and decays with time (at e) and space (e) • Note from (4.3) response is only in u, p and w (easterlies, downward vertical motion, and troughing at the Equator for x>2. • Planetary wave response travels westward at 1/3 KW and decays spatially at 3e • From (4.8), the PW response has a meridional response which enables cyclonic motion on both sides of the Equator and relative ridging at the Equator west of the heating region. • Walker circulation is 5x that of Hadley cells
Symmetric Response in the heating region • Forcing in the region |x|<L (heating region) • As z increases, e goes to zero, from (4.8) w>0 (upward motion) and v>0 for y>0 and v<0 for y<0 (poleward motion-away from heat source) • Relationship is elucidated by vorticity eqn taken in limit e goes to zero. Divergence is balanced by the advection of planetary vorticity: Sverdrop Relation
Response to asymmetric forcing about the Equator (positive north, negative south) • Mixed planetary-gravity wave response which has no effect outside the forcing region, since they don’t propagate • Westward moving planetary wave response in u, v, p, and w per (5.6). • No response to east OUTSIDE heating region (x>2) • Upward (downward) vertical motion north (south) of Equator; cyclone to north and anticyclone to south • Cross-equatorial flow from High to Low pressure • Zonally integrated solution yields dominant Hadley Cell with rising motion in NH and low-level poleward westerly flow.
Heating mostly north of the Equator: combined solution • Symmetric response (Equatorial easterlies) evident to east of forcing region • Upward vertical motion associated with heating dominates to north • Westerlies west of forcing between 0<y<2 • Easterlies south of Equator both east and west of forcing region • Low in NH, High in SH • Zonally integrated solution shows dominant Hadley Cell circulation 70% of Walker Cell
Summary • Walker circulation driven only by the response to symmetric heating • Hadley circulation driven by the heating region and region to west (asymmetric heating) • Effect of large topographic barriers • “Squashing” of pressure contours and low-level jets by boundary
Lindzen and Nigam 1987 : Response of tropical atmosphere to SST gradients • Theory • Observations and Assumptions • Model • Model solutions • Analysis of Sensitivities • Zonally symmetric model • Conclusions
Theory • Observational and model evidence that precipitation anomalies in tropics associated with SSTA and low-level moisture covergence rather than evaporation anomalies • Authors investigate whether SST variations forcing of pressure gradients, which contribute to low-level convergence
Observations and Assumptions • Lower troposphere over tropical oceans is vertically well-mixed to about 700mb • Presence of trade-wind inversion (2-3km) • Isolates lower part of atmosphere from effects of upper atmosphere • Analyzed eddy virtual temperature fields up to 700mb. High degree of vertical correlation.
The “back-pressure” effect • Problem: Unrealistic simulation of zonal and meridional velocities and associated eddy convergence at equator. Sensitivity of near equatorial winds to small variations in equatorial pressure field. • On timescales of less than the cumulus cloud development time (~1hr), in nature, the winds make small-scale adjustments in that finite time to “correct” pressure (decrease the pressure gradient, and thereby the convergence). Therefore before vertical mass flux occurs, there is a horizontal redistribution of mass within the trade inversion
The “back-pressure” effect • Original model instantaneously takes up any convergence by cumulonimbus mass flux • Improved model: To include this back pressure effect, authors incorporate mechanism that allows variations in high of lid (height perturbations) within a specified adjustment or relaxation time, 30 min.
Analysis of sensitivities • Is the low-level tropical flow forced by the zonal or meridional gradients of SST or both? • Meridional gradients are ~2X zonal gradients • Separately set zonal/meridional eddy SST gradients=0 • Results in Figs. 7a and 7b: Convergence forced by zonal gradients~meridional gradients. • Dominance appears regional • Conclusion: East-west gradients in low-level flow and convergence over tropical Pacific are forced not only by zonal gradients in SST, but also by zonal variations in the meridional SST gradient field
Zonal Gradient=0 Meridional Gradient=0
Analysis of sensitivities • What is the essential horizontal momentum balance? • Recall that the momentum balance is between the Coriolis force, the eddy temperature (pressure) gradient and friction. • Tested sensitivity to Rayleigh friction coefficient, e. • Conclusion: The momentum balance in the model’s tropics is essentially geostrophic to within a few degrees of the Equator
Analysis of sensitivities • How important is the contribution of “beta convergence” to the total convergence over tropical oceans? • Eqn 11c. First term on RHS includes effects of geostrophic convergence and friction term. Other major term is essentially Laplacian of net pressure field. • The beta convergence term is important because it largely determines the sign of the convergence field and compensates for the Laplacian term (opposite sign) in the near-Equatorial region. Fig. 9 • Argues against a simple momentum balance between friction and the pressure gradient force in the tropics
Analysis of sensitivities • How sensitive are the model solutions to the value of the adjustment timescale, tc? • tc ~10 minutes or less: Stronger flow and excessive convergence • tc ~3hr: flow and convergence fields weakened • 30 min < tc< 1hr: cumulus development time
Zonally symmetric model • Objective: Determine the surface forced component of the lower tropospheric Hadley circulation through the use of a coupled model • Retain only the zonal mean terms of the back pressure version of the model
Conclusions • SSTs and their associated gradients are an important forcing mechanism of low-level tropical flow and convergence. Low-level forcing is differential heating by SSTs of trade cumulus layer (not latent heat release). • The net eddy tropical convergence is very sensitive to near-Equatorial pressure gradients: To attain a realistic simulation, the Cb mass flux exiting the trade inversion layer must be allowed time to adjust to the horizontal convergence in a finite time (tc) • Momentum balance in model’s tropics is essentially geostrophic except within a few degrees of Equator
Conclusions • Longitudinal gradients in low-level flow and convergence over the tropical Pacific are forced not only by zonal gradients in SST, but also by zonal variations in the meridional SST gradient field. • Although zonal gradients in SST are smaller than their meridional counterparts, they can be of regionally dominant such as in the SPCZ. • The net eddy tropical convergence has important contributions from both the Beta convergence and Laplacian of the net pressure fields terms • The surface temperature field contribute importantly to the mean meridional circulation
References • Gill, A.E., 1980, Some simple solutions for heat-induced tropical circulation, Quart. J. R. Met. Soc. 106, pp. 447-462 • Lindzen, R.S. and S. Nigam, 1987, On the Role of Sea Surface Temperature Gradients in Forcing Low-level Winds and Convergence in the Tropics, J. Atmos. Sci., 44, 2418-2436