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Basic dynamics ●The equations of motion and continuity Scaling Hydrostatic relation

Basic dynamics ●The equations of motion and continuity Scaling Hydrostatic relation Boussinesq approximation ●Geostrophic balance in ocean’s interior. The Equation of Motion. Newton’s second law in a rotating frame. (Navier-Stokes equation).

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Basic dynamics ●The equations of motion and continuity Scaling Hydrostatic relation

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  1. Basic dynamics ●The equations of motion and continuity Scaling Hydrostatic relation Boussinesq approximation ●Geostrophic balance in ocean’s interior

  2. The Equation of Motion Newton’s second law in a rotating frame.(Navier-Stokes equation) : Acceleration relative to axis fixed to the earth. : Pressure gradient force. : Coriolis force, where : Effective (apparent) gravity. : Friction. molecular kinematic viscosity.

  3. Gravity: Equal Potential Surfaces • g changes about 5% 9.78m/s2 at the equator (centrifugal acceleration 0.034m/s2, radius 22 km longer) 9.83m/s2 at the poles) • equal potential surface normal to the gravitational vector constant potential energy the largest departure of the mean sea surface from the “level” surface is about 2m (slope 10-5) • The mean ocean surface is not flat and smooth earth is not homogeneous

  4. In Cartesian Coordinates: where

  5. Accounting for the turbulence and averaging within T:

  6. Given the zonal momentum equation If we assume the turbulent perturbation of density is small i.e., The mean zonal momentum equation is Where Fx is the turbulent (eddy) dissipation If the turbulent flow is incompressible, i.e.,

  7. Eddy Dissipation Reynolds stress tensor and eddy viscosity: , Then Where the turbulent viscosity coefficients are anisotropic. Ax=Ay~102-105 m2/s Az ~10-4-10-2 m2/s >>

  8. Reynolds stress has no symmetry:  A more general definition:   if (incompressible)

  9. Continuity Equation Mass conservation law In Cartesian coordinates, we have or For incompressible fluid, If we define and , the equation becomes

  10. Scaling of the equation of motion • Consider mid-latitude (φ≈45o) open ocean away from strong current and below sea surface. The basic scales and constants: L=1000 km = 106 m H=103 m U= 0.1 m/s T=106 s (~ 10 days) 2Ωsin45o=2Ωcos45o≈2x7.3x10-5x0.71=10-4s-1 g≈10 m/s2 ρ≈103 kg/m3 Ax=Ay=105 m2/s Az=10-1 m2/s • Derived scale from the continuity equation W=UH/L=10-4 m/s  

  11. Scaling the vertical component of the equation of motion   Hydrostatic Equation accuracy 1 part in 106

  12. Boussinesq approximation Density variations can be neglected for its effect on mass but not on weight (or buoyancy). where , we have Assume that where  Then the equations are (1) (2) where (3) (The term (4) is neglected in (1) for energy consideration.)

  13. Geostrophic balance in ocean’s interior

  14. Scaling of the horizontal components  (accuracy, 1% ~ 1‰) Zero order (Geostrophic) balance Pressure gradient force = Coriolis force

  15. Re-scaling the vertical momentum equation Since the density and pressure perturbation is not negligible in the vertical momentum equation, i.e., , and , The vertical pressure gradient force becomes

  16. Taking into the vertical momentum equation, we have , and assume If we scale then  and (accuracy ~ 1‰)

  17. Geopotential Geopotential Φis defined as the amount of work done to move a parcel of unit mass through a vertical distance dz against gravity is The geopotential difference between levels z1 and z2 (with pressure p1 and p2) is (unit of Φ: Joules/kg=m2/s2).

  18. Dynamic height , we have Given where is standard geopotential distance (function of p only) is geopotential anomaly. In general, Φ is sometime measured by the unit “dynamic meter” (1dyn m = 10 J/kg). which is also called as “dynamic distance” (D) Units: δ~m3/kg, p~Pa, D~ dyn m Note: Though named as a distance, dynamic height (D) is still a measure of energy per unit mass.

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