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CEE 262A H YDRODYNAMICS Lecture 7 Conservation Laws Part III.

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Presentation on theme: "CEE 262A H YDRODYNAMICS Lecture 7 Conservation Laws Part III."— Presentation transcript:

1 CEE 262A H YDRODYNAMICS Lecture 7 Conservation Laws Part III

2 The Boussinesq approximation The x 3 momentum equation reads (after neglecting rotation): i.e., part of the pressure is associated with offsetting the weight of the fluid above. We can subtract out a significant part of this as follows: Reference density Background density variation – exists in the absence of motion Perturbation density – association with motion

3 The preferred ordering (which is often valid in oceans, estuaries and lakes) is Likewise we write the pressure as such that in the absence of motion If p 0 is defined by this eqn., then we can subtract out the background hydrostatic pressure gradient and the weight force associated with the density field that exists in the absence of motion.

4 Start with Then define p 0 such that Then since p=p 0 +p', Substitution into NSE gives

5 We can use the ordering of the density field to make an important simplification/approximation: i.e., the mass of each fluid particle that determines what acceleration results from a given force is approximately constant. On the other hand we retain the effect of density variations in the buoyancy (gravity) term (  ’ g). This requires that Particle accelerations << g This approximation is known as the Boussinesq approximation If  '<< , we require that

6 Navier-Stokes equation with the Boussinesq approximation We also need to make the same approximation in the mass- conservation equation, i.e. which implies that, as a consequence of the Boussinesq approximation, Note that we assumed this a priori when writing the viscous term as given above...

7 The difference between incompressibility and the Boussinesq approximation If a flow is incompressible, this implies that the density following a fluid particle is identically zero, which gives the equations for conservation of momentum and mass as Under the Boussinesq approximation, the density following a fluid particle is not constant, but its time rate of change is much smaller than that due to changes resulting from velocity gradients. This enables one to write the momentum and mass conservation equations as The Boussinesq approximation does two things: it linearizes the acceleration term in the Navier-Stokes equations and enables use of the continuity equation while retaining the effects of density in the momentum equation. Incompressible Boussinesq

8 How do we cope with free surfaces? x 3 =0 x3x3  -x 3 From before, we had p=p0+p', where p0 was the pressure field in the absence of motion, while p' was that associated with motion. We can define an alternate splitting of the pressure as p=p h +  0 , where: p h = Hydrostatic pressure arising from weight of fluid (can include motion this time)  0  = Dynamic, or nonhydrostatic, pressure arising from fluid motion

9 Defining the hydrostatic pressure as satisfying the balance we can integrate both sides to obtain p h : Surface pressure Pressure due to depth and free surface: BAROTROPIC PRESSURE Pressure due to density variations: BAROCLINIC PRESSURE

10 Now take gradients of p h : Where we have assumed that (Why is this not obvious?)

11 Adopting very commonly-used shorthand notation for the horizontal gradient, such that we have Surface pressure gradient i.e. Atmospheric pressure. Barotropic pressure gradient due to free-surface gradient. Baroclinic pressure gradient due to density gradient.

12 Substitution into the Navier-Stokes equation with the Boussinesq approximation gives Or, component-wise:

13 Why does water level go down when atmospheric pressure goes up? An example from SF Bay/Delta (observations): 10 cm (water) 15 cm

14 Answer: The ocean likes to tend towards steady state which has Thus, the response to an imposed pressure on the surface would give The “inverse barometer” - water level goes down when pressure goes up


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