CEE 262A H YDRODYNAMICS Lecture 13 Wind-driven flow in a lake.

Slides:



Advertisements
Similar presentations
Basic Governing Differential Equations
Advertisements

Types of flow: Slide from Dr. Isaac.
Monroe L. Weber-Shirk S chool of Civil and Environmental Engineering Basic Governing Differential Equations CEE 331 June 12, 2015.
Basic Governing Differential Equations
D A C B z = 20m z=4m Homework Problem A cylindrical vessel of height H = 20 m is filled with water of density to a height of 4m. What is the pressure at:
1 Numerical Hydraulics Open channel flow 1 Wolfgang Kinzelbach with Marc Wolf and Cornel Beffa.
Lecture 7 Exact solutions
STORM SURGE. Composed of several attributes: A)Barometric – Coastal water response to low pressure at center of storm B) Wind stress – frictional drag.
Monroe L. Weber-Shirk S chool of Civil and Environmental Engineering Basic Governing Differential Equations CEE 331 July 14, 2015 CEE 331 July 14, 2015.
LAMINAR PLANE COUETTE AND OPEN CHANNEL FLOW
Surface Water Equations
Suspended Load Above certain critical shear stress conditions, sediment particles are maintained in suspension by the exchange of momentum from the fluid.
St Venant Equations Reading: Sections 9.1 – 9.2.
Hans Burchard Leibniz Institute for Baltic Sea Research Warnemünde Coastal Ocean Dynamics First course: Hydrodynamics.
The Air-Sea Momentum Exchange R.W. Stewart; 1973 Dahai Jeong - AMP.
Hydraulic Routing in Rivers
CEE 262A H YDRODYNAMICS Lecture 5 Conservation Laws Part I 1.
CP502 Advanced Fluid Mechanics
Basic dynamics  The equations of motion and continuity Scaling Hydrostatic relation Boussinesq approximation  Geostrophic balance in ocean’s interior.
CEE 262A H YDRODYNAMICS Lecture 18 Surface Ekman layer.
USSC3002 Oscillations and Waves Lecture 12 Water Waves Wayne M. Lawton Department of Mathematics National University of Singapore 2 Science Drive 2 Singapore.
Equations that allow a quantitative look at the OCEAN
Momentum Equations in a Fluid (PD) Pressure difference (Co) Coriolis Force (Fr) Friction Total Force acting on a body = mass times its acceleration (W)
Mass Transfer Coefficient
EVAT 554 OCEAN-ATMOSPHERE DYNAMICS FILTERING OF EQUATIONS OF MOTION FOR ATMOSPHERE (CONT) LECTURE 7 (Reference: Peixoto & Oort, Chapter 3,7)
Reynolds Transport Theorem We need to relate time derivative of a property of a system to rate of change of that property within a certain region (C.V.)
CEE 262A H YDRODYNAMICS Lecture 15 Unsteady solutions to the Navier-Stokes equation.
For a rotating solid object, the vorticity is two times of its angular velocity Vorticity In physical oceanography, we deal mostly with the vertical component.
Distributed Flow Routing Surface Water Hydrology, Spring 2005 Reading: 9.1, 9.2, 10.1, 10.2 Venkatesh Merwade, Center for Research in Water Resources.
Fluid Flow in Rivers Outline 1.Flow uniformity and steadiness 2.Newtonian fluids 3.Laminar and turbulent flow 4.Mixing-length concept 5.Turbulent boundary.
1 Equations of Motion Buoyancy Ekman and Inertial Motion September 17.
For a rotating solid object, the vorticity is two times of its angular velocity Vorticity In physical oceanography, we deal mostly with the vertical component.
Ekman Flow September 27, 2006.
Hydraulic Routing in Rivers Reference: HEC-RAS Hydraulic Reference Manual, Version 4.1, Chapters 1 and 2 Reading: HEC-RAS Manual pp. 2-1 to 2-12 Applied.
CEE 262A H YDRODYNAMICS Lecture 7 Conservation Laws Part III.
IIT-Madras, Momentum Transfer: July 2005-Dec 2005 Von Karman Integral Method (BSL) PRANDTL BOUNDARY LAYER EQUATIONS for steady flow are Continuity N-S.
Von Karman Integral Method (BSL) PRANDTL BOUNDARY LAYER EQUATIONS for steady flow are Continuity N-S (approx) 12  If we solve these, we can get V x, (and.
EVAT 554 OCEAN-ATMOSPHERE DYNAMICS TIME-DEPENDENT DYNAMICS; WAVE DISTURBANCES LECTURE 21.
Level of No Motion (LNM)
FREE CONVECTION 7.1 Introduction Solar collectors Pipes Ducts Electronic packages Walls and windows 7.2 Features and Parameters of Free Convection (1)
Mechanical Energy Balance
Conservation of Salt: Conservation of Heat: Equation of State: Conservation of Mass or Continuity: Equations that allow a quantitative look at the OCEAN.
The simplifed momentum equations Height coordinatesPressure coordinates.
Ocean Dynamics Previous Lectures So far we have discussed the equations of motion ignoring the role of friction In order to understand ocean circulations.
OC FLOW: ENERGY CONCEPTS, CHANNEL ANALYSIS
Basic dynamics ●The equations of motion and continuity Scaling Hydrostatic relation Boussinesq approximation ●Geostrophic balance in ocean’s interior.
Basic dynamics The equation of motion Scale Analysis
The sea-breeze circulation Part I: Development w/o Earth rotation.
CEE 262A H YDRODYNAMICS Lecture 12 Steady solutions to the Navier-Stokes equation.
 p and  surfaces are parallel =>  =  (p) Given a barotropic and hydrostatic conditions, is geostrophic current. For a barotropic flow, we have and.
BOUNDARY LAYERS Zone of flow immediately in vicinity of boundary Motion of fluid is retarded by frictional resistance Boundary layer extends away from.
Free Surface Hydrodynamics 2DH and 3D Shallow Water Equations Prof. Dano Roelvink.
Viscosità Equazioni di Navier Stokes. Viscous stresses are surface forces per unit area. (Similar to pressure) (Viscous stresses)
Estuarine Hydrodynamics
Modelling of Marine Systems. Shallow waters Equations.
For a barotropic flow, we have is geostrophic current.
Class Meeting Nov. 26, 2:00pm-4:45pm
Energy Reduction Through Tribology-2
Chapter 4 Fluid Mechanics Frank White
Assume geostrophic balance on -plane approximation, i.e.,
Wind Driven Circulation III
For a barotropic flow, we have is geostrophic current.
Distributed Flow Routing
Subject Name: FLUID MECHANICS
Fluid is contained between two parallel
Navier - Stokes Equation
Convective Heat Transfer
Asst. Prof. Dr. Hayder Mohammad Jaffal
BAE 6333 – Fluvial Hydraulics
Conservation of momentum
Presentation transcript:

CEE 262A H YDRODYNAMICS Lecture 13 Wind-driven flow in a lake

Wind-Driven Flow in a Lake Assumption (i) Steady Forcing (ii) Two-dimensional (iii) H/L<<1 L x 1 =0 x 1 =L H x 3 =0 x 3 =H (A turbulent stress) “Rigid lid”

Mass: x 1 -Momentum: x 3 -Momentum: Simplify (a) (b) Scale Effective viscosity – assumed constant The governing equations with hydrostatic pressures removed are:

To find U and  we use an assumed force balance: pressure ~ friction The free surface condition gives Since we are looking to make We find that ~ ~ ~

Mass: x 1 -Mom: since If we choose which reduces to: From prev. slide:

Likewise the x 3 -momentum eqn. becomes To end up with PC flow we must require two things: If these conditions are both satisfied and we get rid of all of the small stuff, what is left is: 2 Pressure-friction Hydrostatic

Assumption 1: H/L << 1 "The Long Box" Assumption 2: H L Vertical diffusion time scale << Horizontal advection time scale Horizontal acceleration << Vertical friction

The second equation implies that p * = p * (x 1 * ). However, since the boundary conditions are independent of x 1 *, u 1 * should only be a function of x 3 *. This implies that the pressure gradient must be constant, i.e. not a function of x 1 *. Thus, we are back to the PC equations we solved before. But, how do we find ? We obtain an extra condition on u 1 * If we integrate continuity from x 3 * =0 to x 3 * = 1, we find that The pressure gradient we need is the one that imposes no net flow

So to proceed, we now use three conditions to constrain the quadratic velocity profile that results from integration of the x 1 momentum equation No slip on bottom Specified stress on top No net flow =2a=3/2

Thus putting it all together, we find that So that the velocity we find at the top is (to compare to our PC soln.) Since P = 3 (no net flow for PC flow), we can now compute the dimensional pressure gradient using our computed surface velocity and the definition:

Why the 3/2 ? Look at stress distribution and balance of forces 1 -1/2 Net force per unit length = +3/2  0 = Pressure force/unit length = H Shear stress Pressure Note: For turbulent flows it has been found that the stress on the bottom is nearly zero, so that the 3/2 should really be 1 for real flows

What happens when we blow a 7 m/s wind over a 2 km long channel that is 10 m deep?   /  0 =  a C D U 10 2 /  0 =1.0 kg/m 3 * * 49 m 2 /s 2 /  0 = m 2 /s 2 L = 2 km H = 10 m e ~0.005 m 2 /s  H 2 / e = 334 min No stress No slip model (SUNTANS)

What provides the pressure gradient ? In nature, a sloping free surface From hydrostatics: where Water depth without applied stress Super elevation relative to x 1 =0 x 1 =L x 3 =0 x 3 =H Condition required so that domain is still rectangular and that x 1 gradients are small

Now if we compute the horizontal pressure gradient, we can solve for the surface slope This enables us to now integrate to find the water surface change due to winds.

Since generally all of the water that starts in the lake stays there If we integrate the slope equation wrt x 1 Thus, the maximum change up or down is

Previous example: HF oscillation: T = 2L/c 0 = 2L/(gH) 1/2 =6.7 min (time it takes for a shallow water wave to propagate from one end to the other and back) Predicted Computed: m Less bottom stress! zoomed-in view

Relative to the depth this change is: Normal example Lake Okeechobee during a hurricane