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15. Physics of Sediment Transport William Wilcock (based in part on lectures by Jeff Parsons) OCEAN/ESS 410
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Lecture/Lab Learning Goals Know how sediments are characterized (size and shape) Know the definitions of kinematic and dynamic viscosity, eddy viscosity, and specific gravity Understand Stokes settling and its limitation in real sedimentary systems. Understand the structure of bottom boundary layers and the equations that describe them Be able to interpret observations of current velocity in the bottom boundary layer in terms of whether sediments move and if they move as bottom or suspended loads – LAB
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Sediment Characterization Diameter, D Type of material -664 mmCobbles -532 mmCoarse Gravel -416 mmGravel -38 mmGravel -24 mmPea Gravel 2 mmCoarse Sand 01 mmCoarse Sand 10.5 mmMedium Sand 20.25 mmFine Sand 3 125 m Fine Sand 463 μmCoarse Silt 5 32 m Coarse Silt 6 16 m Medium Silt 7 8 m Fine Silt 8 4 m Fine Silt 9 2 m Clay There are number of ways to describe the size of sediment. One of the most popular is the Φ scale. = -log 2 (D) D = diameter in millimeters. To get D from D = 2 -
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Sediment Characterization Sediment grain smoothness Sediment grain shape - spherical, elongated or flattened Sediment sorting
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Sediment Transport Two important concepts Gravitational forces - sediment settling out of suspension Current-generated bottom shear stresses - sediment transport in suspension or along the bottom (bedload) Shield stress - brings these concepts together empirically to tell us when and how sediment transport occurs
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Definitions
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1. Dynamic and Kinematic Viscosity The Dynamic Viscosity is a measure of how much a fluid resists shear. It has units of kg m -1 s -1 The Kinematic viscosity is defined where f is the density of the fluid has units of m 2 s -1, the units of a diffusion coefficient. It measures how quickly velocity perturbations diffuse through the fluid
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2. Molecular and Eddy Kinematic Viscosities The molecular kinematic viscosity (usually referred to just as the ‘kinematic viscosity’), is an intrinsic property of the fluid and is the appropriate property when the flow is laminar. It quantifies the diffusion of velocity through the collision of molecules. (It is what makes molasses viscous). The Eddy Kinematic Viscosity, e is a property of the flow and is the appropriate viscosity when the flow is turbulent flow. It quantities the diffusion of velocity by the mixing of “packets” of fluid that occurs perpendicular to the mean flow when the flow is turbulent
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3. Submerged Specific Gravity, R Typical values: Quartz = Kaolinite = 1.6 Magnetite = 4.1 Coal, Flocs < 1 f
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Sediment Settling
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Stokes settling Settling velocity (w s ) from the balance of two forces - gravitational (F g ) and drag forces (F d )
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Settling Speed Balance of Forces Write balance using relationships on last slide k is a constant Use definitions of specific gravity, R and kinematic viscosity k turns out to be 1/18
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Limits of Stokes Settling Equation 1.Assumes smooth spherical particles - rough particles settle more slowly 2.Grain-grain interference - dense concentrations settle more slowly 3.Flocculation - joining of small particles (especially clays) as a result of chemical and/or biological processes - bigger diameter increases settling rate and has a bigger effect than decrease in specific gravity as a result of voids in floc. 4.Assumes laminar flow (ignores turbulence)
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Shear Stresses
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Bottom Boundary Layers Inner region is dominated by wall roughness and viscosity Intermediate layer is both far from outer edge and wall (log layer) Outer region is affected by the outer flow (or free surface) The layer (of thickness ) in which velocities change from zero at the boundary to a velocity that is unaffected by the boundary is likely the water depth for river flow. is a few tens of meters for currents at the seafloor
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Shear stress in a fluid = shear stress = = force area rate of change of momentum area Shear stresses at the seabed lead to sediment transport
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The inner region (viscous sublayer) Only ~ 1-5 mm thick In this layer the flow is laminar so the molecular kinematic viscosity must be used Unfortunately the inner layer it is too thin for practical field measurements to determine directly
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The log (turbulent intermediate) layer Generally from about 1-5 mm to 0.1 (a few meters) above bed Dominated by turbulent eddies Can be represented by: where e is “turbulent eddy viscosity” This layer is thick enough to make measurements and fortunately the balance of forces requires that the shear stresses are the same in this layer as in the inner region
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Shear velocity u * Sediment dynamicists define a quantity known as the characteristic shear velocity, u * The simplest model for the eddy viscosity is Prandtl’s model which states that Turbulent motions (and therefore e ) are constrained to be proportional to the distance to the bed z, with the constant, , the von Karman constant which has a value of 0.4
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Velocity distribution of natural (rough) boundary layers z 0 is a constant of integration. It is sometimes called the roughness length because it is generally proportional to the particles that generate roughness of the bed (usually z 0 = 30D) From the equations on the previous slide we get Integrating this yields
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What the log-layer actually looks like Plot ln(z) against the mean velocity u to estimate u * and then estimate the shear stress from Z0Z0 lnz 0 Slope = /u * = /u *
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Shields Stress When will transport occur and by what mechanism
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Shields stress and the critical shear stress The Shields stress, or Shields parameter, is: Shields (1936) first proposed an empirical relationship to find c, the critical Shields shear stress to induce motion, as a function of the particle Reynolds number, Re p = u * D/
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Shields curve (after Miller et al., 1977) - Based on empirical observations Sediment Transport No Transport Transitional
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Initiation of Suspension Suspension Bedload No Transport If u* > w s, (i.e., shear velocity > Stokes settling velocity) then material will be suspended. Transitional transport mechanism. Compare u* and w s
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