Density Currents and Stratified Flow Environmental Hydraulics Density Currents and Stratification Already small differences in density give rise to stratification in receiving waters. Stable conditions develop, associated with water motion. ⇒ Reduced exchange between layers ⇒ Consequences for water quality Causes of density differences: • Temperature • Salinity • Suspended matter 1 Characterization of density differences: σ= ρ − ρo ρo Example: 0 oC – 1 oC => Δσ=0.06 10oC – 11oC => Δσ=-0.10 20oC – 21oC => Δσ=-0.21 Density varies approximately linearly with salinity: 0.1% => Δσ=0.80 (independent of temperature) Classification of Stratified Flow • surface flow • bottom flow • inter flow Interface between layers: Thermocline - temperature Halocline - salinity Lutocline - suspended solids Saltwater wedge 2 Net Force due to Density Difference Water volume with density r1 in an ambient with density r2. ρ1 gV Gravity: Buoyancy: ρ 2 gV Net force: ( ρ1 − ρ2 ) gV = ρ1 Reduced acceleration due to gravity: g'= ( ρ1 − ρ2 ) ( ρ1 − ρ2 ) ρ1 ρ1 gV = ρ1 g 'V g Froude Densimetric Number U Fd = g ( ρ1 − ρ2 ) y = momentum buoyancy ρ1 U and y velocity and length scale, respectively Example: Jet discharge U = exit velocity y = D = exit diameter 3 Example of Stratified Flows • wind setup and associated displacement of density interface (e.g., lake) • saltwater wedge in a river mouth Inclination of Water Surface due to Wind Force balance: ρw g 2 h − ρw g 2 (h + dh dx) 2 dx + (τ0 + τb ) dx = 0 2 4 Resulting in: dh τ0 + τb = dx ρ w gh Receiving water with constant depth and length: Δh = τ 0 + τb L ρ w gh Assume that τ0 τb and Δh = τo = CDρair w102 CDρair w102 L ρw gh Numerical Example h = 10 m w10 = 10 m/s CD = 1.3 · 10-3 L = 10 km Which gives a maximum wind setup of: Δh = 1.3 ⋅10−3 ⋅ 1.3 1 102 ⋅104 ⋅ ⋅ = 0.016 m 1000 9.81 10 5 Inclination of Density Interface Surface inclination is small but a compensating tilt in the density interface becomes large. Force balance (neglecting water movement and associated shear stresses): dh2 dh ρ1 =− 1 dx dx ρ 2 − ρ1 Numerical Example ρ1 = 998.2 kg/m3 (20 0C) ρ2 = 1000 kg/m3 (4 0C) dh1 = 10 −6 dx These values yield: dh2 1000 = −10 −6 ⋅ = −0.5 ⋅10−3 dx 1000 − 998.2 With L = 1 km one obtains Δh2 ≈ 0.5 m, whereas the water surface only rises Δh1 = 0.001 m 6 Saltwater Wedge Assume no mixing at interface. Constant velocity along the verticals. Slope of the energy line: S =− d ⎛ U2 ⎞ z + y + y + 2 1 ⎜ ⎟ dx ⎝ 2g ⎠ Definitions: U= q q2 dz , F12 = 3 , So = − y1 gy1 dx Introduce definitions in the equation yields: dy2 dy + (1 − F12 ) 1 = So − S dx dx Steady-state conditions are assumed => net force is zero τi − y 2 dpo + ρ2 gy2 sin φ = 0 dx po = ρ1 gy1 + ρ2 gy2 (pressure at bottom) 7 Shear stress at interface: τi = ρ1 gSy1 Introduce into force balance: S y1 dy1 ρ2 dy2 ρ2 = + − So y2 dx ρ1 dx ρ1 ρ1 y1 dy1 ρ 2 y2 = −S ρ dx 1 − 1 − F12 ρ2 1+ Combine equations: (Equation to determine the shape of the saltwater wedge) y2 is small at the front and dy1/dx < 0. Salt water penetration may only occur if: F12 < ρ2 − ρ1 ρ2 If y2 -> 0, F1 -> Fo and: 1/ 2 ⎛ρ −ρ ⎞ Fo < ⎜ 2 1 ⎟ ⎝ ρ2 ⎠ 8 Numerical example: r1 = 1000 kg/m3 r2 = 1029 kg/m3 => ⎛ 1029 − 1000 ⎞ Fo < ⎜ ⎟ ⎝ 1029 ⎠ 1/ 2 = 0.17 Thus, if Fo > 0.17 there is no risk of a salt water wedge forming. In order to determine the shape of the salt water wedge using the previous equation, a boundary condition is needed at the river mouth: U = g ' y1 Density Interface Large density variation over short vertical distance. Prevents vertical exchange of water. Mixing across interface needs supply of energy (mixing implies increase in the potential energy of the system). The Richardson number characterizes the ability of the interface to prevent mixing: ∂u ∂ρ Ri = − g / ρ ⎛⎜ ⎞⎟ ∂z ⎝ ∂z ⎠ 2 (simpler definition of Ri yields: Ri = 1 Fo2 ) 9 Density Interface Development 0 Water Depth (m) -5 -10 Month FEB -15 APR JUN AUG OCT -20 DEC -25 4 8 12 16 20 24 Water Temperature (degrees) Many laboratory experiments on mixed-layer depening Temperature distribution Nainital Lake rinitial rmixed Internal Waves Similar governing equations as for surface waves, if g is replaced by g’. Additional considerations: • effect of the upper layer (inertia etc) • shear stresses at the interface • thickness of the interface Lake Biwa, Japan 10 Internal Waves in the Ocean Straits of Gibraltar Sulu Sea Breaking of Internal Waves Breaking generates substantial mixing In the atmosphere Laboratory experiments 11
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