Etudes et évaluation de processus océaniques par des hiérarchies ...

Etudes et évaluation de processus océaniques par des hiérarchies ... Etudes et évaluation de processus océaniques par des hiérarchies ...

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236 62 CHAPTER 10. PENETRATION OF SURFACE FLUXES 10.6 Gravity Currents tel-00545911, version 1 - 13 Dec 2010 Gravity currents are currents that evolve due to their different density with respect to the surrounding water masses. We can thus distinguish buoyant gravity currents and dense gravity currents. Buoyant gravity currents are lighter than the surrounding and are thus confined to the surface, an example is fresh river water that enters the ocean. Dense gravity currents on the contrary are composed of water heavier than the surrounding and they thus flow along the topography. Important examples are dense currents that pass through straits (Gibraltar, Denmark, ...) and flow down the continental slopes. We will here consider only the case of dense gravity currents. When a dense gravity current leaves a strait it is deviated to the right by the Coriolis force and flows along the slope of the topography. When we neglect friction, mixing and entrainment (see section 10.5), the parameters determining the dynamics of the gravity current are the reduced gravity g ′ = g∆ρ/ρ the slope α and the Coriolis parameter f. α ⊗ F g ′ ✾ F c ′ ✿ ✲ F g F c Figure ❄10.3: Force balance in gravity currents F g = mg ′ , F ′ g = mg ′ sin α, (10.26) F c = mfu, F ′ c = mfu cos α. (10.27) If we suppose that the gravity current is in a stationary state, the buoyancy force and the Coriolis force projected on the slope have to balance, that is F ′ g ′ = F ′ c (see Fig. 10.6) and thus, u Nof = g′ tanα, (10.28) f which is called the Nof-speed. Exercise 61: What happens when we include bottom friction in the force balance? Exercise 62: What happens when we include entrainment in the dynamics (see section 10.5)?

237 Chapter 11 Solution of Exercises tel-00545911, version 1 - 13 Dec 2010 Exercise 11: The energy of a fluid of density ρ between the two points a and b in a channel of width L is composed of kinetic energy: ∫ b H E kin = ρL a 2 u2 dx, (11.1) and potential energy: ∫ b g E pot = ρL a 2 η2 dx. (11.2) The change of the total energy with time is thus: ∫ b ( ) H ∂ t E total = ∂ t E kin + ∂ t E pot = ρL a 2 ∂ t(u 2 )dx + g∂ t η 2 dx = ∫ b ( ρL − H 2 gu∂ xη − g ) 2 Hη∂ xu dx = −ρL gH ∫ b ∂ x (ηu)dx = −ρL gH 2 2 a a (u(b)η(b) − u(a)η(a)). (11.3) Where we have used eq.5.23 and 5.24. So energy is conserved in the domain [a,b] with the exception of energy entering or leaving at the boundary points. Exercise 12: Yes, the the typical velocity in a Tsunami in deep waters is less than 0.1m/s and its horizontal extension is of the order of 100km so the nonlinear term u∂ x u < 10 −7 m 2 s −1 much less than g∂ x η ≈ 10 −4 m 2 s −1 . Exercise 13: d = ∂ x u + ∂ y v = −∂ xy Ψ + ∂ yx Ψ = 0 Exercise 14: ξ = ∂ x v − ∂ y u = ∂ xx Ψ + ∂ yy Ψ = ∇ 2 Ψ 63

236<br />

62 CHAPTER 10. PENETRATION OF SURFACE FLUXES<br />

10.6 Gravity Currents<br />

tel-00545911, version 1 - 13 Dec 2010<br />

Gravity currents are currents that evolve due to their different <strong>de</strong>nsity with respect to the<br />

surrounding water masses. We can thus distinguish buoyant gravity currents and <strong>de</strong>nse gravity<br />

currents.<br />

Buoyant gravity currents are lighter than the surrounding and are thus confined to the<br />

surface, an example is fresh river water that enters the ocean. Dense gravity currents on<br />

the contrary are composed of water heavier than the surrounding and they thus flow along<br />

the topography. Important examples are <strong>de</strong>nse currents that pass through straits (Gibraltar,<br />

Denmark, ...) and flow down the continental slopes. We will here consi<strong>de</strong>r only the case of<br />

<strong>de</strong>nse gravity currents.<br />

When a <strong>de</strong>nse gravity current leaves a strait it is <strong>de</strong>viated to the right by the Coriolis force<br />

and flows along the slope of the topography. When we neglect friction, mixing and entrainment<br />

(see section 10.5), the <strong>par</strong>am<strong>et</strong>ers d<strong>et</strong>ermining the dynamics of the gravity current are the<br />

reduced gravity g ′ = g∆ρ/ρ the slope α and the Coriolis <strong>par</strong>am<strong>et</strong>er f.<br />

α<br />

⊗<br />

F g<br />

′ ✾<br />

F c<br />

′ ✿<br />

✲<br />

F g<br />

F c<br />

Figure ❄10.3: Force balance in gravity currents<br />

F g = mg ′ , F ′ g = mg ′ sin α, (10.26)<br />

F c = mfu, F ′ c = mfu cos α. (10.27)<br />

If we suppose that the gravity current is in a stationary state, the buoyancy force and the<br />

Coriolis force projected on the slope have to balance, that is F ′ g ′ = F ′ c (see Fig. 10.6) and thus,<br />

u Nof = g′<br />

tanα, (10.28)<br />

f<br />

which is called the Nof-speed.<br />

Exercise 61: What happens when we inclu<strong>de</strong> bottom friction in the force balance?<br />

Exercise 62: What happens when we inclu<strong>de</strong> entrainment in the dynamics (see section 10.5)?

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