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 ...
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
- Page 191 and 192: 185 3.3. θ-S DIAGRAMS 11 3.3 θ-S
- Page 193 and 194: 187 3.6. HEAT CAPACITY 13 tel-00545
- Page 195 and 196: 189 3.7. CONSERVATIVE PROPERTIES 15
- Page 197 and 198: 191 Chapter 4 Surface fluxes, the f
- Page 199 and 200: 193 4.2. FRESH WATER FLUX 19 water.
- Page 201 and 202: 195 Chapter 5 Dynamics of the Ocean
- Page 203 and 204: 197 5.2. THE LINEARIZED ONE DIMENSI
- Page 205 and 206: 199 5.4. TWO DIMENSIONAL STATIONARY
- Page 207 and 208: 201 5.6. THE CORIOLIS FORCE 27 Whic
- Page 209 and 210: 203 5.8. GEOSTROPHIC EQUILIBRIUM 29
- Page 211 and 212: 205 5.10. LINEAR POTENTIAL VORTICIT
- Page 213 and 214: 207 5.13. A FEW WORDS ABOUT WAVES 3
- Page 215 and 216: 209 Chapter 6 Gyre Circulation tel-
- Page 217 and 218: 211 6.1. SVERDRUP DYNAMICS IN THE S
- Page 219 and 220: 213 6.2. THE EKMAN LAYER 39 In the
- Page 221 and 222: 215 6.3. SVERDRUP DYNAMICS IN THE S
- Page 223 and 224: 217 Chapter 7 Multi-Layer Ocean dyn
- Page 225 and 226: 219 7.3. GEOSTROPHY IN A MULTI-LAYE
- Page 227 and 228: 221 7.5. EDDIES, BAROCLINIC INSTABI
- Page 229 and 230: 223 Chapter 8 Equatorial Dynamics t
- Page 231 and 232: 225 Chapter 9 Abyssal and Overturni
- Page 233 and 234: 227 9.2. MULTIPLE EQUILIBRIA OF THE
- Page 235 and 236: 229 9.3. WHAT DRIVES THE THERMOHALI
- Page 237 and 238: 231 Chapter 10 Penetration of Surfa
- Page 239 and 240: 233 10.2. TURBULENT TRANSPORT 59 If
- Page 241: 235 10.5. ENTRAINMENT 61 instabilit
- Page 245 and 246: 239 65 Exercise 32: The moment of i
- Page 247 and 248: 241 INDEX 67 Transport stream-funct
- Page 249 and 250: Annexe A Attestation de reussite au
- Page 251 and 252: Annexe B Rapports du jury et des ra
- Page 253 and 254: tel-00545911, version 1 - 13 Dec 20
- Page 255 and 256: tel-00545911, version 1 - 13 Dec 20
- Page 257 and 258: 251 utilisés avec pertinence. Sur
- Page 259 and 260: 253
- Page 261 and 262: tel-00545911, version 1 - 13 Dec 20
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)?