- •Preface
- •1 A Voyage of Discovery
- •1.2 Goals
- •1.3 Organization
- •1.4 The Big Picture
- •1.5 Further Reading
- •2 The Historical Setting
- •2.2 Eras of Oceanographic Exploration
- •2.3 Milestones in the Understanding of the Ocean
- •2.4 Evolution of some Theoretical Ideas
- •2.5 The Role of Observations in Oceanography
- •2.6 Important Concepts
- •3 The Physical Setting
- •3.1 Ocean and Seas
- •3.2 Dimensions of the ocean
- •3.3 Sea-Floor Features
- •3.4 Measuring the Depth of the Ocean
- •3.5 Sea Floor Charts and Data Sets
- •3.6 Sound in the Ocean
- •3.7 Important Concepts
- •4.1 The Earth in Space
- •4.2 Atmospheric Wind Systems
- •4.3 The Planetary Boundary Layer
- •4.4 Measurement of Wind
- •4.5 Calculations of Wind
- •4.6 Wind Stress
- •4.7 Important Concepts
- •5 The Oceanic Heat Budget
- •5.1 The Oceanic Heat Budget
- •5.2 Heat-Budget Terms
- •5.3 Direct Calculation of Fluxes
- •5.4 Indirect Calculation of Fluxes: Bulk Formulas
- •5.5 Global Data Sets for Fluxes
- •5.6 Geographic Distribution of Terms
- •5.7 Meridional Heat Transport
- •5.8 Variations in Solar Constant
- •5.9 Important Concepts
- •6.2 Definition of Temperature
- •6.4 The Oceanic Mixed Layer and Thermocline
- •6.5 Density
- •6.6 Measurement of Temperature
- •6.7 Measurement of Conductivity or Salinity
- •6.8 Measurement of Pressure
- •6.10 Light in the Ocean and Absorption of Light
- •6.11 Important Concepts
- •7.1 Dominant Forces for Ocean Dynamics
- •7.2 Coordinate System
- •7.3 Types of Flow in the ocean
- •7.4 Conservation of Mass and Salt
- •7.5 The Total Derivative (D/Dt)
- •7.6 Momentum Equation
- •7.7 Conservation of Mass: The Continuity Equation
- •7.8 Solutions to the Equations of Motion
- •7.9 Important Concepts
- •8.2 Turbulence
- •8.3 Calculation of Reynolds Stress:
- •8.4 Mixing in the Ocean
- •8.5 Stability
- •8.6 Important Concepts
- •9 Response of the Upper Ocean to Winds
- •9.1 Inertial Motion
- •9.2 Ekman Layer at the Sea Surface
- •9.3 Ekman Mass Transport
- •9.4 Application of Ekman Theory
- •9.5 Langmuir Circulation
- •9.6 Important Concepts
- •10 Geostrophic Currents
- •10.1 Hydrostatic Equilibrium
- •10.2 Geostrophic Equations
- •10.3 Surface Geostrophic Currents From Altimetry
- •10.4 Geostrophic Currents From Hydrography
- •10.5 An Example Using Hydrographic Data
- •10.6 Comments on Geostrophic Currents
- •10.7 Currents From Hydrographic Sections
- •10.8 Lagrangian Measurements of Currents
- •10.9 Eulerian Measurements
- •10.10 Important Concepts
- •11.2 Western Boundary Currents
- •11.4 Observed Surface Circulation in the Atlantic
- •11.5 Important Concepts
- •12 Vorticity in the Ocean
- •12.2 Conservation of Vorticity
- •12.4 Vorticity and Ekman Pumping
- •12.5 Important Concepts
- •13.2 Importance of the Deep Circulation
- •13.3 Theory for the Deep Circulation
- •13.4 Observations of the Deep Circulation
- •13.5 Antarctic Circumpolar Current
- •13.6 Important Concepts
- •14 Equatorial Processes
- •14.1 Equatorial Processes
- •14.6 Important Concepts
- •15 Numerical Models
- •15.2 Numerical Models in Oceanography
- •15.3 Global Ocean Models
- •15.4 Coastal Models
- •15.5 Assimilation Models
- •15.6 Coupled Ocean and Atmosphere Models
- •15.7 Important Concepts
- •16 Ocean Waves
- •16.1 Linear Theory of Ocean Surface Waves
- •16.2 Nonlinear waves
- •16.3 Waves and the Concept of a Wave Spectrum
- •16.5 Wave Forecasting
- •16.6 Measurement of Waves
- •16.7 Important Concepts
- •17 Coastal Processes and Tides
- •17.1 Shoaling Waves and Coastal Processes
- •17.2 Tsunamis
- •17.3 Storm Surges
- •17.4 Theory of Ocean Tides
- •17.5 Tidal Prediction
- •17.6 Important Concepts
- •References
9.5. LANGMUIR CIRCULATION
of the Ekman flow must be zero. Therefore:
∂MEx |
+ |
∂MEy |
= −ρ wE |
(0) |
|
|
∂x |
∂y |
|||
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H · ME = −ρ wE (0) |
|
147
(9.28a)
(9.28b)
Where ME is the vector mass transport due to Ekman flow in the upper boundary layer of the ocean, and H is the horizontal divergence operator. (9.28) states that the horizontal divergence of the Ekman transports leads to a vertical velocity in the upper boundary layer of the ocean, a process called Ekman Pumping.
If we use the Ekman mass transports (9.26) in (9.28) we can relate Ekman pumping to the wind stress.
wE (0) |
= −ρ |
∂x |
|
f |
− |
∂y |
f |
|
(9.29a) |
|||||
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1 |
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|
∂ |
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Tyz |
(0) |
|
∂ |
Txz (0) |
|
|
|
wE (0) |
= −curlz |
T |
|
|
|
|
|
|
(9.29b) |
|||||
|
|
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|||||||||
ρ f |
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|
|
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|
where T is the vector wind stress and the subscript z indicates the vertical component of the curl.
The vertical velocity at the sea surface w(0) must be zero because the surface cannot rise into the air, so wE (0) must be balanced by another vertical velocity. We will see in Chapter 12 that it is balanced by a geostrophic velocity wG(0) at the top of the interior flow in the ocean.
Note that the derivation above follows Pedlosky (1996: 13), and it di ers from the traditional approach that leads to a vertical velocity at the base of the Ekman layer. Pedlosky points out that if the Ekman layer is very thin compared with the depth of the ocean, it makes no di erence whether the velocity is calculated at the top or bottom of the Ekman layer, but this is usually not true for the ocean. Hence, we must compute vertical velocity at the top of the layer.
9.5Langmuir Circulation
Measurements of surface currents show that winds generate more than Ekman and inertial currents at the sea surface. They also generate a Langmuir circulation (Langmuir, 1938), a current that spiral around an axis parallel to the wind direction. Weller et al. (1985) observed such a flow during an experiment to measure the wind-driven circulation in the upper 50 meters of the sea. They found that during a period when the wind speed was 14 m/s, surface currents were organized into Langmuir cells spaced 20 m apart, the cells were aligned at an angle of 15◦ to the right of the wind, and vertical velocity at 23 m depth was concentrated in narrow jets under the areas of surface convergence (figure 9.9). Maximum vertical velocity was −0.18 m/s. The seasonal thermocline was at 50 m, and no downward velocity was observed in or below the thermocline.
9.6Important Concepts
1.Changes in wind stress produce transient oscillations in the ocean called inertial currents
148 CHAPTER 9. RESPONSE OF THE UPPER OCEAN TO WINDS
T
W
10 U
20
V
10
10 |
0 |
|
-10
-20
Figure 9.9 A three-dimensional view of the Langmuir circulation at the surface of the Pacific observed from the Floating Instrument Platform flip. The heavy dashed line on the sea surface indicate lines of convergence marked by cards on the surface. Vertical arrows are individual values of vertical velocity measured every 14 seconds at 23 m depth as the platform drifted through the Langmuir currents. Horizontal arrows, which are drawn on the surface for clarity, are values of horizontal velocity at 23 m. The broad arrow gives the direction of the wind. After Weller et al. (1985).
(a)Inertial currents are very common in the ocean.
(b)The period of the current is (2π)/f .
2.Steady winds produce a thin boundary layer, the Ekman layer, at the top of the ocean. Ekman boundary layers also exist at the bottom of the ocean and the atmosphere. The Ekman layer in the atmosphere above the sea surface is called the planetary boundary layer.
3.The Ekman layer at the sea surface has the following characteristics:
(a)Direction: 45◦to the right of the wind looking downwind in the Northern Hemisphere.
(b)Surface Speed : 1–2.5% of wind speed depending on latitude.
(c)Depth: approximately 40–300 m depending on latitude and wind velocity.
4.Careful measurements of currents near the sea surface show that:
(a)Inertial oscillations are the largest component of the current in the mixed layer.
(b)The flow is nearly independent of depth within the mixed layer for periods near the inertial period. Thus the mixed layer moves like a slab at the inertial period.
(c)An Ekman layer exists in the atmosphere just above the sea (and
land) surface.
9.6. IMPORTANT CONCEPTS |
149 |
(d)Surface drifters tend to drift parallel to lines of constant atmospheric pressure at the sea surface. This is consistent with Ekman’s theory.
(e)The flow averaged over many inertial periods is almost exactly that calculated from Ekman’s theory.
5.Transport is 90◦ to the right of the wind in the northern hemisphere.
6.Spatial variability of Ekman transport, due to spatial variability of winds over distances of hundreds of kilometers and days, leads to convergence and divergence of the transport.
(a)Winds blowing toward the equator along west coasts of continents produces upwelling along the coast. This leads to cold, productive waters within about 100 km of the shore.
(b)Upwelled water along west coasts of continents modifies the weather along the west coasts.
7.Ekman pumping, which is driven by spatial variability of winds, drives a vertical current, which drives the interior geostrophic circulation of the ocean.
150 CHAPTER 9. RESPONSE OF THE UPPER OCEAN TO WINDS