- •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
6.11. IMPORTANT CONCEPTS |
101 |
The total radiance Lt received by an instrument in space is:
Lt(λi ) = t(λi)LW (λi ) + Lr (λi) + La(λi ) |
(6.15) |
where λi is the wavelength of the radiation in the band measured by the instrument, LW is the radiance leaving the sea surface, Lr is radiance scattered by molecules, called the Rayleigh radiance, La is radiance scattered from aerosols, and t is the transmittance of the atmosphere. Lr can be calculated from theory, and La can be calculated from the amount of red light received at the instrument because very little red light is reflected from the water. Therefore LW can be calculated from the radiance measured at the spacecraft.
Chlorophyll concentration in the water column is calculated from the ratio of LW at two frequencies. Using data from the Coastal Zone Color Scanner, Gordon et al. (1983) proposed
|
|
|
LW (443) |
|
−1.71 |
C13 |
=1.1298 |
|
(6.16a) |
||
LW (550) |
|||||
C23 |
=3.3266 |
|
LW (520) |
|
−2.40 |
|
(6.16b) |
||||
LW (550) |
where C is the chlorophyll concentration in the surface layers in mg pigment/m3, and LW (443), LW (520), andLW (550) is the radiance at wavelengths of 443, 520, and 550 nm. C13 is used when C13 ≤ 1.5 mg/m3, otherwise C23 is used.
The technique is used to calculate chlorophyll concentration within a factor of 50% over a wide range of concentrations from 0.01 to 10 mg/m3.
6.11Important Concepts
1.Density in the ocean is determined by temperature, salinity, and pressure.
2.Density changes in the ocean are very small, and studies of water masses and currents require density with an accuracy of 10 parts per million.
3.Density is not measured, it is calculated from measurements of temperature, salinity, and pressure using the equation of state of sea water.
4.Accurate calculations of density require accurate definitions of temperature and salinity and an accurate equation of state.
5.Salinity is di cult to define and to measure. To avoid the di culty, oceanographers use conductivity instead of salinity. They measure conductivity and calculate density from temperature, conductivity, and pressure.
6.A mixed layer of constant temperature and salinity is usually found in the top 1–100 meters of the ocean. The depth is determined by wind speed and the flux of heat through the sea surface.
7.To compare temperature and density of water masses at di erent depths in the ocean, oceanographers use potential temperature and potential density which remove most of the influence of pressure on density.
8.Water parcels below the mixed layer move along neutral surfaces.
102CHAPTER 6. TEMPERATURE, SALINITY, AND DENSITY
9.Surface temperature of the ocean was usually measured at sea using bucket or injection temperatures. Global maps of temperature combine these observations with observations of infrared radiance from the sea surface measured by an avhrr in space.
10.Temperature and conductivity are usually measured digitally as a function of pressure using a ctd. Before 1960–1970 the salinity and temperature were measured at roughly 20 depths using Nansen bottles lowered on a line from a ship. The bottles carried reversing thermometers which recorded temperature and depth and they returned a water sample from that depth which was used to determine salinity on board the ship.
11.Light is rapidly absorbed in the ocean. 95% of sunlight is absorbed in the upper 100 m of the clearest sea water. Sunlight rarely penetrates deeper than a few meters in turbid coastal waters.
12.Phytoplankton change the color of sea water, and the change in color can be observed from space. Water color is used to measure phytoplankton concentration from space.
Chapter 7
Some Mathematics: The
Equations of Motion
In this chapter I consider the response of a fluid to internal and external forces. This leads to a derivation of some of the basic equations describing ocean dynamics. In the next chapter, we will consider the influence of viscosity, and in chapter 12 we will consider the consequences of vorticity.
Fluid mechanics used in oceanography is based on Newtonian mechanics modified by our evolving understanding of turbulence. Conservation of mass, momentum, angular momentum, and energy lead to particular equations having names that hide their origins (table 7.1).
Table 7.1 Conservation Laws Leading to Basic Equations of Fluid Motion
Conservation of Mass: |
Leads to Continuity Equation. |
Conservation of Energy: |
Conservation of heat leads to Heat Budgets. |
|
Conservation of mechanical energy leads to |
|
Wave Equation. |
Conservation of Momentum: |
Leads to Momentum (Navier-Stokes) Eq. |
Conservation of Angular Momentum: |
Leads to Conservation of Vorticity. |
7.1Dominant Forces for Ocean Dynamics
Only a few forces are important in physical oceanography: gravity, friction, and Coriolis (table 7.2). Remember that forces are vectors. They have magnitude and direction.
1.Gravity is the dominant force. The weight of the water in the ocean produces pressure. Changes in gravity, due to the motion of sun and moon relative to earth produces tides, tidal currents, and tidal mixing in the interior of the ocean.
Buoyancy is the upward or downward force due to gravity acting on a parcel of water that is more or less dense than other water at its level. For example, cold air blowing over the sea cools surface waters causing them
103
104 |
CHAPTER 7. THE EQUATIONS OF MOTION |
to be more dense than the water beneath. Gravity acting on the di erence in density results in a force that causes the water to sink.
Horizontal pressure gradients are due to the varying weight of water in di erent regions of the ocean.
2.Friction is the force acting on a body as it moves past another body while in contact with that body. The bodies can be parcels of water or air.
Wind stress is the friction due to wind blowing across the sea surface. It transfers horizontal momentum to the sea, creating currents. Wind blowing over waves on the sea surface leads to an uneven distribution of pressure over the waves. The pressure distribution transfers energy to the waves, causing them to grow into bigger waves.
3.Pseudo-forces are apparent forces that arise from motion in curvilinear or rotating coordinate systems. For example, Newton’s first law states that there is no change in motion of a body unless a resultant force acts on it. Yet a body moving at constant velocity seems to change direction when viewed from a rotating coordinate system. The change in direction is due to a pseudo-force, the Coriolis force.
Coriolis Force is the dominant pseudo-force influencing motion in a coordinate system fixed to the earth.
Table 7.2 Forces in Geophysical Fluid Dynamics
Dominant Forces |
|
Gravity |
Gives rise to pressure gradients, buoyancy, and tides. |
Coriolis |
Results from motion in a rotating coordinate system |
Friction |
Is due to relative motion between two fluid parcels. |
|
Wind stress is an important frictional force. |
Other Forces |
|
Atmospheric Pressure |
Results in inverted barometer e ect. |
Seismic |
Results in tsunamis driven by earthquakes. |
Note that the last two forces are much less important than the first three.
7.2Coordinate System
Coordinate systems allow us to find locations in theory and practice. Various systems are used depending on the size of the features to be described or mapped. I will refer to the simplest systems; descriptions of other systems can be found in geography and geodesy books.
1.Cartesian Coordinate System is the one I will use most commonly in the following chapters to keep the discussion as simple as possible. We can describe most processes in Cartesian coordinates without the mathematical complexity of spherical coordinates. The standard convention in geophysical fluid mechanics is x is to the east, y is to the north, and z is up.
f-Plane is a Cartesian coordinate system in which the Coriolis force is assumed constant. It is useful for describing flow in regions small compared with the radius of the earth and larger than a few tens of kilometers.