- •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
3.7. IMPORTANT CONCEPTS |
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heard in the sound channel near Bermuda, nearly halfway around the world. Later experiment showed that 57-Hz signals transmitted in the sound channel near Heard Island (75◦E, 53◦S) could be heard at Bermuda in the Atlantic and at Monterey, California in the Pacific (Munk et al. 1994).
Use of Sound Because low frequency sound can be heard at great distances, the US Navy, in the 1950s, placed arrays of microphones on the sea floor in deep and shallow water and connected them to shore stations. The Sound Surveillance System sosus, although designed to track submarines, has found many other uses. It has been used to listen to and track whales up to 1,700 km away, and to find the location of sub-sea volcanic eruptions.
3.7Important Concepts
1.If the ocean were scaled down to a width of 8 inches it would have depths about the same as the thickness of a piece of paper. As a result, the velocity field in the ocean is nearly 2-dimensional. Vertical velocities are much smaller than horizontal velocities.
2.There are only three o cial ocean.
3.The volume of ocean water exceeds the capacity of the ocean basins, and the ocean overflows on to the continents creating continental shelves.
4.The depths of the ocean are mapped by echo sounders which measure the time required for a sound pulse to travel from the surface to the bottom and back. Depths measured by ship-based echo sounders have been used to produce maps of the sea floor. The maps have poor horizontal resolution in some regions because the regions were seldom visited by ships and ship tracks are far apart.
5.The depths of the ocean are also measured by satellite altimeter systems which profile the shape of the sea surface. The local shape of the surface is influenced by changes in gravity due to sub-sea features. Recent maps based on satellite altimeter measurements of the shape of the sea surface combined with ship data have depth accuracy of ±100 m and horizontal resolutions of ±3 km.
6.Typical sound speed in the ocean is 1480 m/s. Speed depends primarily on temperature, less on pressure, and very little on salinity. The variability of sound speed as a function of pressure and temperature produces a horizontal sound channel in the ocean. Sound in the channel can travel great distances. Low-frequency sounds below 500 Hz can travel halfway around the world provided the path is not interrupted by land.
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CHAPTER 3. THE PHYSICAL SETTING |
Chapter 4
Atmospheric Influences
The sun and the atmosphere drive directly or indirectly almost all dynamical processes in the ocean. The dominant external sources and sinks of energy are sunlight, evaporation, infrared emissions from the sea surface, and sensible heating of the sea by warm or cold winds. Winds drive the ocean’s surface circulation down to depths of around a kilometer. Wind and tidal mixing drive the deeper currents in the ocean.
The ocean, in turn, is the dominant source of heat that drives the atmospheric circulation. The uneven distribution of heat loss and gain by the ocean leads to winds in the atmosphere. Sunlight warms the tropical ocean, which evaporate, transferring heat in the form of water vapor to the atmosphere. The heat is released when the vapor condenses as rain. Winds and ocean currents carry heat poleward, where it is lost to space.
Because the atmosphere drives the ocean, and the ocean drives the atmosphere, we must consider the ocean and the atmosphere as a coupled dynamic system. In this chapter we will look mainly at the exchange of momentum between the atmosphere and the ocean. In the next chapter, we will look at heat exchanges. In chapter 14 we will look at how the ocean and the atmosphere interact in the Pacific to produce El Ni˜no.
4.1The Earth in Space
Earth’s orbit about the sun is nearly circular at a mean distance of 1.5 ×108 km. The eccentricity of the orbit is small, 0.0168. Thus earth is 3.4% further from the Sun at aphelion than at perihelion, the time of closest approach to the sun. Perihelion occurs every year in January, and the exact time changes by about 20 minutes per year. In 1995, it occurred on 3 January. Earth’s axis of rotation is inclined 23.45◦ to the plane of earth’s orbit around the sun (figure 4.1). The orientation is such that the sun is directly overhead at the Equator on the vernal and autumnal equinoxes, which occur on or about 21 March and 21 September each year.
The latitudes of 23.45◦ North and South are the Tropics of Cancer and Capricorn respectively. The tropics lie equatorward of these latitudes. As a
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CHAPTER 4. |
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Figure 4.1 The earth in space. The ellipticity of earth’s orbit around the sun and the tilt of earth’s axis of rotation relative to the plane of earth orbit leads to an unequal distribution of heating and to the seasons. Earth is closest to the sun at perihelion.
result of the eccentricity of earth’s orbit, maximum solar insolation averaged over the surface of the earth occurs in early January each year. As a result of the inclination of earth’s axis of rotation, the maximum insolation at any location outside the tropics occurs around 21 June in the northern hemisphere, and around 21 December in the southern hemisphere.
Annual Wind Speed and Sea Level Pressure (hPa) For 1989
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Figure 4.2 Map of mean annual wind velocity calculated from Trenberth et al. (1990) and sea-level pressure for 1989 from the nasa Goddard Space Flight Center’s Data Assimilation O ce (Schubert et al. 1993). The winds near 140◦W in the equatorial Pacific are about 8 m/s.