- •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
70 |
CHAPTER 5. THE OCEANIC HEAT BUDGET |
3.The di erence between insolation and net infrared radiation is the net heat flux across the top of the atmosphere.
Net Meridional Heat Transport To calculate the meridional heat transport in the atmosphere and the ocean, we first average the net heat flux through the top of the atmosphere in a zonal band. Because the meridional derivative of the transport is the zonal-mean flux, we calculate the transport from the meridional integral of the zonal-mean flux. The integral must be balanced by the heat transported by the atmosphere and the ocean across each latitude band.
Calculations by Trenberth and Caron (2001) show that the total, annualmean, meridional heat transport by the ocean and atmosphere peaks at 6 PW toward each pole at 35◦ latitude.
Oceanic Heat Transport The meridional heat transport in the ocean can be calculated three ways:
1.Surface Flux Method calculates the heat flux through the sea surface from measurements of wind, insolation, air, and sea temperature, and cloudiness. The fluxes are integrated to obtain the zonal average of the heat flux (figure 5.7). Finally, we calculate the transport from the meridional integral of the zonal-mean flux just as we did at the top of the atmosphere.
2.Direct Method calculates the heat transport from values of current velocity and temperature measured from top to bottom along a zonal section spanning an ocean basin. The flux is the product of northward velocity and heat content derived from the temperature measurement.
3.Residual Method first calculates the atmospheric heat transport from atmospheric measurements or the output of numerical weather models. This is the direct method applied to the atmosphere. The atmospheric transport is subtracted from the total meridional transport calculated from the top-of-the-atmosphere heat flux to obtain the oceanic contribution as a residual (figure 5.11).
Various calculations of oceanic heat transports, such as those shown in figure 5.11, tend to be in agreement, and the error bars shown in the figure are realistic. The total meridional transport of heat by the ocean is small compared with the total meridional heat transport by the atmosphere except in the tropics. At 35◦, where the total meridional heat transport is greatest, the ocean carries only 22% of the heat in the northern hemisphere, and 8% in the southern (Trenberth and Caron, 2001).
5.8Variations in Solar Constant
We have assumed so far that the solar constant, the output of light and heat from the sun, is steady. Recent evidence based on variability of sunspots and faculae (bright spots) shows that the output varied by ±0.2% over centuries (Lean, Beer, and Bradley, 1995), and that this variability is correlated with changes in global mean temperature of earth’s surface of ±0.4◦C. (figure 5.12). In addition, White and Cayan (1998) found a small 12 yr, 22 yr, and longerperiod variations of sea-surface temperature measured by bathythermographs
5.8. VARIATIONS IN SOLAR CONSTANT |
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Figure 5.11 Northward heat transport for 1988 in each ocean and the total transport summed over all ocean calculated by the residual method using atmospheric heat transport from ecmwf and top of the atmosphere heat fluxes from the Earth Radiation Budget Experiment satellite. After Houghton et al. (1996: 212), which used data from Trenberth and Solomon (1994). 1 PW = 1 petawatt = 1015 W.
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Figure 5.12 Changes in solar constant (total solar irradiance) and global mean temperature of earth’s surface over the past 400 years. Except for a period of enhanced volcanic activity in the early 19th century, surface temperature is well correlated with solar variability. After Lean, personal communication.
72 |
CHAPTER 5. THE OCEANIC HEAT BUDGET |
and ship-board thermometers over the past century. The observed response of earth to solar variability is about that calculated from numerical models of the coupled ocean-atmosphere climate system. Many other changes in climate and weather have been attributed to solar variability. The correlations are somewhat controversial, and much more information can be found in Hoyt and Schatten’s (1997) book on the subject.
5.9Important Concepts
1.Sunlight is absorbed primarily in the tropical ocean. The amount of sunlight changes with season, latitude, time of day, and cloud cover.
2.Most of the heat absorbed by the ocean in the tropics is released as water vapor which heats the atmosphere when water is condenses as rain. Most of the rain falls in the tropical convergence zones, lesser amounts fall in mid-latitudes near the polar front.
3.Heat released by rain and absorbed infrared radiation from the ocean are the primary drivers for the atmospheric circulation.
4.The net heat flux from the ocean is largest in mid-latitudes and o shore of Japan and New England.
5.Heat fluxes can be measured directly using fast response instruments on low-flying aircraft, but this is not useful for measuring heat fluxes over large oceanic regions.
6.Heat fluxes through large regions of the sea surface can be calculated from bulk formula. Seasonal, regional, and global maps of fluxes are available based on ship and satellite observations.
7.The most widely used data sets for studying heat fluxes are the International Comprehensive Ocean-Atmosphere Data Set and the reanalysis of meteorological data by numerical weather prediction models.
8.The atmosphere transports most of the heat needed to warm latitudes higher than 35◦. The oceanic meridional transport is comparable to the atmospheric meridional transport only in the tropics.
9.Solar output is not constant, and the observed small variations in output of heat and light from the sun seem to produce the changes in global temperature observed over the past 400 years.
Chapter 6
Temperature, Salinity, and
Density
Heat fluxes, evaporation, rain, river inflow, and freezing and melting of sea ice all influence the distribution of temperature and salinity at the ocean’s surface. Changes in temperature and salinity can increase or decrease the density of water at the surface, which can lead to convection. If water from the surface sinks into the deeper ocean, it retains a distinctive relationship between temperature and salinity which helps oceanographers track the movement of deep water. In addition, temperature, salinity, and pressure are used to calculate density. The distribution of density inside the ocean is directly related to the distribution of horizontal pressure gradients and ocean currents. For all these reasons, we need to know the distribution of temperature, salinity, and density in the ocean.
Before discussing the distribution of temperature and salinity, let’s first define what we mean by the terms, especially salinity.
6.1Definition of Salinity
At the simplest level, salinity is the total amount of dissolved material in grams in one kilogram of sea water. Thus salinity is a dimensionless quantity. It has no units. The variability of dissolved salt is very small, and we must be very careful to define salinity in ways that are accurate and practical. To better understand the need for accuracy, look at figure 6.1. Notice that the range of salinity for most of the ocean’s water is from 34.60 to 34.80 parts per thousand, which is 200 parts per million. The variability in the deep North Pacific is even smaller, about 20 parts per million. If we want to classify water with di erent salinity, we need definitions and instruments accurate to about one part per million. Notice that the range of temperature is much larger, about 1◦C, and temperature is easier to measure.
Writing a practical definition of salinity that has useful accuracy is di cult (see Lewis, 1980, for the details), and various definitions have been used.
73
74 |
CHAPTER 6. TEMPERATURE, SALINITY, AND DENSITY |
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Figure 6.1 Histogram of temperature and salinity of ocean water colder than 4◦C. Height is proportional to volume. Height of highest peak corresponds to a volume of 26 million cubic kilometers per bivariate class of 0.1◦C and 0.01. After Worthington (1981: 47).
A Simple Definition Originally salinity was defined to be the “Total amount of dissolved material in grams in one kilogram of sea water.” This is not useful because the dissolved material is almost impossible to measure in practice. For example, how do we measure volatile material like gasses? Nor can we evaporate sea-water to dryness because chlorides are lost in the last stages of drying (Sverdrup, Johnson, and Fleming, 1942: 50).
A More Complete Definition To avoid these di culties, the International Council for the Exploration of the Sea set up a commission in 1889 which recommended that salinity be defined as the “Total amount of solid materials in grams dissolved in one kilogram of sea water when all the carbonate has been converted to oxide, the bromine and iodine replaced by chlorine and all organic matter completely oxidized.” The definition was published in 1902. This is useful but di cult to use routinely.
Salinity Based on Chlorinity Because the above definition was di cult to implement in practice, because salinity is directly proportional to the amount of chlorine in sea water, and because chlorine can be measured accurately by a simple chemical analysis, salinity S was redefined using chlorinity:
S = 0.03 + 1.805 Cl |
(6.1) |
where chlorinity Cl is defined as “the mass of silver required to precipitate completely the halogens in 0.328 523 4 kg of the sea-water sample.”
As more and more accurate measurements were made, (6.1) turned out to be too inaccurate. In 1964 unesco and other international organizations appointed a Joint Panel on Oceanographic Tables and Standards to produce a
6.1. DEFINITION OF SALINITY |
75 |
more accurate definition. The Joint Panel recommended in 1966 (Wooster, Lee, and Dietrich, 1969) that salinity and chlorinity be related using:
S = 1.806 55 Cl |
(6.2) |
This is the same as (6.1) for S = 35.
Salinity Based on Conductivity At the same time (6.2) was adopted, oceanographers had began using conductivity meters to measure salinity. The meters were very precise and relatively easy to use compared with the chemical techniques used to measure chlorinity. As a result, the Joint Panel also recommended that salinity be related to conductivity of sea water using:
S = − 0.089 |
96 + 28.297 29 R15 + 12.808 32 R152 |
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0)/C(35, 15, 0) |
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where C(S, 15, 0) is the conductivity of the sea-water sample at 15◦C and atmospheric pressure, having a salinity S derived from (6.4), and C(35, 15, 0) is the conductivity of standard “Copenhagen” sea water. Millero (1996) points out that (6.3) is not a new definition of salinity, it merely gives chlorinity as a function of conductivity of seawater relative to standard seawater.
Practical Salinity Scale of 1978 By the early 1970s, accurate conductivity meters could be deployed from ships to measure conductivity at depth. The need to re-evaluate the salinity scale led the Joint Panel to recommend in 1981 (jpots, 1981; Lewis, 1980) that salinity be defined using only conductivity, breaking the link with chlorinity. All water samples with the same conductivity ratio have the same salinity even though the their chlorinity may di er.
The Practical Salinity Scale of 1978 is now the o cial definition:
S = 0.0080 − 0.1692 K151/2 + 25.3851 K15 + 14.0941 K153/2 |
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K15 = C(S, 15, 0)/C(KCl, 15, 0) |
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where C(S, 15, 0) is the conductivity of the sea-water sample at a temperature of 14.996◦C on the International Temperature Scale of 1990 (its-90, see §6.2) and standard atmospheric pressure of 101 325 Pa. C(KCl, 15, 0) is the conductivity of the standard potassium chloride (KCl) solution at a temperature of 15◦C and standard atmospheric pressure. The standard KCl solution contains a mass of 32.435 6 grams of KCl in a mass of 1.000 000 kg of solution. Millero (1996: 72) and Lewis (1980) gives equations for calculating salinity at other pressures and temperatures.
Comments The various definitions of salinity work well because the ratios of the various ions in sea water are nearly independent of salinity and location in
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CHAPTER 6. TEMPERATURE, SALINITY, AND DENSITY |
the ocean (table 6.1). Only very fresh waters, such as are found in estuaries, have significantly di erent ratios. The result is based on Dittmar’s (1884) chemical analysis of 77 samples of sea water collected by the Challenger Expedition and further studies by Carritt and Carpenter (1959).
The importance of this result cannot be over emphasized, as upon it depends the validity of the chlorinity: salinity: density relationships and, hence, the accuracy of all conclusions based on the distribution of density where the latter is determined by chemical or indirect physical methods such as electrical conductivity. . .—Sverdrup, Johnson, Fleming (1942).
The relationship between conductivity and salinity has an accuracy of around
±0.003 in salinity. The very small error is caused by variations in constituents such as SiO2 which cause small changes in density but no change in conductivity.
Table 6.1 Major Constituents of Sea Water
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Calcium |
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1.1% |
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Reference Seawater and Salinity The Practical Salinity Scale of 1978 introduced several small problems. It led to confusion about units and to the use of “practical salinity units” that are not part of the definition of Practical Salinity. In addition, absolute salinity di ers from salinity by about 0.5%. And, the composition of seawater di ers slightly from place to place in the ocean, leading to small errors in measuring salinity.
To avoid these and other problems, Millero et al (2008) defined a new measure of salinity, the Reference Salinity, that accurately represents the Absolute Salinity of an artificial seawater solution. It is based on a Reference Composition of seawater that is much more accurate than the values in Table 6.1 above. The Reference Composition of the artificial seawater is defined by a list of solutes and their mole fractions given in Table 4 of their paper. From this, they defined artificial Reference Seawater to be seawater having a Reference Composition solute dissolved in pure water as the solvent, and adjusted to its thermodynamic equilibrium state. Finally, the Reference Salinity of Reference Seawater was defined to be exactly 35.16504 g kg−1.
With these definitions, plus many details described in their paper, Millero et al (2008) show Reference Salinity is related to Practical Salinity by:
SR ≈ (35.16504/35)g kg−1 × S |
(6.5) |
The equation is exact at S = 35. Reference Salinity is approximately 0.47% larger than Practical Salinity. Reference Salinity SR is intended to be used as an SI-based extension of Practical Salinity.