Salinity and Temperature of the Oceans
- Salinity in surface waters is controlled by currents and
temperature and averages approximately 35 parts per thousand.
- Salinity values are relatively uniform in well-mixed surface
waters of the open oceans but are
more extreme in restricted waters of coastal seas.
- Salinity and temperature change with depth with the most rapid change
occurring in a depth zone labeled the halocline.
- Ocean temperatures of 27oC are typical of tropical
surface waters and temperatures of 2oC are typical for deep ocean
waters.
- Cold water is more dense than warm water, but ice (frozen solid
water) is less dense than liquid water.
Salinity and Latitude
eawater contains dissolved salts. The concentration of salt in seawater is salinity.
Salinity varies around the world's oceans depending on temperature and
the mixing action of ocean currents. Salinity is measured in
parts per thousand (ppt; 10 ppt = 1%) of salt in water. The salinity of
the warm, well-mixed surface waters over much of the world's major ocean basins ranges
from 33 to 37 parts per thousand (Fig. 6).
 |
| Figure 6. Map of salinity at the ocean surface.
Numbers represent salinity values in parts per thousand. Salinity
in the open ocean is greatest in tropical regions and decreases in the
isolated Arctic Ocean. Map generated at University of Tokyo
website. |
Higher- and lower-salinity values are observed in smaller, restricted
ocean basins and seas (Fig. 7). For example, salinity values of 20 to 30 ppt are recorded for the
high-latitude Arctic Ocean and values of over 40 ppt occur in the narrow
tropical Red Sea basin between north Africa and the Arabian
peninsula. Salinity is higher at low latitudes because high temperatures at these
locations promote evaporation which removes water but leaves the salt it contains behind.
Salinity values are lower at high latitudes because of the lack of evaporation, high
precipitation, and the influx of freshwater from melting ice sheets. The isolated Baltic
Sea between Sweden and Finland has salinity values that approach freshwater along
its northern shore.
 |
Figure 7. High and low salinity in restricted seas in low (Red Sea)
and high (Baltic Sea) latitudes. Click on image to view larger version. Maps generated at
University of Tokyo
website. |
|
Salinity and Depth
Salinity values are variable in the shallow (e.g., 0-200 m) ocean but are much more uniform
in deeper waters below 2,000 meters (6,600 feet; Fig. 8). Salinity may decrease with depth in the tropics but
increases with depth at high latitudes (+60oN/S). The salinity in the
Arctic Ocean (north of 70oN latitude) increases with depth from
30 to 35 ppt.
Salinity in this relatively isolated ocean basin remains uniform below a depth of
approximately 300 meters (1,000 feet).
The change of salinity occurs over a depth zone known as the halocline. The
depth range for the halocline is from approximately 200 to 1,000 meters
(660-3,300 feet) but will show some
variation with location. Salinity is uniform with a value of 34 to 35 ppt below the
halocline.
 |
| Figure 8. North-south profile through the Pacific Ocean
along the 155.5 meridian illustrating the range of salinity with depth and
latitude. Numbers represent salinity values in parts per thousand. Cross section
generated at University
of Tokyo website. |
Temperature and Latitude
Solar
radiation strikes Earth more directly at the equator and tropics than in polar
regions (Fig. 9). Radiation strikes Earth at a lower angle near the poles and the
Suns
rays must therefore penetrate a greater thickness of atmosphere. Some of the solar
radiation is scattered in the atmosphere and more heat energy is lost near the poles as a
result of scattering. Earth's surface at the equator receives 2.5 times more insolation,
incoming solar radiation, than the atmosphere above the poles. The highest average annual
ocean temperatures (~27oC) are present along the equator and temperatures
decrease symmetrically to the north and south approaching 0oC at high
latitudes (Fig. 10).
 |
Figure 9. Solar radiation is distributed over a wider area and must
penetrate a greater thickness of atmosphere at the poles, reducing the amount of solar
energy reaching Earth's surface. Consequently, ocean temperatures are greater near the
equator. |
 |
| Figure 10. Map of world's oceans illustrating the
average annual range of temperature with latitude. Numbers represent
temperature in degrees Celsius. Map generated at University of Tokyo
website. |
Water has two relatively unusual thermal properties
that make the oceans a great storage reservoir for heat energy and contribute to global
oceanic circulation patterns. First, the heat capacity of a material is
measured as the amount of heat required (in calories) to raise the temperature of 1 gram
of the substance by 1oC. Materials with high heat capacity, such as water, can
absorb substantial quantities of heat without any significant change in temperature. The
ability of the oceans to store heat plays a crucial role in controlling global climate
patterns.
Second, cold water can be both less dense and more dense than warm water. Water
density increases as water temperature decreases down to approximately 4oC.
Below that temperature water density decreases, especially when water changes state from a
liquid to solid (ice) form. Consequently, dense cold water can sink below less dense warm
water but ice will float on the ocean's surface.
Temperature and Depth
The major oceans can be divided into layers of relatively warm waters at shallow depths
and cold waters at greater depths (Fig. 11). Surface waters are warmed by solar radiation and
currents cause thermal mixing that results in relatively uniform temperature distributions
by latitude. Sunlight doesn't penetrate more than a few hundred meters below the ocean
surface and the impact of current activity diminishes with depth.
Temperatures exceed 20oC over much of the tropical ocean's surface but
decline to a chilly 2oC below 2,000 meters (6,600 feet)depth. The depth zone in which
temperature decreases rapidly is known as a thermocline. The base of the
thermocline is at a depth of approximately 1,000 meters (3,300 feet).
 |
| Figure 11. North-south profile through the Pacific Ocean
along the 155.5 meridian illustrating the range of temperature with depth and
latitude. Cross section generated at University of Tokyo
website. |
| |
| Think
about it . . . |
| Use
the data found here
to plot two ocean temperature profiles and answer the questions that
follow. |
|