06.12.2012 Views

Principles of terrestrial ecosystem ecology.pdf

Principles of terrestrial ecosystem ecology.pdf

Principles of terrestrial ecosystem ecology.pdf

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

phere, extends to depths <strong>of</strong> 75 to 200 m, depending<br />

on the depth <strong>of</strong> wind-driven mixing. Most<br />

primary production, detrital production, and<br />

decomposition take place in the surface waters<br />

(see Chapter 10). Another major difference<br />

between atmospheric and oceanic circulation is<br />

that density <strong>of</strong> ocean waters is determined by<br />

both temperature and salinity, so, unlike warm<br />

air, warm water can sink, if it is salty enough.<br />

There are relatively sharp gradients in temperature<br />

(thermocline) and salinity (halocline)<br />

between warm surface waters <strong>of</strong> the ocean and<br />

cooler more saline waters at intermediate<br />

depths (200 to 1000m) (Fig. 2.8).These two vertical<br />

gradients cause the surface waters to be<br />

less dense than deep water, creating a stable<br />

vertical stratification. The deep layer therefore<br />

mixes with the surface waters slowly over<br />

hundreds to thousands <strong>of</strong> years. These deeper<br />

layers nonetheless play critical roles in element<br />

cycling, productivity, and climate because they<br />

are long-term sinks for carbon and the sources<br />

<strong>of</strong> nutrients that drive ocean production (see<br />

Chapters 10 and 15). Upwelling areas, where<br />

deep waters move rapidly to the surface,<br />

support high levels <strong>of</strong> primary and secondary<br />

productivity (marine invertebrates and verte-<br />

Depth (m)<br />

0<br />

0<br />

250<br />

500<br />

750<br />

Temperature<br />

Temperature ( o C)<br />

5 10 15<br />

1000<br />

32 33 34 35 36<br />

Salinity (ppt)<br />

Salinity<br />

T / H<br />

Surface<br />

water<br />

Intermediate<br />

water<br />

Figure 2.8. Typical vertical pr<strong>of</strong>iles <strong>of</strong> ocean temperature<br />

and salinity. The thermocline (T) and<br />

halocline (H) are the zones where temperature<br />

and salinity, respectively, decline most strongly<br />

with depth. These transition zones usually coincide<br />

approximately.<br />

The Oceans 29<br />

brates) and are the locations <strong>of</strong> many <strong>of</strong> the<br />

world’s major fisheries.<br />

Ocean Circulation<br />

Ocean circulation plays a critical role in Earth’s<br />

climate system. On average, ocean circulation<br />

accounts for 40% <strong>of</strong> the latitudinal heat transfer<br />

from the equator to the poles, with the<br />

remaining 60% <strong>of</strong> heat transfer occurring<br />

through the atmosphere. The ocean is the dominant<br />

heat transporter in the tropics, and the<br />

atmosphere plays the stronger role at midlatitudes.<br />

The surface currents <strong>of</strong> the oceans<br />

are driven by surface winds and therefore<br />

show global patterns (Fig. 2.9) that are generally<br />

similar to those <strong>of</strong> the prevailing surface<br />

winds (Fig. 2.7). The ocean currents are,<br />

however, deflected 20 to 40° relative to the wind<br />

direction by Coriolis forces. This deflection<br />

and the edges <strong>of</strong> continents cause ocean<br />

currents to be more circular (termed gyres)<br />

than the winds that drive them. In equatorial<br />

regions, currents flow east to west, driven by the<br />

easterly trade winds, until they reach the continents,<br />

where they split and flow poleward along<br />

the western boundaries <strong>of</strong> the oceans, carrying<br />

warm tropical water to higher latitudes. On<br />

their way poleward, currents are deflected by<br />

Coriolis forces. Once the water reaches the high<br />

latitudes, some returns in surface currents<br />

toward the tropics along the eastern edges <strong>of</strong><br />

ocean basins (Fig. 2.9), and some continues<br />

poleward.<br />

Deep ocean waters show a circulation<br />

pattern quite different from the wind-driven<br />

surface circulation. In the polar regions, especially<br />

in the winter <strong>of</strong>f southern Greenland and<br />

<strong>of</strong>f Antarctica, cold air cools the surface waters,<br />

increasing their density. Formation <strong>of</strong> sea ice,<br />

which excludes salt from ice crystals (brine<br />

rejection), increases the salinity <strong>of</strong> surface<br />

waters, also increasing their density. The high<br />

density <strong>of</strong> these cold saline waters causes them<br />

to sink. This downwelling to form the North<br />

Atlantic deep water <strong>of</strong>f <strong>of</strong> Greenland, and the<br />

Antarctic bottom water <strong>of</strong>f <strong>of</strong> Antarctica drives<br />

the global thermohaline circulation in the<br />

middle and deep ocean that ultimately transfers<br />

water between the major ocean basins (Fig.<br />

2.10). The descent <strong>of</strong> cold dense water at high

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!