The Role of the Oceans in the Radiation Balance
The oceans play an important role in storing and redistributing heat absorbed
from incoming solar radiation. Most of the solar radiation is aborbed
near the equator, where the radiation is most intense. Currents then redistribute
this heat throughout the oceans in what is known as the Thermohaline Circulation,
also known as the "Global Ocean Conveyor Belt".
This very simplistic
diagram of thermohaline circulation (below) depicts a cross-section
through a bowl-shaped ocean basin with the polar regions at left
and right.
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Robin Muench (ESR)
Cooling and formation of sea
ice in the polar regions makes the surface ocean water denser
than the underlying water, so that the surface water sinks and moves
towards the equator (light blue arrows). In the central basin a
variety of processes including vertical mixing move the dense bottom
water upwards toward the surface, where it is warmed by the intense
equatorial solar radiation. The warmed water then moves poleward
to take the place of the sinking dense water, thereby completing
thermohaline circulation.
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The previous "simple" diagram evolves into something like this
when applied to the real oceans:
The currents are controlled by complex factors including the shape
of the seafloor and the earth’s rotation, and the picture presented
here is still oversimplified. Nonetheless, the basic mechanisms
shown above can be seen at work. The North Atlantic Ocean and southern
Weddell Sea (black circles) are both sites where intense cooling
creates dense, sinking water. The equatorial Atlantic, Pacific and
Indian oceans (red circles) are all sites where the water has upwelled
from great depths to the surface and is warmed by incoming radiation
("insolation"). |
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Relevance to climate change?
Because the ocean circulation depends so strongly on sinking of dense
water at high latitudes, it is very sensitive to changes in precipitation.
Increased precipitation at high latitudes will lower the density of the
surface water and inhibit sinking of dense water, thereby slowing the
thermohaline circulation. In the extreme case, thermohaline circulation
is shut down.
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