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the tropics polewards, otherwise the tropics would get
hotter and polar regions cooler. It is the winds of the
world, and to a lesser extent the ocean currents, which
bring about the necessary heat transfer.
LATITUDINAL RADIATION BALANCE
To see how much radiant energy we have available at any
location we must know how much radiation is being
lost as well as how much is reaching that location. Long-
wave radiation emission is proportional to the absolute
temperature of the surface. It is far less variable than the
input of solar radiation. The difference between incoming
and outgoing radiation is known as net radiation or the
radiation balance. For Earth's surface, estimates are shown
in Figure 3.7 .
If we include the effects of the atmosphere, the picture
changes. The atmosphere has a negative balance, even in
the tropics ( Figure 3.8 ). In fact, values differ little between
equator and poles. For any particular latitude, we can sum
the surface and atmospheric radiation balances to find out
which areas of Earth have a radiation surplus and which
areas have a deficit. Using satellite data, it is now possible
to determine the radiation balance of the surface and
atmosphere together, as shown in Figure 3.9 . In general
there is a surplus of energy between about 38
350
300
Absorbed Solar
250
Emitted Longwave
200
150
100
Net Radiation
50
0
-50
-100
-150
-90
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-30
0
30
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90
Latitude
S
and a deficit towards the poles. Naturally the magnitude
of the surplus is identical to that of the deficit, but it does
mean that there must be a steady transfer of energy from
N and 38
Figure 3.8 Annual mean absorbed solar radiation, outgoing
long-wave radiation and net radiation averaged around latitude
circles.
Source: After Hartmann (1994)
LONGITUDE
150
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0
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180
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0
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Figure 3.7 Global distribution of mean annual net radiation. Units are W m -2 .
Source: After Budyko et al. (1962)
 
 
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