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The enhanced greenhouse effect

Greenhouse gases are a natural part of the atmo-

sphere. Without these gases the global average

temperature would be around -20ºC. The problem

we now face is that human actions – particularly

burning fossil fuels (coal, oil and natural gas) and

land clearing – are increasing their concentrations.

The more of these gases there are, the more heat

is trapped. This is known as the enhanced green-

house effect. Naturally occurring greenhouse gas-

es include water vapour, carbon dioxide, methane,

nitrous oxide, and ozone. Greenhouse gases that

are not naturally occurring include hydro-fluorocar-

bons (HFCs), perfluorocarbons (PFCs), and sulphur

hexafluoride (SF6), which are generated in a variety

of industrial processes.

On average, about one-third of the solar radiation

that hits the Earth is reflected back into space. The

land and the oceans mostly absorb the rest, with

the remainder trapped in the atmosphere. The solar

radiation that strikes the Earth’s surface heats it up,

and as a result infrared radiation is emitted.

Cooling or heating, a balancing act

THE GREENHOUSE EFFECT

10

Solar radiationpasses through

the clear atmosphere

Incoming solar radiation:

343 Watt per m

2

Solar energy is absorbed by the

Earth’s surface and warms it...

... and is converted into heat causing

the emission of longwave (infrared)

radiation back to the atmosphere

Surface gains more heat and

infrared radiation is emitted again

Some of the infrared radiation is

absorbed and re-emitted by the

greenhouse gas molecules. The

direct effect is the warming of the

Earth’ssurfaceand the troposphere.

Some solar radiation is

reflected by the atmosphere

and Earth’s surface

Outgoing solar radiation:

103 Watt per m

2

Some of the infrared

radiationpasses through

the atmosphere and is

lost in space

Net outgoing infrared radiation:

240 Watt per m

2

Net incoming solar radiation:

240 Watt per m

2

A T M O S P H E R E

E A R T H

G

R

E

E

N

H

O

U

S

E

G

A

S

E

S

The Greenhouse effect

168 Watt per m

2

Sources:OkanaganUniversityCollege,University ofOxford,EPA, IPCC.

UnitedNationsEnvironmentProgramme /GRID-Arendal

-2

-1

0

1

2

3

Global mean radiative forcing (Wm

-2

)

Anthropogenic and natural forcing of the climate for the year 2000, relative to 1750

N

2

O

CO

2

Greenhouse gases

Stratospheric

ozone

The height of a bar indicates a best estimate of the forcing, and the

accompanying vertical line a likely range of values. Where no bar is present

the vertical line only indicates the range in best estimates with no likelihood.

CH

4

UnitedNationsEnvironmentProgramme /GRID-Arendal

Cooling

Halocarbons

Tropospheric

ozone

Sulphate

Organic

carbon

from

fossil

fuel

burning

Black

carbon

from

fossil

fuel

burning

Biomass

burning

Mineral

Dust

Aerosol

indirect

effect

Contrails Cirrus

Aviation

Aerosols + clouds

LEVEL OF SCIENTIFIC

UNDERSTANDING

Warming

Land use

(albedo only)

Solar

Every year the sun delivers an average of 340 watts of energy to every square metre of the Earth. To

produce this amount of energy we would need 440 million large electric power plants, each gener-

ating 100 million watts of power (NASA).

It would get uncomfortably hot on Earth with all this energy, but fortunately for us, the amount of heat we receive from

the sun is balanced by heat radiated back into space by the atmosphere. Radiative forcing is the change in the balance

between radiation coming into the atmosphere and radiation going out. A positive radiative forcing tends on average to

warm the surface of the Earth, and negative forcing tends on average to cool the surface. Greenhouse gases, for example,

produce positive radiative forcing – they trap outgoing terrestrial (infrared) radiation, which causes a temperature rise at

the Earth’s surface – the “greenhouse effect”. In contrast, negative radiative forcing from clouds and aerosols, which can

reflect back into space, acts as a cooling mechanism.

Radiative forcing

The radiative forcing from the increase in

anthropogenic greenhouse gases since the

pre-industrial era is positive (warming) with a

small uncertainty range; that from the direct

effects of aerosols is negative (cooling) and

smaller; whereas the negative forcing from

the indirect effects of aerosols (on clouds and

the hydrologic cycle) might be large but is not

well quantified. Key anthropogenic and natu-

ral factors causing a change in radiative forc-

ing from year 1750 to year 2000 are shown

in this figure, where wide, colored bars mark

the factors whose radiative forcing can be

quantified. Only some of the aerosol effects

are estimated here and denoted as ranges.

Other factors besides atmospheric constitu-

ents -- solar irradiance and land-use change

-- are also shown. Stratospheric aerosols

from large volcanic eruptions have led to

important, but short-lived, negative forcings

(particularly during the periods 1880-1920

and 1960-1994), which are not important

over the time scale since the pre-industrial

era and not shown. The sum of quantified

factors in the figure is positive, but this does

not include the potentially large, negative

forcing from aerosol indirect effects.