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UK Climate Change Programme 2006 - JNCC - Defra

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8<br />

CHAPTER ONE<br />

What is climate change and why does it matter?<br />

The overwhelming majority of scientific<br />

opinion supports the view that human<br />

activities are changing the earth’s climate and<br />

that likely future changes present a serious<br />

threat to human society and the natural<br />

environment.<br />

The ten warmest years globally since<br />

instrumental records began in 1861 have all<br />

occurred since 1994. 1998 was the warmest<br />

year and 2005 was almost as warm.<br />

Without action to reduce greenhouse gas<br />

emissions global temperatures are expected to<br />

rise by between 1.4 and 5.8°C by 2100 and sea<br />

level could also rise by between 0.09 and<br />

0.88 metres compared to 1990 levels.<br />

Such changes will have significant impacts on<br />

human society and on the natural<br />

environment, with increases in drought and<br />

extreme rainfall and greater risks of abrupt<br />

changes in climate.<br />

The greenhouse effect and other<br />

influences on climate<br />

2. The temperature of the earth is determined by<br />

the balance between energy from the sun in the<br />

form of visible radiation (sunlight), and energy<br />

constantly re-radiated from the earth to space in<br />

the form of infra-red radiation. Sunlight passes<br />

through the atmosphere with little direct<br />

warming effect but it warms the earth’s surface<br />

which in turn warms the atmosphere by<br />

convection and the emission of infra-red<br />

radiation, which is absorbed by certain trace<br />

gases – the greenhouse gases. These return some<br />

infra-red radiation back to the surface thereby<br />

warming the surface further. An analogy is often<br />

made with the effect of a greenhouse which<br />

allows sunshine in through clear glass or plastic<br />

that in turn stops the heat inside from escaping,<br />

hence the term ‘greenhouse effect’.<br />

Introduction<br />

1) Visible and near-visible<br />

radiation from the Sun<br />

easily passes through the<br />

glass and heats the ground,<br />

plants, etc.<br />

2) The ground, plants,<br />

etc. act as a thermal<br />

black-body radiator<br />

and emit long-wave<br />

infra-red (IR)<br />

wavelengths<br />

1. The earth’s climate has changed frequently over<br />

the long periods of geological time in responses<br />

to changes in the strength of the sun, the shape<br />

and tilt of the earth’s orbit around the sun, the<br />

position and shape of the continents and the<br />

composition of the atmosphere. There is strong<br />

evidence that greenhouse gas emissions from<br />

human activities are now raising the earth’s<br />

temperature and causing other changes in<br />

climate. Emissions are projected to rise<br />

significantly over the next few decades, and quite<br />

likely beyond this, leading to significant increases<br />

in global temperatures with profound risks for<br />

the natural environment and human society<br />

worldwide. This Chapter provides background<br />

material on the nature of human induced climate<br />

change and its likely impacts.<br />

3) Most of the IR<br />

radiation passes<br />

back through the<br />

glass and escapes<br />

to space ...<br />

4) Some IR radiation<br />

is reflected by the<br />

glass and is trapped<br />

inside the<br />

greenhouse causing<br />

internal temperatures<br />

to rise.<br />

3. The greenhouse effect occurs naturally. Without<br />

it the earth would be over 30°C cooler than it is<br />

and largely uninhabitable. The main naturally<br />

occurring greenhouse gases are water-vapour<br />

(H 2<br />

O), carbon dioxide (CO 2<br />

), methane (CH 4<br />

) and<br />

nitrous oxide (N 2<br />

O). Although water vapour<br />

makes the greatest contribution to the<br />

greenhouse effect, it has a short lifetime in the<br />

atmosphere and its concentration is largely<br />

determined by the temperature of the<br />

atmosphere and not simply by emission or loss<br />

rates. By contrast, the other three gases have<br />

relatively long atmospheric lifetimes – about a

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