EuraStudy
This chapter examines the atmosphere as a dynamic system of energy stores and flows. It covers the composition and vertical layered structure of the atmosphere and how temperature changes with altitude, the Earth's energy budget and the natural greenhouse effect, the global pattern of atmospheric circulation that shapes climate and biomes, and the natural functioning of the stratospheric ozone layer that shields the surface from ultraviolet radiation.
4 sections~14 min reading time3 competenciesLevel Foundation 1 · Standard 2 · Advanced 1
basic level
AS-Level expects you to describe the layers of the atmosphere, the natural greenhouse effect, the broad pattern of circulation and the role of the ozone layer.
higher level
The full A-Level requires you to interpret radiation and temperature data, explain circulation in terms of differential heating, and analyse the ozone balance through the Chapman reactions.
Reading depth: In depth
Text size: Standard
The layers of the atmosphere
A weather balloon records temperature falling from 15 degrees Celsius at the surface to -55 degrees Celsius at 11 km, then rising to about -3 degrees Celsius at 45 km. Identify the layers and explain the reversal.
Temperature falls from the surface to 11 km, so this is the troposphere; the tropopause is at about 11 km where the trend reverses.
Temperature then rises to 45 km, so this is the stratosphere.
In the stratosphere, ozone absorbs ultraviolet radiation and warms the air, so temperature rises with height rather than falling.
Result: The profile shows the troposphere (cooling) then the stratosphere (warming), the reversal caused by ozone absorbing UV.
Typical mistakes
Active revision
Describe how temperature changes with altitude through the troposphere and stratosphere, and explain the difference in terms of where solar energy is absorbed.
Active recall
Recall the key points — then reveal.
Sources: AQA AS and A-level Environmental Science (7447) specification (AQA) · GCE AS and A level subject content (Department for Education)
The Earth's energy budget and the greenhouse effect
A large area of reflective sea ice melts and is replaced by dark open ocean. Predict the effect on the local energy budget and temperature.
Ice has a high albedo and reflects much incoming radiation; dark ocean has a low albedo and absorbs much more.
More short-wave radiation is now absorbed rather than reflected, so more energy enters the system locally.
The extra absorbed energy warms the surface, which can melt more ice, an example of positive feedback.
Result: Lower albedo means more radiation is absorbed, warming the surface and driving further ice loss (positive feedback).
Typical mistakes
Active revision
Explain why greenhouse gases allow incoming solar radiation to pass but absorb the radiation emitted by the Earth's surface.
Active recall
Recall the key points — then reveal.
Sources: AQA AS and A-level Environmental Science (7447) specification (AQA) · GCE AS and A level subject content (Department for Education)
The Hadley cell
Use the three-cell circulation model to explain why a region on the equator has heavy year-round rainfall while a region at 30 degrees latitude is arid.
Intense heating makes air rise; as it rises it cools, water vapour condenses and heavy rain falls, so the equatorial belt is wet.
The air that rose at the equator has lost its moisture and descends at about 30 degrees; as it sinks it warms and dries, so little rain falls.
Rising air at the equatorial low gives rainforest; sinking air at the subtropical high gives desert.
Result: Rising, cooling air at the equator brings rain; sinking, warming air at 30 degrees brings aridity.
Typical mistakes
Active revision
Explain why the world's major hot deserts are found at around 30 degrees north and south of the equator.
Active recall
Recall the key points — then reveal.
Sources: AQA AS and A-level Environmental Science (7447) specification (AQA) · GCE AS and A level subject content (Department for Education)
The Chapman cycle of stratospheric ozone
Explain how the continual formation and breakdown of ozone in the stratosphere reduces the ultraviolet radiation reaching the Earth's surface.
Ultraviolet radiation splits oxygen molecules into atoms, which combine with oxygen to form ozone; this step removes UV energy.
Ozone then absorbs further ultraviolet radiation and splits back into oxygen, again removing UV energy.
Because both steps absorb ultraviolet radiation, much less reaches the surface, and the absorbed energy warms the stratosphere.
Result: The formation and breakdown of ozone each absorb ultraviolet radiation, so the layer shields the surface and warms the stratosphere.
Typical mistakes
Active revision
Explain why the stratospheric ozone layer both protects life at the surface and warms the stratosphere.
Active recall
Recall the key points — then reveal.
Sources: AQA AS and A-level Environmental Science (7447) specification (AQA) · GCE AS and A level subject content (Department for Education)
References & sources
Department for Education