violet radiation by oxygen (O 2 ) and O 3. The rise in temperature with height has
the effect of giving the upper part of the atmosphere great stability against ver-
tical mixing. This is because the heavy cold air at the bottom has no tendency to
rise. This region of the atmosphere has air in distinct layers or strata and is thus
called the stratosphere. The well-known O 3 layer forms at these altitudes. Despite
this stability, even the stratosphere is well mixed compared with the atmosphere
even higher up. Above about 120 km, turbulent mixing is so weak that
individual gas molecules can separate under gravitational settling. Thus the
The Atmosphere 33
200
180
160
140
120
100
80
60
40
20
Altitude (km)
10 –6 10 –4 10 –2 100 102 104
Heterosphere
Homosphere
Turbopause
Mesopause
Stratopause
Tropopause
Troposphere
Stratosphere
Mesosphere
Temperature
100 200 300 400 500 600 700
2000
1000
600
200
104
Concentration (cm–3)
Atomic
oxygen
Molecular
oxygen
Atomic
hydrogen
Helium
Heterosphere
Altitude (km)
Temperature (K)
106 108
Pre
ssu
re
Pressure (Pa)
Fig. 3.2The vertical structure of the atmosphere and associated temperature and pressure variation. Note the
logarithmic scale for pressure. The inset shows gas concentration as a function of height in the heterosphere
and illustrates the presence of lighter gases (hydrogen and helium) at greater heights.