Chapter 2: Atmospheric pressure
Molecular view of atmospheric pressure
EARTH SURFACE
gravity
random
motion
Measurement of atmospheric pressure with the mercury barometer
vacuum
A
h
Atmospheric pressure p = pA = ρHg gh
Mean sea-level pressure:
p = 1.013x105 Pa = 1013 hPa
= 1013 mb
= 1 atm
= 760 mm Hg (torr)
atmospheric pressure
(weight of atmosphere per unit area of surface)
SI unit for pressure is the Pascal (Pa): 1 Pa = 1 kg m-1 s-2
Today’s sea-level pressure map
Pressures are in a narrow range 996-1033 hPa
Why are sea-level pressure gradients so weak?
Consider a pressure gradient at sea level operating on an elementary air parcel dxdydz with mass dm = ρadxdydz where ρa is the air density:
p(x)
p(x+dx)
Vertical area
dydz
Pressure-gradient force
Acceleration
For pressure difference Δp = 10 hPa over Δx = 100 km, with ρa ≈ 1 kg m-3,
we get a ≈ 10-2 m s-2 🢧 100 km/h wind in 3 h!
Wind transports air to from high to low pressure, decreasing Δp
Exerted force
p(x)dydz
So Δp never gets large, except over mountains:
p(z)
p(z+Δz)
p-gradient
gravity
Total mass ma of the atmosphere
Radius of Earth:
6380 km
Mean pressure at Earth's surface: 984 hPa
(less than 1013 hPa because of elevated land)
Total number of moles of air in atmosphere:
Mol. wt. of air: 29 g mole-1 = 0.029 kg mole-1
Molecular weight of air:
9.81 m s-2 (atmosphere is thin enough that this can be considered constant)
Mean vertical profiles of pressure and temperature�
Tropopause
Stratopause
Troposphere has 85% of atmospheric mass, stratosphere has 15%, little above
Decrease of pressure with altitude: barometric law
Consider elementary slab of atmosphere at equilibrium between gravity and p-gradient forces:
p(z)
p(z+dz)
hydrostatic
equation for fluids
Ideal gas law:
Assume uniform T and integrate:
barometric law
unit area
g
Application of barometric law: the sea-breeze effect