Math 2.0

Geophysics Definition

Scale height

Builds on Exponential function

Definition

Let a layer of ideal gas have absolute temperature TT and mean molar mass MM, under a gravitational acceleration gg. Let RR be the molar gas constant. The scale height of the gas is H=RTMg.H = \frac{R T}{M g}.

Remarks

Equivalently, H=kBT/(mg)H = k_B T/(m g), with kBk_B the Boltzmann constant and mm the mean mass of a molecule. If the layer is in hydrostatic balance dp/dz=−ρgdp/dz = -\rho g and obeys the ideal gas law p=ρRT/Mp = \rho R T/M, then dp/dz=−p/Hdp/dz = -p/H. So for constant TT the pressure is p(z)=p(0) e−z/Hp(z) = p(0) \, e^{-z/H}, an exponential function, and it falls by the factor ee over each height HH. Example: for dry air, M=0.02896M = 0.02896 kg/mol, with T=288T = 288 K, g=9.81g = 9.81 m/s² and R=8.314R = 8.314 J/(mol K), one gets H≈8.4H \approx 8.4 km. Non-example: in a layer whose temperature changes with height, HH is a function of height, and the pressure is not a single exponential in zz.

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Further reading

  1. Web https://en.wikipedia.org/wiki/Scale_height
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DefinesScale height
UsesExponential function
Changed3 November 2026

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