Math 2.0

Geophysics Definition

Potential temperature

Builds on Brunt–Väisälä frequency

Definition

Consider dry air treated as an ideal gas with specific gas constant RR and specific heat at constant pressure cpc_p. Fix a reference pressure p0>0p_0 > 0, by convention p0=1000p_0 = 1000 hPa. The potential temperature of air with absolute temperature TT and pressure p>0p > 0 is θ=T(p0p)R/cp.\theta = T \left( \frac{p_0}{p} \right)^{R / c_p}.

Remarks

For dry air R/cp≈0.286R / c_p \approx 0.286. For a reversible adiabatic change of an ideal gas, the first law gives cp dln⁡T−R dln⁡p=0c_p \, d \ln T - R \, d \ln p = 0, that is dln⁡θ=0d \ln \theta = 0. So θ\theta is conserved by a parcel that moves without heating, and cpln⁡θc_p \ln \theta equals the specific entropy up to a constant.

Example: at p=500p = 500 hPa and T=253T = 253 K, θ=253⋅20.286≈253⋅1.219≈308.5\theta = 253 \cdot 2^{0.286} \approx 253 \cdot 1.219 \approx 308.5 K. At p=p0p = p_0 the potential temperature equals the temperature.

Non-example: moist air in which water vapour condenses receives latent heat, so its θ\theta increases as it rises. Then θ\theta is not conserved, and the equivalent potential temperature is used instead.

The vertical gradient of θ\theta measures static stability: the squared Brunt–Väisälä frequency is N2=(g/θ) ∂θ/∂zN^2 = (g / \theta) \, \partial \theta / \partial z, with gg the gravitational acceleration. The atmosphere is statically stable for dry displacements where ∂θ/∂z>0\partial \theta / \partial z > 0.

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Further reading

  1. Web https://en.wikipedia.org/wiki/Potential_temperature
About this page
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WritingW0 stub
MSC86A10, 80A10
DefinesPotential temperature
UsesBrunt–Väisälä frequency
Changed3 November 2026

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