Scale height

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A Scale height is a term often used in scientific contexts for a distance over which a quantity decreases by a factor of e. It is usually denoted by the capital letter H.

For planetary atmospheres, it is the vertical distance upwards, over which the pressure of the atmosphere decreases by a factor of e. The scale height remains constant for a particular temperature. It can be calculated by

[H = \frac]

where:

k = Boltzmann constant = 1.38×10⁻²³ J·K⁻¹
T = temperature in kelvin
m = mean molecular mass of dry air (units Kg·molec⁻¹)
g = acceleration due to gravity

The pressure in the atmosphere is caused by the weight of the atmosphere of the overlying atmosphere [force per unit area]. If at a height of z the atmosphere has density ρ and pressure P, then moving upwards at an infinitesimally small height dz will decrease the pressure by amount dP, equal to the weight of a layer of atmosphere of thickness dz.

Thus:

[d\rho = -g \rho dz]

Where g is used to denote the acceleration due to gravity. For small dz it is possible to assume g to be constant, the minus sign indicates that as the height increases the pressure decreases. Therefore using the equation of state for a perfect gas of mean molecular mass m at temperature T, the density can be expressed as such:

[\rho = \frac]

Therefore combining the equations gives

[\frac = \frac}]

which can then be incorporated with the equation for H given above to give:

[\frac = - \frac]

which will not change unless the temperature does. Integrating the above and assuming where P₀ is the pressure at height z = 0 (pressure at sea level) the pressure at height z can be written as:

[P = P_0e^)}]

This translates as the pressure decreasing exponentially with height.

In the earths atmosphere the pressure at sea level P₀ roughly equals 1.01×10⁵Pa and the mean molecular mass of dry air is 28.964 u (1 u = 1.660×10⁻²⁷ kg).

examples:

T = 290 K, H = 8500 m

T = 210 K, H = 6000 m

Note:

Density is related to pressure by the ideal gas laws. Therefore with some departures caused by varying temperature—density will also decrease exponentially with height from a sea level value of ρ₀ roughly equal to 1.2 kg m⁻³
At heights over 100 km, molecular diffusion means that each molecular atomic species has its own scale height.

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