Atmospheric physics 7: Lapse rate

In fact, the temperature inside the atmosphere is not homogeneous but depends on the altitude. Within the troposphere (lowest atmospheric layer), the temperature decreases with the altitude, which can be seen from the fact that there is a snow cap on high mountains even in tropical regions.

A simple reason for this is the fact that gases cool down on expansion, when they can not exchange heat with their environment. When an air parcel rises in the atmosphere, the pressure decreases, causing the air to expand.

Calculate the temperature decrease of an air package with the height Γ = d T d z z = 0 \Gamma = - \left. \frac{d T}{d z} \right|_{z = 0} near sea level under the following assumptions:

  • The process is adiabatic, so that P V κ = const P V^\kappa =\text{const} , where κ = 1.4 \kappa = 1.4 is the adiabatic index of air.
  • The pressure follows the barametric formula P = P ( z ) P = P(z) from the previous parts with the same scale height H . H.
  • The temperature at sea level is T 0 = 288 K . T_0 = 288 \,\text{K}.
  • Air is an ideal gas with P V T P V \propto T (general gas equation).
Γ 4.3 T / km \Gamma \approx 4.3 \,\text{T}/\text{km} Γ 6.5 T / km \Gamma \approx 6.5\,\text{T}/\text{km} Γ 8.1 T / km \Gamma \approx 8.1\,\text{T}/\text{km} Γ 9.8 T / km \Gamma \approx 9.8\,\text{T}/\text{km}

This section requires Javascript.
You are seeing this because something didn't load right. We suggest you, (a) try refreshing the page, (b) enabling javascript if it is disabled on your browser and, finally, (c) loading the non-javascript version of this page . We're sorry about the hassle.

1 solution

The mass density ρ \rho of the air parcel is inversely proportional to the volume V V : ρ = M n V 1 V \rho = \frac{M n}{V} \propto \frac{1}{V} Therefore, the adiabatic condition P V κ = const PV^\kappa = \text{const} can be rewritten to P ρ κ = const ρ = const P 1 / κ P e z / H = ρ 0 exp [ z κ H ] \begin{aligned} & & \frac{P}{\rho^\kappa} &= \text{const}\\ \Rightarrow & & \rho &= \text{const} \cdot P^{1/\kappa} & & | P \propto e^{-z/H}\\ & & &= \rho_0 \exp\left[ - \frac{z}{\kappa H} \right] \end{aligned} with the density ρ 0 = ρ ( z = 0 ) \rho_0 = \rho(z=0) at sea level. Here we have used the barometric height formula from the last section. Thus, the density also depends exponentially on the height, but drops faster than the pressure P P by the factor κ = 1.4 \kappa = 1.4 . Since we know pressure and density as a function of altitude, we can also use the general gas equation to determine the temperature curve: P = const ρ T T = const P ρ P e z / H , ρ e z / κ H = T 0 exp [ κ 1 κ z H ] \begin{aligned} & & P &= \text{const} \cdot \rho T \\ \Rightarrow & & T &= \text{const} \cdot \frac{P}{\rho} & & | P \propto e^{-z/H}, \rho \propto e^{-z/\kappa H} \\ & & &= T_0 \exp\left[ - \frac{\kappa - 1}{\kappa} \frac{z}{H} \right] \end{aligned} with the temperature T 0 = T ( z = 0 ) T_0 = T(z = 0) . At sea level, therefore, the temperature gradient gives the result Γ = d T d z z = 0 = κ 1 κ T 0 H = 1.4 1 1.4 288 K 8417 m 9.8 1 0 3 K m \begin{aligned} \Gamma &= -\left.\frac{dT}{dz}\right|_{z=0} = \frac{\kappa - 1}{\kappa} \frac{T_0}{H} \\ &= \frac{1.4 - 1}{1.4} \frac{288 \,\text{K}}{8417 \,\text{m}} \approx 9.8 \cdot 10^{-3} \,\frac{\text{K}}{\text{m}} \end{aligned} The quantity Γ \Gamma is also known as the dry adiabatic lapse rate.

0 pending reports

×

Problem Loading...

Note Loading...

Set Loading...