Deriving pressure, density and temperature profile of atmosphere

voxel
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Homework Statement


Derive the pressure, density and temperature profiles of an adiabatically stratified plane-parallel atmosphere under constant gravitational acceleration g. Assume that the atmosphere consists of an ideal gas of mean molecular weight \mu.

Given \mu=14u, g = 9.81m/s^2, z = 8500m, T (@sea level) = 300K, calculate temperature and pressure at the summit.

Homework Equations


Edit: removed the ideal gas law and barometric formula because I think I was on the wrong track with them...

The Attempt at a Solution


I have been able to derive the barometric formula (which doubles as a pressure and density profile) from the ideal gas law, but am stuck in a bit of a circular problem: I need the temperature at the top of the summit to get the pressure, and vice versa. I don't know how to proceed, or maybe I've taken the wrong approach.

Any help would be appreciated!
 
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What does "adiabatically stratified" mean? Is it that pVγ= const. ?
 
kuruman said:
What does "adiabatically stratified" mean?

I interpreted it to mean that the atmosphere can be modeled as planes of thickness dz that are adiabatic.
 
voxel said:
I interpreted it to mean that the atmosphere can be modeled as planes of thickness dz that are adiabatic.
They "are adiabatic" in what way? Could it be that as z changes, the product pVγ remains constant? If so you have three equations: barometric, ideal gas and adiabatic condition and three thermodynamic variables. You can eliminate any two variables and find the other in terms of z.
 
I think you're right in that as z changes, the product PV^\gamma = const.

However, I'm not seeing how I can eliminate P and V to get T(z)..

edit: clarification: I don't see how I can eliminate two of the thermodynamic variables without introducing an unknown constant.
 
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Use the ideal gas law to eliminate the volume in the adiabatic condition to find an expression that says (Some power of p)*(some other power of T) = constant. Find the value of the constant from the initial conditions. Solve for the pressure and replace the expression you get for p in the barometric equation. This will give you an equation with T and z only.
 
To solve this, I first used the units to work out that a= m* a/m, i.e. t=z/λ. This would allow you to determine the time duration within an interval section by section and then add this to the previous ones to obtain the age of the respective layer. However, this would require a constant thickness per year for each interval. However, since this is most likely not the case, my next consideration was that the age must be the integral of a 1/λ(z) function, which I cannot model.
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