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ndgoodburn
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Homework Statement
In this problem, you'll model the lower atmosphere of Venus. The atmospheric pressure reaches 1 bar (100 kPa) in the middle of the dense cloud deck, where T ~ 350 K. At the surface, the pressure is 90 bars (9000 kPa). From the surface to the 1 bar level, the temperature T(z) decreases at a rate of dT/dz = -8 K [itex]km^{-1}[/itex], close to the adiabatic lapse rate of -8 K [itex]km^{-1}[/itex].
(b)Write down the equation for hydrostatic equilibrium, including explicitly the variation T(z).
Homework Equations
We can estimate the adiabatic lapse rate with the approximation:
[itex]\frac{dT}{dz}|_{ad}=-\frac{g}{c_p}[/itex]
The equation for hydrostatic equilibrium:
[itex]\Delta P = -\rho \Delta z g[/itex]
The Attempt at a Solution
Part (a) asks me to confirm the adiabatic lapse rate for Venus, which is simple by plugging in g and cp.
Part (b) (asking for the hydrostatic equilibrium equation) is what is confusing me. I am specifically having trouble including T(z). I can find an expression for T(z) by integrating the adiabatic lapse rate approximation:
[itex]∫\frac{dT}{dz} dz|_{ad}=∫-\frac{g}{c_p} dz[/itex]
[itex]T(z)=T_0-\frac{g}{c_p}z[/itex]
I called the constant of integration T0 because that makes sense conceptually.
Now, what I tried was just solving T(z) for g and plugging it into the hydrostatic equilibrium equation because I'm just trying to find a way to include it, but that just yields
[itex]\Delta P=-\rho \Delta z \frac{c_p}{z}(T_0-T(z))[/itex]
which seems useless to me, because T(z) would quickly reduce out with a tiny bit of simplification.
Maybe someone can help by telling me if what I've done so far makes sense and if I should continue, or if I'm just missing something that would make it more clear. Thanks in advance!
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