Atmospheric Density, exponential decay derivation

In summary, atmospheric density is the measure of mass per unit volume in the Earth's atmosphere. It plays a crucial role in regulating the Earth's climate by affecting the absorption and reflection of solar energy, which impacts temperature and weather patterns. The formula for calculating atmospheric density is ρ = m/V, where ρ is density, m is mass, and V is volume. Exponential decay describes the gradual decrease of atmospheric density as altitude increases, due to decreasing pressure and temperature. Factors such as altitude, temperature, and humidity can influence atmospheric density.
  • #1
tony_cruz
8
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I've read my lecture notes about 100x but can't even begin to see where this derivation can come from. A previous derivation was the equation
dP/dz = -gρ
(P = pressure, z = distance, g= acc due to grav, ρ = density)

If atmosphere can be treated as an isothermal ideal gas of constant mean molecular mass m, show that density drops exponentially with height,
ρ= [ρ0]e^-z/h
where h is a constant*



later i worked through to find it was the scale height ~8.5km but the value is unknown for this question.
 
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bump 2pm deadline ...
 
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The derivation of the exponential decay of atmospheric density with height comes from the ideal gas law and the assumption of isothermal conditions. The ideal gas law states that the pressure of a gas is directly proportional to its density and temperature, and inversely proportional to its volume. In a constant temperature environment, this can be written as P = ρRT, where ρ is the density, R is the gas constant, and T is the temperature.

Using this equation and the previous derivation of dP/dz = -gρ, we can rearrange to solve for ρ and substitute it into the ideal gas law. This gives us ρ = (P/RT) and plugging this into the previous equation gives us:

dP/dz = -g(P/RT)

We can then rearrange this equation to isolate P and integrate both sides with respect to z:

∫dP/P = -g/R∫dz

ln(P) = -gz/R + C

Where C is a constant of integration. We can then exponentiate both sides to eliminate the natural log:

P = e^(-gz/R) * e^C

Since e^C is just another constant, we can combine it with the constant of integration to get a new constant, A. This gives us the final equation of:

P = Ae^(-gz/R)

Since density is directly proportional to pressure, we can substitute ρ for P and get:

ρ = Ae^(-gz/R)

This is the exponential decay equation for atmospheric density with height, where h = R/g is the scale height. This means that for every increase of h in height, the density decreases by a factor of e. This derivation assumes that the atmosphere is an isothermal ideal gas, meaning that the temperature remains constant throughout the atmosphere. However, in reality, the temperature does change with height and this can affect the accuracy of this equation. But for a rough estimate, this derivation provides a good understanding of the exponential decay of atmospheric density.
 

FAQ: Atmospheric Density, exponential decay derivation

1. What is atmospheric density?

Atmospheric density refers to the amount of mass per unit volume in the Earth's atmosphere. It is typically measured in kilograms per cubic meter.

2. How does atmospheric density affect the Earth's climate?

Atmospheric density plays a crucial role in regulating the Earth's climate. It affects the amount of solar energy that is absorbed or reflected by the atmosphere, which in turn impacts temperature and weather patterns.

3. What is the formula for calculating atmospheric density?

The formula for atmospheric density is ρ = m/V, where ρ is density, m is mass, and V is volume. This formula is based on the ideal gas law, which states that the density of a gas is directly proportional to its pressure and inversely proportional to its temperature.

4. How does exponential decay relate to atmospheric density?

Exponential decay refers to the gradual decrease of a quantity over time. In the context of atmospheric density, it describes how the density of the atmosphere decreases as altitude increases. This is due to the decreasing pressure and temperature at higher altitudes.

5. What factors influence atmospheric density?

Several factors can influence atmospheric density, including altitude, temperature, and humidity. Higher altitudes typically have lower atmospheric density due to the lower pressure and temperature. Warmer temperatures can also lead to lower density, as warm air is less dense than cold air. Humidity, or the amount of water vapor in the air, can also impact atmospheric density as water vapor is less dense than dry air.

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