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๐ŸŒฆ๏ธAtmospheric Science Unit 2 Review

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2.3 Atmospheric density, pressure, and temperature profiles

๐ŸŒฆ๏ธAtmospheric Science
Unit 2 Review

2.3 Atmospheric density, pressure, and temperature profiles

Written by the Fiveable Content Team โ€ข Last updated September 2025
Written by the Fiveable Content Team โ€ข Last updated September 2025
๐ŸŒฆ๏ธAtmospheric Science
Unit & Topic Study Guides

The atmosphere's structure and composition play a crucial role in weather patterns, air quality, and aviation. Pressure decreases with altitude, following an exponential relationship, while the ideal gas law governs the interplay between pressure, temperature, and density in the air around us.

The atmosphere's vertical structure is characterized by hydrostatic equilibrium, where gravity balances pressure gradients. Temperature variations with altitude result from solar radiation, greenhouse gases, and convection. These factors shape weather patterns, pollution dispersion, and flight conditions.

Atmospheric Structure and Composition

Atmospheric pressure and altitude

  • Atmospheric pressure is the force per unit area exerted by the weight of the atmosphere above a given point
  • Pressure decreases with increasing altitude due to the decreasing amount of air above a given point
    • At higher altitudes, there is less air mass above, resulting in lower atmospheric pressure (Mount Everest, stratospheric balloons)
  • The relationship between pressure and altitude is approximately exponential, with pressure decreasing by about half for every 5.5 km increase in altitude
    • This relationship is described by the barometric formula: $p = p_0 e^{-z/H}$, where $p$ is pressure, $p_0$ is pressure at sea level, $z$ is altitude, and $H$ is the scale height (Earth's atmosphere, Mars' atmosphere)

Ideal gas law in atmosphere

  • The ideal gas law relates density, pressure, and temperature of a gas: $pV = nRT$, where $p$ is pressure, $V$ is volume, $n$ is the number of moles, $R$ is the universal gas constant, and $T$ is temperature
  • Density ($\rho$) is related to pressure and temperature by the equation: $\rho = p / (RT)$
    • At constant temperature, an increase in pressure leads to an increase in density (compressed air tanks, scuba diving)
    • At constant pressure, an increase in temperature leads to a decrease in density (hot air balloons, convection currents)
  • In the atmosphere, density, pressure, and temperature vary with altitude due to the compressibility of air and the influence of gravity (troposphere, stratosphere)

Vertical Structure of the Atmosphere

Hydrostatic equilibrium in atmosphere

  • Hydrostatic equilibrium is a state in which the upward force of pressure gradient balances the downward force of gravity on a parcel of air
    • In hydrostatic equilibrium, there is no net vertical acceleration of air parcels (stable atmospheric conditions, stratified layers)
  • The hydrostatic equation describes this balance: $dp/dz = -\rho g$, where $dp/dz$ is the vertical pressure gradient, $\rho$ is density, and $g$ is gravitational acceleration
  • The hydrostatic equation explains why pressure decreases with altitude in the atmosphere
    • As altitude increases, the weight of the overlying air decreases, resulting in a decrease in pressure (mountain climbing, aircraft altimeters)

Factors in atmospheric temperature

  • Solar radiation is the primary source of energy for the Earth's atmosphere
    • The amount of solar radiation absorbed by the atmosphere varies with altitude, latitude, and the presence of clouds and aerosols (equatorial regions, polar regions)
  • Greenhouse gases, such as water vapor, carbon dioxide, and methane, absorb and re-emit infrared radiation, trapping heat in the lower atmosphere
    • The greenhouse effect contributes to the warming of the lower atmosphere and the cooling of the upper atmosphere (global warming, climate change)
  • Convection is the vertical transport of heat and moisture in the atmosphere
    • Convection occurs when air parcels become buoyant due to heating from the Earth's surface or the release of latent heat during condensation (thunderstorms, cumulus clouds)
    • Convection can lead to the formation of clouds and the vertical mixing of air, affecting the temperature profile of the atmosphere (atmospheric boundary layer, tropopause)

Implications of atmospheric profiles

  • Weather patterns are influenced by the vertical distribution of temperature, pressure, and density in the atmosphere
    • The formation of high and low-pressure systems, which drive wind patterns and precipitation, is related to the spatial variations in these variables (cyclones, anticyclones)
  • Air pollution dispersion is affected by atmospheric stability, which depends on the vertical temperature gradient
    • In a stable atmosphere, where temperature increases with altitude, vertical mixing is suppressed, leading to the accumulation of pollutants near the surface (temperature inversions, smog)
    • In an unstable atmosphere, where temperature decreases rapidly with altitude, vertical mixing is enhanced, promoting the dispersion of pollutants (clean air, good visibility)
  • Aviation is impacted by the decrease in air density and pressure with altitude
    • As air density decreases, aircraft require higher speeds to generate sufficient lift, affecting takeoff and landing performance (high-altitude airports, longer runways)
    • The decrease in pressure with altitude affects the operation of aircraft systems, such as pressurization and engine performance (cabin pressurization, turbine efficiency)