Lecture 9:Atmospheric temperature, pressure, density, and gases

Atmospheric Pressure

  • Humans experience approximately 1000 millibars (1 atmosphere) of pressure.

    • This pressure is due to the balance of air molecules pressing down against Earth’s surface.

    • Equilibrium is achieved where the pressure from blood and body tissues inside balances the external atmospheric pressure.

    • If there were no external pressure, bodily fluids would expand, potentially leading to severe complications like swelling.

Pressure at Altitude

  • Atmospheric pressure decreases with increasing altitude.

    • At 500 millibars, there is about half the air mass above this level compared to below.

    • At 50 kilometers in height, pressure can drop to 0.1 atmosphere (10 millibars), meaning 99.9% of the atmospheric mass is below you, and thus the sky can be considered about 50 kilometers thick.

The Scale of the Atmosphere

  • When comparing Earth's atmosphere to Earth's radius (approximately 6000 kilometers), the atmosphere is relatively thin.

    • Analogy: If Earth was represented as a basketball, the atmosphere would be akin to a thin sheet of paper.

  • All weather systems and life occur within this thin layer of the atmosphere.

Existence of the Atmosphere

  • Atmospheric pressure is highest at the surface due to gravity pulling gases downwards.

  • The balance between gravitational pull and the tendency of gaseous molecules to expand creates dynamic equilibrium.

Troposphere

  • The troposphere is the lowest layer of the atmosphere.

    • Its height is not fixed but varies with latitude.

    • The tropopause is the upper boundary of the troposphere, typically higher near the equator (around 10 km) and lower towards the poles (around 6 km).

  • Most air and weather phenomena occur within this layer.

    • Important atmospheric features include the polar and subtropical jets.

Heat Distribution in the Atmosphere

  • Heat distribution occurs through conduction and convection.

    • Conduction: Heat transfer through direct contact, which is very inefficient (example: hot sand feels cool until stepped on).

    • Convection: Heat transfer through the movement of air, which is highly efficient.

    • Example: On the Moon, without air to assist in convection, temperature gradients can reach extreme values of 500°C due to conduction alone.

    • On Earth, the temperature gradient from pole to equator is around 100°F due to the efficient movement of atmospheric masses.

Pressure Change with Height

  • As altitude increases, pressure decreases exponentially instead of linearly.

    • This is a key characteristic of gases in the atmosphere due to their compressibility.

    • Understanding exponential decay is similar to concepts like money growth in savings accounts and radioactive decay.

Adiabatic Processes

  • Adiabatic expansion occurs when air rises and cools without heat exchange with the environment.

    • When air expands, its temperature decreases.

    • Conversely, adiabatic compression happens when air is pushed down, causing an increase in temperature without heat input.

  • In atmospheric science, a parcel of air refers to a small volume used to study atmospheric phenomena.

Temperature and Density

  • In the atmosphere, temperature determines the density of air, with warmer air being less dense.

    • This principle explains the lapse rate, which is the temperature change with height in the atmosphere.

    • The lapse rate in the troposphere typically indicates a decrease in temperature with height.

Moisture in the Atmosphere

  • The presence of water vapor in the air changes its energy content.

    • Sensible heat: The heat that can be felt and measured (e.g., air temperature).

    • Latent heat: The heat absorbed or released during phase changes of water (e.g., evaporating vs. condensing).

    • The phase transition from liquid to vapor requires significant energy (540 calories/gram), emphasizing the importance of water vapor in temperature regulation.

Saturation of Air

  • The saturation point of air changes with temperature, with colder air being able to hold less moisture.

    • In winter, cold air leads to drier conditions, with the need for added moisture in indoor spaces.

    • When air is supersaturated, condensation occurs, resulting in precipitation or cloud formation.

Convection in the Atmosphere

  • Convection is essential for transferring heat vertically in the atmosphere, leading to weather patterns.

  • Warm air at the surface rises, cools, and expands, altering the moisture content.

  • This process results in the release of latent heat through condensation, which can further affect temperature and stability of the surrounding air.

Chemical Composition of the Atmosphere

  • The atmosphere consists of approximately 78% nitrogen (N₂), 21% oxygen (O₂), and trace amounts of other gases, including carbon dioxide (CO₂), which currently has about 420 parts per million.

    • CO₂ is a significant greenhouse gas and has been increasing due to human activity.

Seasonal Variation of CO₂ Levels

  • CO₂ levels fluctuate seasonally, typically peaking in late spring and declining in summer due to photosynthesis by vegetation.

    • Higher variability of CO₂ concentration is observed in the Northern Hemisphere due to larger landmasses and seasonal growth cycles.

  • The atmospheric CO₂ fluctuations illustrate the interconnected nature of biological processes and climate change.

Ozone Depletion

  • Certain gases, specifically chlorofluorocarbons (CFCs), contribute to ozone layer depletion, increasing skin cancer risks.

  • The discovery of the ozone hole involved measurements taken at the South Pole that revealed lower ozone concentrations previously unnoticed due to filtration errors in satellite data.

    • The scientific validation of this finding catalyzed international efforts to phase out CFC use and address ozone layer degradation.