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.