☁️Atmospheric Physics Unit 1 – Atmospheric Composition and Structure
The atmosphere is a complex mixture of gases and particles surrounding Earth, structured in layers with distinct properties. Understanding its composition and structure is crucial for grasping weather patterns, climate dynamics, and the delicate balance that sustains life on our planet.
From the troposphere near the surface to the exosphere at the edge of space, each atmospheric layer plays a unique role. The interplay of temperature, pressure, and density variations with altitude shapes atmospheric processes, influencing everything from ozone protection to global circulation patterns.
Atmosphere consists of a mixture of gases, aerosols, and other particles surrounding Earth
Atmospheric composition refers to the types and amounts of gases and particles present in the atmosphere
Atmospheric structure describes the vertical layers of the atmosphere based on temperature variations (troposphere, stratosphere, mesosphere, thermosphere, exosphere)
Atmospheric pressure is the force exerted by the weight of the atmosphere on a unit area
Decreases with increasing altitude due to less air above
Atmospheric density is the mass of air per unit volume
Also decreases with increasing altitude
Atmospheric scale height is the vertical distance over which pressure decreases by a factor of e (approximately 7 km)
Hydrostatic equilibrium is the balance between the upward pressure gradient force and downward gravitational force in the atmosphere
Atmospheric Layers and Their Properties
Troposphere is the lowest layer extending from Earth's surface to an average height of 12 km
Contains 75-80% of the atmosphere's mass and nearly all water vapor and aerosols
Characterized by a decrease in temperature with increasing altitude (negative lapse rate)
Stratosphere extends from the tropopause to about 50 km
Contains the ozone layer which absorbs harmful ultraviolet radiation
Characterized by an increase in temperature with altitude due to ozone heating
Mesosphere extends from the stratopause to about 85 km
Coldest layer with temperatures decreasing with altitude
Noctilucent clouds can form at the top of this layer
Thermosphere extends from the mesopause to about 500 km
Characterized by a rapid increase in temperature with altitude due to absorption of solar radiation by oxygen and nitrogen
Ionosphere is a region within the thermosphere containing electrically charged particles
Exosphere is the outermost layer extending from the thermopause to about 10,000 km
Extremely low density where particles can escape Earth's gravitational pull
Chemical Composition of the Atmosphere
Dry air is composed primarily of nitrogen (78%) and oxygen (21%) by volume
Argon (0.93%), carbon dioxide (0.04%), and trace gases make up the remainder
Water vapor is a highly variable component (0-4% by volume) with higher concentrations in the lower troposphere
Ozone is a critical trace gas in the stratosphere that absorbs ultraviolet radiation
Ozone layer protects life on Earth from harmful UV rays
Aerosols are solid or liquid particles suspended in the atmosphere
Can be natural (dust, sea salt) or anthropogenic (sulfates, nitrates from pollution)
Play important roles in cloud formation, radiation balance, and air quality
Greenhouse gases (carbon dioxide, water vapor, methane, nitrous oxide) absorb and emit infrared radiation
Increasing concentrations due to human activities are driving global climate change
Vertical Structure and Temperature Profile
Temperature varies with altitude in the atmosphere due to different heating and cooling processes
Troposphere exhibits a negative lapse rate (temperature decrease with height) of about 6.5°C/km
Caused by adiabatic cooling as air parcels expand and rise
Tropopause is the boundary between the troposphere and stratosphere
Marked by a temperature inversion where the lapse rate changes sign
Stratospheric temperature increases with altitude due to ozone heating
Positive lapse rate creates a stable layer with little vertical mixing
Mesosphere exhibits a negative lapse rate with the coldest temperatures at the mesopause (~-90°C)
Thermospheric temperature increases rapidly with altitude due to absorption of solar UV and X-ray radiation
Can reach over 1000°C but feels cold due to extremely low density
Atmospheric Pressure and Density
Atmospheric pressure decreases exponentially with altitude following the barometric formula
P(z)=P0exp(−z/H), where P0 is surface pressure, z is altitude, and H is scale height
Sea-level pressure averages around 1013 hPa (1 atm) but varies with weather systems
High pressure systems have sinking air and clear skies
Low pressure systems have rising air and stormy weather
Atmospheric density also decreases exponentially with altitude
Density is related to pressure by the ideal gas law: P=ρRsT
Scale height is the e-folding distance for pressure and density
Varies with temperature (higher scale height in warmer air)
Hydrostatic balance is the equilibrium between the vertical pressure gradient force and gravity
dP/dz=−ρg, where ρ is density and g is gravitational acceleration
Energy Balance and Radiative Transfer
Earth's climate is driven by the balance between incoming solar radiation and outgoing terrestrial radiation
Incoming shortwave radiation is mostly in the visible and near-infrared
Outgoing longwave radiation is in the thermal infrared
Albedo is the fraction of incoming solar radiation reflected back to space
Varies with surface type (higher for snow and ice, lower for oceans and forests)
Greenhouse effect is the trapping of outgoing infrared radiation by atmospheric gases
Warms the surface and lower atmosphere compared to a transparent atmosphere
Radiative transfer equation describes the change in radiation intensity along a path
Includes absorption, emission, and scattering processes
Absorption and emission of radiation by gases depend on their molecular structure and wavelength
H2O, CO2, O3 are important absorbers in the thermal infrared
Scattering of radiation by air molecules and aerosols affects the transmission of light
Rayleigh scattering by molecules is stronger at shorter (blue) wavelengths
Mie scattering by aerosols is more wavelength-independent
Atmospheric Dynamics and Circulation
Atmospheric motion is driven by pressure gradients, Coriolis force, and friction
Pressure gradient force points from high to low pressure
Coriolis force is an apparent force due to Earth's rotation (deflects to the right in the Northern Hemisphere)
Geostrophic balance is the equilibrium between pressure gradient force and Coriolis force
Results in parallel flow along isobars (lines of constant pressure)
General circulation of the atmosphere is characterized by three main cell types
Hadley cells are thermally direct circulations in the tropics (rising near equator, sinking in subtropics)
Ferrel cells are thermally indirect circulations in the mid-latitudes (rising in subpolar regions, sinking in subtropics)
Polar cells are thermally direct circulations at high latitudes (rising in subpolar regions, sinking over poles)
Jet streams are narrow bands of strong upper-level winds
Polar jet stream is associated with the polar front (boundary between cold polar air and warm subtropical air)
Subtropical jet stream is associated with the descending branch of the Hadley cell
Rossby waves are large-scale meandering patterns in the upper-level flow
Caused by the variation of Coriolis force with latitude (beta effect)
Play a key role in the development and propagation of weather systems
Measurement Techniques and Instrumentation
Surface observations provide direct measurements of atmospheric variables at fixed locations
Include temperature, pressure, humidity, wind speed and direction, precipitation
Automated weather stations and human observers contribute to global observing network
Radiosondes are balloon-borne instruments that measure vertical profiles of atmospheric properties
Launched twice daily at hundreds of sites worldwide
Provide crucial input data for weather forecasting models
Radar and lidar are active remote sensing techniques that use electromagnetic waves to probe the atmosphere
Weather radars measure precipitation and wind velocity
Doppler lidars measure wind speed and turbulence
Satellites provide global coverage of atmospheric observations from space
Geostationary satellites (GOES) provide continuous imagery over a fixed area
Polar-orbiting satellites (NOAA, NASA) provide global coverage with varying overpass times
Instruments include radiometers, spectrometers, and sounders for measuring temperature, moisture, and composition
Aircraft and drones are mobile platforms for atmospheric measurements
Research aircraft are equipped with a wide range of in-situ and remote sensing instruments
Drones (UAVs) offer flexibility and high-resolution sampling in the lower atmosphere