Atmospheric Physics

☁️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.

Key Concepts and Definitions

  • 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 ee (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)P(z) = P_0 \exp(-z/H), where P0P_0 is surface pressure, zz is altitude, and HH 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=ρRsTP = \rho R_s T
  • 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=ρgdP/dz = -\rho g, where ρ\rho is density and gg 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


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© 2024 Fiveable Inc. All rights reserved.
AP® and SAT® are trademarks registered by the College Board, which is not affiliated with, and does not endorse this website.
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