☁️Atmospheric Physics Unit 5 – Atmospheric Dynamics and Circulation
Atmospheric dynamics and circulation form the backbone of weather patterns and climate systems. These processes involve complex interactions between air pressure, temperature, and Earth's rotation, driving global wind patterns and weather phenomena.
Understanding atmospheric motion is crucial for predicting weather and climate change. From local sea breezes to global circulation patterns, these principles explain how energy moves through the atmosphere, shaping our planet's weather and climate systems.
Atmospheric motion is driven by differences in pressure, temperature, and density
Wind is the horizontal movement of air from high pressure to low pressure areas
Vertical motion in the atmosphere is caused by buoyancy forces and convection
Coriolis effect deflects wind to the right in the Northern Hemisphere and to the left in the Southern Hemisphere due to Earth's rotation
Geostrophic wind is a theoretical wind that results from the balance between the pressure gradient force and the Coriolis force
Flows parallel to isobars (lines of constant pressure) at a constant speed
Gradient wind is a more realistic approximation of wind flow that includes the effects of friction and centrifugal force
Thermal wind is the difference in geostrophic wind between two pressure levels, caused by horizontal temperature gradients
Thermodynamics and Stability
Atmospheric thermodynamics deals with the transfer of heat and energy in the atmosphere
First law of thermodynamics states that energy cannot be created or destroyed, only converted from one form to another
Second law of thermodynamics states that entropy always increases in a closed system
Adiabatic processes occur without heat exchange between a system and its surroundings (e.g., rising or sinking air parcels)
Dry adiabatic lapse rate (DALR) is the rate at which unsaturated air cools as it rises (~9.8°C/km)
Moist adiabatic lapse rate (MALR) is the rate at which saturated air cools as it rises (varies with temperature and pressure)
Atmospheric stability refers to the atmosphere's resistance to vertical motion
Stable atmosphere: air parcel displaced vertically will return to its original position
Unstable atmosphere: air parcel displaced vertically will continue to rise or sink
Conditionally unstable atmosphere: stability depends on the saturation state of the air parcel
Atmospheric Forces and Equations
Pressure gradient force (PGF) is the force that moves air from high to low pressure areas
Coriolis force is an apparent force caused by Earth's rotation that deflects moving objects to the right in the Northern Hemisphere and to the left in the Southern Hemisphere
Friction is a force that opposes motion and is most significant near the Earth's surface
Centrifugal force is an apparent outward force experienced by an object moving in a curved path
Hydrostatic balance is the balance between the vertical pressure gradient force and gravity in a stationary atmosphere
Hydrostatic equation: ∂z∂p=−ρg, where p is pressure, z is height, ρ is density, and g is gravitational acceleration
Equation of state relates pressure, density, and temperature in a gas: p=ρRdT, where Rd is the gas constant for dry air and T is temperature
Equations of motion describe the acceleration of air due to various forces (e.g., PGF, Coriolis, friction)
Global Circulation Patterns
Global circulation is driven by uneven heating of the Earth's surface and the rotation of the planet
Hadley cells are large-scale atmospheric circulations that transport heat from the equator to about 30° latitude
Rising motion near the equator, poleward flow aloft, descending motion around 30°, and equatorward flow near the surface
Ferrel cells are mid-latitude circulations that transport heat from about 30° to 60° latitude
Rising motion around 60°, equatorward flow aloft, descending motion around 30°, and poleward flow near the surface
Polar cells are small-scale circulations that transport cold air from the poles to about 60° latitude
Jet streams are fast-moving, narrow bands of strong winds in the upper troposphere that flow from west to east
Polar jet stream is located around 60° latitude and is stronger in the winter
Subtropical jet stream is located around 30° latitude and is stronger in the summer
Intertropical Convergence Zone (ITCZ) is a region near the equator where the trade winds converge, leading to rising motion, cloudiness, and precipitation
Synoptic-Scale Weather Systems
Synoptic-scale weather systems are large-scale systems (1,000-5,000 km) that can be identified on weather maps
Extratropical cyclones (mid-latitude cyclones) are low-pressure systems that form along frontal boundaries in the mid-latitudes
Characterized by counterclockwise rotation in the Northern Hemisphere and clockwise rotation in the Southern Hemisphere
Associated with fronts, precipitation, and strong winds
Anticyclones are high-pressure systems with clockwise rotation in the Northern Hemisphere and counterclockwise rotation in the Southern Hemisphere
Associated with descending motion, clear skies, and light winds
Fronts are boundaries between air masses with different temperatures and densities
Cold fronts occur when cold air advances and displaces warmer air, often associated with strong convection and severe weather
Warm fronts occur when warm air advances over colder air, often associated with steady precipitation and stratiform clouds
Occluded fronts form when a cold front overtakes a warm front, lifting the warm air off the surface
Upper-level troughs and ridges are disturbances in the upper-level flow that can influence surface weather patterns
Troughs are associated with lower pressure and rising motion
Ridges are associated with higher pressure and sinking motion
Mesoscale and Local Circulations
Mesoscale circulations are smaller-scale systems (10-1,000 km) that are influenced by local factors such as topography, land-sea contrasts, and urban heat islands
Sea and land breezes are diurnal circulations driven by temperature differences between land and water surfaces
Sea breeze: onshore flow during the day as land heats up faster than water
Land breeze: offshore flow at night as land cools down faster than water
Mountain and valley breezes are diurnal circulations driven by temperature differences between mountain slopes and valleys
Valley breeze: upslope flow during the day as mountain slopes heat up
Mountain breeze: downslope flow at night as mountain slopes cool down
Urban heat islands are areas of elevated temperature in cities compared to surrounding rural areas due to human activities and modified land surfaces
Thunderstorms are convective systems that develop in unstable environments with sufficient moisture and lifting mechanisms
Characterized by strong updrafts, downdrafts, lightning, and heavy precipitation
Tornadoes are violently rotating columns of air that extend from a thunderstorm to the ground
Associated with strong wind shear and specific types of thunderstorms (supercells)
Climate Dynamics and Variability
Climate is the long-term average of weather conditions in a given area
Climate variability refers to variations in climate on timescales ranging from months to decades
El Niño-Southern Oscillation (ENSO) is a coupled ocean-atmosphere phenomenon that affects global weather patterns
El Niño: warming of the eastern tropical Pacific Ocean, associated with increased precipitation in some regions and droughts in others
La Niña: cooling of the eastern tropical Pacific Ocean, often associated with opposite impacts to El Niño
North Atlantic Oscillation (NAO) is a fluctuation in atmospheric pressure differences between the Icelandic Low and the Azores High
Positive NAO: stronger pressure gradient, more intense and frequent storms in the North Atlantic
Negative NAO: weaker pressure gradient, fewer and weaker storms in the North Atlantic
Arctic Oscillation (AO) is a variation in atmospheric pressure patterns over the Arctic and mid-latitudes
Positive AO: lower pressure over the Arctic, higher pressure in mid-latitudes, and stronger westerly winds
Negative AO: higher pressure over the Arctic, lower pressure in mid-latitudes, and weaker westerly winds
Climate change refers to long-term changes in climate due to natural factors and human activities
Greenhouse gases (e.g., carbon dioxide, methane) trap heat in the atmosphere, leading to global warming
Impacts include rising sea levels, changes in precipitation patterns, more frequent and intense extreme weather events, and shifts in ecosystems
Atmospheric Modeling and Forecasting
Atmospheric models are mathematical representations of the atmosphere used for weather forecasting and climate simulations
Numerical weather prediction (NWP) models simulate the evolution of the atmosphere using the equations of motion and thermodynamics
Global models cover the entire Earth and have lower spatial resolution (e.g., GFS, ECMWF)
Regional models cover a limited area and have higher spatial resolution (e.g., WRF, NAM)
Data assimilation is the process of incorporating observations into atmospheric models to improve initial conditions and forecasts
Methods include 3D-Var, 4D-Var, and ensemble Kalman filtering
Ensemble forecasting involves running multiple model simulations with slightly different initial conditions or model physics to account for uncertainty
Ensemble mean and spread provide information about the most likely outcome and the range of possible outcomes
Model output statistics (MOS) are statistical techniques used to correct systematic biases in model forecasts based on past performance
Forecast verification is the process of evaluating the accuracy and skill of weather forecasts using various metrics
Measures include bias, root mean square error (RMSE), and anomaly correlation coefficient (ACC)
Climate models are used to simulate long-term changes in the Earth's climate system
Coupled atmosphere-ocean general circulation models (AOGCMs) include interactions between the atmosphere, oceans, land surface, and sea ice
Earth system models (ESMs) incorporate additional components such as the carbon cycle and dynamic vegetation