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Precipitation
Occurs when water droplets or ice crystals grow large enough to overcome the updrafts of rising air that form clouds
Must fall to the ground and not evaporate
Types of Precipitation
Rain
Drizzle
Sleet
Freezing rain
Snow
Hail
Temperature Profile of the Atmosphere
Determines what type of precipitation reaches the ground
Typical Cloud Droplets
Are 10 micrometres in radius
Need to grow for precipitation to occur
Terminal velocity is 0.01 m/s
Typical Raindrops
Are 1000 micrometres (1 mm)
Terminal Velocity
Is reached when the force of gravity is balanced by air resistance in still air
Smaller drops have larger surface area to mass ratio, so smaller drops have slower terminal velocities
Stratiform Updraft Velocity
0.1 m/s
Cumulonimbus Updraft Velocity
10 m/s
Large Cloud Droplet Characteristics
Droplet radius → 50 micrometres
Terminal velocity → 0.3 m/s
Drizzle Characteristics
Droplet radius → 100 micrometres
Terminal velocity → 0.7 m/s
Typical Raindrop Characteristics
Droplet radius → 1.0 mm
Terminal velocity → 6.5 m/s
Large Raindrop Characteristics
Droplet radius → 2.0 mm
Terminal velocity → 10 m/s
Mechanisms by Which Droplets Grow in Clouds
Collision and coalescence
The Bergeron-Findeisen process
Collision & Coalescence
Happens in warm clouds, happens when temperature is above 0 degrees throughout
Large drops fall faster than small ones, collector drops grow by absorbing smaller drops
Are promoted by a variety of drop sizes
Collector Drops
Grow by absorbing smaller drops
Collision Efficiency
Probability that two drops will collide
Increases for larger collector drops, must be >20 micrometres in size or when drops are of similar size (or if they are smaller), they will be deflected if these conditions are not met
Coalescence Efficiency
Likelihood that two colliding drops will coalesce
Colliding drops do not always coalesce, it is more likely when drops are either very similar or different in size
Cloud Droplets Growth
Grow larger the longer they remain within the cloud
Thins Clouds
Produce small drops, such as drizzle
Deep Clouds
With strong updrafts, can enhance droplet growth and produce large drops
Cumulonimbus Clouds
Produce the largest drops
Cloud Temperature Between 0 deg C and -40 deg C
Contain both ice crystals and water droplets
Saturation Vapour Pressure is Higher
Over water than ice
Air can be saturated for ice but unsaturated for water
Water Droplets Shrink
Through net evaporation
Ice Crystals Grow
Through net deposition
Once Ice Crystals Reach a Certain Size Through Deposition
They are likely to grow by:
Accretion
Aggregation
Accretion
Ice crystals grow by colliding with supercooled water droplets
Droplets immediately freeze onto the ice crystal
Aggregation
Ice crystals grow by colliding with other ice crystals
All Cold Clouds
Are mostly ice
Temperature determines type of precipitation that reaches the ground
Virga
Streaks or shafts of precipitation (rain or snow) fall from a cloud base but evaporate or sublimate before reaching the ground
Air below is very dry so precipitation can evaporate
Sleet & Freezing Rain
When precipitation may melt in a warm layer, but then falls through a cold layer
If the cold layer is deep enough (>250 m), the precipitation will refreeze into ice pellets (sleet)
If the cold layer is shallow, the water may become supercooled (freezing rain) and rain freeze on contact
Layers of ice deposited on cold surfaces
Sleet is Likely to Form
When the cold layer is >250 m deep
Freezing Rain is Likely to Form
When the surface cold layer is <250 m deep
Hail
Begins with small ice particles. Is generally larger than 5 mm and considered severe when larger than 2 cm
Strong updrafts in cumulonimbus clouds cycle the particles through the cloud over and over
Growth occurs through accretion
Action of Forces that Result in Wind
Gravity
Pressure gradient
Coriolis force
Centripetal force
Friction
These forces explain the relationship between the winds we observe and the patterns of isobars or height contours on weather maps
Pressure Gradient (PG)
Is the change in pressure (P) over a distance (x)
Causes a pressure gradient force (PGF) directed from higher to lower pressure
Is directed from equator to pole
Pressure Gradient Force
Driving force of atmospheric motions
All other forces deflect or slow it down
Is the force that starts the movement of air
The Coriolis Force
Occurs due to Earth’s rotation
On a large scale, it causes freely moving objects to deviate from a straight path
Affects movements of air, water, aircraft, artillery shells that travel relatively quickly and/or over very long distances
Is dependent on latitude and wind speed
Produces upper-air westerlies
The Coriolis Force - Northern Hemisphere
Apparent force deflects moving objects to the right
The Coriolis Force - Southern Hemisphere
Apparent force deflects moving to the left
Earth’s Rotation at the Equator
Causes purely translational movement of the surface
Coriolis force is zero
The Coriolis Force - The Poles
Rotation causes purely rotational movement of the surface
Coriolis force is maximised
The Coriolis Force - In Between
Force is between zero and maximum
The Coriolis Parameter
Relates the strength of the force to the Earth’s rotation rate and latitude
Centripetal Force
Force required to keep an object moving along a curved path
Must be larger for faster objects
Must be larger for smaller radii
Frictional Force
Opposes movement
Increases with wind speed and surface roughness
Planetary Boundary Layer (PBL)
The lowest part of the troposphere, directly influenced by the Earth’s surface through turbulent exchange of heat, moisture, and momentum
Is near the surface where winds are slowed by friction
Is deeper for faster winds, rougher surfaces, unstable/rising air
Resulting Winds - As Air Accelerates
The effects of other forces will increase because they depend on wind speed
Feedback processes operate among the forces until they become balanced
Geostrophic Winds
Occur where friction is negligible, above the PBL
Resultant flow is parallel to the isobars, isobars are straight
When Isobars are Curved
Balance of forces must include CLF
Net force must be directed at the centre of rotation
Gradient Wind
Occurs above the PBL
Is the feedback between pressure gradient force (PGF), wind speed, and centripetal force (CF) keeps the flow parallel to isobars
Gradient Wind Around Areas of Low Pressure
Is cyclonic in nature
PGF begins acting against the wind, so winds around cyclones are slower than geostrophic winds (subgeostrophic)
Rotation is cyclonic and spins counter-clockwise in the Northern hemisphere and clockwise in the Southern hemisphere
Gradient Wind Around Areas of High Pressure
Is anticyclonic in nature
Centripetal forces (CF) begins to act against the wind, so winds around anticyclones are faster than geostrophic winds (subgeostrophic)
Rotation is anticyclonic and spins clockwise in the Northern hemisphere and counter-clockwise in the Southern hemisphere
Ridges
Are areas of high pressure in the upper atmosphere
Winds decelerate coming out (assuming a constant PGF)
Troughs
Are areas of low pressure in the upper atmosphere
Winds accelerate coming out (assuming a constant PGF)
As Air Slows Down
It converges
Area Downwind of a Ridge
There is speed convergence
This area is often associated with high pressure at the surface
As Air Speeds up
It diverges
Area Downwind of a Trough
There is speed divergence
This area is often associated with low pressure at the surface
Friction
Acts opposite of pressure gradient force (PGF), which reduces wind speed
Coriolis force is now weaker than pressure gradient force (PGF) as a result
Resultant wind crosses isobars at an angle
Surface Wind
Spirals into cyclones and out of anticyclone
Local Winds
Are caused by pressure differences that are linked to spatial differences in surface temperature due to:
Variations in surface properties (land and sea breezes)
Variations in terrain (mountain and valley winds)
Local Winds - Differences in Thermal Properties of Land & Water
Generate daytime sea breezes and night-time land breezes
Local Winds - Daytime Heating in High-Relief Terrain
Generates upslope anabatic winds and valley winds
Local Winds - Nocturnal Cooling
Generates downslope katabatic winds and mountain winds
Global Circulation - Theoretical Balance & Latitudinal Imbalance
Drives atmospheric circulation, and in turn oceanic circulation
Temperature gradient determines the strength of circulation
Latitudinal Radiation Imbalance
Dictates that there must be a poleward transfer of energy, there must also be poleward transfer of momentum (from tropical easterlies to mid-latitude westerlies)
Simplified Circulation on a Simple Earth
Surface pressure systems: low pressure at the equator and high pressure at the poles
Pressure patterns in the upper troposphere: high pressure at the equator and low pressure at the poles
Simplified Circulation on a Simple Earth in Rotation
Surface pressure systems: low pressure a the equator and mid-latitudes, high pressure at subtropics and poles
Pressure patterns in the upper troposphere: high pressure at the equator and low pressure at the poles
Earth’s Pressure Patterns Influences
Seasonal shifts in declination of the Sun
The location of large land masses Vs. bodies of water
Differences in heating of land and ocean
Topography
Tropical Circulation - The Hadley Cell
Is a thermally driven cell with warm air rising near the equator and colder air forced to descend and warm adiabatically in the subtropics
Mid-Latitude Westerlies (Extra-Tropical - Mid-Latitude Circulation)
Are produced by flow from subtropical highs northward towards subpolar lows
Polar Highs (Extra-Tropical - Polar Circulation)
Produce southward pressure gradient towards subpolar lows, which results in polar easterlies
Polar Easterlies
Are produced by polar highs producing southward pressure gradients towards subpolar lows
Regional Circulation - Monsoons
ITCZ migrates northward over Southeast Asia in the summer and southward over the Indian Ocean in the winter
Results in seasonally reversing wind patterns
Summertime onshore flows produce heavy rainfall
High Pressure Aloft
Created by air expanding upwards at the equator
Low Pressure Aloft
Created by air compressing downwards at the poles
The Subtropical Jet Streams
Form over the subtropical highs
Happen when poleward flow aloft becomes increasingly affected by Coriolis force and becomes westerly
Poleward movement brings air closer to the centre of rotation (Earth’s axis). Conservation of momentum causes velocity to greatly increase
Polar Jet Streams
Form along the Polar Front
The Polar Front
Is the boundary between cold/dry and warm/moist air masses
The Polar Front Jet Stream
Is created when large latitudinal temperature gradients generate strong pressure gradients
Are stronger in the winter due to greater temperature differences
Results in faster movement
Rossby Waves
Are associated with the polar front jet stream
Are 3 to 7 waves that are slowly circling the planet that increase and decrease in amplitude
Strongly influence mid-latitude weather due to occurrence of cyclonic activity
Ocean Currents
Account for about 1/3 of the poleward heat transfer from tropics to poles
Surface currents are driven by prevailing winds
Deep currents are driven by differences in density; called thermohaline circulation
Operate over a long time:
Lateral circulation ca. 1 year
Deep ocean circulation ca. 1000 years
Thermohaline Circulation
Deep currents driven by differences in density
Surface Currents
Friction between water layers transfer momentum to a depth of about 100 m (Coriolis force acts on each layer)
Layers at successive depths are deflected further, producing an Ekman spiral
Moves at ~45 degrees to the wind direction
Ekman Spiral
When layers of water currents at successive depths are deflected further away than normal
Describes how ocean water moves in layers, influenced by wind and the Coriolis effect, resulting in a spiral effect where water moves at different angles as you go deeper
Temperature & Salinity
Affect ocean water density
Downwelling
Occurs when water is more dense
Upwelling
Occurs when water is less dense
Primary Zones of Downwelling
North Atlantic Ocean
Southern Atlantic Ocean
Areas of Upwelling
Are less clear and poorly understood
Air Masses
Are large bodies of air with uniform temperature and moisture conditions
Develop over source regions where they adopt the characteristics of the land/water surfaces below
Migrate from different source regions and meet at transition zones known as fronts
Continental Arctic
Air-mass Symbol → cA
Characteristics → very cold and dry
Source region → arctic and antarctic (winter only)
Continental Antarctic
Air-mass → cAA
Characteristics → very stable
Source region → (winter only)
Continental Polar
Air-mass → cP
Characteristics → cold and dry, stable in winter but slightly unstable in summer
Source region → high-latitude continents and ice-covered oceans
Maritime Polar
Air-mass → mP
Characteristics → cool and moist, unstable
Source region → high-latitude oceans
Maritime Tropical
Air-mass → mT
Characteristics → warm and moist, unstable on west side of oceans, stable on east side of oceans
Source region → subtropical oceans
Continental Tropical
Air-mass → cT
Characteristics → hot and dry, very unstable
Source region → subtropical deserts (in the summer only in North America)
Source Regions - Winter Pattern
Continental arctic - very cold, dry, and stable
Continental polar - cold, dry, stable, and high pressure
Maritime polar - cool, humid, and unstable all year
Maritime tropical - warm, humid, and unstable
Source Regions - Summer Pattern
Continental tropical - hot, low relative humidity, stable aloft, and unstable at the surface
Continental polar - cool, dry, and moderately stable
Maritime polar - cool, humid, and unstable all year
Maritime tropical - warm, very humid, and very unstable