Lecture 7

R
The Atmosphere
The Blue Planet: Chapter 11
Outline
• The Habitable Planet
• Composition and Structure of our
Atmosphere
• Moisture in the Atmosphere
• The Atmosphere in the Earth System
The Habitable Planet
• The atmosphere is the gaseous envelope
that surrounds a celestial body
• Air is the invisible, odorless mixture of
gases and suspended particles that
surrounds Earth
• In addition to supporting life chemically, it
protects it, stores moisture and solar
energy and moves Earth materials
The Habitable Planet
• After accretion, Earth had a primordial or
primary atmosphere, which was stripped
away by solar winds early in solar system
history
• Little by little, through volcanic outgassing,
abundant volatiles were released to surface,
forming Earth’s secondary atmosphere
– Unlike today’s atmosphere, this would have
been composed of water vapor, methane,
hydrogen, nitrogen, carbon dioxide and argon
The Habitable Planet
The Habitable Planet
• Earth had virtually no oxygen in its
atmosphere more than 4 billion years ago,
and now it makes up 21%
• Traces of oxygen were probably generated
through breakdown of water molecules by
ultraviolet light
• Almost all the free oxygen originated through
photosynthesis
– The oxygen combined with other elements to
make compounds, eventually oxygenating the
atmosphere around 2.5 to 1.8 billion years ago
The Habitable Planet
The Habitable Planet
• The transition from an oxygen-poor to
an oxygen-rich atmosphere is recorded
in the alternating black (reduced) and
red (oxidized) banded iron formations
• With the buildup of molecular oxygen
came and eventual increase in ozone
– By absorbing harmful UV radiation, ozone
made it possible for life to flourish in
shallow water and finally on land
The Habitable Planet
• The critical stage in the evolution of the
atmosphere was reached between 1100 and
542 Ma
– Explosive diversification of life occurred 542 million
years ago
• Oxygen levels have fluctuated over the past 200
million years from 10% to 25%
• The other major chemical change in the
atmosphere was the removal of carbon dioxide
by sinking it into limestone and organic sediment
Outline
• The Habitable Planet
• Composition and Structure of our
Atmosphere
• Moisture in the Atmosphere
• The Atmosphere in the Earth System
Composition and Structure of
our Atmosphere
Composition and Structure of our
Atmosphere
• The air of our present day atmosphere
varies in composition from region to
region due to the presence of
– Aerosols: tiny suspended liquid or solid
particles
– Water vapor: humidity from evaporation
• The remaining “dry” gases in the
atmosphere are consistent
– Nitrogen, oxygen and argon
– Carbon dioxide, methane, ozone and NOx
Composition and Structure of
our Atmosphere
Composition and Structure of
our Atmosphere
Composition and Structure of
our Atmosphere
Composition and Structure of our
Atmosphere
• Two things energize the atmosphere
– The Sun’s energy
• Warms the atmosphere
• Energy source for clouds, rain, snowstorms,
wind, and weather
– The Earth’s rotation
• Axial tilt is responsible for seasons
• Large scale flow patterns in the atmosphere
– Jet stream, global wind patterns
Composition and Structure of our
Atmosphere
• There are 4 thermal layers of the
atmosphere, separated by pauses
– Troposphere: temperature decreases with
altitude, most of our weather occurs here
– Stratosphere: temperature increases with
altitude because of the presence of ozone
– Mesosphere: temperature decreases with
altitude, the coldest layer of the atmosphere
– Thermosphere: temperature increases with
altitude, reaches the highest temperatures,
hosts the ionosphere, where auroras occur
Composition and Structure of
our Atmosphere
Composition and Structure of
our Atmosphere
Composition and Structure of our
Atmosphere
• Air pressure is the force exerted by the
weight of the overlying air
– Air pressure decreases smoothly with
altitude
– Because air is highly compressible, 50% of
the of the atmosphere lies below 5.5 km,
99% lies below 32 km, the remaining 1%
extends from 32 km to 500 km
– It is measured with a barometer, and
changes can indicate imminent changes in
weather
Composition and Structure of
our Atmosphere
Composition and Structure of
our Atmosphere
Composition and Structure of
our Atmosphere
Outline
• The Habitable Planet
• Composition and Structure of our
Atmosphere
• Moisture in the Atmosphere
• The Atmosphere in the Earth System
Moisture in the Atmosphere
• Relative humidity
– When the number of molecules that evaporate
equals the number that condense, the vapor is
saturated, this is the dew point temperature
– The amount of water vapor in under-saturated air
is the relative humidity
– This is the ratio of the actual vapor pressure to
the saturation vapor pressure
– Temperature exerts a strong control on water
vapor capacity of air
Moisture in the Atmosphere
• Relative humidity can be changed
either by the addition of water vapor or
by a change in temperature
Moisture in the Atmosphere
• Adiabatic lapse rate
– When air is compressed, it warms
– When compressed air expands, it cools
– Warm air rises, but since air pressure
decreases, the air expands and cools
– Cool air descends, but with increased air
pressure it compresses and warms
– The rate of temperature change over these
processes is called
• Dry adiabatic lapse rate (unsaturated air)
• Moist adiabatic lapse rate (saturated air)
Moisture in the Atmosphere
Moisture in the Atmosphere
• Clouds are visible aggregates of minute
water droplets, ice crystals, or both
• They form when air rises and becomes
saturated with moisture in response to
adiabatic cooling and condensation
• There are four principal reasons for the
upward movement of air, which in turn
leads to the formation of clouds
Moisture in the Atmosphere
1. Density lifting
• Warm, low-density air rises convectively
1. Frontal lifting
• Two flowing air masses of different density
meet, one forcing the other up
1. Orographic lifting
• Flowing air is forced upward due to terrain
1. Convergence lifting
• Flowing air masses converge and are both
forced upward
Moisture in the Atmosphere
Moisture in the Atmosphere
• When the dew point is reached one of
two things happens
– Water condenses
– Ice crystals form
• These nucleation processes require
energy to form a new surface
– Nucleation sites may be
• The ground, aerosols
Moisture in the Atmosphere
Moisture in the Atmosphere
• Clouds are classified on the basis of
shape, appearance, and height
– Cumulus: puffy individual clouds, where
the flat base marks the condensation level
– Stratus: sheets of cloud cover spread
laterally rather than vertically
– Cirrus: highest of the clouds, wispy
feathers composed of ice crystals
– Nimbus: rain, as in cumulonimbus
Moisture in the Atmosphere
Moisture in the Atmosphere
Outline
• The Habitable Planet
• Composition and Structure of our
Atmosphere
• Moisture in the Atmosphere
• The Atmosphere in the Earth System
The Atmosphere in the Earth
System
• The atmosphere and the life zone
– Most organisms live in conditions of fairly
stable temperatures
– Humans need moist air for proper lung
function, and our brains, hearts, lungs,
livers, and digestive systems cannot
function within a +/- 2˚C temperature
variation
– Over 90% of the human population lives
where the annual mean temperature is
between 6˚C and 27˚C
The Atmosphere in the Earth
System
• Considering our total dependence on
air and the atmospheric blanket
maintaining conditions supportive of life,
one might expect us to know and care a
lot about the atmosphere
– A wide variety of anthropogenic
contaminants cause pollution at low levels
in the atmosphere
– Many common air pollutants are known to
have negative impacts on human and
ecosystem health
The Atmosphere in the Earth
System
• Today there is growing concern about
anthropogenic pollutants causing
changes in the concentration of
radiatively active gases in the
atmosphere, which, it is thought, will
lead to changes in the greenhouse
effect, and ultimately, global climatic
change
Extras
Extras
Extras
Extras
Wind and Weather Systems
The Blue Planet: Chapter 12
Outline
• Why Air Moves
• Global Air Circulation
• Regional Wind and Weather Systems
• Local Wind and Weather Systems
• Severe Weather
• Weather and the Earth System
Why Air Moves
• Weather is the state of the atmosphere at a
given time and place, determined by five
variables
1. Temperature
2. Air pressure
3. Humidity
4. Cloudiness
5. Wind speed and direction
• Weather is short-term, climate is long-term;
the average weather condition of a place
Why Air Moves
• Wind is air movement that arises from
differences in air pressure
– Flowing from an area of high pressure to an area
of low pressure
• Most places have wind speeds that average
between 10 and 30 km/hr
• In places where temperatures drop below
freezing, the windchill factor is reported
– This is a measure of the heat loss from exposed
skin due to low temperature and wind
Why Air Moves
Why Air Moves
• Wind speed and direction are affected
by three factors
1. Pressure-gradient force: drop in air
pressure per unit of distance
2. Coriolis force: the deviation from a
straight line of the path of a moving body
as a result of Earth’s rotation
3. Friction: the resistance to movement that
results when two bodies are in contact
Why Air Moves
• Pressure-gradient force
– Air always moves from an area of high
pressure to an area of low pressure, the
stronger the pressure gradient, the stronger
the resulting flow of air
– Places of equal air pressure are shown on
weather maps by lines called isobars
• Analogous to contour lines on topographic maps
• Isobars close together show a steep gradient
• Isobars far apart show a low gradient
Why Air Moves
Why Air Moves
• Coriolis force
– Includes all freely moving objects on the
surface of a rotating planet - such as wind
– The directions of all winds, like ocean
currents, are subject to this force
• Friction
– From topography, trees, and other solid
objects, friction slows the speed of wind
Why Air Moves
• Geostrophic winds
– Winds are always subject to more than one factor,
even the least complicated example
– A high-altitude wind, not in contact with the
ground, starts to flow due to air pressure gradient,
the Coriolis effect deflects the wind so that it is no
longer perpendicular to the isobars
– Eventually the pressure-gradient force and the
Coriolis effect are in balance, and the wind flows
parallel to the isobars
– This is a geostrophic wind
Why Air Moves
Why Air Moves
• The three effects interact such that winds
around a low-pressure center develop an
inward spiral motion (convergence, cyclone)
• By the same process, winds around a high-
pressure center develop an outward spiral
motion (divergence, anticyclone)
• In the northern hemisphere, convergent
centers rotate counterclockwise and
divergent centers rotate clockwise - the
reverse is true for the southern hemisphere
Why Air Moves
Why Air Moves
Why Air Moves
Outline
• Why Air Moves
• Global Air Circulation
• Regional Wind and Weather Systems
• Local Wind and Weather Systems
• Severe Weather
• Weather and the Earth System
Global Air Circulation
• Air masses, enormous volumes of air
driven by the pressure-gradient force
and the Coriolis force, are responsible
for our wind and weather systems
• Earth’s axial tilt, the Coriolis force, and
the solar heat imbalance, also means
that warm equatorial air must flow to the
poles and cold air to the equator in
several huge convection cells
Global Air Circulation
Global Air Circulation
Global Air Circulation
Global Air Circulation
• Hadley cells and the ITCZ
– Major circulatory cell that stretches from
the equator to 30˚ N and S latitude
– Warm air rises in the tropics and creates a
low-pressure zone of convergence (ITCZ)
– Air piles up here, creating two belts of high-
pressure air sinking towards the surface,
and creating a zone of divergence and
completing the convection cells
– Contains high-level winds: the westerlies
and low-level winds: the trade winds
Global Air Circulation
Global Air Circulation
• Ferrel cells
– On the poleward side of the Hadley cells
are midlatitude convection cells
– Surface winds are westerlies
• Polar fronts and Jet streams
– On the poleward side of the Ferrel cells,
meeting along a zone called a polar front
– Dry, high-altitude air descends near the
pole, creating a zone of divergence
Global Air Circulation
• Polar fronts and Jet streams
– Surface air then moves toward the equator,
forming the polar easterlies
– High-level winds in the polar cells are
westerly
– Upper atmosphere westerlies associated
with steep pressure gradient are called jet
streams
Global Air Circulation
Global Air Circulation
Outline
• Why Air Moves
• Global Air Circulation
• Regional Wind and Weather Systems
• Local Wind and Weather Systems
• Severe Weather
• Weather and the Earth System
Regional Wind and Weather
Systems
• Monsoons
– A seasonally reversing wind system
– Most distinct in Asia and Africa
– The controlling factor is the intertropical
convergence zone
• In India, ITCZ lies on the equator in winter and
moves north in summer, bringing with it
southwesterlies and warm, moisture-laden air
that result in humidity and torrential rains
Regional Wind and Weather
Systems
Regional Wind and Weather
Systems
• El Niño and the Southern Oscillation
– Off the coast of Peru, cold upwelling sustains
fishing grounds with nutrients
– Periodically a mass of unusually warm water
appears off the coast, when this happens, the
trade winds slacken, upwelling is reduced, fish
population declines and coastal birds die off
– Dry parts of Peru receive heavy rains, Australia
experiences drought conditions, and cyclones
appear in Hawaii and French Polynesia
Regional Wind and Weather
Systems
• El Niño and the Southern Oscillation
– There is a link between El Niño and changing
atmospheric pressure anomalies over the equator,
the Southern Oscillation
• A periodic variation in air pressure differential across the
tropical Pacific
– Which disrupts the Walker circulation wind pattern
– During an El Niño event, the pressure differential
weakens, weakening the Walker circulation and the
trade winds, which allows anomalously warm
surface water to accumulate and stop cold
upwelling
Regional Wind and Weather
Systems
Regional Wind and Weather
Systems
Regional Wind and Weather
Systems
Outline
• Why Air Moves
• Global Air Circulation
• Regional Wind and Weather Systems
• Local Wind and Weather Systems
• Severe Weather
• Weather and the Earth System
Local Wind and Weather Systems
• Coupled local wind systems
– Near coasts, the land heats up more
rapidly than the sea during the day, and
causes air to heat up and expand
– This develops a pressure gradient, and air
flows onto the land, creating a sea breeze
– An upper level reverse flow sets in, forming
a convection cell
– During the night, heat is radiated more
rapidly from the land and the situation
reverses, creating a land breeze
Local Wind and Weather Systems
Local Wind and Weather Systems
• Kabatic wind: high-speed, cold wind
– The flow of cold, dense air under the
influence of gravity
– Occur in places where a mass of cold air
accumulates over a high plateau or valley
• Chinook wind: warm, dry wind
– Strong regional winds rise and compress
higher-level air masses as they pass over
a mountain range, forcing the air
downslope, it warms as it compresses
Outline
• Why Air Moves
• Global Air Circulation
• Regional Wind and Weather Systems
• Local Wind and Weather Systems
• Severe Weather
• Weather and the Earth System
Severe Weather
• Cyclones
– Refers to any cyclonic circulating wind
system around a low-pressure center
• Wave cyclones
– Extratropical or midlatitude cyclones
– Form between 30˚ and 60˚ N and S
– Up to 2000 km across
– Last many days, responsible for most
everyday weather events in the midlatitude
regions of the world
Severe Weather
Severe Weather
• Tropical cyclones
– A hurricane or tropical storm that develops at
5˚N or S or higher when sea-surface
temperature is 26.5˚C or higher
– Draws energy from the water, so wind speeds
quickly diminish when it moves on shore
– Most hurricane damage occurs within 250 km
of the coast
• Wind damage, storm surge, and torrential rain
Severe Weather
Severe Weather
Severe Weather
• Thunderstorms
– Develop when an updraft of warm, humid
air releases a lot of latent heat very quickly
and becomes unstable
– Most form along cold fronts, pulling in
warm, moist air, releasing more heat and
intensifying updrafts
– Cumulonimbus clouds form and heavy
rainfall, hail, thunder and lightening result
Severe Weather
Severe Weather
• Tornadoes
– Violent windstorms produced by a spiraling
column of air that extends downward from a
cumulonimbus cloud
– Develop from large thunderstorms that have
multiple updrafts (supercell thunderstorms)
– Approximately funnel shaped
– Tornado activity from April to August
– Small relative to the thunderstorms they are
associated with, but incredibly violent and
destructive
Severe Weather
Severe Weather
Severe Weather
• Drought
– A region experiencing below-average
rainfall for an extended period
• Often with emphasis on affected water supply
or harvests
– Semi-arid areas adjacent to deserts are
highly susceptible to drought
– The expansion of desert conditions into
adjacent areas is called desertification
• Due to natural causes (drought)
• Overgrazing and poor land-use practices
Severe Weather
Severe Weather
Severe Weather
• Dust storms
– Once in the air, dust constitutes the wind’s
suspended load
– Grains of dust are tossed around in eddies
– Strong winds associated with large dust
storms can carry very fine dust into the
upper troposphere
– Most frequent in arid and semi-arid areas
• Related to cycles of drought
Severe Weather
Severe Weather
Outline
• Why Air Moves
• Global Air Circulation
• Regional Wind and Weather Systems
• Local Wind and Weather Systems
• Severe Weather
• Weather and the Earth System
Weather and the Earth System
• Weather and climate are sensitive
indicators of changes in the Earth
system as a whole
• Effects from small differences can
propagate quickly due to feedbacks
• Earth’s weather system is full of
feedbacks, both positive and negative
– Prolonged drought -> vegetation dies ->
dust storm
Weather and the Earth System
• In a positive feedback situation, a
prolonged drought might reach a point
where it becomes impossible to recover to
its former state
• A new drier “normal” would be established
• This is a threshold situation, meaning a
system can handle and respond to changes
by returning to its starting point, but only up
to a certain point
Extras
Extras
Extras
Extras
Extras
Extras
Extras
Extras
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Lecture 7

  • 1. The Atmosphere The Blue Planet: Chapter 11
  • 2. Outline • The Habitable Planet • Composition and Structure of our Atmosphere • Moisture in the Atmosphere • The Atmosphere in the Earth System
  • 3. The Habitable Planet • The atmosphere is the gaseous envelope that surrounds a celestial body • Air is the invisible, odorless mixture of gases and suspended particles that surrounds Earth • In addition to supporting life chemically, it protects it, stores moisture and solar energy and moves Earth materials
  • 4. The Habitable Planet • After accretion, Earth had a primordial or primary atmosphere, which was stripped away by solar winds early in solar system history • Little by little, through volcanic outgassing, abundant volatiles were released to surface, forming Earth’s secondary atmosphere – Unlike today’s atmosphere, this would have been composed of water vapor, methane, hydrogen, nitrogen, carbon dioxide and argon
  • 6. The Habitable Planet • Earth had virtually no oxygen in its atmosphere more than 4 billion years ago, and now it makes up 21% • Traces of oxygen were probably generated through breakdown of water molecules by ultraviolet light • Almost all the free oxygen originated through photosynthesis – The oxygen combined with other elements to make compounds, eventually oxygenating the atmosphere around 2.5 to 1.8 billion years ago
  • 8. The Habitable Planet • The transition from an oxygen-poor to an oxygen-rich atmosphere is recorded in the alternating black (reduced) and red (oxidized) banded iron formations • With the buildup of molecular oxygen came and eventual increase in ozone – By absorbing harmful UV radiation, ozone made it possible for life to flourish in shallow water and finally on land
  • 9. The Habitable Planet • The critical stage in the evolution of the atmosphere was reached between 1100 and 542 Ma – Explosive diversification of life occurred 542 million years ago • Oxygen levels have fluctuated over the past 200 million years from 10% to 25% • The other major chemical change in the atmosphere was the removal of carbon dioxide by sinking it into limestone and organic sediment
  • 10. Outline • The Habitable Planet • Composition and Structure of our Atmosphere • Moisture in the Atmosphere • The Atmosphere in the Earth System
  • 11. Composition and Structure of our Atmosphere
  • 12. Composition and Structure of our Atmosphere • The air of our present day atmosphere varies in composition from region to region due to the presence of – Aerosols: tiny suspended liquid or solid particles – Water vapor: humidity from evaporation • The remaining “dry” gases in the atmosphere are consistent – Nitrogen, oxygen and argon – Carbon dioxide, methane, ozone and NOx
  • 13. Composition and Structure of our Atmosphere
  • 14. Composition and Structure of our Atmosphere
  • 15. Composition and Structure of our Atmosphere
  • 16. Composition and Structure of our Atmosphere • Two things energize the atmosphere – The Sun’s energy • Warms the atmosphere • Energy source for clouds, rain, snowstorms, wind, and weather – The Earth’s rotation • Axial tilt is responsible for seasons • Large scale flow patterns in the atmosphere – Jet stream, global wind patterns
  • 17. Composition and Structure of our Atmosphere • There are 4 thermal layers of the atmosphere, separated by pauses – Troposphere: temperature decreases with altitude, most of our weather occurs here – Stratosphere: temperature increases with altitude because of the presence of ozone – Mesosphere: temperature decreases with altitude, the coldest layer of the atmosphere – Thermosphere: temperature increases with altitude, reaches the highest temperatures, hosts the ionosphere, where auroras occur
  • 18. Composition and Structure of our Atmosphere
  • 19. Composition and Structure of our Atmosphere
  • 20. Composition and Structure of our Atmosphere • Air pressure is the force exerted by the weight of the overlying air – Air pressure decreases smoothly with altitude – Because air is highly compressible, 50% of the of the atmosphere lies below 5.5 km, 99% lies below 32 km, the remaining 1% extends from 32 km to 500 km – It is measured with a barometer, and changes can indicate imminent changes in weather
  • 21. Composition and Structure of our Atmosphere
  • 22. Composition and Structure of our Atmosphere
  • 23. Composition and Structure of our Atmosphere
  • 24. Outline • The Habitable Planet • Composition and Structure of our Atmosphere • Moisture in the Atmosphere • The Atmosphere in the Earth System
  • 25. Moisture in the Atmosphere • Relative humidity – When the number of molecules that evaporate equals the number that condense, the vapor is saturated, this is the dew point temperature – The amount of water vapor in under-saturated air is the relative humidity – This is the ratio of the actual vapor pressure to the saturation vapor pressure – Temperature exerts a strong control on water vapor capacity of air
  • 26. Moisture in the Atmosphere • Relative humidity can be changed either by the addition of water vapor or by a change in temperature
  • 27. Moisture in the Atmosphere • Adiabatic lapse rate – When air is compressed, it warms – When compressed air expands, it cools – Warm air rises, but since air pressure decreases, the air expands and cools – Cool air descends, but with increased air pressure it compresses and warms – The rate of temperature change over these processes is called • Dry adiabatic lapse rate (unsaturated air) • Moist adiabatic lapse rate (saturated air)
  • 28. Moisture in the Atmosphere
  • 29. Moisture in the Atmosphere • Clouds are visible aggregates of minute water droplets, ice crystals, or both • They form when air rises and becomes saturated with moisture in response to adiabatic cooling and condensation • There are four principal reasons for the upward movement of air, which in turn leads to the formation of clouds
  • 30. Moisture in the Atmosphere 1. Density lifting • Warm, low-density air rises convectively 1. Frontal lifting • Two flowing air masses of different density meet, one forcing the other up 1. Orographic lifting • Flowing air is forced upward due to terrain 1. Convergence lifting • Flowing air masses converge and are both forced upward
  • 31. Moisture in the Atmosphere
  • 32. Moisture in the Atmosphere • When the dew point is reached one of two things happens – Water condenses – Ice crystals form • These nucleation processes require energy to form a new surface – Nucleation sites may be • The ground, aerosols
  • 33. Moisture in the Atmosphere
  • 34. Moisture in the Atmosphere • Clouds are classified on the basis of shape, appearance, and height – Cumulus: puffy individual clouds, where the flat base marks the condensation level – Stratus: sheets of cloud cover spread laterally rather than vertically – Cirrus: highest of the clouds, wispy feathers composed of ice crystals – Nimbus: rain, as in cumulonimbus
  • 35. Moisture in the Atmosphere
  • 36. Moisture in the Atmosphere
  • 37. Outline • The Habitable Planet • Composition and Structure of our Atmosphere • Moisture in the Atmosphere • The Atmosphere in the Earth System
  • 38. The Atmosphere in the Earth System • The atmosphere and the life zone – Most organisms live in conditions of fairly stable temperatures – Humans need moist air for proper lung function, and our brains, hearts, lungs, livers, and digestive systems cannot function within a +/- 2˚C temperature variation – Over 90% of the human population lives where the annual mean temperature is between 6˚C and 27˚C
  • 39. The Atmosphere in the Earth System • Considering our total dependence on air and the atmospheric blanket maintaining conditions supportive of life, one might expect us to know and care a lot about the atmosphere – A wide variety of anthropogenic contaminants cause pollution at low levels in the atmosphere – Many common air pollutants are known to have negative impacts on human and ecosystem health
  • 40. The Atmosphere in the Earth System • Today there is growing concern about anthropogenic pollutants causing changes in the concentration of radiatively active gases in the atmosphere, which, it is thought, will lead to changes in the greenhouse effect, and ultimately, global climatic change
  • 45. Wind and Weather Systems The Blue Planet: Chapter 12
  • 46. Outline • Why Air Moves • Global Air Circulation • Regional Wind and Weather Systems • Local Wind and Weather Systems • Severe Weather • Weather and the Earth System
  • 47. Why Air Moves • Weather is the state of the atmosphere at a given time and place, determined by five variables 1. Temperature 2. Air pressure 3. Humidity 4. Cloudiness 5. Wind speed and direction • Weather is short-term, climate is long-term; the average weather condition of a place
  • 48. Why Air Moves • Wind is air movement that arises from differences in air pressure – Flowing from an area of high pressure to an area of low pressure • Most places have wind speeds that average between 10 and 30 km/hr • In places where temperatures drop below freezing, the windchill factor is reported – This is a measure of the heat loss from exposed skin due to low temperature and wind
  • 50. Why Air Moves • Wind speed and direction are affected by three factors 1. Pressure-gradient force: drop in air pressure per unit of distance 2. Coriolis force: the deviation from a straight line of the path of a moving body as a result of Earth’s rotation 3. Friction: the resistance to movement that results when two bodies are in contact
  • 51. Why Air Moves • Pressure-gradient force – Air always moves from an area of high pressure to an area of low pressure, the stronger the pressure gradient, the stronger the resulting flow of air – Places of equal air pressure are shown on weather maps by lines called isobars • Analogous to contour lines on topographic maps • Isobars close together show a steep gradient • Isobars far apart show a low gradient
  • 53. Why Air Moves • Coriolis force – Includes all freely moving objects on the surface of a rotating planet - such as wind – The directions of all winds, like ocean currents, are subject to this force • Friction – From topography, trees, and other solid objects, friction slows the speed of wind
  • 54. Why Air Moves • Geostrophic winds – Winds are always subject to more than one factor, even the least complicated example – A high-altitude wind, not in contact with the ground, starts to flow due to air pressure gradient, the Coriolis effect deflects the wind so that it is no longer perpendicular to the isobars – Eventually the pressure-gradient force and the Coriolis effect are in balance, and the wind flows parallel to the isobars – This is a geostrophic wind
  • 56. Why Air Moves • The three effects interact such that winds around a low-pressure center develop an inward spiral motion (convergence, cyclone) • By the same process, winds around a high- pressure center develop an outward spiral motion (divergence, anticyclone) • In the northern hemisphere, convergent centers rotate counterclockwise and divergent centers rotate clockwise - the reverse is true for the southern hemisphere
  • 60. Outline • Why Air Moves • Global Air Circulation • Regional Wind and Weather Systems • Local Wind and Weather Systems • Severe Weather • Weather and the Earth System
  • 61. Global Air Circulation • Air masses, enormous volumes of air driven by the pressure-gradient force and the Coriolis force, are responsible for our wind and weather systems • Earth’s axial tilt, the Coriolis force, and the solar heat imbalance, also means that warm equatorial air must flow to the poles and cold air to the equator in several huge convection cells
  • 65. Global Air Circulation • Hadley cells and the ITCZ – Major circulatory cell that stretches from the equator to 30˚ N and S latitude – Warm air rises in the tropics and creates a low-pressure zone of convergence (ITCZ) – Air piles up here, creating two belts of high- pressure air sinking towards the surface, and creating a zone of divergence and completing the convection cells – Contains high-level winds: the westerlies and low-level winds: the trade winds
  • 67. Global Air Circulation • Ferrel cells – On the poleward side of the Hadley cells are midlatitude convection cells – Surface winds are westerlies • Polar fronts and Jet streams – On the poleward side of the Ferrel cells, meeting along a zone called a polar front – Dry, high-altitude air descends near the pole, creating a zone of divergence
  • 68. Global Air Circulation • Polar fronts and Jet streams – Surface air then moves toward the equator, forming the polar easterlies – High-level winds in the polar cells are westerly – Upper atmosphere westerlies associated with steep pressure gradient are called jet streams
  • 71. Outline • Why Air Moves • Global Air Circulation • Regional Wind and Weather Systems • Local Wind and Weather Systems • Severe Weather • Weather and the Earth System
  • 72. Regional Wind and Weather Systems • Monsoons – A seasonally reversing wind system – Most distinct in Asia and Africa – The controlling factor is the intertropical convergence zone • In India, ITCZ lies on the equator in winter and moves north in summer, bringing with it southwesterlies and warm, moisture-laden air that result in humidity and torrential rains
  • 73. Regional Wind and Weather Systems
  • 74. Regional Wind and Weather Systems • El Niño and the Southern Oscillation – Off the coast of Peru, cold upwelling sustains fishing grounds with nutrients – Periodically a mass of unusually warm water appears off the coast, when this happens, the trade winds slacken, upwelling is reduced, fish population declines and coastal birds die off – Dry parts of Peru receive heavy rains, Australia experiences drought conditions, and cyclones appear in Hawaii and French Polynesia
  • 75. Regional Wind and Weather Systems • El Niño and the Southern Oscillation – There is a link between El Niño and changing atmospheric pressure anomalies over the equator, the Southern Oscillation • A periodic variation in air pressure differential across the tropical Pacific – Which disrupts the Walker circulation wind pattern – During an El Niño event, the pressure differential weakens, weakening the Walker circulation and the trade winds, which allows anomalously warm surface water to accumulate and stop cold upwelling
  • 76. Regional Wind and Weather Systems
  • 77. Regional Wind and Weather Systems
  • 78. Regional Wind and Weather Systems
  • 79. Outline • Why Air Moves • Global Air Circulation • Regional Wind and Weather Systems • Local Wind and Weather Systems • Severe Weather • Weather and the Earth System
  • 80. Local Wind and Weather Systems • Coupled local wind systems – Near coasts, the land heats up more rapidly than the sea during the day, and causes air to heat up and expand – This develops a pressure gradient, and air flows onto the land, creating a sea breeze – An upper level reverse flow sets in, forming a convection cell – During the night, heat is radiated more rapidly from the land and the situation reverses, creating a land breeze
  • 81. Local Wind and Weather Systems
  • 82. Local Wind and Weather Systems • Kabatic wind: high-speed, cold wind – The flow of cold, dense air under the influence of gravity – Occur in places where a mass of cold air accumulates over a high plateau or valley • Chinook wind: warm, dry wind – Strong regional winds rise and compress higher-level air masses as they pass over a mountain range, forcing the air downslope, it warms as it compresses
  • 83. Outline • Why Air Moves • Global Air Circulation • Regional Wind and Weather Systems • Local Wind and Weather Systems • Severe Weather • Weather and the Earth System
  • 84. Severe Weather • Cyclones – Refers to any cyclonic circulating wind system around a low-pressure center • Wave cyclones – Extratropical or midlatitude cyclones – Form between 30˚ and 60˚ N and S – Up to 2000 km across – Last many days, responsible for most everyday weather events in the midlatitude regions of the world
  • 86. Severe Weather • Tropical cyclones – A hurricane or tropical storm that develops at 5˚N or S or higher when sea-surface temperature is 26.5˚C or higher – Draws energy from the water, so wind speeds quickly diminish when it moves on shore – Most hurricane damage occurs within 250 km of the coast • Wind damage, storm surge, and torrential rain
  • 89. Severe Weather • Thunderstorms – Develop when an updraft of warm, humid air releases a lot of latent heat very quickly and becomes unstable – Most form along cold fronts, pulling in warm, moist air, releasing more heat and intensifying updrafts – Cumulonimbus clouds form and heavy rainfall, hail, thunder and lightening result
  • 91. Severe Weather • Tornadoes – Violent windstorms produced by a spiraling column of air that extends downward from a cumulonimbus cloud – Develop from large thunderstorms that have multiple updrafts (supercell thunderstorms) – Approximately funnel shaped – Tornado activity from April to August – Small relative to the thunderstorms they are associated with, but incredibly violent and destructive
  • 94. Severe Weather • Drought – A region experiencing below-average rainfall for an extended period • Often with emphasis on affected water supply or harvests – Semi-arid areas adjacent to deserts are highly susceptible to drought – The expansion of desert conditions into adjacent areas is called desertification • Due to natural causes (drought) • Overgrazing and poor land-use practices
  • 97. Severe Weather • Dust storms – Once in the air, dust constitutes the wind’s suspended load – Grains of dust are tossed around in eddies – Strong winds associated with large dust storms can carry very fine dust into the upper troposphere – Most frequent in arid and semi-arid areas • Related to cycles of drought
  • 100. Outline • Why Air Moves • Global Air Circulation • Regional Wind and Weather Systems • Local Wind and Weather Systems • Severe Weather • Weather and the Earth System
  • 101. Weather and the Earth System • Weather and climate are sensitive indicators of changes in the Earth system as a whole • Effects from small differences can propagate quickly due to feedbacks • Earth’s weather system is full of feedbacks, both positive and negative – Prolonged drought -> vegetation dies -> dust storm
  • 102. Weather and the Earth System • In a positive feedback situation, a prolonged drought might reach a point where it becomes impossible to recover to its former state • A new drier “normal” would be established • This is a threshold situation, meaning a system can handle and respond to changes by returning to its starting point, but only up to a certain point
  • 103. Extras
  • 104. Extras
  • 105. Extras
  • 106. Extras
  • 107. Extras
  • 108. Extras
  • 109. Extras
  • 110. Extras