Chapter 6: Air-sea interaction
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Transcript Chapter 6: Air-sea interaction
Seasons
Earth’s axis of rotation
tilted with respect to
ecliptic orbit around sun
Tilt responsible for
seasons
Vernal (spring) equinox
(3/21)
○ sun overhead at equator
○ Equal day/night periods
Summer solstice
(6/21)
○ sun overhead at Tropic of
Cancer (23.5O N)
○ Longest day of the year
in Northern hemisphere
Autumnal (fall)
equinox (9/23)
○ sun overhead at equator
○ Equal day/night periods
Winter solstice
(12/22)
○ sun overhead at Tropic of
Capricorn (23.5O S)
○ Shortest day of the year
in Northern hemisphere
Seasons
Seasonal changes and
day/night cause unequal solar
heating of Earth’s surface
Arctic circle (66.5O N)
latitude receives direct sunlight all
day on summer solstice
no direct sunlight during winter
solstice
Antarctic circle – reverse of above
Uneven solar heating
Angle of incidence of solar
rays per area
Greater the angle, solar
energy spread over more
area
Equatorial regions more heat
Polar regions less heat
Thickness of atmosphere –
absorbs or reflects energy
○ Think about South Florida
compared to Maine
Uneven solar heating
Albedo
Albus = white
% incident radiation reflected back into space
Affected by angle of sun – more angle , more
reflected
Affected by type of surface
○ Snow/ice reflects more
○ Water surface absorbs more
○ Land absorbs most
Day/night and seasonal cycles affect solar
heating
Physical properties of atmosphere
http://www.ux1.eiu.edu/~cfjps/1400
Atmosphere is
comprised of gases and
dust
mostly nitrogen (N2)
– 78%
Oxygen (O2) – 21%
CO2, water vapor,
ozone (O3) are
variable
Fig. 6.4
Physical properties of atmosphere
Warm air, less
dense (rises)
Cool air, more
dense (sinks)
Moist air, less
dense (rises)
Dry air, more
dense (sinks)
Fig. 6.5
Winds, Wind Belts and Climate
Introductory geography
○
○
○
Equator = 0O latitude
Earth rotates from west to east
Wind direction indicated by direction
winds are blowing from
Movements in atmosphere
Fig. 6.6
Air (wind) always moves from regions of high
pressure to low
Cool dense air, higher surface pressure
Warm less dense air, lower surface pressure
Air movements over non-rotating Earth
•
Convection or circulation cell
• Air heated at equator
warm (less dense) air rises
• Surface air moves in to
replace rising air mass
• Air expands & cools as it
rises
• As it cools, becomes more
dense
• Warm air holds more
moisture than cooler air
• As air cools moisture
condenses & forms
clouds/precipitation
Fig. 6.7
Air movements over a rotating Earth
Coriolis effect causes deflection in moving
body due to Earth’s rotation to east
Most pronounced on objects that move long
distances across latitudes
Deflection to right in Northern Hemisphere
Deflection to left in Southern Hemisphere
Maximum Coriolis effect at poles
No Coriolis effect at equator
Movements in air on a rotating Earth
Rotational velocity increases approaching
equator
Fig. 6.9
Global atmospheric circulation
Circulation cells as air changes density
due to:
Changes in air temperature
Changes in water vapor content
Circulation cells
Hadley cells (0o to 30o N and S)
Ferrel cells (30o to 60o N and S)
Polar cells (60o to 90o N and S)
6 cells of
windbelts and
boundaries:
Intertropical
convergence
zone
Doldrums
Horse latitudes
Tradewinds
Westerlies
Polar front
Polar easterlies
1. Intertropical convergence zone (boundary)
•
Air warms and rises at equator
•
low surface pressure
(rising air) poduce light winds
= doldrums
•
Long ago sailing
ships became
stuck here
because of lack
of winds
•
Sink at about 30O N & S latitude
•
2. Horse latitudes (boundary)
– low winds, high pressure
ridge
•
Dry, cool, sinking air
•
Sailors would also get
“stuck” here and would
through horses overboard
to conserve water
•
Winds:
•
3. Tradewinds return
to Equator, deflected
west
•
4. Westerlies move
toward poles,
deflected east
•
Winds converge at 50-60O N & S with polar air
•
•
•
5. Polar Front (boundary) - warm air rises (low
press./clouds)
Upper air splits & cools sinks near poles
Winds:
•
6. Polar Easterlies – air sinks near poles, moves
from poles toward equator
Global atmospheric circulation
High pressure zones
Subtropical highs
Polar highs
Clear skies
Low pressure zones
Equatorial low
Subpolar lows
Overcast skies with lots of precipitation
Modifications to idealized 3-cell
model of atmospheric circulation
Winds are more complex in nature due
to…
Seasonal changes
Distribution of continents and
ocean
Differences in heat capacity
between continents and ocean
○ Monsoon winds
Ocean weather and climate patterns
Weather – conditions of
atmosphere at particular time and
place
Climate – long-term average of
weather
Northern hemisphere winds move
counterclockwise (cyclonic) around
a low pressure region
Southern hemisphere winds move
clockwise (anticyclonic) around a
low pressure region
http://www.wunderground.com/US/Region/US/2xFronts.html
Coastal winds
Caused by solar heating &
different heat capacities
of land and water
Sea breeze
From ocean to land
During day, land heats air
rises draws cooler ocean
air onto coast
Land breeze
From land to ocean
At night, warmer ocean
water rises, draws cooler
land air over coast
Fig. 6.13
Fronts and storms
Air masses
Storms
Large volumes of air, meet at fronts
Disturbances with strong winds, precipitation, often
with thunder and lightning
typically develop at fronts
Warm front
contact between moving warm
air mass with cooler air mass
More extensive, lighter rains
Cold front
contact between moving cold
air mass with warmer air
mass
Usually steep front, with
heavier, but briefer, rains
Clear skies follow behind
Tropical cyclones (hurricanes)
Caused by release of energy (latent heat of condensation)
Low-pressure system breaks off equatorial low-pressure belt
Surface winds feed moisture into storm
○ As water vapor condenses, heat released warms air
○ Rising warm air draws in more moist air fueling cyclone
○ Large rotating masses of low pressure with calm “eye” (< 25 mph
winds)
Strong winds, torrential rain outside eye
Fig. 6.16
Hurricane movement
At low latitudes, affected by trades
move west
Curve toward right in No. hemisphere cooler
water, influenced by westerlies
Hurricane Wilma
10/25/2005
http://cimss.ssec.wisc.edu/tropic/archive/montage/atlantic/2005/WILMA-track.gif
Table 6.5
Hurricane destruction
Fast winds
Flooding from torrential rains
Storm surge most damaging
increased water levels from low pressure at eye
On top of tide, most damaging at high tides
Storm waves on top of storm surge
Historical examples:
Galveston, TX, 1900
Hurricane Andrew, 1992
Hurricane Mitch, 1998
Hurricane Katrina, 2005
Ocean climate patterns
Equatorial regions
○ Warm, lots of rain
Tropical regions
○ Warm, less rain, trade winds
○ South Florida is tropical, defined rainy and dry season
Subtropical regions
○ Warm, lots of wind and evaporation, find dessert areas
Temperate regions
○ Strong westerlies
Subpolar regions
○ Cool, winter sea ice, lots of snow
Polar regions
○ Cold, ice
Polar oceans and sea ice
Sea ice or masses of frozen seawater form
in high latitude oceans
Begins as small needle-like ice crystals
○ Pushes out dissolved salts dense brine
○ Ice is much lower salinity
Rate of formation depends on temperature
http://static.howstuffworks.com/gif/iceberg-calving.
Polar oceans and icebergs
Icebergs – fragments of
glaciers or shelf ice
Global warming (Climate Change)
Average global temperature increased
Part of warming due to anthropogenic greenhouse
(heat-trapping) gases such as CO2
http://healthandenergy.com/images/carbon%20d
ioxide%201700-2000.jpg
http://earthobservatory.nasa.gov/Library/Global
Warming/Images/temperature_vs_co2_rt.gif
Greenhouse effect
Solar radiation enter
atmosphere
Some of that radiation
is reflected to space
Some of it is reflected
back towards Earth by
trace gases and
particles in the
atmosphere
Elevated levels of
carbon dioxide,
methane, etc can
increase that effect
Literally “trapping” more
heat in the atmosphere
close to the Earth
Fig. 6.24
Greenhouse gases
Absorb longer wave radiation from Earth
Many “greenhouse gases”
Water vapor – most common and important
Carbon dioxide (CO2)
Other trace gases: methane, nitrous oxide, ozone,
and chlorofluorocarbons
Current controversy is not whether global
temperatures are increasing, but in the extent of
human impact
The climate is changing, we cannot deny that
The last time this happen human population
was not as large, even small changes in
climate can effect agricultural crops, larger
storms hitting populated areas, etc.
Is it significantly above natural background
change?
Can we afford to keep our heads in the sand?
Consequences of global warming are
not certain, but can be predicted…
When scientists say “uncertain” it DOES NOT mean that they do not
know what they are talking about
It does not mean that there will not be consequences
It is just difficult to predict the extent of those consequences, the
timing of those consequences, etc.
○ This is the first time we are experiencing these changes with
today’s society
○ The Earth and it’s systems are dynamic – constantly changing
- But when we talk about these changes, we are talking about
thousands, millions of years
- Our society, population boom, building of extensive cites along
coastlines, etc has been very recent
- So, let’s say for a moment that man isn’t making it worse by
putting more carbon dioxide into the atmosphere – changes are
still happening……and we have to be prepared to deal with
them….
Consequences of Climate Change
Sea level rise
Contamination of freshwater sources
Vulnerability of more low-lying areas to storm surges
Shift in species distribution
Shifts in climate patterns will affect all living organisms
Melting ice caps & expanding deserts threaten wildlife
Extreme weather patterns
Heat waves, extreme winters, larger storms in populated
areas
Droughts will affect productivity and crops
Changing ocean chemistry
Ocean water will become more acidic, warmer
Changes in ocean circulation
Spread of tropical diseases
Possible Impacts of Climate Change on South
Florida
Possible sea level rise of 15-20 inches by 2060
○ South Florida Water Management plays a delicate
balancing game to ensure that areas in South Florida don’t
flood during rain events (canal system), higher sea level
would make that more difficult – areas would be more
vulnerable to flooding
○ Greater vulnerability to storm surges and erosion
○ Salt water intrusion – fresh water supply for the
population could be threatened
Reducing greenhouse gases
Greater fuel efficiency
Alternative fuels
Re-forestation
Eliminate chlorofluorocarbons
Reduce CO2 emissions
Intergovernmental Panel on Climate Change
1988
Kyoto Protocol 1997
Ocean’s role in reducing CO2
Oceans absorbs CO2
from atmosphere
CO2 incorporated in
organisms and carbonate
shells (tests)
Stored as biogenous
calcareous sediments and
fossil fuels
Ocean is repository or sink
for CO2
Increases ocean acidity
enough to affect
organisms (corals)
http://www.whoi.edu/science/MCG/cafethorium/website/images/tzex_img1.j
Ocean Literacy Principles
1c - Throughout the ocean there is one interconnected circulation system powered by wind, tides, the
force of the Earth’s rotation (Coriolis effect), the Sun, and water density differences. The shape of
ocean basins and adjacent land masses influence the path of circulation.
1d - Sea level is the average height of the ocean relative to the land, taking into account the
differences caused by tides. Sea level changes as plate tectonics cause the volume of ocean basins
and the height of the land to change. It changes as ice caps on land melt or grow. It also changes as
sea water expands and contracts when ocean water warms and cools.
3a - The ocean controls weather and climate by dominating the Earth’s energy, water and carbon
systems.
3b - The ocean absorbs much of the solar radiation reaching Earth. The ocean loses heat by
evaporation. This heat loss drives atmospheric circulation when, after it is released into the
atmosphere as water vapor, it condenses and forms rain. Condensation of water evaporated from
warm seas provides the energy for hurricanes and cyclones.
3c - The El Niño Southern Oscillation causes important changes in global weather patterns because it
changes the way heat is released to the atmosphere in the Pacific.
3d - Most rain that falls on land originally evaporated from the tropical ocean.
3f - The ocean has had, and will continue to have, a significant influence on climate change by
absorbing, storing, and moving heat, carbon and water.
3g - Changes in the ocean’s circulation have produced large, abrupt changes in climate during the last
50,000 years.