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Exam I Wednesday, September 16th
Study Guide: Today
Review Session: Monday
Water, Heat, and Climate
Heat capacity
1 Cal
g . oC
It requires 1 calorie of heat input
to raise the temperature of 1 g
of water by 1 degree Celsius
2
Temperatures of large standing bodies of
water remain relatively constant.
Heat Capacity
Sun Warms water
Low pressure
cools
Florida
Sand
Asphalt
Vegetation
Gulf of Mexico Atlantic Ocean
Vaporization and Condensation
How much heat?
3
Quantified by Latent Heat
Amount of heat added or removed
from water to effect a phase change.
Liquid Gas
Latent Heat of Vaporization
Amount of heat added to water to
change it from a liquid to a gas.
Liquid Gas
580 cal of heat added for each gram of water
580 cal/g
Water 580 cal/g
Ammonia 350 cal/g
Alcohol 215 cal/g
Acetone 133 cal/g
Latent Heats of Vaporization
Amount of heat input to the liquid to change it to a gas
4
Latent Heat of Condensation
Amount of heat removed from gaseous
water to change it from a gas to a liquid.
Liquid Gas
580 cal of heat removed for each gram of water
580 cal/g
Liquid
Gas
580 cal/g
Conservation of Energy
Heat required to vaporize or condense 1 g of water = 580 cal
How much heat is needed to evaporate or condense 1 L of water?
1000 g x 580 cal = 580,000 cal
g 11
1 L of water = g water1000
5
Importance
Latent Heat and Climate
Water stores energy (heat) in the gas
580 cal/g
Liquid gas
Water releases energy (heat) from gas
580 cal/g
Liquid
500,000 km3/day
5 x 1014 L/day
5 x 1017 g/day
2.7 x 1020 cal/day
200,000 MT TNT
Ocean Evaporation
500,000 km3/day
How Much Energy?
Roughly equivalent to 10,000 atomic bombs
6
Effect on Climate
Equinox
Latent Heat and Climate
Equinox
Equinox
Low
Pressure
7
Low
Pressure
Latent Heat Transport
580 cal/g
580 cal/g
Surface
wind
Surface
wind
1. Equatorial latitudes receive more solar energy than other latitudes
2. Equatorial regions are dominated by oceans
3. Solar heat evaporates water near the equator (water absorbs 580 cal/g)
4. Warm, moist air rises from the equator
5. Rising moist air creates low pressure at the surface
6. Cooler air from northern and southern latitudes moves to the equator
7. Air rising from the equator eventually moves to northern and southern
latitudes carrying latent heat of vaporization obtained at the equator.
8. This air eventually cools and descends near 30o latitude
9. Cool air condenses, releasing energy (580 cal/g) obtained at equator
10. The overall process cools the equator and warms northern and
southern latitudes, redistributing heat globally.
8
85o
55o
55o
0
30
60
Air flows southward between 0 and 30 degrees
Air flows northward between 30 and 60 degrees
Redistribution of Heat
30o
0o
60o
Northern Hemisphere
Do Winds Really Blow in these Directions?
9
Today: mostly cloudy
Tomorrow: Rain
30o
30o
0o
60o
equator
30o N
wind
Hurricanes
30o
0o
60o
30o
0o
60o
Northern Hemisphere
Something is redirecting the wind
Hurricanes
Fronts
10
The Coriolis Effect
Due to the rotation of a spherical earth
What is the circumference of the Earth? ~ 25,000 miles
How long does it take for the earth to make one rotation? 24 hours
25,000 mi at 0o latitude
1042 mi/hr
0 mi/hr
stationary
1042 mi/hr
The Coriolis Effect
Velocity at 90o latitude
zero
Velocity at equator
1042 mi hr
Objects moving in the northern hemisphere deflect to the right of the direction of travel.
11
The Coriolis Effect
Velocity at 90o latitude
zero
Velocity at equator
1042 mi hr
Objects moving in the northern hemisphere deflect to the right of the direction of travel.
1042 mi/hr
Stationary
30o
0o
60o
Northern Hemisphere
The Coriolis Effect deflects the wind
to the right of the direction of travel
30o
0o
60o
The Coriolis Effect deflects the wind
to the right of the direction of travel
12
Equator
30o
30o
60o
60o
Surface Winds
Prevailing
Westelies
Tropical
Easterlies
In the Northern Hemisphere moving objects, including air,
are deflected to the right of the direction of travel
In the Southern Hemisphere moving objects, including air,
are deflected to the left of the direction of travel
stationary
1042 mi/hr
13
The Coriolis Effect
Velocity at 90o latitude
zero
Velocity at equator
1042 mi hr
Objects moving in the southern hemisphere deflect to the left of the direction of travel.
Equator
30o
30o
60o
60o
In the Southern Hemisphere moving objects, including air,
are deflected to the left of the direction of travel
Equator
30o
30o
60o
60o
14
Calm air
Calm air
descending
descending
rising
Hurricane Track
30o
0o
30o
15
Sailing, sailing…
30o
Trade winds
(easterlies)
Westerlies
1. The Coriolis force is due to the spherical shape of the earth.
2. Points at the equator move faster than points at other latitudes.
3. In the northern hemisphere air is deflected to the right of the
direction of travel
4. In the southern hemisphere air is deflected to the left of the
direction of travel
8. Winds are named with respect to the direction from which
they originate.
9. Winds between 30o and the equator are called easterlies.
10. Winds between 30o and 60o are called westerlies.
Summary
16
equator

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Lecture 7 water, heat, and climate

  • 1. 1 Exam I Wednesday, September 16th Study Guide: Today Review Session: Monday Water, Heat, and Climate Heat capacity 1 Cal g . oC It requires 1 calorie of heat input to raise the temperature of 1 g of water by 1 degree Celsius
  • 2. 2 Temperatures of large standing bodies of water remain relatively constant. Heat Capacity Sun Warms water Low pressure cools Florida Sand Asphalt Vegetation Gulf of Mexico Atlantic Ocean Vaporization and Condensation How much heat?
  • 3. 3 Quantified by Latent Heat Amount of heat added or removed from water to effect a phase change. Liquid Gas Latent Heat of Vaporization Amount of heat added to water to change it from a liquid to a gas. Liquid Gas 580 cal of heat added for each gram of water 580 cal/g Water 580 cal/g Ammonia 350 cal/g Alcohol 215 cal/g Acetone 133 cal/g Latent Heats of Vaporization Amount of heat input to the liquid to change it to a gas
  • 4. 4 Latent Heat of Condensation Amount of heat removed from gaseous water to change it from a gas to a liquid. Liquid Gas 580 cal of heat removed for each gram of water 580 cal/g Liquid Gas 580 cal/g Conservation of Energy Heat required to vaporize or condense 1 g of water = 580 cal How much heat is needed to evaporate or condense 1 L of water? 1000 g x 580 cal = 580,000 cal g 11 1 L of water = g water1000
  • 5. 5 Importance Latent Heat and Climate Water stores energy (heat) in the gas 580 cal/g Liquid gas Water releases energy (heat) from gas 580 cal/g Liquid 500,000 km3/day 5 x 1014 L/day 5 x 1017 g/day 2.7 x 1020 cal/day 200,000 MT TNT Ocean Evaporation 500,000 km3/day How Much Energy? Roughly equivalent to 10,000 atomic bombs
  • 6. 6 Effect on Climate Equinox Latent Heat and Climate Equinox Equinox Low Pressure
  • 7. 7 Low Pressure Latent Heat Transport 580 cal/g 580 cal/g Surface wind Surface wind 1. Equatorial latitudes receive more solar energy than other latitudes 2. Equatorial regions are dominated by oceans 3. Solar heat evaporates water near the equator (water absorbs 580 cal/g) 4. Warm, moist air rises from the equator 5. Rising moist air creates low pressure at the surface 6. Cooler air from northern and southern latitudes moves to the equator 7. Air rising from the equator eventually moves to northern and southern latitudes carrying latent heat of vaporization obtained at the equator. 8. This air eventually cools and descends near 30o latitude 9. Cool air condenses, releasing energy (580 cal/g) obtained at equator 10. The overall process cools the equator and warms northern and southern latitudes, redistributing heat globally.
  • 8. 8 85o 55o 55o 0 30 60 Air flows southward between 0 and 30 degrees Air flows northward between 30 and 60 degrees Redistribution of Heat 30o 0o 60o Northern Hemisphere Do Winds Really Blow in these Directions?
  • 9. 9 Today: mostly cloudy Tomorrow: Rain 30o 30o 0o 60o equator 30o N wind Hurricanes 30o 0o 60o 30o 0o 60o Northern Hemisphere Something is redirecting the wind Hurricanes Fronts
  • 10. 10 The Coriolis Effect Due to the rotation of a spherical earth What is the circumference of the Earth? ~ 25,000 miles How long does it take for the earth to make one rotation? 24 hours 25,000 mi at 0o latitude 1042 mi/hr 0 mi/hr stationary 1042 mi/hr The Coriolis Effect Velocity at 90o latitude zero Velocity at equator 1042 mi hr Objects moving in the northern hemisphere deflect to the right of the direction of travel.
  • 11. 11 The Coriolis Effect Velocity at 90o latitude zero Velocity at equator 1042 mi hr Objects moving in the northern hemisphere deflect to the right of the direction of travel. 1042 mi/hr Stationary 30o 0o 60o Northern Hemisphere The Coriolis Effect deflects the wind to the right of the direction of travel 30o 0o 60o The Coriolis Effect deflects the wind to the right of the direction of travel
  • 12. 12 Equator 30o 30o 60o 60o Surface Winds Prevailing Westelies Tropical Easterlies In the Northern Hemisphere moving objects, including air, are deflected to the right of the direction of travel In the Southern Hemisphere moving objects, including air, are deflected to the left of the direction of travel stationary 1042 mi/hr
  • 13. 13 The Coriolis Effect Velocity at 90o latitude zero Velocity at equator 1042 mi hr Objects moving in the southern hemisphere deflect to the left of the direction of travel. Equator 30o 30o 60o 60o In the Southern Hemisphere moving objects, including air, are deflected to the left of the direction of travel Equator 30o 30o 60o 60o
  • 15. 15 Sailing, sailing… 30o Trade winds (easterlies) Westerlies 1. The Coriolis force is due to the spherical shape of the earth. 2. Points at the equator move faster than points at other latitudes. 3. In the northern hemisphere air is deflected to the right of the direction of travel 4. In the southern hemisphere air is deflected to the left of the direction of travel 8. Winds are named with respect to the direction from which they originate. 9. Winds between 30o and the equator are called easterlies. 10. Winds between 30o and 60o are called westerlies. Summary