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The Energy Cycle
(Reading AK Chapter-2)
Transferring Energy in the Atmosphere
Conduction: Requires Touching
Convection: Hot Air Rises
Temperature Advection: Horizontal Movement of Air
Latent Heating: Changing the Phase of Water
Adiabatic Cooling and Warming: Expanding and Compressing Air
Diabatic Cooling and Warming: Adding and Subtracting Heat
Radiative Heat Transfer: Exchanging Energy with Space
Sun and Seasons
Radiative Properties of the Atmosphere
Global Energy Budget
Simple C to F conversion:
F = ( TempC + TempC ) –10% +32
Example: 30deg C
86 F = (30degC + 30DegC ) – 6 + 32
C = 5 / 9 * (F – 32 )
F = (9 / 5 * C) + 32
K = 273.16 + C
No Atmosphere
Facing the Sun
(121degC) ((250F)
No Atmosphere
Shadow and darkness
(-157degC) (-250F)
Mars 218K
Venus 457o C (855o F)
Temperature
--Definition – A measure of the average
kinetic energy of all particles within a
sample.
HEAT – Energy produced by motions of
molecules and is the total kinetic energy of a
sample.
Energy Transfer
The transfer of energy between two objects due to a
difference in temperature is called HEAT energy.
Methods of Heat transfer include Conduction,
Convection, Advection, and Radiation
Adiabatic heating/cooling are constant entropy processes
and have no transfer of heat
Transferring Energy in the
Atmosphere
-Conduction Requires Touching (land/ sea - air)
-Convection Vertical Movement--Hot Air Rises
-Temperature Advection Horizontal Movement
-Latent Heating Phase Change of Water (Diabatic)
-Adiabatic (heating-cooling) Expanding - Compressing
-Radiative Heat Transfer With Space
-Conduction
-Convection
-Temperature Advection
-Latent Heating
-Adiabatic (heating-cooling)
-Radiative Heat Transfer
Surface and Air Temperature
D. L. Walters
Cook an egg on sidewalk
Hot Enough to Fry an Egg
Need a surface air temperature (2m)
warmer than 35º C ~ 95 º F
• Egg white begins to coagulate at 62°C (144°F)
while yolk begins to coagulate at 65°C (149°F).
Note: This will take a few minutes
Midday Air Temperature-Desert
D. L. Walters
15 min
-Conduction
-Convection
-Temperature Advection
-Latent Heating
-Adiabatic (heating-cooling)
-Radiative Heat Transfer
1km Vis at 1 min interval from GOES-8
7204vis.avi
http://www.shodor.org/metweb/
Measured Versus Calculated Variables
TEMPERATURE
ADVECTION
5 10 15
COLD WARM
CO LD
AD V
WA RM
AD V
500 mb
1000 mb
-Conduction
-Convection
-Temperature Advection
-Latent Heating
-Adiabatic (heating-cooling)
-Radiative Heat Transfer
-Conduction
-Convection
-Temperature Advection
-Latent Heating
-Adiabatic (heating-cooling)
-Radiative Heat Transfer
0 C
-Conduction
-Convection
-Temperature Advection
-Latent Heating
-Adiabatic (heating-cooling)
-Radiative Heat Transfer
Parcel does not exchange
heat with its surroundings
Latent Heat
release
Expansion cooling  Compression warming
Atm Avg
Lapse rate
~6.5 °C/km
-Conduction
-Convection
-Temperature Advection
-Latent Heating
-Adiabatic (heating-cooling)
-Radiative Heat Transfer
I-80
The Sun
Solar Constant 1368 W/m2
Radiation – The transfer of energy through electromagnetic
waves. Does not involve the movement of matter
-Conduction
-Convection
-Temp Advection
-Latent Heating
-Adiabatic (heating-cooling)
-Radiative Heat Transfer IR
VIS
E ~5.7x10-8 x T**4
Emax ~ 2900/T
Stefan-Boltzman Law
(Sun 160,000 more E than Earth)
Weins Law
emitted
emitted λ
Fade
Absorption of Radiation by Atmosphere
Greenhouse Effect
Venus to Hot(450C) 97%C02, 90x Sfc Pres of Earth
, Mars to Cold (-53C)95% CO2, ~1% Sfc Pres Earth,
and Earth 0.04% CO2…Just Right (15C)
• Recycles energy and makes the planet suitable for life as we know it.
• Some Trace Gases Absorb and Emit Heat
(H2Ovapor,CO2,CH4,Ozone)
• Albedo also has important influence on Earth’s Temperature
• Without Greenhouse effect Earth would be about -18C
• Water Vapor most important Greenhouse Gas
(Absorbs at different wavelengths and abundant in Atmosphere)
• Rough Approximation of contributions to Greenhouse effect by trace gases:
-60% water vapor
-20% Carbon dioxide
-20% the rest to others (Ozone, Nitrous Oxide, Methane, and other species)
UCAR 2006
Other
Planets
https://www.ucar.edu/learn/1_3_1.htm
Annual Average Energy Balance of Earth
342 W/m2 from Earth to Space 342 W/m2 from Space to Earth
In Space Solar Constant is ~1368 W/m2 (half due to night and half again due to solar zenith angle)
Earth Albedo ~ 30% (107W) Aprox 50% solar energy reaches earth
(AK)
Solar Zenith Angle
(AK)
Tropic of
Capricorn
~23.5 deg S
Tropic of
Cancer
~23.5 deg N
SUN- EARTH min/max 146-152 million km
1 complete orbit every 365.25 days
Daylight Length
http://en.wikipedia.org/wiki/Twilight
Tilt of the Earth’s axis
defines length of daylight
for a given latitude
Earth Rotation .25 deg / min
Hours Daylight
Net radiation = net short-wave radiation +
net long-wave radiation.
https://www.ncdc.noaa.gov/cag/time-series/global/globe/land_ocean/1/8/1880-2017
Image from Andy Armstrong/National Oceanic and
Atmospheric Administration
"There is considerable uncertainty in future model projections. The
more important message from models is that all but a few outliers
predict enormous sea ice retreat this century," Oceanographer of the Navy
Rear Adm. Titley July 2009

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2-Energy.ppt

  • 1. The Energy Cycle (Reading AK Chapter-2) Transferring Energy in the Atmosphere Conduction: Requires Touching Convection: Hot Air Rises Temperature Advection: Horizontal Movement of Air Latent Heating: Changing the Phase of Water Adiabatic Cooling and Warming: Expanding and Compressing Air Diabatic Cooling and Warming: Adding and Subtracting Heat Radiative Heat Transfer: Exchanging Energy with Space Sun and Seasons Radiative Properties of the Atmosphere Global Energy Budget
  • 2. Simple C to F conversion: F = ( TempC + TempC ) –10% +32 Example: 30deg C 86 F = (30degC + 30DegC ) – 6 + 32 C = 5 / 9 * (F – 32 ) F = (9 / 5 * C) + 32 K = 273.16 + C No Atmosphere Facing the Sun (121degC) ((250F) No Atmosphere Shadow and darkness (-157degC) (-250F) Mars 218K Venus 457o C (855o F) Temperature --Definition – A measure of the average kinetic energy of all particles within a sample. HEAT – Energy produced by motions of molecules and is the total kinetic energy of a sample.
  • 3. Energy Transfer The transfer of energy between two objects due to a difference in temperature is called HEAT energy. Methods of Heat transfer include Conduction, Convection, Advection, and Radiation Adiabatic heating/cooling are constant entropy processes and have no transfer of heat
  • 4. Transferring Energy in the Atmosphere -Conduction Requires Touching (land/ sea - air) -Convection Vertical Movement--Hot Air Rises -Temperature Advection Horizontal Movement -Latent Heating Phase Change of Water (Diabatic) -Adiabatic (heating-cooling) Expanding - Compressing -Radiative Heat Transfer With Space
  • 6. Surface and Air Temperature D. L. Walters Cook an egg on sidewalk
  • 7. Hot Enough to Fry an Egg Need a surface air temperature (2m) warmer than 35º C ~ 95 º F • Egg white begins to coagulate at 62°C (144°F) while yolk begins to coagulate at 65°C (149°F). Note: This will take a few minutes
  • 9. -Conduction -Convection -Temperature Advection -Latent Heating -Adiabatic (heating-cooling) -Radiative Heat Transfer 1km Vis at 1 min interval from GOES-8 7204vis.avi http://www.shodor.org/metweb/
  • 10. Measured Versus Calculated Variables TEMPERATURE ADVECTION 5 10 15 COLD WARM CO LD AD V WA RM AD V 500 mb 1000 mb
  • 12. -Conduction -Convection -Temperature Advection -Latent Heating -Adiabatic (heating-cooling) -Radiative Heat Transfer 0 C
  • 13. -Conduction -Convection -Temperature Advection -Latent Heating -Adiabatic (heating-cooling) -Radiative Heat Transfer Parcel does not exchange heat with its surroundings Latent Heat release Expansion cooling  Compression warming Atm Avg Lapse rate ~6.5 °C/km
  • 14. -Conduction -Convection -Temperature Advection -Latent Heating -Adiabatic (heating-cooling) -Radiative Heat Transfer I-80
  • 15. The Sun Solar Constant 1368 W/m2 Radiation – The transfer of energy through electromagnetic waves. Does not involve the movement of matter
  • 16. -Conduction -Convection -Temp Advection -Latent Heating -Adiabatic (heating-cooling) -Radiative Heat Transfer IR VIS E ~5.7x10-8 x T**4 Emax ~ 2900/T Stefan-Boltzman Law (Sun 160,000 more E than Earth) Weins Law emitted emitted λ Fade
  • 17. Absorption of Radiation by Atmosphere
  • 18. Greenhouse Effect Venus to Hot(450C) 97%C02, 90x Sfc Pres of Earth , Mars to Cold (-53C)95% CO2, ~1% Sfc Pres Earth, and Earth 0.04% CO2…Just Right (15C) • Recycles energy and makes the planet suitable for life as we know it. • Some Trace Gases Absorb and Emit Heat (H2Ovapor,CO2,CH4,Ozone) • Albedo also has important influence on Earth’s Temperature • Without Greenhouse effect Earth would be about -18C • Water Vapor most important Greenhouse Gas (Absorbs at different wavelengths and abundant in Atmosphere) • Rough Approximation of contributions to Greenhouse effect by trace gases: -60% water vapor -20% Carbon dioxide -20% the rest to others (Ozone, Nitrous Oxide, Methane, and other species) UCAR 2006 Other Planets
  • 20. Annual Average Energy Balance of Earth 342 W/m2 from Earth to Space 342 W/m2 from Space to Earth In Space Solar Constant is ~1368 W/m2 (half due to night and half again due to solar zenith angle) Earth Albedo ~ 30% (107W) Aprox 50% solar energy reaches earth (AK)
  • 21. Solar Zenith Angle (AK) Tropic of Capricorn ~23.5 deg S Tropic of Cancer ~23.5 deg N SUN- EARTH min/max 146-152 million km 1 complete orbit every 365.25 days
  • 22. Daylight Length http://en.wikipedia.org/wiki/Twilight Tilt of the Earth’s axis defines length of daylight for a given latitude Earth Rotation .25 deg / min Hours Daylight
  • 23. Net radiation = net short-wave radiation + net long-wave radiation.
  • 25. Image from Andy Armstrong/National Oceanic and Atmospheric Administration "There is considerable uncertainty in future model projections. The more important message from models is that all but a few outliers predict enormous sea ice retreat this century," Oceanographer of the Navy Rear Adm. Titley July 2009