Radiation Understanding



•Muhammad
 Fahad Ansari
      12IEEM14
15 Lecture Material for Introduction of
            Environmental Physics
              Class 12 EE Batch
1. Sound and Light
2. Radiation Understanding
3. Global Warming
4. Terrestrial Environment
5. Extra-Terrestrial Environment
6. Natural and Man made radiation
7. Universe understanding
8. Understanding water
9. Cloud formation
10. Climate
11. Climate change
Radiation Understanding



1.   EATRH’S ATMOSPHERE
2.   STRUCTURE
3.   SUN’S ELECTROMAGNETIC SPECTRUM
4.   Energy from the Sun
5.   Atmospheric Greenhouse Effects
Radiation and Earth’s Atmosphere
• The earth’s global average surface temperature in present
  climate is 15C (59F). Without the atmosphere, it would be -18C
  (-0.4F),
• About 33C or 59.4F colder! Atmosphere is the most important
  component of the earth’s climate.

• Radiation vs. other heat sources:
• Total energy enter the earth’s atmosphere: 174 petawatts or
  174X1015 Watts
• Solar: 99.978%, Geothermal: 0.013%, waste and fossil fuel:
  0.007%, tidal: 0.002%
Earth’s Atmosphere
1. What is it?
  A thin gaseous envelope around the planet.
                         Blue sky!
2. Composition
  Today’s atmosphere: nitrogen (78%), oxygen
  (21%), other (1%) – trace gases!

  Nitrogen, oxygen, argon, water vapor, carbon dioxide, methane, and most
  other gases are invisible.
  Clouds are not gas, but condensed vapor in the form of
  liquid droplets or ice particles.

   Ground based smog, which is visible, contains reactants of
   nitrogen and ozone.
3. Structure        Four layers:
   Troposphere (overturning) From surface to 8-18 km
  Stratosphere (stratified)     From troposphere top to 50 km
  Mesosphere
  Thermosphere
The Structure of Earth’s Atmosphere
1. Four layers defined by

         temperature
  Troposphere: T decreases with elevation
  Stratosphere: T increases with elevation
  Mesosphere:    T decreases with elevation
  Thermosphere: T increases with elevation

2. Importance to climate and climate change
  Troposphere:
     80% of Earth’s gases
     Most of Earth’s weather happens
     Most of the measurements
  Stratosphere:
     19.9% of Earth’s gases
     Ozone layer:
        Blocking Sun’s ultraviolet radiation
Energy from the Sun
1. Characteristics

  Travels through space (vacuum)
      in a speed of light
  In the form of waves:
      Electromagnetic waves
  In stream of particles      (Photons)
  Releases heat when absorbed
2. Electromagnetic spectrum

  From short wavelength, high energy,
  gamma rays to long wavelength, low
  energy, radio waves

3. Importance to climate and
climate change
  Primary driving force of Earth’s climate engine
  Ultraviolet, Visible, Infrared
Sun’s Electromagnetic Spectrum




Solar radiation has peak intensities in the shorter
wavelengths, dominant in the region we know as visible, thus
shortwave radiation
Longwave & Shortwave Radiation

                            The hot sun
                            radiates at
                            shorter
                            wavelengths
                            that carry more
                            energy, and the
                            fraction
                            absorbed by the
                            cooler earth is
                            then re-radiated
                            at longer
                            wavelengths.
Atmospheric Greenhouse Effects




           T= 15°C
           (59°F)
Surface Temperature With the
Atmosphere                               T= –18°C
                                         (0°F)
                               Surface Temperature Without the
                               Atmosphere

   Greenhouse effects make Earth’s surface warmer!
Radiation understanding by Muhammad Fahad Ansari 12IEEM14
Greenhouse Gases
    What are they?
                              Water vapor (H2O)

                 Carbon dioxide (CO2)         Methane (CH4)

       Ozone (O3)           Chlorofluorocarbons        Nitrous oxide (N2O)
                                  (CFC’s)

   Water vapor accounts for 60% of the atmospheric greenhouse effect, CO2 26%,
    and the remaining greenhouse gases 14%.



   CO2 contributes most (55-60%) to the anthropogenic greenhouse effect,
    and methane is a distant second (16%).


   CFCs cause the strongest greenhouse warming on a molecule-for-molecule
    basis.
Nitrous
Atmospheric Absorption                                   Oxide


                                                         Methane
Solar radiation passes
rather freely through
Earth's atmosphere.                                           Ozone




                          Absorption
Earth emits longwave
                                                         Water Vapor




                          (100%)
energy, which either
leaks through a narrow
window or                              Carbon
                                       Dioxide
is absorbed by
                                         UV
greenhouse gases and                                     IR
radiated back to Earth.
                                         Total Atmo

                                                  Wavelength
Solar Intensity and Latitude




Solar intensity, defined as the energy per area, is different at
different latitude.

A sunlight beam that strikes at an angle is spread across a greater
surface area, and is a less intense heat source than a beam
impinging directly.
Unequal Radiation on a Sphere



                         Insolation is
                         stronger in the
                         tropics (low
                         latitudes) than in
                         in the polar
                         regions (high
                         latitudes).
Pole-to-Equator Heating Imbalances
What controls the elevation of the Sun above the horizon?




       Earth’s Tilt Primarily Determines Season
Earth's Annual Energy Balance
The balance is
achieved locally
                                    Incoming Solar
at only two lines
                                       Radiation
of latitude.

A global balance
                                 Outgoing Longwave
is maintained by                     Radiation
excess heat from
the equatorial
region
transferring
toward the
poles.



                     Unequal heating of tropics and poles
The Global Energy Budget: Driver of Atmospheric Motion
                                       A balance exists between
                                       the incoming solar and
                                       outgoing longwave energy
                                       averaged over the globe
                                       and the year




                                         However, the tilt of the
SURPLUS   DEFICIT                      Earth means this balance
                                       is not maintained for each
                                       latitude
Questions:

• What is the current global mean surface temperature?

• Why it is 33C or 59F warmer than it would be without the
  atmosphere?

• Why is climate dominated by the radiation balance of the
  atmosphere?

• What are the main greenhouse gases in the earth’s
  atmosphere?

• In what latitudes the earth’s gain and lost radiative energy
  (heat), respectively?
Questions:
• What is the current global mean surface temperature?
    – 15C or 59F
• Why it is 33C or 59F warmer than it would be without the
  atmosphere?
    – Because of greenhouse effect of the atmosphere
• Why is climate dominated by the radiation balance of the
  atmosphere?
    – It contributes to 99.978% of total heat flux into the atmosphere
• What are the main greenhouse gases in the earth’s
  atmosphere?
    – H2O, CO2, CH4, O3, CFCs, NO2
• In what latitudes the earth’s gain and lost radiative energy
  (heat), respectively?
    – Gain heat in the tropics or 40S-40N, loss heat in high latitudes
      (50S-50N)
Interested in more questions? Try these
               questions:
• Can you name one or more main causes of glacier
  and interglacier climate change?

• What is the most important greenhouse gases for
  modern climate change? What is the fastest growing
  greenhouse gas?

• Earth’s climate has been much colder and warmer
  than that of today. Do you know in what ways the
  earth’s radiation balance was altered?

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Radiation understanding by Muhammad Fahad Ansari 12IEEM14

  • 2. 15 Lecture Material for Introduction of Environmental Physics Class 12 EE Batch 1. Sound and Light 2. Radiation Understanding 3. Global Warming 4. Terrestrial Environment 5. Extra-Terrestrial Environment 6. Natural and Man made radiation 7. Universe understanding 8. Understanding water 9. Cloud formation 10. Climate 11. Climate change
  • 3. Radiation Understanding 1. EATRH’S ATMOSPHERE 2. STRUCTURE 3. SUN’S ELECTROMAGNETIC SPECTRUM 4. Energy from the Sun 5. Atmospheric Greenhouse Effects
  • 4. Radiation and Earth’s Atmosphere • The earth’s global average surface temperature in present climate is 15C (59F). Without the atmosphere, it would be -18C (-0.4F), • About 33C or 59.4F colder! Atmosphere is the most important component of the earth’s climate. • Radiation vs. other heat sources: • Total energy enter the earth’s atmosphere: 174 petawatts or 174X1015 Watts • Solar: 99.978%, Geothermal: 0.013%, waste and fossil fuel: 0.007%, tidal: 0.002%
  • 5. Earth’s Atmosphere 1. What is it? A thin gaseous envelope around the planet. Blue sky! 2. Composition Today’s atmosphere: nitrogen (78%), oxygen (21%), other (1%) – trace gases! Nitrogen, oxygen, argon, water vapor, carbon dioxide, methane, and most other gases are invisible. Clouds are not gas, but condensed vapor in the form of liquid droplets or ice particles. Ground based smog, which is visible, contains reactants of nitrogen and ozone. 3. Structure Four layers: Troposphere (overturning) From surface to 8-18 km Stratosphere (stratified) From troposphere top to 50 km Mesosphere Thermosphere
  • 6. The Structure of Earth’s Atmosphere 1. Four layers defined by temperature Troposphere: T decreases with elevation Stratosphere: T increases with elevation Mesosphere: T decreases with elevation Thermosphere: T increases with elevation 2. Importance to climate and climate change Troposphere: 80% of Earth’s gases Most of Earth’s weather happens Most of the measurements Stratosphere: 19.9% of Earth’s gases Ozone layer: Blocking Sun’s ultraviolet radiation
  • 7. Energy from the Sun 1. Characteristics Travels through space (vacuum) in a speed of light In the form of waves: Electromagnetic waves In stream of particles (Photons) Releases heat when absorbed 2. Electromagnetic spectrum From short wavelength, high energy, gamma rays to long wavelength, low energy, radio waves 3. Importance to climate and climate change Primary driving force of Earth’s climate engine Ultraviolet, Visible, Infrared
  • 8. Sun’s Electromagnetic Spectrum Solar radiation has peak intensities in the shorter wavelengths, dominant in the region we know as visible, thus shortwave radiation
  • 9. Longwave & Shortwave Radiation The hot sun radiates at shorter wavelengths that carry more energy, and the fraction absorbed by the cooler earth is then re-radiated at longer wavelengths.
  • 10. Atmospheric Greenhouse Effects T= 15°C (59°F) Surface Temperature With the Atmosphere T= –18°C (0°F) Surface Temperature Without the Atmosphere Greenhouse effects make Earth’s surface warmer!
  • 12. Greenhouse Gases  What are they? Water vapor (H2O) Carbon dioxide (CO2) Methane (CH4) Ozone (O3) Chlorofluorocarbons Nitrous oxide (N2O) (CFC’s)  Water vapor accounts for 60% of the atmospheric greenhouse effect, CO2 26%, and the remaining greenhouse gases 14%.  CO2 contributes most (55-60%) to the anthropogenic greenhouse effect, and methane is a distant second (16%).  CFCs cause the strongest greenhouse warming on a molecule-for-molecule basis.
  • 13. Nitrous Atmospheric Absorption Oxide Methane Solar radiation passes rather freely through Earth's atmosphere. Ozone Absorption Earth emits longwave Water Vapor (100%) energy, which either leaks through a narrow window or Carbon Dioxide is absorbed by UV greenhouse gases and IR radiated back to Earth. Total Atmo Wavelength
  • 14. Solar Intensity and Latitude Solar intensity, defined as the energy per area, is different at different latitude. A sunlight beam that strikes at an angle is spread across a greater surface area, and is a less intense heat source than a beam impinging directly.
  • 15. Unequal Radiation on a Sphere Insolation is stronger in the tropics (low latitudes) than in in the polar regions (high latitudes).
  • 17. What controls the elevation of the Sun above the horizon? Earth’s Tilt Primarily Determines Season
  • 18. Earth's Annual Energy Balance The balance is achieved locally Incoming Solar at only two lines Radiation of latitude. A global balance Outgoing Longwave is maintained by Radiation excess heat from the equatorial region transferring toward the poles. Unequal heating of tropics and poles
  • 19. The Global Energy Budget: Driver of Atmospheric Motion A balance exists between the incoming solar and outgoing longwave energy averaged over the globe and the year However, the tilt of the SURPLUS DEFICIT Earth means this balance is not maintained for each latitude
  • 20. Questions: • What is the current global mean surface temperature? • Why it is 33C or 59F warmer than it would be without the atmosphere? • Why is climate dominated by the radiation balance of the atmosphere? • What are the main greenhouse gases in the earth’s atmosphere? • In what latitudes the earth’s gain and lost radiative energy (heat), respectively?
  • 21. Questions: • What is the current global mean surface temperature? – 15C or 59F • Why it is 33C or 59F warmer than it would be without the atmosphere? – Because of greenhouse effect of the atmosphere • Why is climate dominated by the radiation balance of the atmosphere? – It contributes to 99.978% of total heat flux into the atmosphere • What are the main greenhouse gases in the earth’s atmosphere? – H2O, CO2, CH4, O3, CFCs, NO2 • In what latitudes the earth’s gain and lost radiative energy (heat), respectively? – Gain heat in the tropics or 40S-40N, loss heat in high latitudes (50S-50N)
  • 22. Interested in more questions? Try these questions: • Can you name one or more main causes of glacier and interglacier climate change? • What is the most important greenhouse gases for modern climate change? What is the fastest growing greenhouse gas? • Earth’s climate has been much colder and warmer than that of today. Do you know in what ways the earth’s radiation balance was altered?