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Physical basis of the Greenhouse Effect -The “wavelength shift”-

Online at: http://www.umich.edu/~twod/energy/resources/greenhouse_lecture. Physical basis of the Greenhouse Effect -The “wavelength shift”-. Solar insolation calculation (doc file) Blackbody radiation, Absorption spectra Conservation of energy Energy & Environment 263.

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Physical basis of the Greenhouse Effect -The “wavelength shift”-

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  1. Online at: http://www.umich.edu/~twod/energy/resources/greenhouse_lecture Physical basis of the Greenhouse Effect-The “wavelength shift”- Solar insolation calculation (doc file) Blackbody radiation, Absorption spectra Conservation of energy Energy & Environment 263

  2. Black body radiation • Continuous spectra 400 500 600 700 Wavelength [nm, nanometers] ColorScience.htm

  3. Black body radiation • Continuous spectra – we see as white light 400 500 600 700 Wavelength [nm, nanometers] ColorScience.htm

  4. Black body radiation • Continuous spectra & human cones, rods 400 500 600 700 Wavelength [nm, nanometers] Warning: shows range of three types of cones, but not relative sensitivities (green has ~ 10x sensitivity of red). ColorScience.htm

  5. Black body radiation • Continuous visible spectra – higher temp. 400 500 600 700 Wavelength [nm, nanometers] ColorScience.htm

  6. Black body radiation Note peak shift   And flatter shape with lower Temperature • Continuous visible spectra -- lower temperature 400 500 600 700 Wavelength [nm, nanometers] ColorScience.htm

  7. Black body radiation • Continuous visible spectra -- lower temperature 400 500 600 700 Wavelength [nm, nanometers] -- Wavelength vs. temp is Stephan-Boltzmann law -- Peak is Wein’s law -- Shape or ‘distribution’ of intensity with frequency is Plank’s Readiation Law … A big deal in Quantum Mechanics’ history (Einstein, Plank, et al) -More on this & math later ColorScience.htm

  8. Black body vs. atomic line spectra • Continuous spectra – from bulk solids with complex modes • Atomic line spectra – discrete energy levels 400 500 600 700 Wavelength [nm, nanometers] Hydrogen EMISSION line spectra ColorScience.htm

  9. Solar black body radiation • Solar spectra … ~5800 K at surface • Yellow-green at middle. Combo ~ white. But, some parts missing … 400 500 600 700 Wavelength [nm, nanometers] ColorScience.htm

  10. Blackbody radiation 400 500 600 700 Wavelength [nm, nanometers] But, what we actually get from the sun is: Hydrogen ABSORPTION spectra ColorScience.htm

  11. Atomic physics: • ATOMISTIC • and QUANTUM • view of • micro-world • Larger jump • more energy  bluer color 400 500 600 700 Hydrogen EMISSION line spectra Hydrogen ABSORPTION spectra Hydrogen emits/absorbs same energies. ColorScience.htm

  12. Atomic physics: ATOMISTIC and QUANTUM view of micro-world 400 500 600 700 Hydrogen EMISSION line spectra Hydrogen ABSORPTION spectra Hydrogen emits/absorbs same energies. ColorScience.htm

  13. Greenhouse: Black body radiation Three concepts crucial to understand greenhouse effect: • Blackbody radiation is E&M radiation a) Continuous spectra b) Shifts with temperature • Physics of radiant energy

  14. Greenhouse: Black body radiation Three concepts crucial to understand greenhouse effect: • Blackbody radiation is E&M radiation a) Continuous spectra b) Shifts with temperature 2) Line Spectra of atoms (or bands of molecules) a) Discrete lines (bands) b) Emission and absorption at same energies • Physics of radiant energy

  15. Greenhouse: Black body radiation Three concepts crucial to understand greenhouse effect: • Blackbody radiation is E&M radiation a) Continuous spectra b) Shifts with temperature 2) Line Spectra of atoms (or bands of molecules) a) Discrete lines (bands) b) Emission and absorption at same energies 3) Equilibrium temperature reached when earth’s emission = earth’s absorption. - Slight change in either -> colder or hotter earth

  16. Greenhouse: and “Wavelength shift” • Fourth issue: CO2 emissions and H2O already in atmosphere • Look in detail now Physics of radiant energy … • We’ll need couple students with calculators … (And remember Sun = 6000 K, earth = 288 K, sigma = 5.67 x 10-8 Watts m-2) Later: solar-earth spectra compared 

  17. Fourth issue: CO2 emissions, and H2O already in atmosphere Source: http://www.lenntech.com/The-greenhouse-effect.htm

  18. Fourth issue: CO2 emissions, and H2O already in atmosphere Source: http://www.lenntech.com/The-greenhouse-effect.htm

  19. Fourth issue: CO2 emissions, and H2O already in atmosphere Earth shine Source: http://www.lenntech.com/The-greenhouse-effect.htm

  20. Fourth issue: CO2 emissions, and H2O already in atmosphere Earth shine WATER VAPOR “Water molecules, always abundant I air, absorb thermal IR light due to the H-O-H bending vibration, the peak in the spectrum for this absorption occurs at about 6.3 µm. Thus almost all the relatively small amount of outgoing IR in the 5.5-7.5 µm regions is intercepted by water vapor. There are other water vibrations the remove thermal infrared light of wavelength 12 µm and longer. In fact the water is the most important greenhouse gas in the earth’s atmosphere, though on a per molecule basis it is a less efficient absorber than is CO2. “ “The equilibrium vapor pressure of liquid water, and consequently the maximum concentration of water vapor in air, increases exponentially with temperature. Thus the amount of thermal IR redirected by water vapor will rise as a result of any global warming induced by the other greenhouse gases and will amplify the temperature increase. Since it comes about as an indirect effect of increasing the levels of other gases. Consequently, water is not usually listed explicity among gases whose increasing concentrations are enhancing the greenhouse effect.  Water in the liquid form droplets in clouds also absorbs thermal IR. “ Source: http://www.lenntech.com/The-greenhouse-effect.htm

  21. Greenhouse: and “Wavelength shift”

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