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Natural Environments: The Atmosphere GG 101 – Spring 2005 Boston University. Myneni Lecture 07: Atmosphere-Surface-Energy-Budget Feb-04-05 (1 of 12). Further Reading: Chapter 04 of the text book. Outline. - matter-energy interactions. - shortwave radiation balance.

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Outline

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  1. Natural Environments: The Atmosphere GG 101 – Spring 2005 Boston University Myneni Lecture 07: Atmosphere-Surface-Energy-Budget Feb-04-05 (1 of 12) Further Reading: Chapter 04 of the text book Outline - matter-energy interactions - shortwave radiation balance - longwave radiation balance - global radiation balance

  2. Natural Environments: The Atmosphere GG 101 – Spring 2005 Boston University Myneni Lecture 07: Atmosphere-Surface-Energy-Budget Feb-04-05 (2 of 12) Introduction • Previously,we studied • Insolation • (a) Seasonal/latitudinal patterns in incident radiation • (b) Latitude zones • Composition of the Atmosphere (a) Evolution (b) Current composition (c) State variables • The first determines the amount of radiation moving through the atmosphere • The second determines the fate of this radiation as it moves through the atmosphere • Today, we begin by looking at the fate, transformations, and exchanges of • absorbed radiation within system • To do this we begin to look at how radiation interacts with matter

  3. Natural Environments: The Atmosphere GG 101 – Spring 2005 Boston University Myneni Lecture 07: Atmosphere-Surface-Energy-Budget Feb-04-05 (3 of 12) Radiation and Matter • Absorption: • Radiation is absorbed by matter (liquid and gases) in the atmosphere • Leads to heating • Transmission: • Radiation passes through the atmosphere and does not interact with matter • Does not affect the atmosphere • Scattering: • Radiation is reflected and scattered by matter in the atmosphere, but is not absorbed • Also does not affect the atmosphere • Results in a change of wavelength and/or direction of travel Interactions depend on wavelength and type of matter

  4. Natural Environments: The Atmosphere GG 101 – Spring 2005 Boston University Myneni Lecture 07: Atmosphere-Surface-Energy-Budget Feb-04-05 (4 of 12) Example: The Ozone Hole • In the upper part of the atmosphere, there is a layer with high concentrations of ozone • Although transparent to most solar radiation, ozone selectively absorbs high-energy UV • solar radiation • This is actually vital for life on earth - high-energy UV radiation can easily break • molecular bonds in biological organisms, leading to mutations, particularly in the form • of cancer • When this disappears, this UV energy gets through to the ground

  5. Natural Environments: The Atmosphere GG 101 – Spring 2005 Boston University Myneni Lecture 07: Atmosphere-Surface-Energy-Budget Feb-04-05 (5 of 12) Incoming Solar Radiation • As the above example suggests, what happens to • radiation depends on its wavelength • Atmosphere is transparent to solar radiation (i.e. it reaches the surface and heats it) • Atmosphere absorbs longwave radiation (i.e. it heats the atmosphere) • Lets first consider solar radiation • It turns out that the clear atmosphere relatively • transparent to solar radiation • However, when we introduce clouds, we find that • the transmission is cut down. In addition there is • more reflection as well as more absorption in the • atmosphere • For right now though, we will just be considering • average conditions

  6. Natural Environments: The Atmosphere GG 101 – Spring 2005 Boston University Myneni Lecture 07: Atmosphere-Surface-Energy-Budget Feb-04-05 (6 of 12) Shortwave Radiation Budget • Typically, to aid with discussion, we use ‘dimensionless units’ where 100 represents an • amount equal to what comes from the sun • Reflection (Albedo): • 3% reflected to space by atmosphere • 19% reflected by clouds • 9% reflected by the surface • Absorption in the atmosphere: • 18% absorbed by atmosphere • 3% absorbed by clouds • Absorption by the surface: • 48% absorbed at the surface • This radiation is absorbed, heats the surface • and is converted to • Longwave radiation • Sensible and latent heat

  7. Natural Environments: The Atmosphere GG 101 – Spring 2005 Boston University Myneni Lecture 07: Atmosphere-Surface-Energy-Budget Feb-04-05 (7 of 12) Longwave Radiation • The surface emits longwave radiation (A and B), some of which escapes to the free space (A) • As opposed to solar radiation, the atmosphere is strongly absorptive to longwave radiation • Hence, the atmosphere “traps” outgoing longwave flux emitted by the surface (B) • This absorbed long-wave radiation goes to heating the gas molecules in the atmosphere • In turn, the atmosphere emits longwave radiation • Some of this radiation is emitted to space (C) • But some of it is also emitted back towards the earth (D) • Hence emission of longwave radiation from the atmosphere back to the surface represents • another form of radiative heating of the surface

  8. Natural Environments: The Atmosphere GG 101 – Spring 2005 Boston University Myneni Lecture 07: Atmosphere-Surface-Energy-Budget Feb-04-05 (8 of 12) Longwave Radiation Budget • We will continue use the dimensional units • From surface: • 6% escapes to space • 107% is radiated by surface and absorbed by atmosphere • From Atmosphere: • 97% is re-radiated by atmosphere and is • absorbed by the surface • 63% is re-radiated to atmosphere and escapes • Why is more radiation emitted from the surface of the earth than is absorbed through solar radiation? • Because of the “Natural GreenhouseEffect”

  9. Natural Environments: The Atmosphere GG 101 – Spring 2005 Boston University Myneni Lecture 07: Atmosphere-Surface-Energy-Budget Feb-04-05 (9 of 12) The Greenhouse Effect • Refers to the emission of longwave radiation by the surface, absorption by the • atmosphere, and re-radiation back to the surface • Because of the re-radiated longwave energy, the earth receives more than just energy • from the sun • Note that the earth receives more longwave energy from the atmosphere than it does • directly from the sun • Can consider this to be ‘recycling’ of energy within the earth system • This is why the surface temperature of the earth is greater than 255K expected by simple • radiation balance considerations

  10. Natural Environments: The Atmosphere GG 101 – Spring 2005 Boston University Myneni Lecture 07: Atmosphere-Surface-Energy-Budget Feb-04-05 (10 of 12) Surface Radiation Balance 48 Solar Radiation Heating Incoming Solar Radiation 48 Incoming Longwave Radiation 97 Total 145 Cooling Outgoing Longwave Radiation 113 Latent Heat 22 Sensible Heat 10 Total 145

  11. Natural Environments: The Atmosphere GG 101 – Spring 2005 Boston University Myneni Lecture 07: Atmosphere-Surface-Energy-Budget Feb-04-05 (11 of 12) Atmospheric Radiation Balance Heating Cooling Incoming Solar Radiation 21 Incoming Longwave Radiation 107 Latent Heat 22 Sensible Heat 10 Total 160 Outgoing Longwave Radiation (to space) 63 Outgoing Longwave Radiation (to Earth) 97 Total 160

  12. Natural Environments: The Atmosphere GG 101 – Spring 2005 Boston University Myneni Lecture 07: Atmosphere-Surface-Energy-Budget Feb-04-05 (12 of 12) Global Radiation Balance Incoming Solar Radiation 100 Total 100 Reflected to space 31 Longwave Radiation from Earth 6 Longwave Radiation from Atmos. 63 Total 100

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