Teaching the Science of Climate Change

1. Teaching the Science of Climate Change Keith Burrows AIP Education Committee STAVCON November 2007 This ppt available on www.vicphysics.org - Teachers Please read the Notes pages for more info

2. A declaration of vested interests • This presentation is dedicated to our wonderful grandchildren – and all the others who will inherit the results of our efforts in this decade – the last that has the option to act to avoid dangerous climate change.

3. Overview • Climate science • Earth’s energy balance • Interactions between emr and the atmosphere • The effect of changes in the system • Human induced changes • The release of millions of years of stored energy • Is the climate changing? • How can we understand it? • Climate models and their predictions. • What can we do? • Fossil fuels • Reduce energy use • Lower CO2 options • Sustainable options • The human response • Sceptics, deniers, avoiders • Change the light bulbs • The need for real change • Education • That’s where we come in

4. Climate science • Earth’s energy balance • The average temperature of the Earth is determined by the balance between incoming solar radiation and outgoing ‘heat’ radiation

5. Climate science • ~ 1/3 reflected • ~ 2/3 absorbed then re-radiated as IR emr. • 175,000 TW in • 175,000 TW out

6. Climate science • Earth’s energy balance • The average temperature of the Earth is determined by the balance between incoming solar radiation and outgoing ‘heat’ radiation • Not all the IR radiation from the surface escapes immediately... • or the average temperature would be about – 15ºC • and there would be much greater swings between night—day, cloud—no cloud

7. Climate science • Earth’s energy balance

8. Climate science • Earth’s energy balance • The average temperature of the Earth is determined by the balance between incoming solar radiation and outgoing ‘heat’ radiation • Not all the IR radiation from the surface escapes immediately... • or the average temperature would be about – 15ºC • and there would be much greater swings between night—day, cloud—no cloud • The Greenhouse effect: • Natural: • Water vapour • Carbon dioxide • Human produced: • Carbon dioxide • Methane etc.

9. Climate science • Interactions between emr and the atmosphere: EMR • Blackbody spectra. All objects at ANY temperature emit emr • Hot metal emits lots of shorter IR and some visible

10. Climate science • Interactions between emr and the atmosphere: EMR • Blackbody spectra. All objects at ANY temperature emit emr • Cold objects only long IR and no visible • Slightly shorter IR

11. Climate science • Interactions between emr and the atmosphere: EMR • Blackbody spectra • Spectra of stars • or anything else that hot – UV Vis IR –

12. Climate science • Interactions between emr and the atmosphere: EMR • Blackbody spectra • Sun and Earth but note that Earth is less than a millionth of the Sun – UV Vis short IR – long IR

13. Climate science • Interactions between emr and the atmosphere: EMR • Types of spectra • Blackbody continuous spectrum

14. Climate science • Interactions between emr and the atmosphere: EMR • Types of spectra • Emission line spectrum

15. Climate science • Interactions between emr and the atmosphere: EMR • Types of spectra This is what we are interested in.

16. Climate science • Interactions between emr and the atmosphere: EMR • First we need to know something about emr (light). • Quantum physics tells us that it comes as ‘photons’ • Here’s a red one • Here’s a violet one • Notice that the red one has a longer wavelength • It also has less energy • (Violet is more violent!)

17. Climate science • Interactions between emr and the atmosphere: EMR • First we need to know something about emr (light). • Quantum physics tells us that it comes as ‘photons’ • Here’s an ultraviolet (UV) one • Here’s an infrared (IR) one • Notice that the IR one has a longer wavelength again • It also has much less energy – • but it’s IR that is of interest to us

18. Climate science • Interactions between emr and the atmosphere: EMR • The gases in the atmosphere absorb, and then re-radiate some parts of the spectrum but not others. • The structure of the molecule determines what sort of energy is absorbed. • Oxygen and Nitrogen molecules are ‘tight’ and it takes a lot of energy to ‘shake’ them. • IR goes right past • High energy UV can give its energy to oxygen • but there’s very little of that even in sunlight

19. Climate science • Interactions between emr and the atmosphere: EMR • The gases in the atmosphere absorb, and then re-radiate some parts of the spectrum but not others. • The structure of the molecule determines what sort of energy is absorbed. • H2O and CO2 molecules (and other GHGs) are more ‘floppy’ • IR gives them energy • Which they re-radiate – in random directions • So some goes back down to Earth • keeping us warmer • The Greenhouse effect!

20. Climate science • The effect of changes • Remember we wouldn’t be here without it! • Water vapour is the main GHG • But what if we add more CO2?

21. Climate science • The effect of changes – Feedback and Forcing • More CO2→ more warmth → more H2O (evaporation) → more warmth → more H2O → more warmth → ??? • Water vapour goes in and out of the atmosphere very quickly • Carbon dioxide is there for ~ 100 years • That makes a big difference in the way they act • Adding H2O is not a problem.

22. Climatepseudo science “the combined effect of these greenhouse gases is to warm Earth's atmosphere by about 33 ºC, from a chilly -18 ºC in their absence to a pleasant +15 ºC in their presence. 95% (31.35 ºC) of this warming is produced by water vapour, which is far and away the most important greenhouse gas. The other trace gases contribute 5% (1.65 ºC) of the greenhouse warming, amongst which carbon dioxide corresponds to 3.65% (1.19 ºC). The human-caused contribution corresponds to about 3% of the total carbon dioxide in the present atmosphere, the great majority of which is derived from natural sources. Therefore, the probable effect of human-injected carbon dioxide is a miniscule 0.12% of the greenhouse warming, that is a temperature rise of 0.036 ºC. Put another way, 99.88% of the greenhouse effect has nothing to do with carbon dioxide emissions from human activity.” Prof. Bob Carter, Research Professor at James Cook University, palaeontologist, stratigrapher, marine geologist and environmental scientist. • The effect of changes – Feedback and Forcing

23. Climatepseudo science • The effect of changes – Feedback and Forcing • In short: • GHE → 31°C • H2O → 95% • OGHG → 5% of which CO2 → 3.6% • Human CO2 is 3% of CO2 so 0.1% of GHE • ie. 0.04°C No worries ☺

24. Climatepseudo science • The effect of changes – Feedback and Forcing • Sounds impressive – if only – but  • www.realclimate.org A group of real climate scientists who try to help people like Carter – and us. RealClimate.org Gavin A. Schmidt: climate modeller at the NASA Goddard Institute for Space Studies Dr. Michael E. Mann: Penn State University Departments of Meteorology and Geosciences and the Earth and Environmental Systems Institute, IPCC lead author Dr. Caspar Ammann: National Center for Atmospheric Research (NCAR). Dr. Rasmus E. Benestad: Norwegian project called RegClim, Norwegian Meteorological Institute Prof. Raymond S. Bradley: Director of the Climate System Research Center University of Massachusetts, Ray Bradley: Advisor to U.S., Swiss, Swedish, and U.K. National Science Foundations, NOAA, IPCC, IGBP, Stockholm. William M. Connolley: Climate modeller with the British Antarctic Survey. Prof. Stefan Rahmstorf: New Zealand Oceanographic Institute, Institute of Marine Science in Kiel, Potsdam Institute for Climate Impact Research in Germany, IPCC. Dr. Eric Steig: Isotope geochemist, University of Washington Dr. Thibault de Garidel: Institute of Marine and Coastal Sciences at Rutgers University. Dr. David Archer: Computational ocean chemist at the University of Chicago.

25. Climatepseudo science • The effect of changes – Feedback and Forcing • 95% should actually be 90-95% and is for clouds also. • Can’t simply subtract leaving 5-10% for GHGs. • H2O and CO2 absorb different parts of the IR radiation.

26. Climatepseudo science • The effect of changes – Feedback and Forcing • Take away all H2O: OGHGs absorb ~34% • Take away OGHGs: H2O absorb ~85% • So effect of H2O ~ 66% – 85% • Not a linear problem! • So 5% for OGHGs should be ~ 15% – 34% • CO2 on its own 9% – 26% → ΔT ~ 3 to 9°C • (But that assumes Carter’s linearity which it isn’t)

27. Climatepseudo science • The effect of changes – Feedback and Forcing • Reminder – Carter’s figures: • GHE → 31°C • H2O → 95% • OGHG → 5% of which CO2 → 3.6% • Human CO2 is 3% of CO2 so 0.1% of GHE • ie. 0.04°C No worries ☺ ?

28. Climatepseudo science • The effect of changes – Feedback and Forcing • Anthropogenic CO2 is NOT 3%!

29. Climatepseudo science • The effect of changes – Feedback and Forcing • Anthropogenic CO2: 300 ppm → 380 ppm • Rise of 30% • linear extrapolation: AGHG → 1 to 2.6°C (AGHG = Anthropogenic GHGs)

30. Climate science • The effect of changes – Feedback and Forcing • Carter ignores complex mechanisms of the GHE. Assumes effects are linear – Just plain wrong. • Overlaps: gases absorb overlapping wavelengths. • Saturation: more gas makes no difference. • Feedback: Particularly important. Positive and negative. • Positive feedback:

31. Climate science • The effect of changes – Feedback and Forcing • Examples of feedback: • Increased water vapour → more clouds • reflect sunlight (negative feedback) • trap IR radiation (positive feedback)

32. Climate science • The effect of changes – Feedback and Forcing • Water vapour is a ‘feedback’ GHG • CO2, CH4, O3 etc are ‘forcing’ agents • They stay in the atmosphere whatever and ‘force’ more heat into the climate system. • Effect measured by ‘Radiative forcing constant’ • or: the extra heat flowing into (or out of) the climate system as a result of a change in some part of the system "The radiative forcing of the surface-troposphere system due to the perturbation in or the introduction of an agent (say, a change in greenhouse gas concentrations) is the change in net (down minus up) irradiance (solar plus long-wave; in Wm-2) at the tropopause AFTER allowing for stratospheric temperatures to readjust to radiative equilibrium, but with surface and tropospheric temperatures and state held fixed at the unperturbed values". (IPCC)

33. Climate science • The effect of changes – Feedback and Forcing • Computer models are the only way of taking all this into account – a little later.

34. Overview • Climate science • Earth’s energy balance • Interactions between emr and the atmosphere • The effect of changes in the system • Human induced changes • The release of millions of years of stored energy • Is the climate changing? • How can we understand it? • Climate models and their predictions. • What can we do? • Fossil fuels • Reduce energy use • Lower CO2 options • Sustainable options • The human response • Sceptics, deniers, avoiders • Change the light bulbs • The need for real change • Education • That’s where we come in

35. Human induced changes • The release of solar energy and carbon stored over 100 million years ...

36. Human induced changes • The release of solar energy and carbon stored over 100 million years in only 100’s of years We have to ask whether it might have an effect!

37. Human induced changes • Is the climate changing?

38. IPCC SynRep

39. Human induced changes • Is the climate changing?

40. Human induced changes • Is the climate changing?

41. Human induced changes • Is the climate changing?

42. Human induced changes • We now know it has:

43. Human induced changes • Is the climate changing?

44. Human induced changes • Is the climate changing? IPCC SynRep

45. Human induced changes • Is the climate changing?

46. IPCC SynRep

47. IPCC SynRep

48. Human induced changes • How can we understand it? • It’s all a matter of physics!

50. IPCC SynRep