1 / 44

Why do climates change ?

Why do climates change ?. Climate changes over the last millennium. Take away ideas and understandings. What factors influence climate change over decadal to century timescales? Solar variability, volcanic eruptions, and greenhouse gases. How we can quantify their effects ?

delling
Download Presentation

Why do climates change ?

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Why do climates change ? Climate changes over the last millennium

  2. Take away ideas and understandings • What factors influence climate change over decadal to century timescales? • Solar variability, volcanic eruptions, and greenhouse gases. • How we can quantify their effects ? • Climate history of the last millennium

  3. Our first climate model Recall how to calculate Earth’s effective temperature, or the temperature the Earth would be without an atmosphere. The Stefan-Bolzmann equation: Blackbody radiation: I (w/m2) = s T4 Earth’s incoming radiation (a = Earth albedo, or reflectivity) I incoming = (1-a) s Tsun4

  4. Our first climate model Earth incoming radiation (a = Earth albedo, or reflectivity) I incoming = ((1-a) Isolar ) / 4, or ((1-a) s Tsun4 )/ 4 Earth outgoing radiation I outgoing = s Tearth4 • is ~0.3, or 30% • e (emissivity) = 1 • s = 5.67 x 10-8 Wm-2 K-4 Archer Fig. 3.3 (p. 23)

  5. Earth’s temperature with no greenhouse effectTeffective = 254.8K (-18°C) At equilibrium, I incoming = I outgoing ((1-a) s Tsun4 ) / 4 = s T4earth Solve for Tearth Eqn. 3.1 in Archer Chapter 3

  6. Surface temperature readings Galileo’s Thermoscope (1500s) Daniel Fahrenheit (1714) closed thermometer First weather stations established ~250 years ago Widespread measurements for last 150 years only.

  7. Stockholm Observatory 31 December, 1768: “No one can recall such a mild Autumn: the ground is as green as in the Spring, and today I have picked sufficient young nettles, dandelions, and other herbs to cook green cabbage tomorrow, which is New Year's day.”

  8. Many 1000s of stations

  9. http://data.giss.nasa.gov/gistemp/

  10. There are only 3 ways to change Earth’s temperature Change input • Solar variability • Earth reflectivity (volcanoes) Change output c) Greenhouse gases

  11. 1. Volcanoes cool climate, briefly Mt. Tambora - 1815 Mt. Pinatubo - 1994

  12. Volcanic eruption can change albedo by 1%  = ~30% on average Teffective = 254.8K Recalling Iin = (1-a) s T4 ((1-a) s Tsun4 )/ 4 = s T4earth Increase  to 31% New Teffective = 253.9K or -1°C cooler due a volcanic eruption

  13. Climate Impacts of Volcanic Eruptions • Volcanoes inject aerosols and particles into the stratosphere which can scatter and/or absorb incoming solar radiation. • Cools the troposphere by up to 0.5-1.0°C for only 2-4 years. • Warms the Stratosphere by 2-3°C (!) • Short-term but significant impact

  14. Mt. Tambora 1815 eruption “Year Without a Summer” “Poverty Year” “1800-and-froze-to-death”

  15. Mt. Merapi (Indonesia)tropical volcanoes cool climate most

  16. 2. Solar Variability

  17. Sunspots, Facular brightening, and Irradiance

  18. 30 years of satellite observations: ±1 W/m2

  19. What if the solar radiation changes by +2 W/m2 ? Recalling Isolar = 1365 W/m2 Set Isolar = 1367 W/m2 • = 0.3 Solve for Tearth ((1-a) Isolar)/ 4 = s T4earth ∆T = 0.1°C (Small !)

  20. Sunspot Cycles - Sunspots + ~0.1% 1600 1700 1800 1900 2000 Very weak forcing, but significant climate responses to it.

  21. Little Ice Age (1500-1850 AD) LIA Cooling was the result of lower solar radiation and some big volcanic eruptions

  22. Little Ice Age (1500-1850) London Frost Fair (1814)

  23. 2001 1859 Rhône Glacier

  24. Solar Variability • Forcing is very weak (in visible spectrum), only ±0.1-0.2%, so climate response should be weak. • Climate response is actually quite high - still not sure why. • One possibility is UV part of spectrum - much greater changes (±10%) … suggests that global climate is very sensitive

  25. http://data.giss.nasa.gov/gistemp/

  26. How do we estimate past climate change, before there were thermometers

  27. b) Calibrate ring widths C) Validate and Apply warm T (°C) cool Year AD “Proxies” - getting temperatures from trees a) Measure ring widths

  28. Temperatures over the last 2,000 years *2005 Date (AD)

  29. Measured CO2 trends since 1958

  30. Atmospheric CO2: Last 250 years

  31. Natural forcing only Natural + Human …most of modern warming is due to humans Results from the IPCC AR4 report

  32. Natural only Natural + GHG

  33. Modeling the climate of the last 1000 years…

  34. Climate = Solar Irrad. + Volcanoes + GHG

  35. 4 lights per square meter * Sum of all forcings (1850-2000) Net = +1.6 W * *

  36. Another way to imagine global warming

  37. What global warming really looks like Data source: NASA / GISS

  38. Timescales of Natural Climate Variability • Short time scales (1-2 years): Random weather-related variations of turbulent, chaotic atmosphere. • Interannual (2-8 years): Primarily ENSO and Volcanic eruptions. • Decadal-to-century scale: • Solar Variability (decades to centuries) • Anthropogenic greenhous gas emissions (decades to centuries)

  39. What’s in store for the future? • Most probable estimate is +2 to +4°C in next 100 years • All scenarios warmer. past future Today

  40. Global Temperature in 2050

  41. 2010 * +3°C warming Recent warming is unusual, Future warming is “another world”

More Related