vii. climate change blackbody model windows and saturation feedbacks aerosols
TRANSCRIPT
VII. Climate Change
Blackbody modelWindows and saturationFeedbacksAerosols
Blackbody model
Energy In = Energy Out
Energy In = 1368 W/m2 Earth cross-section (1-reflectivity)Energy Out = Earth surface Area SB Tearth
4
SB is Stefan-Boltzmann constant
Tearth = 255 K ignores clouds and greenhouse gases
Energy Balance beyond Blackbody
Earth’s IR Emissions
Energy Balance beyond Blackbody
CO2
Concentration increasing, seasonal variationAbsorptions are nearly saturated
Saturation
Strong CO2 absorptions almost saturated.Window regions between strong absorbances:
Activity: model greenhouse gases X and Ya) Consider [Y] = 2.5 x 1013 molecules cm-3
at 1 in IR, Y = 1 x 10-19 cm2 molecule-1 What is A(1), the absorbance at 1 ?
b) Add [X] = 2.5 x 1011 molecules cm-3
at 1 in IR, X = 4 x 10-18 cm2 molecule-1
at 2 in IR, X = 1 x 10-18 cm2 molecule-1
What is the total A(1) and what is A(2) ?
c) Does the addition of X reduce heat emission more at 1 or 2?
Global mean radiative forcing of climatefor year 2000 relative to 1750 (IPCC)
Human Affects on Radiation Budget
Greenhouse Gases
See Coursepack Section E Table 3
Seinfeld and Pandis Figures 21.17-19
Instantaneouse Radiative Forcing (IRF)
of a compound (Watts m-2 kg-1)
Absolute Global Warming Potential (W m-2 kg-1 yr)
t
t
t
dttIRFAGWP
etIRFtIRF
0
/
)(
)0()(
Greenhouse Gases
Global Warming Potential (w/respect to CO2)
(dimensionless)
t
t
tCO
t
t
ti
t
t
CO
t
t
i
dtetIRF
dtetIRF
dttIRF
dttIRF
iGWPCO
i
0
/2
0
/
0
2
0
2)0(
)0(
)(
)(
)(
Key Points
• Radiative balance is complicated• Greenhouse Gas effect real, global• Greenhouse Gas effects not isolated
- feedbacks with biosphere
- feedback with geosphere
• Aerosol effects messy, local (temporary)
• Climatic effects hard to see (weather)