earth’s radiative balance or, how i learned to stop worrying and love the greenhouse effect if the...

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Earth Earth s radiative balance s radiative balance or, how I learned to stop worrying and love the greenhouse effect or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T T 4 = S / 4 (1 — A) T = 255 T = 255 K K -18 ˚C -18 ˚C 0 ˚F 0 ˚F Albedo (reflectivity) Solar constant (1370 W/m 2 ) Stefan-Boltzmann constant (5.67x10 -8 ) reflected Absorbed and re-radiated as heat

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Page 1: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =

EarthEarth’’s radiative balances radiative balanceor, how I learned to stop worrying and love the greenhouse effector, how I learned to stop worrying and love the greenhouse effect

If the Earth had no atmosphere:

TT4 = S/4(1 — A)

T = 255 KT = 255 K

-18 ˚C-18 ˚C

0 ˚F0 ˚F

Albedo (reflectivity)

Solar constant (1370 W/m2) Stefan-Boltzmann constant

(5.67x10-8)

reflected

Absorbed and re-radiated as heat

Page 2: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =
Page 3: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =
Page 4: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =

288 - 255 = 33 ˚ of 288 - 255 = 33 ˚ of ‘‘normalnormal’’ greenhouse warming greenhouse warming

Actual surface

No atmosphere

Sunlight Infra-red radiation

Air

Page 5: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =

0

-0.4

0.4

1900 1940 19801860

Te

mp

era

ture

ano

mal

y (˚

C)

Global Temperatures for the last 150 yearsGlobal Temperatures for the last 150 years(5-year running average; as of ~2005)(5-year running average; as of ~2005)

Civil war

Model T

World War II

Al Gore inventsthe internet

Page 6: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =

After Jones and Wigley, 1980

“ . . . a global deterioration of climate, by order of magnitude larger than any hitherto experienced by civilized mankind, is a very real possibility and indeed may be due very soon.”

Climate change in the age of DiscoClimate change in the age of Disco

Page 7: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =

The last ~10 years: another plateau resembling ~1950

Page 8: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =

Currently favored explanation of the plateaus is thatthese are periods when accumulated heat gets

preferentially stored in ocean instead of atmosphere…

Page 9: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =

Warming has a strong geographic bias(2000-2009 avg. vs. 1950-1980 mean)

±2.5 ˚C scale

Page 10: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =

A long-suspected driving force — rise in COA long-suspected driving force — rise in CO22

Global average 1700-2000 AD

Mauna Loa 1958-2004 AD

Page 11: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =

The COThe CO22 Greenhouse Effect Greenhouse EffectWhat should physical principles lead me to expect of global warming?What should physical principles lead me to expect of global warming?

Complications • Solar ‘constant’ is a variable• Water-vapor feedback• Albedo

• Ice• Clouds• Aerosols and dust• Ground cover

33 ˚ of warming = 20˚ from H2Ov + 10 ˚ from CO2 + 3 ˚ from other things

COCO22 has risen 10 has risen 10’’s of %, so T shoulds of %, so T should

have risen by a degree or morehave risen by a degree or more

Arrhenius, 1896

Doubling CO2 = 5-6 ˚C warming

Page 12: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =

Cylon invasion happens here

Page 13: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =
Page 14: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =
Page 15: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =

Reid, 1999; by way of www.oar.noaa.gov

Sunspots and early 20th century temperatures

Page 16: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =
Page 17: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =
Page 18: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =
Page 19: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =
Page 20: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =
Page 21: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =
Page 22: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =
Page 23: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =
Page 24: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =
Page 25: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =
Page 26: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =
Page 27: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =
Page 28: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =

So what factor is to blame for 20So what factor is to blame for 20thth century T rise? century T rise?Wrong question — lots of things are to Wrong question — lots of things are to ‘‘blameblame’’ but some but some

are more important than others, and at different timesare more important than others, and at different times

Page 29: Earth’s radiative balance or, how I learned to stop worrying and love the greenhouse effect If the Earth had no atmosphere: T  T 4 = S / 4 (1 — A) T =