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29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

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Page 1: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

29th Macaulay LectureAberdeen, 14 Nov 2005

Planetary Co-Evolution:Where On Earth Are We Going

John Schellnhuber

Page 2: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber
Page 3: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

An Integrated Earth System

Page 4: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber
Page 5: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber
Page 6: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

COCO22 Emissions from Scenarios with Technological Uncertainty Emissions from Scenarios with Technological Uncertainty

5 10 15 20 25 30

5.5

5.0

4.5

4.0

3.5

3.0

2.5

2.0

1.5

1.0

0.5

0.0

Set of 130,000 Scenarios

Optimal set of13,250 scenarios

GtC in 2100

Rel

ativ

e F

req

uen

cy in

Per

cen

t

Gritsevkyi&NakicenovicGritsevkyi&Nakicenovic IIASA 2000IIASA 2000

Page 7: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Co-evolution Timeline

Global tipping points:• Great oxidation• Snowball Earths• Cambrian explosion

T. M. Lenton et al. (Working Group 1) 91st Dahlem Workshop on Earth System Analysis for Sustainability (2003)

Ages in Ga (109 yr BP)

Page 8: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Environment-Information LadderCo-Evolution of Information Processing and Environmental

Complexification

Lenton, Schellnhuber & Szathmáry (2004):Nature, forthcoming

Pseudo-Time

Degree of Complexity

Environmental Make-up

Informational Organization

E1 I1

I2

I3

I4

I5

I6

E2

E3

E4

E5

E6

Coevolution

Degree of Complexity

Environmental Make-up

Informational Organization

E1 I1

I2

I3

I4

I5

I6

E2

E3

E4

E5

E6

ForcingEvolution

Coevolution

Page 9: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

EARTH SYSTEM MODELLING

ToPIK Days 2003

Page 10: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

MODEL DESCRIPTION

Franck et al. (2002): Tellus 54B 325.

Page 11: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

MODEL RESULTS

Evolution of global surface temperature.

Evolution of the cumulative biosphere pools for prokaryotes, eukaryotes,

and complex multicellular life.

von Bloh, Bounama & Franck (2003): Geophys. Res. Lett. 30 (18) 1963

Page 12: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

CAMBRIAN EXPLOSION

• Biological Big Bang 540 million years ago• Most modern animal groups appear

Page 13: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Mid-Holocene Saharan desertification• Non-linear change in a

single equilibrium• Followed by the rise of

“hydraulic societies” in Egypt, Mesopotamia…

• A tipping point in human systems linked to a tipping point in vegetation-climate?

De Menocal, P. J. et al. (2000). Quaternary Science Reviews 19: 347-361.

Page 14: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Human co-evolution

Civilisations collapse!Read Jared Diamond

Tipping points:• Food production• Freshwater• Displacement• Disease• Economy• Technology• Governance

102

Yr BP

Global industrialisation

Anthropogenicclimate change

Hydraulic societies

Hominins

Mega-fauna extinctions

African-Asianclimate drying

Quaternary climate changes

104

106

Environment Bio-information

Global governance?

Organised groups(syntax?)

Yr APEngineeredplanetary

environment??

Page 15: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Vitousek (1994)

What is Global Change?

• Nitrogen fixation • Temperature• Biodiversity………..

• Global-scale changes that affect the functioning of the Earth System

• Much more than climate change• Socio-economic as well as biophysical

For example, changes in:

Reid

& M

iller (1989)

Page 16: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

NOAA

What is Global Change?

• Nitrogen fixation • Temperature • Biodiversity • Atmosphere composition• Population• N in the coastal zone• Forest cover• Fisheries exploitation

For example, changes in:

U.S

. Bu

rea

u o

f the

Ce

ns

us

Ma

ck

en

zie e

t al (2

00

2)

Ric

ha

rds

(19

91

), WR

I (19

90

)

FAO

Page 17: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Temperature Since 850 AD

Science, 10 February 2005

Page 18: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

• an integrated study of the Earth System, • the changes occurring to the System, and• the implications for global sustainability.

Earth System Science PartnershipDIVERSITAS, IGBP, IHDP, WCRP

Page 19: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Food Provision

Food demands are changing:

• How will global environmental change (GEC) affect food provision and vulnerability?

• How might societies and producers adapt their food systems to cope with GEC?

• What would be the environmental and socioeconomic consequences of such adaptations?

Page 20: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Carbon Cycle

• Patterns and variability: what are the geographical and temporal patterns of carbon sources and sinks?

• Processes, controls and interactions: what are the controls and feedback mechanisms - natural and anthropogenic - that determine the dynamics of the carbon cycle on scales of years to millennia?

• Management of the carbon cycle: what are the future dynamics of the carbon-climate system and what are the points of intervention and windows of opportunity for managing this system?

Page 21: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Water Resources

• What are the relative magnitudes of changes in the global water system (GWS) due to human activities and environmental factors?

• What are the social and Earth System feedbacks of human-driven change to the global water system?

• To what extent is the GWS resilient and adaptable to global change?

Page 22: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Human HealthUnder Development

Project Goals:

• To determine the past, current, and future health impacts of global environmental change.

• To enrich the policy discussion about mitigation and adaption from a human health perspective.

Page 24: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Earth System Achilles Heels

Page 25: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

EuropeEurope’’ssFree HeatingFree Heating

SystemSystem

Page 26: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

West Antarctic Ice Sheet Greenland Ice Sheet

Page 27: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

0o 2.5o E

50o N

52.5o N

London

The coastline of south-eastern UK, assuming 6m of

sea level rise in the wake of Greenland Ice Sheet melting

Page 28: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

A Global Inventory of Natural Gas Hydrate Occurrence

USGS, 2001. More information: http://walrus.wr.usgs.gov/globalhydrate/

Page 29: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Tibetan Plateau

Page 30: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Broadleaf tree cover (gridbox fraction)

in coupled climate-carbon cycle

simulation

Hadley Centre for Climate Prediction and Research

Page 31: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Thanks to Joseph M. Prospero

RSMAS, Univ. of Miami

Dust Storm - Bodele Depression, Chad

The location of dry lakes

in the Bodele Depression

Page 32: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

(N. Petit-Maire, 1990)

deMenocal et al., 2000deMenocal et al., 2000

Will Greenhouse Green the Sahara?

Page 33: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Years of Simulation[1800] [2000]

Veg

eta

tion

fr

acti

on

Transient CO2 scenario (1%, 1000 ppm)

Changes in Potential Vegetation Cover in the Sahara

Claussen et al., 2003Claussen et al., 2003

Page 34: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Anthropogenic Global Warming

Re-Greening of Sahara

Amazon Forest Die-Back

Lifestyle & Recreation

ChangeGlobal Change Synergism

(+)

(+)

(+)

(+)

(+)

(-)

Reduced Dust Export

Regional Climate Change

Regional Climate Change

Additional Carbon

Release

Additional GHG

Emissions

Land Surface

Disturbance

Page 35: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Arabian Sea

Image: WJ Schmitz, WHOI

Southwesterly Summer Monsoon

Northeasterly Winter Monsoon

Page 36: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Worst Case Scenario for Monsoon Development

Roller-Coaster Trajectory

Zickfeld et al. 2005, GRL 32, 15707 (see also Ball 2005, Nature, August 15th)

Wet Regime Bi-stability

Dry Regime

Page 37: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

|  Thursday, August 18, 2005 |

Man’s murder of monsoon - German climate researchers issue India warning

G.S. MUDUR

New Delhi, Aug. 17: Increasing air pollution and loss of forest cover in South Asia may trigger a sudden breakdown of the Indian monsoon and sharply reduce rainfall in the subcontinent within decades, climate scientists said.

Researchers at Germany’s Potsdam Institute for Climate Impact Research who set out to explore the stability of the summer monsoon over India have discovered that it’s particularly vulnerable to human influences.

“The stage seems to be set for a man-made reduction of the Indian summer monsoon,” climate physicist Kirsten Zickfeld and her colleagues said in a paper published in the latest issue of the journal, Geophysical Research Letters.

The scientists have shown that tiny particles called aerosols, spewed into the atmosphere during the burning of coal and firewood, reduce monsoon rainfall, while rising greenhouse gases such as carbon dioxide tend to increase rainfall.

A steady rise in aerosols will reduce the amount of sunlight striking land and lower land temperatures. This will decrease the supply of moisture-laden air from the sea and lower rainfall. Shrinking forest cover will also have the same effect.

“When these effects exceed a critical threshold, the monsoon could experience a sudden breakdown,” Zeckfeld told The Telegraph in a telephone interview. “We’d then see a very weak monsoon consistently over many years,” she said.

“This is something we should be concerned about,” said Sourendra Bhattacharya, a climate scientist at the Physical Research Laboratory in Ahmedabad.

Climate records have revealed that the Indian monsoon has undergone abrupt changes over the past 8,000 years. “There have been some dramatic ups and downs in the monsoon,” said Bhattacharya who specialises in ancient climate studies.

“While those ancient changes in rainfall were driven by natural phenomena, we’re now anticipating changes influenced by human activities,” he said.

Zeckfeld said her study could not quantify the reduction in the rainfall, nor predict when exactly the breakdown of the monsoon might occur.

But with rising aerosol levels, it could happen over the next few decades, she said.

If India adopts new technologies to reduce its aerosol emissions, Zeckfeld said, the monsoon may display a “roller-coaster” behaviour. After a suppression over the next decades, as aerosol-reduction policies begin to take effect and economic growth drives up carbon dioxide emissions, the monsoon may abruptly intensify and re-establish the “wet-monsoon” regime within a few years.

“It might be hard for India to have the monsoon doing really weird things — reducing and then abruptly increasing,” she said. The study has also cautioned that India might find it a challenge to adapt to such a roller-coaster scenario.

This is not the first study to signal the danger that aerosols pose to the monsoon. A study by climate scientist Murari Lal, formerly at the Indian Institute of Technology, New Delhi, in 1995 was the first to show that aerosols can weaken rainfall.

Bhattacharya said the impact of aerosols would depend on what type they were. Some aerosols such as soot absorb sunlight and will tend to increase rainfall, while sulphur-containing particles will reflect sunlight and tend to reduce rainfall.

“We might also have a scenario where the effects of aerosols and greenhouse gases cancel each other out,” Bhattacharya said.

Page 38: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Monsoon Chaos?

TTS

Sss FFAFHLE

t

TC

)1(

THT

SYHSTT

SSA

A ALPFAFFFAFHt

TC

,, )1()1(

VV

q APEt

qC

12

1

1 WW

f

REP

t

W

21

2

12 WW

f

f

t

W

Ts: surface temperature

TA: near-the-surface atmosphere temperature qv: near-the-surface specific humidityW1,2: wetness of the upper and the lower soil layerE: evaporationP: precipitationH: sensible heat flux from the surface

Physically based Lorenz-type model for the Indian summermonsoon:

Page 39: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Lorenz Attractor

283

81,,

10

r

b

dca

Parameter Settings

YXX

cYrXaXZY

,bZdXYZ

0,0

1

0

2 ';

';

'

V

V

q

qZ

W

WY

W

WX

where

Page 40: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

“I believe that climate change is the most important long-term issue we face as a global community. It is an issue that will require sustained action over the coming decades. A sound understanding of the science must be the basis for this action.”

Tony Blair, UK Prime Minister

3 Nov 2004

One view of climate change

Page 41: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

“Much of the debate over global warming is predicated on fear, rather than science. I called the threat of catastrophic global warming the greatest hoax ever perpetrated on the American people.”

James M. Inhofe, US Senator &

Chairman of Environment and Public Works Committee

4 Jan 2005

….and another

Page 42: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Hurrican Katrina Hurrican Rita

Page 43: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Consolidated Results:

Schellnhuber et al. (Eds.)

„Avoiding Dangerous Climate Change“

CUP, forthcoming

Page 44: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber
Page 45: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Carbon Management

Page 46: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Macro-Engineering Options

Page 47: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Practical Geoengineering Options to PreventAbrupt and Long-Term Climate Change

Alvia Gaskill, PresidentEnvironmental Reference Materials, Inc.

Research Triangle Park, [email protected]

888-645-7645

Charles E. Reese, Ph.D.Consultant

St. Julians, [email protected]

356-2137-1223

Presented to:

U.S. Climate Change Technology ProgramU.S. Department of Energy

Washington, D.C.

June 16, 2004

Page 48: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Our Conclusion

• GHG emissions will NOT be reduced in time to prevent a climate catastrophe!

Page 49: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Albedo modification potential for Southern California

Example: urban albedo increase 5km cells: 1291>0, 625>0.01,456>0.02, 256>0.05, 143>0.10, 40>0.15, 17>0.16

Los AngelesSan Diego

Page 50: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Candidates for Albedo Enhancement

• Las Vegas, NV

• Phoenix, AZ

• Covering 5-20 square miles outside each city may cool off the cities themselves.

• This can be done much sooner than the whitening of urban surfaces and large scale tree planting which may take decades to complete.

Page 51: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber
Page 52: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber
Page 53: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Cost Benefit Equation for Climate Policy Implemented through

Mitigation (M) and Adaptation (A)

B(M,A) = AD(M,A) – C1(M) – C2(A)Net

BenefitsAvoided Damages

Mitigation Costs

Adaptation Costs

Claims:AD(M,A)

M

AD(M,A)

A

>>

C1(M) < 1% Global GDP~

1.

2.

Page 54: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Learning Curves

20000

10000

5000

1000

100

10 100 1000 10000 100000

1982

1987

1963

1980

Windmills (USA)(learning rate ~ 20%)

RD&D phase

Commercializationphase

USAJapan

Cumulative MW installed

19811983

500

Photovoltaics(learning rate ~ 20%)

Gas turbines (USA)(learning rate ~ 20%, ~10%)

US

(19

90

)$/k

W

1995

1992

200

2000

Nakicenovic et al. IIASA 1998

IEA (2000): Experience Curves for Energy

Technology Policy; p. 21

Page 55: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

0%

1%

2%

3%

4%

5%

6%

7%

8%

9%

10%

11%

12%

5 10 15 20 25 30

Ranges, GtC

Rela

tive

Freq

uenc

yNear-optimal set of 53 technology dynamics

Based on Gritsevkyi & Nakicenovic, IIASA 2000

Page 56: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

0

400

800

1200

1600

2000

400

800

1200

1600

2000

400

800

1200

1600

2000

0

0

0

400

800

1200

1600

2000

400

800

1200

1600

2000

400

800

1200

1600

2000

0

0

0

400

800

1200

1600

2000

400

800

1200

1600

2000

400

800

1200

1600

2000

0

0

Page 57: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Relative losses of global GDP as a consequence of Climate Change

mitigation measures

Page 58: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

The Model MIND

Technological change is driven by investment decisions

• Learning-by-doing in the energy sectors

• Assessment of Mitigation Options– Energy efficiency

– Renewable energy sources

– Carbon Capturing and Sequestration

Page 59: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Intertemporal welfarefunction

Optimize ConstraintGuardrail

Per capitaconsumption

Budget

Industrialproduction

Labour efficiencyunits

Energy efficiencyunits

Labour

Labourknowledge

capital

Energy Energyknowledge

capital

Renewableenergy

Secondaryfossil

energyTraditionalnon-fossil energy

(exog.)

Capital

Learning by doing

Capital stockren. energy

sector

Capital stockfossil energy

sector

Fossilprimaryenergy

carbonintensity (exog.)

Fossil fuelextraction

Capital stockextraction

Learning by doingResource scarcity

CO2concentration

Land usechange

CO2 emission

Fossil fuelCO2

emissions

SO2 emissions

Leakage

Energy

Capital stocksequestration

sector

Rad. forcing ofother GHG (exog.)

Global mean temperature change

Total radiative forcing

Captured CO2and SO2

Desulphurization(exog.)

Page 60: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Costs of Reducing Climate Change

Mitigation costs

0

0,5

1

1,5

2

2,5

3

300 400 500 600 700 800

CO2 stabilization level [ppmv]

Pre

se

nt

va

lue

of

wo

rld

G

WP

los

s [

%] AIM A1B

MARIA A1T

MARIA A1B

MiniCAM A1Fl

MIND CPP

Page 61: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

IMPC-Kostenvergleich für DO2-Stabilisierung bei 450, 500 bzw. 550 ppm. Erfaßt sind nur Modelle, die in vergleichbarer Weise geeignet sind, den technischen Fortschritt darzustellen.

Page 62: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

Vostok Ice Core – the record of the last 420,000 years

Images from WDCP/IPCC

Human Impact on Atmosphere

Page 63: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

The Future?

Mann et al (1999) and IPCC 2000

N.H

. T

emp

(°C

)

0

0.5

1

-0.5

1000 1500 2000

Page 64: 29th Macaulay Lecture Aberdeen, 14 Nov 2005 Planetary Co-Evolution: Where On Earth Are We Going John Schellnhuber

The Future?IPCC Projections2100 AD

2

4

3

5

6

1

0

Glo

bal

Tem

p (°

C)

N.H

. T

emp

(°C

)

0

0.5

1

-0.5

1000 1500 2000

Mann et al (1999) and IPCC 2000