Evolution of the El Ni ño Southern Oscillation (ENSO) from the Last Ice Age to Today

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lution of the El Niño Southern Oscillat ENSO) from the Last Ice Age to Today Andy Bush Dept. of Earth & Atmospheric Sciences University of Alberta Winds of Change:

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Winds of Change:. Evolution of the El Ni ño Southern Oscillation (ENSO) from the Last Ice Age to Today. Andy Bush Dept. of Earth & Atmospheric Sciences University of Alberta. Winds of Change:. Evolution of the El Ni ño Southern Oscillation - PowerPoint PPT Presentation

Transcript of Evolution of the El Ni ño Southern Oscillation (ENSO) from the Last Ice Age to Today

Page 1: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Evolution of the El Niño Southern Oscillation (ENSO) from the Last Ice Age to Today

Andy BushDept. of Earth & Atmospheric Sciences University of Alberta

Winds of Change:

Page 2: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Evolution of the El Niño Southern Oscillation (ENSO) from the Last Ice Age to Today

Andy BushDept. of Earth & Atmospheric Sciences University of Alberta

Winds of Change:

A.B.G. Bush, 2006, Journal of Climate, in press.

Page 3: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Evolution of the El Niño Southern Oscillation (ENSO) from the Last Ice Age to Today

Andy BushDept. of Earth & Atmospheric Sciences University of Alberta

Winds of Change:

A.B.George Bush, 2006, Journal of Climate, in press.

Page 4: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Evolution of the El Niño Southern Oscillation (ENSO) from the Last Ice Age to Today

Andy BushDept. of Earth & Atmospheric Sciences University of Alberta

Winds of Change:

A.B.George Bush, 2006, Journal of Climate, in press. [email protected]

Page 5: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Motivation: To understand the climatological factorsthat determine the period and intensity of interannualvariability (ENSO).

Page 6: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Motivation: To understand the climatological factorsthat determine the period and intensity of interannualvariability (ENSO).

Past climates provide altered mean states within which interannual variability exists.

Page 7: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 8: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 9: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Animation of TOPEX/Poseidon sea surface height data

QuickTime™ and aCinepak decompressor

are needed to see this picture.

Page 10: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Some human impacts of ENSO: 1) Impact on disease spread (malaria and dengue) 2) Food production

Page 11: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 12: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 13: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 14: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 15: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

El Niño winter snow anomalies

Page 16: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Observed CompositeTemperature Anomalies

El Niño

La Niña

Page 17: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

SST anomalies, Aug.-Sept. 2006: El Niño’s coming…

Page 18: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Existing numerical models for ENSO prediction are anomaly models in which a background climate state is assumed. Predicted variables are perturbations on that background state. The two climate variables that must be assumed are:1) Mean depth of the thermocline2) Strength of the climatological easterly trade winds

These quantities are known for today’s climate, so anomaly models work quite well for ENSO prediction.

Page 19: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 20: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Existing numerical models for ENSO prediction are anomaly models in which a background climate state is assumed. Predicted variables are perturbations on that background state. The two climate variables that must be assumed are:1) Mean depth of the thermocline2) Strength of the climatological easterly trade winds

These quantities are known for today’s climate, so anomaly models work quite well for ENSO prediction.

However, one or both of these quantities appear to havebeen different in the past (aeolian deposits, upwelling indices,planktonic foraminifera, etc.). Changes in the strength of thegeneral circulation can cause changes in these quantities.

Page 21: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Our atmosphere exhibits dynamic variability associated with midlatitude baroclinic waves, or eddies.

Page 22: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Our atmosphere exhibits dynamic variability associated with midlatitude baroclinic waves, or eddies.

Eddies may be either TRANSIENT (not fixed to a specificgeographic location) or STATIONARY (fixed geographically; caused by mountain ranges, continent-ocean contrasts, etc.)

Eddies play a very important role in governing the strength of the general circulation.

Page 23: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

QuickTime™ and aFLIC Animation decompressorare needed to see this picture.

Page 24: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Atmospheric eddies are the primary mechanism by which low latitude HEAT is transported poleward (v’T’>0). This occurs in the growth phase of baroclinic waves. (Idealized life cycle)

Page 25: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Atmospheric eddies are the primary mechanism by which low latitude HEAT is transported poleward (v’T’>0). This occurs in the growth phase of baroclinic waves.

They are also the primary mechanism by which the zonal mean(and, by angular momentum conservation, the meridional mean)flow is forced (u’v’>0). This occurs in the Rossby wave decayphase of the baroclinic wave, in which easterly momentum istransported equatorward.

Page 26: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Atmospheric eddies are the primary mechanism by which low latitude HEAT is transported poleward (v’T’>0). This occurs in the growth phase of baroclinic waves.

They are also the primary mechanism by which the zonal mean(and, by angular momentum conservation, the meridional mean)flow is forced (u’v’>0). This occurs in the Rossby wave decayphase of the baroclinic wave, in which easterly momentum istransported equatorward.

Global Implications?

Page 27: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Atmospheric eddies are the primary mechanism by which low latitude HEAT is transported poleward (v’T’>0). This occurs in the growth phase of baroclinic waves.

They are also the primary mechanism by which the zonal mean(and, by angular momentum conservation, the meridional mean)flow is forced (u’v’>0). This occurs in the Rossby wave decayphase of the baroclinic wave, in which easterly momentum istransported equatorward.

Global Implications?

More Eddy ActivityStronger Circulation

Page 28: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 29: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Eddy activity depends on the meridional temperature gradients of the climatological background state.

Stronger temperature gradients increase the rate of eddy formation (can be shown from linear theory).

Page 30: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Eddy activity depends on the meridional temperature gradients of the climatological background state.

Stronger temperature gradients increase the rate of eddy formation (can be shown from linear theory).

Meridional temperature gradients were quite different in the past for a variety of reasons (ice sheets, orbitalparameters, greenhouse gases, etc.).

Page 31: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Eddy activity depends on the meridional temperature gradients of the climatological background state.

Stronger temperature gradients increase the rate of eddy formation (can be shown from linear theory).

Meridional temperature gradients were quite different in the past for a variety of reasons (ice sheets, orbitalparameters, greenhouse gases, etc.).

Also, during an Ice Age, topographic forcing of stationary waves was very different because of the massive ice sheets.

Page 32: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

The numerical experiments

A global coupled atmosphere-ocean general circulation model isused to simulate 80 years of climate for:

Page 33: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

The numerical experiments

A global coupled atmosphere-ocean general circulation model isused to simulate 80 years of climate for:

1) Last Glacial Maximum (LGM, 21,000 years ago) -massive continental ice sheets -decreased atmospheric carbon dioxide -sea level lowering of 120 m -surface vegetation different

Page 34: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Schematics of ice sheet extent at the Last Glacial Maximum

Page 35: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

The numerical experiments

A global coupled atmosphere-ocean general circulation model isused to simulate 80 years of climate for:

1) Last Glacial Maximum (LGM, 21,000 years ago) -massive continental ice sheets -decreased atmospheric carbon dioxide -sea level lowering of 120 m -surface vegetation different

2) 9,000 years ago -orbital parameters -remnants of Laurentide ice sheet

Page 36: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Obliquity was high in the early-mid Holocene (9,000-6,000 years ago).This accentuates the seasonal cycle; warmer summers and colder winters.

Page 37: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

The numerical experiments

A global coupled atmosphere-ocean general circulation model isused to simulate 80 years of climate for:

1) Last Glacial Maximum (LGM, 21,000 years ago) -massive continental ice sheets -decreased atmospheric carbon dioxide -sea level lowering of 120 m -surface vegetation different

2) 9,000 years ago -orbital parameters -remnants of Laurentide ice sheet

3) 6,000 years ago -orbital parameters

Page 38: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

The numerical experiments

A global coupled atmosphere-ocean general circulation model isused to simulate 80 years of climate for:

1) Last Glacial Maximum (LGM, 21,000 years ago) -massive continental ice sheets -decreased atmospheric carbon dioxide -sea level lowering of 120 m -surface vegetation different

2) 9,000 years ago -orbital parameters -remnants of Laurentide ice sheet

3) 6,000 years ago -orbital parameters

4) Today (control)

Page 39: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

The numerical experiments

A global coupled atmosphere-ocean general circulation model isused to simulate 80 years of climate for:

1) Last Glacial Maximum (LGM, 21,000 years ago) -massive continental ice sheets -decreased atmospheric carbon dioxide -sea level lowering of 120 m -surface vegetation different

2) 9,000 years ago -orbital parameters -remnants of Laurentide ice sheet

3) 6,000 years ago -orbital parameters

4) Today (control)

5) Doubling of atmospheric carbon dioxide (2xCO2)

Page 40: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 41: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 42: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 43: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 44: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

El Niño and La Niña events are defined by sea surfacetemperature anomalies in the Nino 3.4 region. Valuesare typically normalized by the standard deviation.

Page 45: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Control simulation produces good statistics for ENSO.

QuickTime™ and aGIF decompressor

are needed to see this picture.

Page 46: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 47: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

S.D.=0.83

S.D.=0.87

Control

Observations

Page 48: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Wavelet analysisPower Spectrum:

Averaged in time:

Observations

Page 49: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

S.D.=0.83

S.D.=0.87

Control

Observations

Page 50: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Values Normalized byTheir standardDeviation

LGM

9,000 B.P.

6,000 B.P.

Control

Observations

2xCO2

Page 51: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Values Normalized byTheir standardDeviation

LGM

9,000 B.P.

6,000 B.P.

Control

Observations

2xCO2

Page 52: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Values Normalized byTheir standardDeviation

LGM

9,000 B.P.

6,000 B.P.

Control

Observations

2xCO2

Page 53: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Values Normalized byTheir standardDeviation

LGM

9,000 B.P.

6,000 B.P.

Control

Observations

2xCO2

Page 54: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Values NOTNormalized byThe standardDeviation

S.D.=0.58

S.D.=0.55

S.D.=0.81

S.D.=0.83

S.D.=0.87

S.D.=1.05

IncreasingPeriod of ENSO

(decrease inFrequency)

Page 55: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Not much changein mean thermoclinedepth (except forCO2 case)

Change in east-west tiltof thermocline consistentwith change in strength of mean atmospheric trade winds

Changes in the climatological mean states

Page 56: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Not much changein mean thermoclinedepth (except forCO2 case)

Change in east-west tiltof thermocline consistentwith change in strength of mean atmospheric trade winds

Changes in the climatological mean states

~20% reduction in Easterly trade winds from LGM to today

Page 57: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Linear Stability Analysis of the coupled atmosphere-ocean system (Fedorov and Philander, Science, 2001)

(increases withdecreasing windspeed)

Control

Growth Rate

PERIOD

Page 58: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Linear Stability Analysis of the coupled atmosphere-ocean system (Fedorov and Philander, Science, 2001)

(increases withdecreasing windspeed)

Control

Growth Rate

PERIOD

* LGM* 9,000* 6,000

*2xCO2

Page 59: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Is there a reason why the strength of the atmospheric winds should be different in these simulations?

Page 60: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Is there a reason why the strength of the atmospheric winds should be different in these simulations?

Yes. The eddy fields are very different.

Page 61: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Is there a reason why the strength of the atmospheric winds should be different in these simulations?

Yes. The eddy fields are very different.

LGM: enhanced meridional temperature gradient (transient eddies) presence of massive continental ice sheets (stationary eddies)

Page 62: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Is there a reason why the strength of the atmospheric winds should be different in these simulations?

Yes. The eddy fields are very different.

LGM: enhanced meridional temperature gradient (transient eddies) presence of massive continental ice sheets (stationary eddies)

9,000 and 6,000 B.P.: more seasonal climate because of enhanced obliquity of the planet and summertime perihelion. Effect is stronger at 9,000 B.P. than 6,000 B.P. Hotter summers and colder winters should produce more wintertime transient eddy activity.

Page 63: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Is there a reason why the strength of the atmospheric winds should be different in these simulations?

Yes. The eddy fields are very different.

LGM: enhanced meridional temperature gradient (transient eddies) presence of massive continental ice sheets (stationary eddies)

9,000 and 6,000 B.P.: more seasonal climate because of enhanced obliquity of the planet and summertime perihelion. Effect is stronger at 9,000 B.P. than 6,000 B.P. Hotter summers and colder winters should produce more wintertime transient eddy activity.

CO2: reduced meridional temperature gradient (transient eddies)

Page 64: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

The Eliassen-Palm (E-P) flux vector:

Z

Y

Poleward heat flux(v’T’>0)

Equatorward momentum flux(u’v’>0)

E-P flux

Page 65: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 66: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 67: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 68: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Increased midlatitudeeddies drive strongersubtropical subsidence,a stronger Hadleycell and, through angular momentumconservation,stronger equatorialeasterlies.

Page 69: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Peak easterly (i.e. negative)winds over the Pacificoccur near the solstices ofend-December and end-June when baroclinic eddy activity is greatest

Coupled modelTAO winds

Zonally symmetricatmosphere-onlyintegration for aland-covered planet--wind changes are notrelated to the Asian monsoon.

Page 70: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Changing TeleconnectionPatterns:Temperature

LGM

9K BP

6K BP

Today

2xCO2

Page 71: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

LGM

9K BP

6K BP

Today

2xCO2

ChangingTeleconnection Patterns:Precipitation

Page 72: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Implications of changing teleconnection patterns:

Page 73: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Implications of changing teleconnection patterns:

Caution must be used when interpreting paleoclimate proxy recordsfor ENSO. For example, Rodbell et al (1999) interpreted the absence of a distinct ENSO signal from early Holocene sediments ofcoastal Peru to mean that ENSO was absent between 15,000 and~6,000 years ago. This assumed “stationarity” of the teleconnectionpattern is incorrect.

Page 74: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Implications of changing teleconnection patterns:

Caution must be used when interpreting paleoclimate proxy recordsfor ENSO. For example, Rodbell et al (1999) interpreted the absence of a distinct ENSO signal from early Holocene sediments ofcoastal Peru to mean that ENSO was absent between 15,000 and~6,000 years ago. This assumed “stationarity” of the teleconnectionpattern is incorrect.

Also, Koutavas et al (2002) interpreted a reduced zonal SST gradientin the tropical Pacific at the LGM to mean the glacial climate was in an El Niño state. This assumption does not take into account the changed mean state of the LGM climate.

Page 75: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Implications of changing teleconnection patterns:

Caution must be used when interpreting paleoclimate proxy recordsfor ENSO. For example, Rodbell et al (1999) interpreted the absence of a distinct ENSO signal from early Holocene sediments ofcoastal Peru to mean that ENSO was absent between 15,000 and~6,000 years ago. This assumed “stationarity” of the teleconnectionpattern is incorrect.

Also, Koutavas et al (2002) interpreted a reduced zonal SST gradientin the tropical Pacific at the LGM to mean the glacial climate was in an El Niño state. This assumption does not take into account the changed mean state of the LGM climate.

Teleconnections produce high latitude fingerprints of ENSO changes.

Page 76: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Conclusions

The period of ENSO increases from the LGM to today

Page 77: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Conclusions

The period of ENSO increases from the LGM to today

The amplitude of ENSO increases from the LGM to today

Page 78: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Conclusions

The period of ENSO increases from the LGM to today

The amplitude of ENSO increases from the LGM to today

These changes are consistent with the decrease in strength of the climatological easterly trade winds overthe Pacific

Page 79: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Conclusions

The period of ENSO increases from the LGM to today

The amplitude of ENSO increases from the LGM to today

These changes are consistent with the decrease in strength of the climatological easterly trade winds overthe Pacific

Decrease in trade wind strength is consistent with thedecrease in midlatitude eddy activity

Page 80: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Conclusions

The period of ENSO increases from the LGM to today

The amplitude of ENSO increases from the LGM to today

These changes are consistent with the decrease in strength of the climatological easterly trade winds overthe Pacific

Decrease in trade wind strength is consistent with thedecrease in midlatitude eddy activity

Decrease in eddy activity related to topographic forcingat the LGM, to orbital forcing at 9,000 and 6,000 B.P., andto radiative forcing in the 2xCO2 environment

Page 81: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

What’s been observed?

Increased tropical Pacific wind speeds during the LGM(aeolian deposits, upwelling indices from ocean cores)

Page 82: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

What’s been observed?

Increased tropical Pacific wind speeds during the LGM(aeolian deposits, upwelling indices from ocean cores)

Increased tilt of the tropical Pacific thermocline duringthe LGM (planktonic foraminifera)

Page 83: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

What’s been observed?

Increased tropical Pacific wind speeds during the LGM(aeolian deposits, upwelling indices from ocean cores)

Increased tilt of the tropical Pacific thermocline duringthe LGM (planktonic foraminifera)

Increase in ENSO amplitude and period from LGM to todayfrom corals (Tudhope et al, 2001)

Page 84: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

What’s been observed?

Increased tropical Pacific wind speeds during the LGM(aeolian deposits, upwelling indices from ocean cores)

Increased tilt of the tropical Pacific thermocline duringthe LGM (planktonic foraminifera)

Increase in ENSO amplitude and period from LGM to todayfrom corals (Tudhope et al, 2001)

Decrease in easterly trade wind strength (Nature, May 2006)

Page 85: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

With many thanks to…

Canadian Foundation for Climate andAtmospheric Research (CFCAS; PolarClimate Stability Network)

Page 86: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

With many thanks to…

Canadian Foundation for Climate andAtmospheric Research (CFCAS; PolarClimate Stability Network)

…and all of you!

Page 87: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Wavelet analysisPower Spectrum:

Averaged in time:

Page 88: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Seasonal Cycle

Page 89: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Seasonal Cycle

QBO?

Page 90: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Seasonal Cycle

QBO?

Decadal Variability

Page 91: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Seasonal Cycle

QBO?

ENSO

Decadal Variability

Page 92: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 93: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 94: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 95: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 96: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today

Changing teleconnection patterns: composite temp. anomaliesControl 6,000 B.P.

9,000 B.P. LGM

Page 97: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today
Page 98: Evolution of the El Ni ño Southern Oscillation    (ENSO) from the Last Ice Age to Today