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QuickTime™ and a decompressor are needed to see this picture. Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. [email protected] Linear interference effects on tropical-extratropical teleconnections EGU General Assembly 2010, Vienna, Austria.

Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. [email protected] Linear interference effects

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Page 1: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

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are needed to see this picture.Christopher G Fletcher and Paul J KushnerDepartment of Physics, University of Toronto, [email protected]

Linear interference effects on tropical-extratropical teleconnectionsLinear interference effects on tropical-extratropical teleconnections

EGU General Assembly 2010, Vienna, Austria.

Page 2: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 2

Motivation

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ENSO+

Trend

[Shin and Sardeshmukh 2010]

Page 3: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 3

Motivation

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[Cagnazzo and Manzini 2009][Garfinkel and Hartmann 2008]

[Bell et al. 2009]

ENSO+ NAM—

also:[Ineson and Scaife 2009]

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TIO+ NAO+

[Annamalai et al. 2007][Hoerling et al. 2004]

[Bader and Latif 2005]

also:[Sanchez-Gomez et al. 2009]

Page 4: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 4

Main findings

• We compare the extratropical NAM response to tropical Pacific and Indian Ocean SST warming.

• Both forcings produce Rossby wave trains but the NAM responses are opposite-signed.

• The NAM response is determined by linear interference between the wave response and the climatological stationary wave

• Perturbing the climatological stationary wave results in very different NAM responses.

Page 5: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 5

GFDL AM2.1 Experiments:

TIO TPO

TIP

Amplitude0.4 ~ 1.0

- N = 100- Independent ICs- Repeating Seas Cycle- JF response

Page 6: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 6

OLR and Chi200hPa Response

TIO TPO

TIP

Page 7: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 7

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TIOTPOTIP

TIOTPOTIP

wavenumber-1

wavenumber-2

Page 8: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 8

[∆Z]

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TIO

TPO

TIP

Page 9: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 9

[∆Z]

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TIO

TPO

TIP

[Thompson and Wallace 2000]

NAM—

NAM+

NAM Pattern (+)

why?

Page 10: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 10

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TIO

TPOQuickTime™ and a

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Z*(60N)

Page 11: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 11

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Eddy Meridional Heat Flux Response (mK s-1)

[∆Z] ~ [v*T*]

Page 12: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 12

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Eddy Meridional Heat Flux Response (mK s-1)

[v*T*] decomposition: TOTAL = EM + FL

Page 13: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 13

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Eddy Meridional Heat Flux Response (mK s-1)

[v*T*] decomposition: TOTAL = EM + FLEM = LIN + NONLIN

Page 14: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 14

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[v*T*] decomposition: TOTAL = EM + FLEM = LIN + NONLINLIN ~ wv_1 + wv_2

Eddy Meridional Heat Flux Response (mK s-1)

Page 15: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 15

What happens to the NAM response when we perturb the climatological stationary wave?

Page 16: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 16

Flatten the topography over:1. Tibet and northern Eurasia (NOTIBET)2. Rocky Mountains (NOROCK)

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Standard Model NOTIBET case difference

500 hPa Geopotential Heights

Page 17: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 17

[∆Z]

NOTIBET cases NOROCK case

TIOTPO TPO

Eddy Meridional Heat Flux Response (mK s-1)

Page 18: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 18

Concluding Remarks

Linear interference determines the sign and amplitude of the zonal mean (NAM) response to tropical SST forcing

The phase and amplitude of the climatological wave are critical for NAM teleconnections; example of flattening Eurasia/Rockies.

Indian Ocean is a “sweet-spot” for forcing NAM responses: implications for future SST trends?

See Karen Smith’s poster XY103 today, which explores midlatitude forcings.

Page 19: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 19

Reference

Fletcher, C. G., and P. J. Kushner, 2010: The role of linear interference in the Annular Mode response to tropical SST forcing, J. Climate, in review.

Preprint available at: www.atmosp.physics.utoronto.ca/people/cgf

Page 20: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 20

Page 21: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 21

Winter 2009/10

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Page 22: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 22

Pattern of Tropical SST trends

[Shin and Sardeshmukh 2010]

[Barsugli et al. 2006]

Page 23: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 23

∆Z*200hPa

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TIO TPO

TIP

Page 24: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 24

Page 25: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 25

Control (unforced) climatologies: STD and NOTIBET

Page 26: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 26

Control (unforced) climatologies: STD and NOTIBET

Page 27: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 27

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TIOTPOTIP

TIOTPOTIP

wavenumber-1

wavenumber-2

Page 28: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 28

The Problem

• The model is forced by two tropical warmings: one strong (TPO), the other weaker (TIO).

• Both forcings produce poleward propagating wave trains that scale roughly with forcing amplitude.

• But the NAM responses are of opposite sign and similar in strength. Why?

Page 29: Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca Linear interference effects

EGU General Assembly 2010, Vienna, Austria. 29