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Linear interference effects on tropical-extratropical teleconnections. Christopher G Fletcher and Paul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca. EGU General Assembly 2010, Vienna, Austria. Motivation. ENSO+. Trend.
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Linear interference effects on tropical-extratropical teleconnections Christopher G FletcherandPaul J Kushner Department of Physics, University of Toronto, Canada. chris.fletcher@utoronto.ca EGU General Assembly 2010, Vienna, Austria.
Motivation ENSO+ Trend [Shin and Sardeshmukh 2010] EGU General Assembly 2010, Vienna, Austria.
Motivation ENSO+ NAM— [Ineson and Scaife 2009] also: [Garfinkel and Hartmann 2008] [Cagnazzo and Manzini 2009] [Bell et al. 2009] TIO+ NAO+ [Sanchez-Gomez et al. 2009] also: [Hoerling et al. 2004] [Annamalai et al. 2007] [Bader and Latif 2005] EGU General Assembly 2010, Vienna, Austria.
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. EGU General Assembly 2010, Vienna, Austria.
- N = 100 - Independent ICs - Repeating Seas Cycle - JF response GFDL AM2.1 Experiments: TIP TIO TPO Amplitude 0.4 ~ 1.0 EGU General Assembly 2010, Vienna, Austria.
OLR and Chi200hPa Response TIP TIO TPO EGU General Assembly 2010, Vienna, Austria.
wavenumber-1 TIP TPO TIO wavenumber-2 TIP TPO TIO EGU General Assembly 2010, Vienna, Austria.
[∆Z] TIP TPO TIO EGU General Assembly 2010, Vienna, Austria.
NAM Pattern (+) [Thompson and Wallace 2000] NAM— NAM+ [∆Z] TIP TPO why? TIO EGU General Assembly 2010, Vienna, Austria.
Z*(60N) TPO TIO EGU General Assembly 2010, Vienna, Austria.
[∆Z] ~ [v*T*] Eddy Meridional Heat Flux Response (mK s-1) EGU General Assembly 2010, Vienna, Austria.
[v*T*] decomposition: TOTAL = EM + FL Eddy Meridional Heat Flux Response (mK s-1) EGU General Assembly 2010, Vienna, Austria.
[v*T*] decomposition: TOTAL = EM + FLEM = LIN + NONLIN Eddy Meridional Heat Flux Response (mK s-1) EGU General Assembly 2010, Vienna, Austria.
[v*T*] decomposition: TOTAL = EM + FLEM = LIN + NONLINLIN ~ wv_1 + wv_2 Eddy Meridional Heat Flux Response (mK s-1) EGU General Assembly 2010, Vienna, Austria.
What happens to the NAM response when we perturb the climatological stationary wave? EGU General Assembly 2010, Vienna, Austria.
Flatten the topography over: • Tibet and northern Eurasia (NOTIBET) • Rocky Mountains (NOROCK) difference NOTIBET case Standard Model 500 hPa Geopotential Heights EGU General Assembly 2010, Vienna, Austria.
NOTIBET cases NOROCK case [∆Z] TPO TPO TIO Eddy Meridional Heat Flux Response (mK s-1) EGU General Assembly 2010, Vienna, Austria.
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. EGU General Assembly 2010, Vienna, Austria.
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 EGU General Assembly 2010, Vienna, Austria.
Winter 2009/10 EGU General Assembly 2010, Vienna, Austria.
Pattern of Tropical SST trends [Shin and Sardeshmukh 2010] [Barsugli et al. 2006] EGU General Assembly 2010, Vienna, Austria.
∆Z*200hPa TIP TIO TPO EGU General Assembly 2010, Vienna, Austria.
Control (unforced) climatologies: STD and NOTIBET EGU General Assembly 2010, Vienna, Austria.
Control (unforced) climatologies: STD and NOTIBET EGU General Assembly 2010, Vienna, Austria.
wavenumber-1 TIP TPO TIO wavenumber-2 TIP TPO TIO EGU General Assembly 2010, Vienna, Austria.
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? EGU General Assembly 2010, Vienna, Austria.