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Low-frequency variability in the mid-latitude atmosphere induced by an oceanic thermal front: Application to the North Atlantic Ocean Yizhak Feliks 1,2 Michael Ghil 2,3 and Andrew W. Robertson 4 1 Mathematics Dept., Israel Institute of Biological Research, Ness Ziona, Israel. 2 Dept. of Atmospheric & Oceanic Sciences and Institute of Geophysics & Planetary Physics, UCLA, Los Angeles, CA, USA. 3 Geosciences Department and Laboratoire de Météorologie Dynamique (CNRS and IPSL), Ecole Normale Supérieure, Paris, France. 4 International Research Institute for Climate and Society, Columbia University, Palisades, NY, USA.
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Outline A model of atmospheric response to SST fronts ‣ Marine atmospheric boundary layer (MABL) + QG free atmosphere SST front specification ‣ Steady SST front 6 o C/100 km ‣ Adding interannual oscillations of 1 o C /100 km to the SST front Gulf Stream SST front ‣ spectral analyses of the SST field (SODA reanalysis, 1958–2007) in two regions along the Gulf Stream front, in which the interannual oscillations are prominent ‣ atmospheric model response to SODA monthly history
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Evolution of the barotropic mode in a domain 5000 km x 5000 km
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Three kinds of unstable oscillatory modes First, antisymmetric instabilities are baroclinic; they have a standing dipole structure. The dominant mode has a period of 270 days.
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Second, symmetric instabilities are barotropic; they develop at the eastern edge of the eastward jet. This mode was also obtained in an equivalent-barotropic model. The dominant mode has a period of 30 days, cf. Feliks et al. (JAS, 2004).
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Third, northward propagating instabilities can be decomposed into two standing parts, an antisymmetric and a symmetric part. The dominant mode has a period of 103 days. The spatio-temporal evolution of this mode resembles the observed 70-day mode of Plaut and Vautard (1994).
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Conclusion: The SST front spins up an eastward jet in the free atmosphere. Three kinds of unstable oscillatory modes are obtained: (1) antisymmetric due to baroclinic instability, with a period of 6–8 months. (2) Symmetric due to barotropic instability, with a period of 30 days. (3) Northward propagating, with an antisymmetric and a symmetric part, and a period of 2-3 months. These effects depend of the atmospheric model’s high resolution of 50 km x 50 km (not shown)! The role of interannual oscillations of the SST front in the atmospheric evolution was studied next.
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Evolutive spectral analysis 30-day oscillation 70-day oscillation
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The atmospheric response to the observed North Atlantic SST field
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10 km
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Next we examined the atmospheric effects of SST anomalies over and near the Gulf Stream with the general circulation model (GCM) of the Laboratoire de Météorologie Dynamique (LMD-Z) that has a zooming capability over the Gulf Stream. Francis Codron’s talk will summarize this study.
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Additional slides
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In the barotropic model, the instability is symmetric. A bifurcation point appears at ΔT=6 0 C: Δ t < 6 0 C, the eddies are weak and the dominant mode has a period of 30 days; Δ t > 6 0 C, the eddies are strong and the dominant mode has a period of 70 days.
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Schematic illustration of the FGS mechanism [FGS(a,b)] of SST front impacts. The sharp SST gradient forces a mesoscale cross-front circulation. The resulting vertical velocity at the top of the MABL induces vorticity anomalies in the free troposphere and a jet parallel to the surface isotherms. The vertical velocity at the top of the MABL has a thermal component, similar to that of Lindzen and Nigam (1987) in the tropics, and a mechanical one, which is substantial in mid-latitudes.
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