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The unpredictable nature of the atmospheric jet stream Frank Selten, KNMI Satellite view of the general circulation water vapour channel • what sets the atmosphere into motion? • what causes the strong westerly jets? Differential heating Net cooling in high latitudes Net warming in tropics Poleward heat transports 5 PW = 300 x world energy consumption Available potential energy due to differential heating sets the atmosphere in motion unstable L Cold air H Warm air pressure higher in warm air region: air starts flowing towards lower pressure gravity force height stable pressure H L extra-tropics tropics no pressure gradient Hydrostatic balance: the pressure is approximately equal to the weight of the air column above: warm air is lighter, pressure drops less quickly with height Hadley cells Hadley Cells Ferrel Cell Ferrel Cell Between equator and 30 degrees: direct mean poleward transport by the thermally driven Hadley circulation In the poleward moving air, westerlies develop: conservation of angular momentum, an apparent force in the rotating earth frame deflects particles to the right 13 Geostrophic balance • In the extra-tropics on synoptic spatial and temporal scales the flow is approximately in a geostrophic balance (Law of Buys Ballot): the coriolis force balances the pressure gradient force. Low Fp = -dP/dy U f = 2Ωsinφ is coriolis parameter Ω= angular velocity of the earth High Fcor = -f U Valid for small Rossby number: Klimaatcursus Velocity U and spatial scale L of synoptic motions set a time scale on the order of days, long enough to feel the rotation of the earth In the upper branch of the Hadley circulations strong westerlies develop zonal mean zonal circulation General circulation observed zonal mean meridional circulation Thermal wind balance Combines the hydrostatic balance with the geostrophic balance: A horizontal temperature gradient leads to an increase of the geostrophic wind with height that is a vertical wind shear. Cold air Warm air L H pressure becomes higher in warm air region: a geostrophic flow develops proportional to the pressure gradient dp/dy = f U dp/dy increases with height so does zonal wind U no pressure gradient y Klimaatcursus Strong horizontal temperature gradients • what drives the jetstream: radiation imbalance at the top of the atmosphere: net heating of tropics, net cooling of poles: creates temperature gradient, pressure gradient, flow: westerlies due to rotation of the earth: == subtropical jet: two approximate balances: geostrophic and hydrostatic balance • jetstream unstable: baroclinic instability: available potential energy is converted into kinetic energy of storms by lowering the center of mass of the atmosphere: warm air rises, cold air sinks in extratropical storms: storms reduce the temperature gradient which gets restored by the radiation imbalance Baroclinic instability Instabilities develop if horizontal temperature gradients/ vertical wind shears become too large Baroclinic instability • Small disturbances grow through conversion of available potential energy of the background flow into kinetic energy • Hydrostatic en geostrophic balance lead to a typical spatial scale of disturbances that become unstable first as temperature gradients cross a critical value A baroclinically growing wave warm air is advected underneath the upper air ridge: growth ! warm air rises Westward tilt with height cold cold air sinks L warm cold air is advected underneath the upper air trough: growth ! Baroclinic wave observed At 500 hPa At surface Role of the ‘eddies’ in climate • Transport heat poleward • Transport water vapor • Transport westward momentum into the jet region: vortex stripping through wave breaking: eddy driven jet • Mix air masses • strong scale interactions: jet steers the storms, storms feedback on the jet: zonal - blocked flow transitions: implications for local weather: stripping effect of breaking waves; mixing of momentum to the surface: waves can form jets: eddy-driven jets Position of subtropical and eddydriven jets • strong subtropical jet - weaker southward displaced eddy-driven jet • North Atlantic Oscillation (NAO): multi-scale interactions, split-single jet transitions, large impact on European climate Rotation of the earth: Rossby wave motions Rossby waves: conservation of absolute vorticity d ⎛⎜ζ + f ⎞⎟ = 0 ⎟ dt ⎜⎝ ⎠ ζ : relative vorticity f = 2Ωsinφ : planetary vorticity Rossby waves move westward in the planetary vorticity field with respect to the flow The phase speed depends on the wavelength: long waves move faster Dispersive character: c=U − β2 k β =δ f δy for a wave of the form: ζ = Acos(k(x−ct)) L = > 30 days Standing waves M= <30 days > 6 days Retrogressing waves H= < 6 days Baroclinic waves Rennert and Wallace, 2009 A toy model of the extra-tropical atmosphere E.N. Lorenz, 1984: “Irregularity, a fundamental property of the atmosphere”,Tellus, 36A, 98-110 X The Lorenz 84 system dX = −Y 2 − Z 2 −aX +aF dt dY = XY −bXZ −Y +G dt Y • • • • • Z dZ =bXY + XZ − Z dt Interaction of a wave (Y,Z) with a zonal flow (X) Solutions depend on parameters F, G, a and b Solutions are found by numerical integrations Solutions in the 3D phase space: trajectories Solutions in real space: traveling wave on a zonal flow ζ (x,t)= X(t)×ζ zonal (x)+Y (t)×sin(kx)+ Z(t)×cos(kx) Strange attractor X Z Y • Sensitive dependence on initial conditions • Evolution never exactly repeated Solutions in phase space X y z • unstable periodic orbits: quasi-periodic behaviour of waves in the jetstream • origin of Rossby wave energy: tropical convection with upper level divergence, mountain ranges, baroclinic instability, barotropic instability • traveling and standing waves lead to teleconnections: correlations between wind/ pressure fluctuations over large distances: example tropical forcing experiment • weather regimes: multiple equilibria, interaction with mountain ranges, stationary waves, resonant interaction: in low-order models: chaotic transitions between zonal and block flows along preferred paths, continuous temporal spectrum, limited predictability due to sensitive dependence on initial conditions Crommelin, 2003 “zonal” stable Zon al flo w unstable = forcing “blocked” stable Dynamisch seminarium Homoclinic and heteroclinic orbits PDF in chaotic regime Conclusion: UPO’s as remnants of heteroclinic connections guide transitions between regimes on the chaotic attractor Ingredients: orographic and barotropic instability • jet stream influenced by: a interaction with diabatic heating processes (condensation, radiation), b interaction with earth surface (land/ocean/sea-ice), c turbulent heat and momentum transports • predictability from lower boundary (soil moisture, sea surface temperatures, sea-ice cover) on the seasonal time-scales • climate change due to CO2 increase: jets will respond to change in radiative forcing: need to compute feedbacks from a-b-c: high-resolution coupled atmosphere-oceanland sea-ice models with radiative transfer, moisture and clouds, aerosols • examples: pole ward shift due to shift in baroclinic zones, high pressure over British Isles due to cooling sub polar surface waters in summer, shift in stationary waves due to change in tropical convection, hints of change in regime frequencies • detection of change difficult due to existence of large internal fluctuations “Warming Hole” MSLP SAT Reduced upward heat flux Z500 Sens. + latent heat flux