Presentation is loading. Please wait.

Presentation is loading. Please wait.

The Atmosphere: Part 3: Unsaturated convection Composition / Structure Radiative transfer Vertical and latitudinal heat transport Atmospheric circulation.

Similar presentations


Presentation on theme: "The Atmosphere: Part 3: Unsaturated convection Composition / Structure Radiative transfer Vertical and latitudinal heat transport Atmospheric circulation."— Presentation transcript:

1 The Atmosphere: Part 3: Unsaturated convection Composition / Structure Radiative transfer Vertical and latitudinal heat transport Atmospheric circulation Climate modeling Suggested further reading: Hartmann, Global Physical Climatology (Academic Press, 1994)

2 Full calculation of radiative equilibrium surface much too warm tropopause too cold stratosphere about right tropospheric lapse rate too large

3 Atmospheric energy balance

4 Hydrostatic balance

5 Pressure and density profiles in a compressible atmosphere hydrostatic balance perfect gas law Isothermal atmosphere More generally, H=H(z) and gas constant for dry air R = 287 J kg -1 K -1

6 Pressure and density profiles in a compressible atmosphere hydrostatic balance perfect gas law Isothermal atmosphere More generally, H=H(z) and (T=237K)

7 Convection I: Incompressible fluid, no condensation T and ρ are conserved under adiabatic displacement stable unstable

8 Thermodynamics of dry air C p = 1005 J kg -1 K -1

9 Thermodynamics of dry air C p = 1005 J kg -1 K -1 specific entropy

10 Thermodynamics of dry air C p = 1005 J kg -1 K -1 p 0 = 1000 hPa κ = R/c p = 2/7 (diatomic ideal gas) potential temperature (+ constant) specific entropy

11 Thermodynamics of dry air C p = 1005 J kg -1 K -1 p 0 = 1000 hPa κ = R/c p = 2/7 (diatomic ideal gas) potential temperature Adiabatic processes : θ is conserved under adiabatic displacement (N. B. θ=T at p =p 0 = 1000 hPa) (+ constant) specific entropy

12 Convection II: Compressible ideal gas, no condensation adiabatic displacement

13 Convection II: Compressible ideal gas, no condensation hydrostatic balance adiabatic displacement

14 Convection II: Compressible ideal gas, no condensation hydrostatic balance adiabatic displacement — adiabatic lapse rate Following displaced parcel

15 Convection II: Compressible ideal gas, no condensation hydrostatic balance adiabatic displacement — adiabatic lapse rate Following displaced parcel unstable stable

16 Convection II: Compressible ideal gas, no condensation hydrostatic balance adiabatic displacement — adiabatic lapse rate Following displaced parcel unstable stable

17 Stability of Radiative Equilibrium Profile Radiative equilibrium is unstable in the troposphere -10 K/km radiative equilibrium solution

18 Effects of convection Model aircraft observations in an unsaturated convective region (Renno & Williams)

19 Effects of convection radiative-convective equilibrium

20 Effects of convection radiative-convective equilibrium TROPOSPHERE STRATOSPHERE

21 Radiative-Convective Equilibrium Radiative equilibrium is unstable in the troposphere Re-calculate equilibrium subject to the constraint that tropospheric stability is rendered neutral by convection. -10 K/km radiative equilibrium solution

22 Radiative-convective equilibrium (unsaturated) Better, but: surface still too warm tropopause still too cold

23 Moist convection Above a thin boundary layer, most atmospheric convection involves phase change of water: condensation releases latent heat


Download ppt "The Atmosphere: Part 3: Unsaturated convection Composition / Structure Radiative transfer Vertical and latitudinal heat transport Atmospheric circulation."

Similar presentations


Ads by Google