0. The sequence on atmosphere-ocean interactions
1. Tropical Observations
Handouts
Annual cycle (Mitchell and Wallace, 1992)
2. The role of the tropics
On time scales less than decadal, the only effects of SST on the rest of the globe are from the tropics
Sterl and Hazeleger, 2005
Thermal forcing (organized by SST but not caused by SST) to rest of globe. Forcing effects determined by location and magnitude of forcing and transmission properties of atmosphere.
Divergence crucial to tropics and large
Trenberth et al, 2000
Tropical ocean participates in effects of tropics on rest of globe through oceanic heat transport and through ENSO.
3. Tropical Thermodynamics
Notes from Cane and Sarachik, 2006
4. Tropical Divergence
In midlatitudes: quasi-geostrophy gives: f:ζ:δ = 1:R0:R02
In the tropics, the divergence is of the same order as the vorticity.
In the tropics, divergence is thermally forced by the latent heat released in cumulonimbus:
wN2 Å Q
Reed and Recker, 1971
5. How clouds heat.
Yanai, Esbensen and Chu, 1973)
6. Convective Boundary Layers
Tennekes, 1973
7. The
maintenance of the vertical stratification---Radiative-Convective Equilibrium
Sarachik, 1978; 1985
8. A 2d Example of Thermal Forcing--The Hadley
Circulation
Schneider and Lindzen, 1978,
Schneider, 1978
9. Thermal Forcing by an isolated heat source
Matsuno (1966); Gill (1980
Lindzen (1967)
Wu et al. (1999,2000,2001)
Chiang et al (2001)
10. How SST determines the location of the thermal sources:
Lindzen and Nigam. 1987
Battisti et al., 1999
Neelin, 1989
11. Teleconecting to higher latitudes
Trenberth et al., 1998.
12. The Walker Circulation
Geisler,
1981
Notes from Cane and Sarachik, 2006
References:
Battisti, D. S., E. S. Sarachik, and A. C. Hirst, 1999: A Consistent Model for the Large-Scale Steady Surface Atmospheric Circulation in the Tropics. J. Climate, 12, 2956-2964.
Chiang, J. C. H., S. E. Zebiak, and M. A. Cane, 2001: Relative
roles of elevated heating and surface temperature gradients in driving anomalous
surface winds over tropical oceans. J Atmos. Sci., 58, 1371-1394.
Geisler,
J.E., 1981: A linear model of the Walker circulation. J. Atmos. Sci., 38, 1390-1400.
Gill, A. E., 1980: Some simple solutions for heat induced tropical circulation. Quart. J. Roy. Meteor. Soc., 106, 447–462
Lindzen, R. D, 1967: Planetary waves on beta-planes. Mon. Wea. Rev., 95, 441-451.
Lindzen, R.S., and S. Nigam, 1987: On the role of sea surface temperature gradients in forcing low-level winds and convergence in the tropics. J. Atmos. Sci., 44, 2418-2436.
Matsuno, T., 1966: Quasi-geostrophic motions in the equatorial area. J. Met. Soc. Japan, 44, 25-43.
Mitchell, T.P. and J.M. Wallace, 1992: The annual cyucle in equatorial convection and sea surface temperature. J. Clim., 5, 1140-1156.
Neelin, J.D., 1989: On the interpretation of the Gill model. J. Atmos. Sci.,46, 2466–2468.
Reed, R. J. and E..Recker. 1971: Structure
and Properties of Synoptic-Scale Wave Disturbances in the Equatorial Western
Pacific. J.Atmos. Sci., 28,
1117–1133.
Sarachik,
E. S., 1978: Tropical sea surface temperature: An interactive one-dimensional
atmosphere‑ocean model, Dyn. Atmos.& Oceans., 2, 455‑469.
Sarachik, E. S., 1985: A simple theory for the vertical structure of the tropical atmosphere. Pure Appl. Geophys., 123, 261–271.
Schneider, E.K., 1977: Axially symmetric steady-state models of the basic
state for instability and climate studies. Part II. Nonlinear calculations. J. Atmos. Sci., 34, 280-297.
Schneider, E.K., and R. S. Lindzen, 1977a: A discussion of the parameterization of momentum exchange by cumulus convection. J. Geophys. Res., 81, 3158-3160.
Schneider, E.K., and R. S. Lindzen, 1977b: Axially symmetric steady-state models of the basic state for instability and climate studies. I. Linearized calculations. J. Atmos. Sci., 34, 263-279.
Sterl, A. and W. Hazeleger, 2005: The relative roles of tropical and extratropical forcing on atmospheric variability. Geophys. Res. Lett., 32, doi: 10.1029/2005GL023757.
Tennekes. H., 1973: A model for the dynamics of the inversion above a convective boundary layer. J. Atmos. Sci., 30, 558–567.
Trenberth, K. E., G. W. Branstator, D. Karoly, A. Kumar, N.-C. Lau, and C. Ropelewski. 1998: Progress during TOGA in understanding and modeling global teleconnections associated with tropical sea surface temperatures. J. Geophys. Res., 103 (C7), 14,291–14,324.
Trenberth,
K.E., D.P. Stepaniak, and J.M. Caron, 2000: The global monsoon as seen through
the divergent atmospheric circulation. J. Climate, 13, 3969-3993.
Wu, Z., E.S. Sarachik, and D.S. Battisti, 1999: Thermally forced surface winds on an equatorial beta-plane. J. Atmos. Sci., 56, 2029-2037.
Wu,
Z., D.S. Battisti, and E.S. Sarachik 2000a: Rayleigh Friction, Newtonian
Cooling, and the Linear Response to Steady Tropical Heating. J. Atmos. Sci., 57,
1937-1957.
Wu, Z., E.S. Sarachik, and D.S. Battisti, 2000b: The vertical structure of convective heating and the three-dimensional structure of the forced circulation in the tropics. J. Atmos. Sci., 57, 2169-2187.
Wu, Z., E.S. Sarachik, and D.S.
Battisti, 2001: Thermally driven tropical circulations under Rayleigh friction
and Newtonian cooling: Analytic solutions. J. Atmos. Sci., 58, 724-741.
Yanai, M., S. Esbensen and J-H. Chu. 1973: Determination of bulk properties of tropical cloud clusters from large-scale heat and moisture budgets. J. Atmos. Sci., 30, 611–627.
Radius
of Earth 6370 km
Area
of Earth 0.51x1015 m2
Solar
Constant 1367 W/m2
Area
covered by Oceans 0.36x1015
m2
Heat
capacity of Water Cpw
= 1cal/gmK = 4.19 x103 J/kgK
Heat
Capacity of Dry Air
Cpa = 0.24 cal/gmK = 1.0x103 J/kgK
Density
of Air at surface 1.23 kg/m3
Density
of Water 1gm/cm3 = 103 kg/m3 = 1 tonne/m3
1
year has 3.15x107 sec (which can be remembered as ¹ x107
sec)
Latent
heat of water L = 2.5 x 106 J/kgK
Universal
Gas Constant R = 8.31x103 J/Kmol
Gravity
at Sea Level g=9.81m/s2
Stefan-Boltzman
Constant σ=5.67 x 10-8
J/m2K4s
Derived
Quantities:
The
mass of a water column of area 1m2 area and 10 m deep is 10 tonnes
The
mass of the total air column exerting 1020hPa at surface is about 10 tonnes
50
W/m2 into a column of area 1m2 of water 50 meters deep
heats the column 1K in 50 days (ÒThe 50-50-50 ruleÓ)
100
W/m2 into a unit column of water 100 m deep heats that column
0.6K/mo.
100
W/m2 into a unit column of air to the top of the atmosphere heats
the air column 0.8K/day
It
takes 29W/m2 to evaporate 1mm/day of water from the surface.
For
the mean temperature of surface of the earth, T=15¼C=288K, σT4
= 390 W/m2 For T=300K, σT4 = 459 W/m2