Skip to main content

Advertisement

Log in

The effect of ocean mixed layer depth on climate in slab ocean aquaplanet experiments

  • Published:
Climate Dynamics Aims and scope Submit manuscript

Abstract

The effect of ocean mixed layer depth on climate is explored in a suite of slab ocean aquaplanet simulations with different mixed layer depths ranging from a globally uniform value of 50–2.4 m. In addition to the expected increase in the amplitude of the seasonal cycle in temperature with decreasing ocean mixed layer depth, the simulated climates differ in several less intuitive ways including fundamental changes in the annual mean climate. The phase of seasonal cycle in temperature differs non-monotonically with increasing ocean mixed layer depth, reaching a maximum in the 12 m slab depth simulation. This result is a consequence of the change in the source of the seasonal heating of the atmosphere across the suite of simulations. In the shallow ocean runs, the seasonal heating of the atmosphere is dominated by the surface energy fluxes whereas the seasonal heating is dominated by direct shortwave absorption within the atmospheric column in the deep ocean runs. The surface fluxes are increasingly lagged with respect to the insolation as the ocean deepens which accounts for the increase in phase lag from the shallow to mid-depth runs. The direct shortwave absorption is in phase with insolation, and thus the total heating comes back in phase with the insolation as the ocean deepens more and the direct shortwave absorption dominates the seasonal heating of the atmosphere. The intertropical convergence zone follows the seasonally varying insolation and maximum sea surface temperatures into the summer hemisphere in the shallow ocean runs whereas it stays fairly close to the equator in the deep ocean runs. As a consequence, the tropical precipitation and region of high planetary albedo is spread more broadly across the low latitudes in the shallow runs, resulting in an apparent expansion of the tropics relative to the deep ocean runs. As a result, the global and annual mean planetary albedo is substantially (20 %) higher in the shallow ocean simulations which results in a colder (7C) global and annual mean surface temperature. The increased tropical planetary albedo in the shallow ocean simulations also results in a decreased equator-to-pole gradient in absorbed shortwave radiation and drives a severely reduced (≈50 %) meridional energy transport relative to the deep ocean runs. As a result, the atmospheric eddies are weakened and shifted poleward (away from the high albedo tropics) and the eddy driven jet is also reduced and shifted poleward by 15° relative to the deep ocean run.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Fig. 1
Fig. 2
Fig. 3
Fig. 4
Fig. 5
Fig. 6
Fig. 7
Fig. 8

Similar content being viewed by others

Notes

  1. We note that the seasonal cycle of temperature in the deep runs is delayed aloft in the vicinity of 40°. This phase lag is a consequence of reduced eddy energy flux divergence during the warm season that is driven by extratropical atmospheric heating which leads to a reduced meridional temperature gradient aloft during the late summer. This acts as a phase delayed source of heating in the subtropical troposphere which is driven non-locally

  2. We note that, the seasonal amplitude of extratropical shortwave radiation absorbed at the surface is in phase with the insolation but has 57 % of the seasonal amplitude of the insolation (125 W m−2 as compared to 220 W m−2) which represents the shortwave opacity of the atmosphere times the surface co-albedo (0.92). Thus, in the limit of zero surface heat capacity we would expect that approximately 57 % of the seasonal insolation to enter the atmospheric column via SHF as compared to the 20 % of insolation absorbed directly in the atmospheric column (SWABS). In this case, there is an approximatley 3:1 heating ratio of SHF:SWABS, similar to the observed annual mean ratio (Donohoe and Battisti 2013).

  3. The stationary eddies make a negligible contribution to the total energy transport. The stationary eddy energy transport is included in the eddy energy transport term for completeness.

  4. The equatorward MOC energy transport in the deep tropics of the 50 m run is a consequence of the moist static energy decreasing with height in the boundary layer due to a very moist and warm boundary layer. This results in the Hadley cell transporting energy in the same direction as the meridional flow at the surface.

References

  • Andrews D, McIntyre M (1976) Planetary waves in horizontal and vertical shear: the generalized eliassen-palm relation and the zonal mean acceleration. J Atmos Sci 33:2031–2048

    Article  Google Scholar 

  • Chiang J, Friedman A (2012) Extratropical cooling, interhemispheric thermal gradients, and tropical climate change. Annu Rev Earth Planet Sci 40:383–412

    Article  Google Scholar 

  • Chou M, Lee K (1996) Parameterizations for the absorption of solar radiation by water vapor and ozone. J Atmos Sci 53:1203–1208

    Article  Google Scholar 

  • Czaja A, Marshall J (2006) The partitioning of poleward heat transport between the atmosphere and the ocean. J Atmos Sci 63:1498–1511

    Article  Google Scholar 

  • Danabasoglu G, Gent P (2009) Equilibrium climate sensitivity: is it accurate to use a slab ocean model? J Clim 22:2494–2499

    Article  Google Scholar 

  • Delworth TL, Broccoli AJ, Rosati A, Stouffer RJ, Balaji V, Beesley JA, Cooke WF (2006) Gfdl’s cm2 global coupled climate models. part I: formulation and simulation characteristics. J Clim 19:643–674

    Article  Google Scholar 

  • Donohoe A (2011) Radiative and dynamic controls of global scale energy fluxes. Ph.D. thesis, University of Washington, p 137

  • Donohoe A, Battisti D (2012) What determines meridional heat transport in climate models? J Clim 25:3832–3850

    Article  Google Scholar 

  • Donohoe A, Battisti D (2013) The seasonal cycle of atmospheric heating and temperature

  • Donohoe A, Marshall J, Ferreira D, McGee D (2013) The relationship between ITCZ location and atmospheric heat transport across the equator: from the seasonal cycle to the last glacial maximum. J Clim 26(11):3597–3618

    Article  Google Scholar 

  • Edmon HJ, Hoskins B, McIntyre M (1980) Eliassen-palm cross sections for the troposphere. J Atmos Sci 37:2600–2616

    Article  Google Scholar 

  • Eliassen A, Palm E (1961) On the transfer of energy in staionary mountain waves. Geofys Publ 22(5):1–23

    Google Scholar 

  • Enderton D, Marshall J (2009) Controls on the total dynamical heat transport of the atmosphere and oceans. J Atmos Sci 66:1593–1611

    Article  Google Scholar 

  • Fasullo JT, Trenberth KE (2008a) The annual cycle of the energy budget: part 1. Global mean and land-ocean exchanges. J Clim 21:2297–2312

    Article  Google Scholar 

  • Fasullo JT, Trenberth KE (2008b) The annual cycle of the energy budget: part 2. Meridional structures and poleward transports. J Clim 21:2313–2325

    Article  Google Scholar 

  • Frierson D, Hwang Y, Fuckar N, Seager R, Kang S, Donohoe A, Maroon E, Liu X, Battisti D (2013) Why does tropical rainfall peak in the northern hemisphere? The role of the oceans meridional overturning circulation. Nature (submitted)

  • Johanson C, Fu Q (2009) Hadley cell widening: model simulations versus observations. J Clim 22:2713–2725

    Article  Google Scholar 

  • Kang S, Held I, Frierson D, Zhao M (2008) The response of the ITCZ to extratropical thermal forcing: idealized slab-ocean experiments with a GCM. J Clim 21:3521–3532

    Article  Google Scholar 

  • Lin SJ (2004) A “vertically lagrangian” finite-volume dynamical core for global models. Mon Weather Rev 132:2293–2307

    Article  Google Scholar 

  • Lindzen R, Hou A (1988) Hadley circulations of zonally averaged heating centered off the equator. J Atmos Sci 45:2416–2427

    Article  Google Scholar 

  • North GR (1975) Theory of energy-balance climate models. J Atmos Sci 32:2033–2043

    Article  Google Scholar 

  • Rose B, Ferreira D (2013) Ocean heat transport and water vapor greenhouse in a warm equable climate: a new look at the low gradient paradox. J Clim (in press)

  • Schneider EK (1996) A note on the annual cycle of sea surface temperature at the equator. Technical Report. Center for Ocean-Land-Atmosphere Studies, 18 p

  • Stone P (1978) Constraints on dynamical transports of energy on a spherical planet. Dyn Atmos Oceans 2:123–139

    Article  Google Scholar 

  • Stone P, Salustri G (1984) Generalization of the quasi-geostrophic eliassen-palm flux to include eddy forcing of condensational heating. J Atmos Sci 41:3527–3535

    Article  Google Scholar 

  • Trenberth KE, Caron JM (2001) Estimates of meridional atmosphere and ocean heat transports. J Clim 14:3433–3443

    Article  Google Scholar 

  • Vallis GK (2006) Atmospheric and oceanic fluid dynamics. Cambridge University Press, Cambridge

    Book  Google Scholar 

  • Wielicki B, Barkstrom B, Harrison E, Lee R, Smith G, Cooper J (1996) Clouds and the earth’s radiant energy system (CERES): An earth observing system experiment. Bull Am Meteorol Soc 77:853–868

    Article  Google Scholar 

Download references

Acknowledgments

AD was funded by the NOAA Global Change Postdoctoral Fellowship.

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to Aaron Donohoe.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Donohoe, A., Frierson, D.M.W. & Battisti, D.S. The effect of ocean mixed layer depth on climate in slab ocean aquaplanet experiments. Clim Dyn 43, 1041–1055 (2014). https://doi.org/10.1007/s00382-013-1843-4

Download citation

  • Received:

  • Accepted:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/s00382-013-1843-4

Keywords

Navigation