eISSN 1942-2466
Vol. 2, 2010
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J. Adv. Model. Earth Syst., Vol. 2, Art. #5, 24 pp.

Published Online 7 Apr. '10

Intraseasonal Variability in an Aquaplanet General Circulation Model

Eric D Maloney, Adam H Sobel, Walter M Hannah

Abstract


An aquaplanet atmospheric general circulation model simulation with a robust intraseasonal oscillation is analyzed. The SST boundary condition resembles the observed December-April average with continents omitted, although with the meridional SST gradient reduced to be one-quarter of that observed poleward of 10 ̊ latitude. Slow, regular eastward propagation at 5 m s21 in winds and precipitation with amplitude greater than that in the observed MJO is clearly identified in unfiltered fields. Local precipitation rate is a strongly non-linear and increasing function of column precipitable water, as in observations. The model intraseasonal oscillation resembles a moisture mode that is destabilized by wind-evaporation feedback, and that propagates eastward through advection of anomalous humidity by the sum of perturbation winds and mean westerly flow.

A series of sensitivity experiments are conducted to test hypothesized mechanisms. A mechanism denial experiment in which intraseasonal latent heat flux variability is removed largely eliminates intraseasonal wind and precipitation variability. Reducing the lower-troposphere westerly flow in the warm pool by reducing the zonal SST gradient slows eastward propagation, supporting the importance of horizontal advection by the low-level wind to eastward propagation. A zonally symmetric SST basic state produces weak and unrealistic intraseasonal variability between 30 and 90 day timescales, indicating the importance of mean low-level westerly winds and hence a realistic phase relationship between precipitation and surface flux anomalies for producing realistic tropical intraseasonal variability.


 Article Spotlight
Time-longitude diagrams of 0oS-20oS averaged unfiltered precipitation and 850 hPa zonal winds in the Quarter Meridional Gradient (QM) simulation indicate a very regular oscillation that propagates eastward at approximately 5 m s-1 in the Eastern Hemisphere (Figure 5).
Cite this article in JAMES:
Maloney, E. D., A. H. Sobel and W. M. Hannah, 2010: Intraseasonal Variability in an Aquaplanet General Circulation Model. J. Adv. Model. Earth Syst., Vol. 2, Art. #5, 24 pp., doi:10.3894/JAMES.2010.2.5
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