84th AMS Annual Meeting

Tuesday, 13 January 2004: 11:45 AM
The Madden-Julian Oscillation in GCMs
Room 608
Kenneth R. Sperber, LLNL/PCMDI, Livermore, CA; and J. M. Slingo, P. M. Inness, S. Gualdi, W. Li, P. J. Gleckler, and C. Doutriaux
Using AVHRR OLR and model simulated OLR we analyze intraseasonal convection in the AMIP models and coupled ocean-atmosphere models to determine the extent to which the Madden-Julian Oscillation (MJO; Madden and Julian 1971, 1972) is simulated, and the influence that air-sea interaction has on the representation of the MJO. All data are bandpassed with a 20-100 day Lanczos filter.

Sperber (2003) identified seven years when the boreal winter MJO was notably active as a well-defined eastward propagating mode. Using these periods, the eastward propagation of convection was isolated via EOF analysis of filtered AVHRR OLR. For EOF-1 (EOF-2) enhanced convection covers 105oE-180oE, 20oN-20oS (60oE-140oE, 15oN-20oS). In the present study, filtered AVHRR OLR and the model OLR is projected onto the afore-mentioned EOF's. Thus, all models are evaluated relative to a common metric. The analysis is for the months November-March, for 1979/80-1994/95 for the observations and the AMIP II models, and for 9-19 winters from the coupled models. Confining the analysis to years during which eastward propagation of MJO convection occurs yields improved model results.

For the AVHRR OLR data, a one standard deviation perturbation of PC-1 and PC-2 gives rise to convective anomalies of about +/-25Wm-2. The vast majority of models have much weaker MJO convective signals. The maximum positive correlation, R, between PC-2 and PC-1, and the time lag at which it occurred indicates basic propagation characteristics of the MJO. For the AVHRR OLR, on average, PC-2 leads PC-1 by 12 days with a maximum positive correlation of 0.67. For all models, R is smaller than observed indicating that eastward propagation is not as coherent as observed. The characteristic timescale of propagation exhibits a wide-range of variability, with some models incorrectly exhibiting weak westward propagation. Comparing AMIP II and AMIP I we find that HADAM3 has a weaker MJO amplitude and less coherent eastward propagation compared to HADAM2. Importantly, air-sea interaction has a beneficial influence. Three of the coupled models have an AMIP II atmospheric component. In each case the coupled models have a larger R, indicating that the MJO convection has a more realistic propagating structure. That coupling to an ocean yields improvement to the representation of the MJO is consistent with Waliser et al. (1999), Inness and Slingo (2003) and Inness et al. (2003)

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