资源环境科技发展态势分析平台

This work aims at detecting to what extent the El Nino Southern Oscillation (ENSO) modulation influences the upper warm temperature anomaly (UWTA) formation in Tanzania during March to May (MAM) season of 1980-2010. The UWTA has known to influence heavy rainfall events through enhanced vertical uplift and deepening surface low pressure. The study is thus critical towards improved early warning system through a better understanding of the mechanisms in the climate system responsible for the above average rainfall. The empirical orthogonal function analysis in this study, revealed the dominant interannual variability mode of the UWTA to be concentrated over the study region. The interannual variability of ENSO and the UWTA shows a moderate relationship during MAM (r = .5328) while a robust association (r = .7905) exists during the previous September to November (SON). Thus, the anomalous sea surface temperature anomaly (SSTA) of the central tropical Pacific (e.g., over Nino 3.4) leads 6 months before the UWTA of the study region and anomalous SSTA over the tropical Indian Ocean (TIO) peak up. Comparatively, the warm phase of ENSO during SON and December to February (DJF) is in phase relationship with the strengthened ascending branch of the Walker circulation over the warm TIO. Further analysis demonstrates that in SON the rising limb of the Walker circulation is the dominant source of uplift and convection enhancement over the warm TIO and later transports warm and moist air (i.e., diabatic heating) aloft for the UWTA formation during SON and DJF. Meanwhile, the Hadley circulation (HC) induced by the SSTA associated with ENSO exhibits the symmetric mode during SON and asymmetric mode in MAM. The asymmetric mode of the HC plays its role in transporting the warm and moist air from the warm TIO towards the study area for the UWTA formation during MAM.