DYNAMICAL RESPONSE OF THE OCEANIC CIRCULATION AND TEMPERATURE TO INTERDECADAL VARIABILITY IN THE SURFACE WINDS OVER THE INDIAN-OCEAN

Citation
Cjc. Reason et al., DYNAMICAL RESPONSE OF THE OCEANIC CIRCULATION AND TEMPERATURE TO INTERDECADAL VARIABILITY IN THE SURFACE WINDS OVER THE INDIAN-OCEAN, Journal of climate, 9(1), 1996, pp. 97-114
Citations number
30
Categorie Soggetti
Metereology & Atmospheric Sciences
Journal title
ISSN journal
08948755
Volume
9
Issue
1
Year of publication
1996
Pages
97 - 114
Database
ISI
SICI code
0894-8755(1996)9:1<97:DROTOC>2.0.ZU;2-P
Abstract
A global ocean general circulation model (OGCM) is used to investigate the sensitivity of the circulation and temperature fields to observed interdecadal variability in Indian Ocean winds for the austral summer (January, February, March). Focus is placed on the dynamical response of the model to the imposed winds. These comprise the observed winds from GOADS for the region 46 degrees S-30 degrees N, 17 degrees-152 de grees E organized into four 21-yr epochs ( 1900-1920, 1921-1941, 1942- 1962, and 1963-1983). During the first two epochs, the southern Indian anticyclone, African monsoonal flow, and associated trades were anoma lously weak, whereas during the 1963-1983 period the reverse was true. The 1942-1962 epoch appears to be a transition between the 1921-1941 and 1963-1983 periods. The model indicates an overall decrease (increa se) in the transports of the southern Indian and tropical Indian gyres for the 1900-1920, 1921-1941 (1963-1983) cases in dynamical response to the variability in the surface winds over the Indian Ocean. Sea sur face temperature(SST) perturbations in the southern Indian Ocean have the same sign as the observed anomalies but are smaller in magnitude ( 0.05 degrees-0.1 degrees C model, 0.1 degrees-0.3 degrees C observed). The model SST patterns are restricted to the southern Indian Ocean mi dlatitudes, occurring particularly in the region of the Agulhas retrof lection and outflow zones, whereas observations indicate anomalies thr oughout the Indian Ocean basin. Analysis of the streamfunction anomali es induced by the epoch winds in the model indicates that the JEBAR te rm is important in modulating the Indian gyre transports. While it is noted that thermodynamic effects not explicitly included in the model may contribute toward the observed SST variability in certain regions and that previous model studies have shown that SST in the southern In dian Ocean is sensitive to variations in the Indonesian throughflow an d the Pacific trade winds, the results lend support to the hypothesis that changes in the basin-scale ocean circulation driven by the Indian Ocean epoch winds may contribute significantly toward the observed in terdecadal variability in SST in the southern regions of this ocean.