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Title: | Super El Niño Years Potentially Diversify the Indian Summer Monsoon Circulation and Rainfall Patterns |
Authors: | Mahendra, Nimmakanti Chilukoti, Nagaraju Chowdary, Jasti S Attada, Raju |
Keywords: | Super El Niño monsoon circulation rainfall patterns Indian summer |
Issue Date: | Mar-2023 |
Citation: | Annual Monsoon Workshop (AMW-2022) and National Symposium on Challenges in climate services for health sector in the warming environment, IITM, Pashan, Pune, 28-30 March 2023 |
Abstract: | In general, the Indian Summer Monsoon (ISM) rainfall over India is deficit (excess) during El Niño (La Niña) years, although this is not true for all the El Niño years. In this work, we noted that the spatial rainfall patterns over the Indian region exhibited large diversity among the super El Niño events such as 1982, 1997, and 2015. Differences in magnitudes of Positive Indian Ocean Dipole (IOD) and changes in Sea surface temperature (SST) anomaly patterns over the Indo-Western Pacific (IWP) are noteworthy features of these events. Mainly strong southeast-northwest tilted cold SST anomalies were noticeable from the southwest Pacific to the southeast Indian Ocean (SEIO) through the Indonesian islands during 1982 and 1997 than that of 2015. These anomalies were caused by the interaction of cyclonic circulation over the South Pacific Convergence Zone(SPCZ) with anticyclonic circulation south of Australia. However, it is feeble in 2015, which was led by the occurrence of an asymmetric equatorial circulation over the IWP. Furthermore, we observed the equatorial Indian Ocean zonal winds are modulated by southern annular mode (SAM) forcing, which plays a substantial role in altering the strength of the IOD. It emphasizes that SAM has an influence on ISM rainfall along with super El Niño induced SST anomalies coupled with circulation over the IWP. Though upper-level convergence over the ISM region is somewhat similar among these super El Niño events, more frequent and organized northward propagating convective activity over Central India was observed in 1982 and 1997 than in 2015. High-frequency intraseasonal variability with rainfall peaks is evident due to the northward propagation of convective activity. The influence of WNP convection on active and break signals of the ISM is evident in Quasi-biweekly (10–20-day) oscillations, even in deficit monsoon years associated with El Niño. Even though the super El Niño may occur in the future, the background conditions over the IWP along with Southern Hemisphere synoptic (such as SAM) events influence the rainfall changes over India. |
Description: | Copyright belongs to proceeding publisher |
URI: | http://hdl.handle.net/2080/4003 |
Appears in Collections: | Conference Papers |
Files in This Item:
File | Description | Size | Format | |
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2023_IMSP-AMW_NMahendra_Super.pdf | Poster | 4.45 MB | Adobe PDF | View/Open |
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