Preprints
https://doi.org/10.5194/egusphere-2025-2303
https://doi.org/10.5194/egusphere-2025-2303
10 Jun 2025
 | 10 Jun 2025

The multi-year negative Indian Ocean Dipole of 2021–2022

Ankur Srivastava, Gill M. Martin, Maheswar Pradhan, Suryachandra A. Rao, and Sarah Ineson

Abstract. The years 2021 and 2022 witnessed negative Indian Ocean Dipole (nIOD) conditions, with the 2022 event being the strongest on record. The dipole mode index was negative since the summer of 2021 and remained negative until early winter 2022, an unprecedented duration of 19 months. This makes it the first such occurrence of a multi-year nIOD. It co-existed with a triple-dip La Niña event during 2020–2022. In this study, we explore the dynamics behind the occurrence of this multi-year nIOD event. The tropical Indian Ocean (TIO) witnessed predominant westerly wind anomalies starting in the summer of 2021 and lasting till the end of 2022, with a record number and duration of westerly wind bursts (WWBs). The anomalous westerlies were supported by the background La Niña state and anomalous convection over the eastern TIO associated with tropical intra-seasonal oscillations. Occurrences of WWBs outside their preferred climatological months and strong westerly wind anomalies modulated the intensity of the zonal currents and the Wyrtki jets in the TIO. The associated heat and mass transfer caused the depression of the thermocline in the eastern TIO, resulting in the sustenance of nIOD conditions. Anomalous westerly wind activity in the TIO during the spring of 2022 served as a bridge between the two nIOD events and sustained it for a record duration. This multi-year nIOD event thus prevented the Indian summer monsoon rainfall from being in large excess, as the monsoon conducive modulation of the Walker circulation was counteracted by the anomalous subsidence over India by the nIOD-modulated regional Hadley circulation.

Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.
Share
Ankur Srivastava, Gill M. Martin, Maheswar Pradhan, Suryachandra A. Rao, and Sarah Ineson

Status: final response (author comments only)

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2025-2303', Anonymous Referee #1, 10 Jul 2025
    • AC1: 'Reply on RC1', Ankur Srivastava, 27 Jul 2025
  • RC2: 'Comment on egusphere-2025-2303', Anonymous Referee #2, 05 Aug 2025
    • AC2: 'Reply on RC2', Ankur Srivastava, 09 Aug 2025
Ankur Srivastava, Gill M. Martin, Maheswar Pradhan, Suryachandra A. Rao, and Sarah Ineson
Ankur Srivastava, Gill M. Martin, Maheswar Pradhan, Suryachandra A. Rao, and Sarah Ineson

Viewed

Total article views: 520 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
392 112 16 520 34 54
  • HTML: 392
  • PDF: 112
  • XML: 16
  • Total: 520
  • BibTeX: 34
  • EndNote: 54
Views and downloads (calculated since 10 Jun 2025)
Cumulative views and downloads (calculated since 10 Jun 2025)

Viewed (geographical distribution)

Total article views: 513 (including HTML, PDF, and XML) Thereof 513 with geography defined and 0 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 
Latest update: 06 Sep 2025
Download
Short summary
This study documents the dynamics behind the first occurrence of a multi-year negative Indian Ocean Dipole (nIOD) event during 2021–2022, which lasted for an unprecedented 19 months! The event was sustained by the triple-dip La Niña event of 2020–2022. The conducive background state led to anomalous westerly wind activity and a record number and duration of westerly-wind bursts in the equatorial Indian Ocean. The resulting modulation of Wyrtki jets aided the sustenance of the nIOD event.
Share