EGU23-3440, updated on 22 Feb 2023
https://doi.org/10.5194/egusphere-egu23-3440
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

New insight into multi-year La Niña dynamics from the perspective of a near-annual ocean process 

Fangyu Liu1, Wenjun Zhang1, Fei-Fei Jin2, Feng Jiang1, Julien Boucharel2,3, and Suqiong Hu1
Fangyu Liu et al.
  • 1Key Laboratory of Meteorological Disaster of Ministry of Education (KLME), Nanjing University of Information Science and Technology, Nanjing, China (fangyu.liu@nuist.edu.cn)
  • 2Department of Atmospheric Sciences, School of Ocean and Earth Science and Technology (SOEST), University of Hawai’i at Mānoa, Honolulu, HI, USA (jff@hawaii.edu)
  • 3University of Toulouse, LEGOS, IRD, 14 avenue Edouard Belin, 31400, Toulouse, France (julien.boucharel@ird.fr)

The El Niño-Southern Oscillation (ENSO) exhibits highly asymmetric temporal evolutions between its warm and cold phases. While El Niño events usually terminate rapidly after their mature phase and show an already established transition into the cold phase by the following summer, many La Niña events tend to persist throughout the second year and even re-intensify in the ensuing winter. While many mechanisms were proposed, no consensus has been reached yet and the essential physical processes responsible for the multi-year behavior of La Niña remain to be illustrated. Observations show that a unique ocean physical process operates during multi-year La Niña events. It is characterized by rapid double reversals of zonal ocean current anomalies in the equatorial Pacific which exhibits a fairly regular near-annual periodicity. Analyses of mixed-layer heat budget reveal comparable contributions of the thermocline and zonal advective feedbacks to the SST anomaly growth for the first year of multi-year La Niña events; however, the zonal advective feedback plays a dominant role in the re-intensification of La Niña events. Furthermore, the unique ocean process is identified to be closely associated with the preconditioning heat content state in the central to eastern equatorial Pacific before the first year of La Niña, which sets the stage for the future re-intensification of La Niña. The above-mentioned oceanic process can be largely reproduced by state-of-the-art climate models despite systematic underestimation, providing a potential predictability source for the multi-year La Niña events.

How to cite: Liu, F., Zhang, W., Jin, F.-F., Jiang, F., Boucharel, J., and Hu, S.: New insight into multi-year La Niña dynamics from the perspective of a near-annual ocean process , EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-3440, https://doi.org/10.5194/egusphere-egu23-3440, 2023.