EGU25-1871, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-1871
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Wednesday, 30 Apr, 10:45–12:30 (CEST), Display time Wednesday, 30 Apr, 08:30–12:30
 
Hall X5, X5.117
On the Slow Decay of El Niño in CMIP6 Models
Yihua wei
Yihua wei
  • Nanjing University of Information Science and Technology, China (evawei0324@gmail.com)

The decay pace of El Niño can significantly modify its impacts on the Asian climate during the post-El Niño summer. Hence, accurately reproducing the observed decay pace in state-of-art coupled models is essential for realistic climate simulations. In the CMIP6 models, El Niño decays slower than observed. This slower decay can be attributed to weaker-than-observed air-sea coupling in the models that causes a weaker atmospheric convective response and smaller westerly anomalies along the equatorial Pacific during the El Niño life cycle. The smaller westerly anomalies result in a slower discharge of equatorial ocean heat, weaker negative/positive thermocline anomalies along/off the equator and thus a weaker meridional gradient of the thermocline anomalies. This weakens the easterly current anomalies, diminishes the zonal advection feedback, and ultimately slows the decay pace of El Niño in the models.

How to cite: wei, Y.: On the Slow Decay of El Niño in CMIP6 Models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1871, https://doi.org/10.5194/egusphere-egu25-1871, 2025.