EGU21-3222
https://doi.org/10.5194/egusphere-egu21-3222
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Simulated disruptions of the Quasi-Biennial Oscillation

Kevin DallaSanta and Clara Orbe
Kevin DallaSanta and Clara Orbe
  • NASA Goddard Institute for Space Studies, New York, United States of America (kevin.dallasanta@nasa.gov)

The Quasi-Biennial Oscillation has exhibited remarkable stability over the observational record—until a well-documented 2015/16 disruption and an emerging disruption in 2020/21. The possibility that disruptions are more frequent in a changing climate is important to consider, as the QBO affects predictability, stratospheric composition, and surface weather. However, this possibility is challenging to assess for a variety of reasons. For instance, the 2015/16 disruption has been attributed to anomalous easterly momentum flux from extratropical waves. By comparison, the 2020/21 disruption involves anomalous westerly forcing, less likely to originate from the same mechanism.

We present a rich variety of QBO disruptions that spontaneously arise in integrations of the high-top NASA GISS Model E2.2. The disruptions loosely fall into several categories, some of which are analogous to the 2015/16 disruption and the 2020 disruption, as well as a previously undocumented possible disruption in 1988. Several factors appear to influence QBO disruptions in the model: natural variability, climate change, tropical SSTs, volcanic eruptions, and model physics/tuning. Although QBO representation is an ongoing challenge for models, the results point to a model-independent framework for assessment of disruptions.

 

How to cite: DallaSanta, K. and Orbe, C.: Simulated disruptions of the Quasi-Biennial Oscillation, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-3222, https://doi.org/10.5194/egusphere-egu21-3222, 2021.

Corresponding displays formerly uploaded have been withdrawn.