EGU2020-8339
https://doi.org/10.5194/egusphere-egu2020-8339
EGU General Assembly 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

The downward propagation of split- and displacement-type SSWs in an idealised model

Ian White1, Chaim Garfinkel1, Edwin Gerber2, and Martin Jucker3
Ian White et al.
  • 1Institute of Earth Sciences, Hebrew University of Jerusalem, Jerusalem, Israel (ian.white@mail.huji.ac.il)
  • 2Courant Institute of Mathematical Sciences, New York University, New York, USA (gerber@cims.nyu.edu)
  • 3Climate Change Research Centre, University of New South Wales, Sydney, Australia (martin.jucker@unsw.edu.au)

Sudden stratospheric warmings (SSWs) have a significant downward influence on the tropospheric circulation below, although the mechanisms governing this downward impact are not well understood. It is also not known if the type of SSW event – be them splits or displacements – play a role in determining the magnitude of the tropospheric response. We here examine the impacts of split- and displacement-type SSWs on the troposphere.

To do this, we use the recently developed model of an idealised moist atmosphere to impose zonally-asymmetric warming perturbations to the extratropical stratosphere, extending the work of a recent study by the authors in which a zonally-symmetric heating perturbation was imposed. This model of ‘intermediate complexity’ is particularly suited to this study as it incorporates the radiation scheme that is utilised by operational forecast systems, including both the ECMWF and NCEP. The radiation scheme also allows us to force the model with a realistic ozone profile, and thus to simulate realistic radiative timescales in the stratosphere. From a control run with a realistic climatology, we perform an ensemble of spin-off runs every January 1st with imposed high-latitude stratospheric heating perturbations of varying degrees of magnitude. The heating perturbation is switched on for a limited period of time to mimic the sudden nature of a SSW event and the troposphere is allowed to evolve freely. We compare the evolution of the tropospheric response to the forced split and displacement-type SSWs with free-running SSWs of the same type in the control run.

By modifying only the temperature tendency equation as opposed to the momentum budget, our experiments allow us to isolate the tropospheric response associated with changes in the polar-vortex strength (e.g., a direct or indirect modulation of planetary waves and synoptic waves), rather than due to any planetary-wave momentum torques that initially drive the SSW. Nevertheless, the imposition of wave-1 and wave-2 heating perturbations provide a more realistic post-onset SSW state than that which occurs in response to zonal-mean heating perturbations as performed in our previous study.

How to cite: White, I., Garfinkel, C., Gerber, E., and Jucker, M.: The downward propagation of split- and displacement-type SSWs in an idealised model , EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-8339, https://doi.org/10.5194/egusphere-egu2020-8339, 2020

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