Kurzfassungen der Meteorologentagung DACH
DACH2022-7, 2022
https://doi.org/10.5194/dach2022-7
DACH2022
© Author(s) 2022. This work is distributed under
the Creative Commons Attribution 4.0 License.

A deeper insight into the dynamics and effects of the Hiccup of the fall transition

Vivien Matthias, Daniela Banys, and Marc Hansen
Vivien Matthias et al.
  • DLR Institute for Solar-Terrestrial Physics, Solar-Terrestrial Coupling Processes, Neustrelitz, Germany (vivien.matthias@dlr.de)

In autumn the prevailing wind in the middle atmosphere at mid and high latitudes changes from summer easterly to winter westerly.  This process is not smooth but interrupted by the Hiccup of the fall transition with characteristics similar to a mini sudden stratospheric warming (SSW) which occurs in fall even though the zonal mean zonal wind does not reverse to easterly again. Combining global reanalysis data and satellite observations we improve our knowledge and understanding of the dynamics of the Hiccup of the fall transition in the middle atmosphere. The introduction of a new definition for the onset of the Hiccup focusing now on its core region in the lower mesosphere allows us the automatic detection of a Hiccup in almost every year and thus a deeper insight into its dynamics. For example, we found a latitudinal and altitudinal shift in the zonal wind regime during the Hiccup. We also investigate its 3D-structure and compare the characteristics of the Hiccup in the Northern hemisphere with those in the Southern hemisphere. We found that the latitudinal and altitudinal shift of the zonal wind regime occurs in both hemispheres but is more pronounced in the Northern hemisphere and smoother in the Southern hemisphere.  Additionally, we discuss the possible impact of the Hiccup on the D-region.

How to cite: Matthias, V., Banys, D., and Hansen, M.: A deeper insight into the dynamics and effects of the Hiccup of the fall transition, DACH2022, Leipzig, Deutschland, 21–25 Mar 2022, DACH2022-7, https://doi.org/10.5194/dach2022-7, 2022.