EGU24-9151, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-9151
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Lagrangian analysis of ice supersaturated air masses in connection with low level fronts of extratropical cyclones

Philipp Reutter1, Stefan Niebler2, Annette Miltenberger1, and Peter Spichtinger1
Philipp Reutter et al.
  • 1Johannes Gutenberg University, Institute for Atmospheric Physics, Mainz, Germany (preutter@uni-mainz.de)
  • 2Johannes Gutenberg University, Institute of Computer Science, Mainz, Germany

Ice supersaturation is often found in the upper troposphere. The so-called ice supersaturated regions (ISSRs), i.e. air masses in the status of supersaturation with respect to ice, are formation regions of in-situ cirrus clouds. While an ISSR alone has a rather small effect on the radiation budget, this changes significantly when cirrus clouds develop within the ISSR. Hence, the transition from an ISSR to a cirrus cloud has important implications. In order to understand how ISSR and the embedded in-situ cirrus clouds form and develop, the transport pathways of water vapour have to be understood.

Therefore, to better understand the life cycle of extratropical ice-supersaturated regions (ISSRs), we utilize backward and forward trajectories initiated within ISSRs and analyze them. Furthermore, we connect these trajectories with information about the location of low-level frontal systems to investigate connections between ISSRs and extratropical cyclones. Particularly interesting is the relative position to the so-called warm conveyor belt (WCB) trajectories.

 

How to cite: Reutter, P., Niebler, S., Miltenberger, A., and Spichtinger, P.: Lagrangian analysis of ice supersaturated air masses in connection with low level fronts of extratropical cyclones, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-9151, https://doi.org/10.5194/egusphere-egu24-9151, 2024.