Identifying atmospheric fronts based on diabatic processes using the dynamic state index (DSI)
Laura Mack, Annette Rudolph, Peter N\'evir

TL;DR
This paper introduces a novel front detection algorithm based on the dynamic state index (DSI), improving identification of weak warm fronts and providing insights into front speed and movement in atmospheric flows.
Contribution
A new front detection method using DSI is developed, addressing limitations of existing algorithms and enabling better analysis of atmospheric front dynamics.
Findings
DSI shows a coherent dipole structure along fronts.
Fronts identified with DSI have higher specific humidity.
DSI-based fronts exhibit higher estimated front speeds.
Abstract
Atmospheric fronts are associated with precipitation and strong diabatic processes. Therefore, detecting fronts objectively from reanalyses is a prerequisite for the long-term study of their weather impacts. For this purpose, several algorithms exist, e.g., based on the thermic front parameter (TFP) or the F diagnostic that combines relative vorticity and horizontal temperature gradient. It is shown that both methods have problems to identify weak warm fronts since they are characterized by low baroclinicity. To avoid this inaccuracy, a new algorithm is developed that considers fronts as deviation from an adiabatic and steady state. These deviations can be accurately measured using the dynamic state index (DSI). The DSI shows a coherent dipole structure along fronts and is strongly correlated with precipitation sums. Using the DSI, a new front detection algorithm is developed (called…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsClimate variability and models · Meteorological Phenomena and Simulations · Tropical and Extratropical Cyclones Research
