Building transport models from baroclinic wave experimental data

Abstract

In this paper, we study baroclinic waves from both the experimental and the theoretical perspective. We obtain data from a rotating annulus experiment capable of producing a series of baroclinic eddies similar to those found in the mid-latitude atmosphere. We analyze the experimental outputs using two methods. First, we apply a technique that involves filtering data using the empirical orthogonal function (EOF) analysis, which is applied to both velocity and surface temperature fields. The second method relies on the construction of a simple kinematic model based on key parameters derived from the experimental data. To analyze eddy-driven fluid transport, we apply the method of Lagrangian descriptors to the underlying velocity field, revealing the attracting material curves that act as transport barriers in the system. These structures effectively capture the essential characteristics of the baroclinic flow and the associated transport phenomena. Our results show that these barriers are in good agreement with the transport patterns observed in the rotating annulus experiment. In particular, we observe that the structures obtained from the kinematic model, or the one derived in terms of filtered velocities, perform well in this regard.

Generation and Life Cycle of Solar Spicules

“…It may be mentioned here that the baroclinic flow, baroclinic waves, and instabilities are well-known in atmospheric physics. The equations used in different models are solved under appropriate boundary conditions applicable in the atmosphere (De-Leon et al 2020;Baran et al 2022;Agaoglou et al 2024).…”