As a first example of the application of such methods, we will show how Lagrangian tracking can be used to study the mechanisms through which cold pools trigger new convective cells in a case in radiative-convective equilibrium with no large-scale organization. Our results show that Lagrangian particles reach their level of free convection only through a cooperation between gust front lifting and thermodynamic forcing, rather than only because of the latter factor, as previously believed. Then, we will apply Lagrangian tracking also to investigate the moisture-rich areas at the edges of expanding cold pools and that are also considered as important players in the thermodynamic forcing. We will present results regarding the structure of these areas and we will assess the relative role played by surface fluxes and rain evaporation in generating them.