“…Unlike previous models claiming a progressive deepening of the explosion locus and, relevantly, the crater formation (Lorenz, 1986), recent experiment-based studies of maar eruption dynamics favor a vertical (with respect to the scaled depth (SD), an empirical ratio between depth and energy of the explosion; Goto et al, 2001) and lateral movement of explosions and suggest that pre-existing topography (Sweeney et al, 2018;Acocella, 2021) and substrata lithology are the main factors affecting maar formations (Graettinger et al, 2015;Valentine et al, 2017;Sweeney et al, 2018). These factors have been tested by an increasing number of field observations, mostly on mafic maars (Amin and Valentine, 2017;Chako-Tchamabé et al, 2020;De León-Barragán et al, 2020;Ureta et al, 2021), which are significantly more common as compared to their felsic counterparts (Graettinger, 2018). There is still less information on felsic maars due to the limited exposure (Borrero et al, 2017), and hence, their characteristics have been mostly adopted by tuff rings (Ross et al, 2017).…”