“…The methodology used could provide a significant contribution to the key debate regarding the style of resurfacing on Venus. Their results demonstrate what can be still achieved using the (relatively low resolution) Magellan radar dataset but it also shows what could be potentially obtained by higher resolution radar data which are going to be provided from future missions to Venus, such as the European Space Agency's EnVision mission (Ghail et al, 2012(Ghail et al, , 2020 or the NASA's Venus Emissivity, Radio Science, InSAR, Topography & Spectroscopy (VERITAS) mission (i.e., Smrekar et al, 2020). The Deep Atmosphere of Venus Investigation of Noble gases, Chemistry and Imaging, Plus (DAVINCI+) (Glaze et al, 2017;2018;Garvin et al, 2020) and Venera-D (Senske et al, 2017;Zasova et al, 2019) missions will instead provide more detailed data on the structure and thermal profiles of the Venusian atmosphere.…”