FORMISANO, MichelangeloMichelangeloFORMISANOFederico, CostanzoCostanzoFedericoDE SANCTIS, MARIA CRISTINAMARIA CRISTINADE SANCTISDE ANGELIS, SimoneSimoneDE ANGELISMagni, GianfrancoGianfrancoMagni2022-07-142022-07-142018http://hdl.handle.net/20.500.12386/32494Core dynamo is one of the most efficient mechanism to produce magnetic field in the planetary bodies as well as in the minor bodies of the solar system. It is interesting to study and to evaluate how the thickness and composition of the overlying rocky lid influences the thermal convective evolution of the core. <P />ELETTRONICOenConference abstracthttps://www.epsc2018.eu/information/general_information.html2018EPSC...12..740FFIS/05 - ASTRONOMIA E ASTROFISICA