A Mars GCM simulation of the 2018 global dust storm, nudged by observed dust opacities, traces dust from different source regions and identifies rapid exchange between Arabia/Sabaea and Tharsis reservoirs as a storm-sustaining feedback.
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Simulation of the 2018 Global Dust Storm on Mars Using the NASA Ames Mars GCM: A Multi-Tracer Approach
A Mars GCM simulation of the 2018 global dust storm, nudged by observed dust opacities, traces dust from different source regions and identifies rapid exchange between Arabia/Sabaea and Tharsis reservoirs as a storm-sustaining feedback.