We present a seismic model of the African Plate, made with the technique
of full-waveform inversion. The purpose of our model is to become a
foundation for future use and research, such as quantitative geodynamic
interpretations, earthquake-induced ground motion predictions, and
earthquake source inversion. Starting from the first-generation
Collaborative Seismic Earth Model (CSEM), we invert seismograms filtered
to a minimum period of 35 s and compute gradients of the misfit function
with respect to the model parameters using the adjoint state method. In
contrast to the conventional FWI approach, we use dynamically changing
data subsets (mini-batches) of the complete dataset to compute
approximate gradients at each iteration. This approach has three
significant advantages: (1) it reduces computational costs for model
updates and the inversion, (2) it enables the use of larger datasets
without increasing iteration costs, and (3) it makes it trivial to
assimilate new data since we can add it to the complete dataset without
changing the misfit function, thereby enabling “evolutionary FWI”. We
perform 130 mini-batch iterations and invert data from 397 unique
earthquakes and 184,356 unique source-receiver pairs at the cost of
approximately 10 full-data iterations. We clearly image tectonic
features such as the Afar triple junction. Particularly interesting are
the low-velocity zones below the Hoggar, Aïr, and Tibesti Mountains,
pronounced more than in earlier works. Finally, we introduce a new
strategy to assess model uncertainty. We deliberately perturb the final
model, perform additional mini-batch iterations, and compare the result
with the original final model. This test uses actual seismic data
instead of artificially generated synthetic data and requires no
assumptions about the linearity of the inverse problem.