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based on observed dynamics, and to link these processes to evolutionary dynamics. To this end, we plan to adapt multivariate autoregressive models for density-class data, whilst paying particular
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, the precipitation of carbides disrupts the macroscopic flow of carbon. Additional complexities come from the process, which includes pulses of enrichment separated by diffusion stages, and from the coexistence
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by scale separation and scale-local interactions, which is precisely a major feature of turbulent flows. Besides, many useful operators (Fourier transforms, convolutions, finite differences, …) accept
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