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We observe:  \begin{itemize}  \item The majority of the identified hybrid cloud regimes are strongly associated with observed cloud regimes, with the exception of H4 and H6, which appear to be optically-thinner versions of the deep low cloud regimes (H5) and the optically thin mid-topped cloud regimes (H7), respectively.  \item The pre-frontal cirrus (H10) and frontal cloud regimes (H11) are relatively well-represented in the model. model, within a few percent of the observed RFOs.  \item The thin thinnest hybrid cloud regime (H1) is strongly over-produced in the model, which identifies H1 around more than $40\%$ of the time, compared with $9\%$ in observations.  \end{itemize}  Figure~\ref{fig:hists_sim-obs} shows the