As in all centerline evolution models, the first centerline is a straight line, with some noise added. Initial curvature values of the noisy centerline are large (and, therefore, the mean radius of curvature is small), but they decrease as the centerline gets smoother and a characteristic wavelength is being established. A peak value of R is reached early on and then the radius of curvature declines rapidly (Fig. \ref{693028}). The increase in sinuosity lags behind the increase in curvature, so that there is barely any departure from a straight line during the early phase of high values of R (Fig. \ref{693028}A). If the Coriolis effect was suppressing the development of sinuosity, this phase of large radiuses of curvature would represent the time period during which the Coriolis force could and should limit the development of the instability that leads to meandering. However, our numerical simulations suggest that by the time the centerline has a visually noticeable sinuosity, curvature values have increased significantly and the radius of curvature has dropped to a value that remains characteristic for the system for the rest of its evolution (Fig. 7A). A similar early phase of low curvature values that rapidly transitions to larger curvatures characteristic of the sinuous channel has been documented using other, more sophisticated numerical models as well \citep{Camporeale_2005}.
The implication of this analysis is that channels with low but clearly visible sinuosity are likely to have already established a characteristic radius of curvature that is not going to significantly decrease any further. More sinuous stretches of the NAMOC have an overall sinuosity of ~1.06, a value high enough to suggest that this system is past its early phase, characterized by small curvatures (Fig. \ref{693028}A). In other words, the NAMOC has large values of R because it is a large system, not because of its low sinuosity. The presence of an obvious sinuosity is evidence for an inertial instability in the first place; as \citet{Klaucke:1997wi} have stated in their study of the NAMOC, ‘‘in general, the thalweg appears to be located on the outside of meander bends, which demonstrates the predominant effect of the centrifugal force on the lowest and fastest parts of the flows.’’
Thus, the low sinuosity of very large channels like the NAMOC and Tanzania is unlikely to be caused by the Coriolis effect. Both of these systems reflect important differences compared to the highly sinuous channels that are more or less directly linked to their feeding rivers/deltas: (1) they are about an order of magnitude larger than even the largest ‘‘typical’’ submarine channel (Fig. \ref{777085}); and (2) they are fed by a tributary channel system, as opposed to the typical avulsion-related distributary channel pattern characteristic of channels on submarine fans.