The accuracy of the long-baseline technique is tested in several ways. First, the recovered low-resolution kinematic fields are compared with data obtained for the same MCS from other observational platforms. Then, observed structures and morphologies of similar MCSs during TOGA COARE will be subjectively compared to those recovered using the long-baseline technique. Further, the evolution of this MCS is examined for continuity of the observed structures over a 60-minute period. Using the low-resolution flow field, the area-averaged divergence profiles of various regions within the MSC are computed. The low-resolution flow fields and area-averaged divergence profiles derived from this method show a zone of enhanced convergence along the southern edge of the convective band. This results in a slight (25∞) counter-clockwise rotation of the convective band. This finding is consistent with the results from other observational studies of this particular MCS.
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