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Cross-correlation coefficient maps for Venusian mesoscale cloud morphology, generated from images acquired by the Akatsuki orbiter's cameras at various wavelengths. The data consists of CSV files with 2880 longitude grids (0-360 degrees) and 1440 latitude grids (-90 to +90 degrees) at a 0.125-degree pixel resolution. This archive was created by researchers including Takeshi Imamura of The University of Tokyo for the paper 'Correlation of Venusian Mesoscale Cloud Morphology Between Images Acquired at Various Wavelengths' published in the Journal of Geophysical Research - Planets.
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