Iwas hoping that, someone can estimate the h (thickness of net pay) from one of the published seismic lines comparing Venus, Mopane, Saturn?OldGeo - I think the published seismic lines over Venus and proximal to Mopane are in time, not depth, so a comparison with any seismic lines in depth published over Saturn would be difficult to compare with Venus, Mopane.
Could we assume that the Saturn targets (reservoir) could have more or less the same seismik velocity as if available a seismic line within Mopane/Venus reservoir? If yes we could compare the travel times through the potential reservoirs in Saturn to the travel times through the Mopane/Venus reservoirs? I think that could give you an idea about the thickness of the reservoir formation thickness. But I would agree, not for the thickness of the payzone .
...again you end up there: you have to drill to find out.
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