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Now that everyone has more-or-less recovered from NAPC I guess it's time to get back to the business of wringing information out of the universal paleo. mind. Lately I've been looking into the question of Late Paleozoic marine surface-water circulation patterns (don't ask why) and I need to know whether the existence of circum-global equatorial circulation (such as existed in the Early Carboniferous and Cretaceous would have increased or decreased the intensity of gyral circulation relative to time periods when there was no circum-global equatorial circulation (such as the Permian or now)? Any paleo-oceanographers out there who feel like sticking their necks out on this one? Thanks in advance. Norm MacLeod ---------------------------------------------------------------------------- Norman MacLeod Micropalaeontological Research N.MacLeod@nhm.ac.uk (Internet) N.MacLeod@uk.ac.nhm (Janet) Address: Dept. of Palaeontology, The Natural History Museum, Cromwell Road, London, SW7 5BD Office Phone: 0171-938-9006 Dept. FAX: 0171-938-9277 ----------------------------------------------------------------------------
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