Computer Science
Scientific paper
Jan 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988gecoa..52..201h&link_type=abstract
Geochimica et Cosmochimica Acta, vol. 52, Issue 1, pp.201-207
Computer Science
3
Scientific paper
Sediment samples (32) from DSDP Holes 516 and 516F, Leg 72 were subjected to INAA (instrumental neutron activation analysis). Thirty-two major, minor and trace elements were determined. Ce anomalies, Ce A Ce ( obs .)/ Ce * (interpolated between La and Nd and relative to the N.A.S.C. (North American Shale Composite)) = Ce ( obs .)/[1.44 La ( obs .) + 0.66 Nd ( obs .)], in the carbonate phase were obtained. Calculations indicate that the Ce anomaly changed from 0.80 (80 My), 0.68 (67 My) to 0.30 (56 My), 0.27 (39 My) and 0.12-0.43 (avg. 0.26) (15-0.3 My). The Ce A change observed at ~55 My coincides with the Ce A change at ~58 My in marine carbonates from the Walvis Ridge, Hole 525A. These changes are attributed to improved water circulation caused by either the widening of the north-south Atlantic passage, subsidence of the Rio Grande Rise or subsidence of the Romanche Fracture Zone. The ultimate driving force behind the Ce A changes is related to the pH and P O 2 of the seawater and also related to global circulation of bottom ocean water and transport of the external terrestrial input from riverine or/and aeolian sources.
Hu Xiao
Schmitt Roman A.
Wang L. Y.
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