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Applications of PB-210/RA-226 and PO-210/PB-210 disequilibria in the study of marine geochemical processes

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Author(s)
Bacon, Michael P.
Keywords
Pb-210/Po-210
Distribution
Removal
Meteor (Ship) Cruise M32
Atlantis II (Ship : 1963-) Cruise AII85

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URI
http://hdl.handle.net/20.500.12424/1045720
Online Access
http://hdl.handle.net/1912/1254
Abstract
Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy at the Massachusetts Institute of Technology and the Woods Hole Oceanographic Institution November, 1975
The distribution of Pb-210 and Po-210 in dissolved (<O.4 micron) and particulate (>0.4 micron) phases has been measured at ten stations in the tropical and eastern North Atlantic and at two stations in the
 Pacific. Both radionuclides occur principally in the dissolved phase.
 Unsupported Pb-210 activities, maintained by flux from the atmosphere, are present in the surface mixed layer and penetrate into the thermocline to depths of about 500 m. Dissolved Po-210 is ordinarily present
 in the mixed layer at less than equilibrium concentrations, suggesting rapid biological removal of this nuclide. Particulate matter is enriched in Po-210, with Po-210/Pb-210 activity ratios greater than 1.0, similar to those reported for phytoplankton. Box-model calculations yield a 2-y residence time for Pb-210 and a 0.6-y residence time for
 Po-210 in the mixed layer. These residence times are considerably longer than the time calculated for turnover of particles in the mixed layer (about 0.1 y). At depths of 100-300 m, Po-210 maxima occur and
 unsupported Po-210 is frequently present. 
 Calculations indicate that at least 50% of the Po-210 removed from the mixed layer is recycled within the thermocline. Similar calculations for Pb-210 suggest much
 lower recycling efficiencies. Comparison of the Pb-210 distribution with the reported distribution of Ra-226 at nearby GEOSECS. stations has confirmed the widespread
 existence of a Pb-210/Ra-226 disequilibrium in the deep sea. Vertical profiles of particulate Pb-210 were used to test the hypothesis that Pb-210 is removed from deepwater by in situ scavenging. With the
 exception of one profile taken near the Mid-Atlantic Ridge, significant
 vertical gradients in particulate Pb-210 concentration were not observed, and it is necessary to invoke exceptionally high particle sinking velocities (>10 m/d) to account for the inferred Pb-210 flux. It is proposed that an additional sink for Pb-210 in the deep sea must be sought. Estimates of the dissolved Pb-210/Ra-226 activity ratio at
 depths greater than 1,000 m range from 0.2 to 0.8 and reveal a systematic increase, in both vertical and horizontal directions, with
 increasing distance from the sea floor. This observation implies rapid scavenging of Pb-210 at the sediment-water interface and is
 consistent with a horizontal eddy diffusivity of 3-6 x 107 cm2/s. The more reactive element Po, on the other hand, shows evidence of rapid in situ scavenging. In filtered sea water, Po-210 is deficient, on the
 average, by ca. 10% relative to Pb-210; a corresponding enrichment is
 found in the particulate phase. Total inventories of Pb-210 and Po-210
 over the entire water column, however, show no significant departure from secular equilibrium, and reliable estimates of particle sinking rates cannot be made.
Prepared under National Science Foundation Grant GA-41061 and U.S.A.E.C. Contract AT(11-1).
Date
2006-10-02
Type
Technical Report
Identifier
oai:localhost:1912/1254
http://hdl.handle.net/1912/1254
10.1575/1912/1254
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