Autor: |
Hansjakob Hofmann, K.J. Hsu, M. Suter, Friedrich Heller, J. Beer, G. Bonani, W.U. Henken-Mellies, C. Shen, Willy Wolfli |
Rok vydání: |
1990 |
Předmět: |
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Zdroj: |
Earth and Planetary Science Letters. 98:267-276 |
ISSN: |
0012-821X |
DOI: |
10.1016/0012-821x(90)90029-w |
Popis: |
A high-resolution10Be profile has been measured on DSDP Site 519 (central South Atlantic) in order to search for changes in the flux of10Be into a pelagic sediment during geomagnetic reversals as compared with times of constant magnetic polarity. The decay corrected10Be concentrations range from 1 to 9 × 108 at/g. The average10Be flux rate is 5 × 108 [at cm−2 kyr−1].9Be and CaCO3 were measured on the same samples. The10Be vs. depth curve is overall similar to the9Be vs. depth curve, while the CaCO3 vs. depth curve anticorrelates the beryllium isotope curves closely, implying that Be is carried mainly by the non-CaCO3 phases of the sediment. The positive correlation between10Be and9Be along with the fact that the average 10Be/9Be ratio of 5.5 × 10−8 is within the range of 10Be/9Be ratios reported for deep ocean water leads us to conclude (1) that the beryllium isotopes come close to an equilibrium in the open ocean, and (2) that the 10Be/9Be in deep sea sediments with a low detrital component monitors the 10Be/9Be of deep ocean water through time. Relative increases of the 10Be/9Be ratio are observed in the vicinity of the geomagnetic reversals, but the relationship between reversals and higher 10Be/9Be remains doubtful. Other mechanisms which could alter the 10Be/9Be ratio are discussed (input of10Be by melting of glacial ice; changing input of9Be due to changes in continental erosion; changing deep ocean circulation; changing scavenging activity at ocean margins), but as yet no conclusive explanation for the observed behavior of the beryllium isotopes can be given. |
Databáze: |
OpenAIRE |
Externí odkaz: |
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