Changes in the carbon cycle during the last deglaciation as indicated by the comparison of 10Be and 14C records

被引:155
作者
Muscheler, R
Beer, J
Wagner, G
Laj, C
Kissel, C
Raisbeck, GM
Yiou, F
Kubik, PW
机构
[1] Lund Univ, Dept Geol, GeoBiosphere Sci Ctr, SE-22362 Lund, Sweden
[2] Swiss Fed Inst Environm Sci & Technol, EAWAG, CH-8600 Dubendorf, Switzerland
[3] CEA, CNRS, Lab Sci Climat & Environm, F-91198 Gif Sur Yvette, France
[4] CNRS, Ctr Spectrometrie Nucl & Spectrometrie Masse, F-91405 Orsay, France
[5] ETH Honggerberg, Paul Scherrer Inst Particle Phys, CH-8093 Zurich, Switzerland
关键词
cosmogenic radionuclides; ice cores; carbon cycle; ocean circulation; paleomagnetism;
D O I
10.1016/S0012-821X(03)00722-2
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The variations in atmospheric radiocarbon (C-14) concentration during the last 50 000 years can be attributed to changes in the C-14 production rate (due to changes in solar activity, the geomagnetic field and/or interstellar galactic cosmic ray flux) and to changes in the global carbon cycle. The relative contributions of these processes is the subject of current debate. Although the discrepancies between the various reconstructions of the past atmospheric radiocarbon concentration increase with age, the relatively good agreement over the last 25 000 years allows a quantitative discussion of the causes of the observed C-14 variations for this period. Using Be-10 measurements from Greenland Summit ice cores, we show that, in addition to solar and geomagnetically induced production rate changes, significant changes in the carbon cycle have to be considered to explain the measured C-14 concentrations. There is evidence that these changes are connected to: (1) global deglaciation and (2) climate changes in the North Atlantic region on centennial to millennial time scales related to changes in the ocean circulation. Differences between Be-10 and geomagnetic field records, however, suggest that uncertainties of about 20% still exist in determinations of past changes in the C-14 production rate. (C) 2004 Elsevier B.V. All rights reserved.
引用
收藏
页码:325 / 340
页数:16
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