Hostname: page-component-6bf8c574d5-t27h7 Total loading time: 0 Render date: 2025-02-21T16:42:09.300Z Has data issue: false hasContentIssue false
  • English
  • Français

Temporal 10Be Variations in Ice

Published online by Cambridge University Press:  18 July 2016

Juerg Beer ,
Michael Andree ,
Hans Oeschger ,
Bernhard Stauffer ,
Richard Balzer ,
Georges Bonani ,
Christian Stoller ,
Martin Suter ,
Willy Woelfli  and
Robert C Finkel
Juerg Beer
Affiliation:
Physics Institute, University of Bern, Sidlerstrasse 5, 3012 Bern, Switzerland
Michael Andree
Affiliation:
Physics Institute, University of Bern, Sidlerstrasse 5, 3012 Bern, Switzerland
Hans Oeschger
Affiliation:
Physics Institute, University of Bern, Sidlerstrasse 5, 3012 Bern, Switzerland
Bernhard Stauffer
Affiliation:
Physics Institute, University of Bern, Sidlerstrasse 5, 3012 Bern, Switzerland
Richard Balzer
Affiliation:
Laboratorium für Kernphysik, Swiss Federal Institute of Technology ETHZ, 8093 Zürich, Switzerland
Georges Bonani
Affiliation:
Laboratorium für Kernphysik, Swiss Federal Institute of Technology ETHZ, 8093 Zürich, Switzerland
Christian Stoller
Affiliation:
Laboratorium für Kernphysik, Swiss Federal Institute of Technology ETHZ, 8093 Zürich, Switzerland
Martin Suter
Affiliation:
Laboratorium für Kernphysik, Swiss Federal Institute of Technology ETHZ, 8093 Zürich, Switzerland
Willy Woelfli
Affiliation:
Laboratorium für Kernphysik, Swiss Federal Institute of Technology ETHZ, 8093 Zürich, Switzerland
Robert C Finkel
Affiliation:
Mt Soledad Laboratory, Scripps Institution of Oceanography S - 002, La Jolla, California 92093, U S A
Rights & Permissions [Opens in a new window]

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

10Be (T1/2 = 1.5·106y) is mainly produced in the atmosphere by cosmic ray spallation reactions on nitrogen and oxygen. About 70 % of the production takes place in the stratosphere. 10Be becomes attached to aerosols within a very short time. If 10Be is produced in the stratosphere some latitudinal mixing occurs. Most of the 10Be is transferred to the troposphere during spring and early summer when, mainly at median latitudes, large stratospheric air masses enter the troposphere. Tropospheric 10Be is deposited rapidly on the earth's surface by precipitation. The mean residence time of 10Be in the atmosphere is ca 1 to 2 years. 10Be removed from the atmosphere by precipitation is either preserved in snow and ice layers, in the topsoil and the biosphere, or it enters the hydrosphere (oceans and lakes), where it is transported to the sediments.

Type
I. Natural 14C Variations
Information
Radiocarbon , Volume 25 , Issue 2: 11th International Radiocarbon Conference , 1983 , pp. 269 - 278
Copyright
Copyright © The American Journal of Science 

References

Amin, BS, Lal, D, and Somayajulu, BLK, 1975, Chronology of marine sediments using the 10Be method: intercomparison with other methods: Geochim et Cosmochim Acta, v 39, p 1187–1192.CrossRefGoogle Scholar
Elmore, D, Tubbs, LE, Newman, D, Ma, XZ, Finkel, R, Nishiizumi, K, Beer, J, Oeschger, H, and Andrée, M, in press, The 36Cl bomb pulse measured in a 100 m ice core from Dye 3, Greenland: submitted to Nature.Google Scholar
Finkel, R, Krishnaswami, S, and Clarck, DL, 1977, 10Be in arctic ocean sediments: Earth Planetary Sci Letters, v 35, p 199–204.CrossRefGoogle Scholar
Hammer, CU, Clausen, HB, Dansgaard, W, Gundestrub, N, Johnsen, SJ, and Reeh, N, 1978, Dating of Greenland ice cores by flow models, isotopes, volcanic debris and continental dust: Jour Glaciol, v 20, p 3–26.CrossRefGoogle Scholar
Herron, MM, and Langway, CC, 1982, Chloride, nitrate and sulfate in the Dye 3 and Camp Century, Greenland, ice cores: Am Geophys Union mtg, Philadelphia, May 31-June 14, 1982.Google Scholar
Lal, D, and Peters, B, 1967, Cosmic ray produced radioactivity on the earth, in Flügge, S, ed, Handbuch Physik: Berlin, Springer, v 462, p 551–612.Google Scholar
McCorkell, R, Fireman, EL, and Langway, CC, 1967, Aluminum-26 and Beryllium-10 in Greenland ice: Science, v 158, p 1690–1692.CrossRefGoogle ScholarPubMed
Moller, F, 1951, Vierteljahreskarten des Niederschlages für die ganze Erde: Petermanns Geog Mitt, v 95, p 1–7.Google Scholar
Nishiizumi, K, Arnold, JR, Elmore, D, Ferraro, RD, Gove, HE, Finkel, RC, Beukens, RO, Chang, KH, and Kilius, LR, 1979, Measurements of 36Cl in antarctic meteorites and antarctic ice using a van de Graaff accelerator, in Earth Planetary Sci Letters. v 45, p 285–292.CrossRefGoogle Scholar
Oeschger, H, Beer, J, Loosli, HH, and Schotterer, U, 1981, Low level counting systems in deep underground laboratories, in Methods of low-level-counting and spectrometry: IAEA symposium, Berlin 1981, Proc: p 459–474.Google Scholar
Oeschger, H, Houtermans, J, Loosli, HH, and Wahlen, M, 1970, The constancy of cosmic radiation from isotope studies in meteorites and on the Earth, in Olsson, IU, ed, Radiocarbon variations and absolute chronology: New York, John Wiley + Sons, p 471–498.Google Scholar
Raisbeck, GM, Yiou, F, Fruneau, M, Loiseaux, JM, Lieuvin, M, and Ravel, JC, 1979, Cosmogenic 10Be; mean deposition rate and seasonal concentration variations in precipitation: Nature, v 282, p 279–280.CrossRefGoogle Scholar
Raisbeck, GM, Yiou, F, Lieuvin, M, Ravel, JC, Fruneau, M, and Loiseaux, JM, 1981, 10Be in the environment: some recent results and their applications, in Kutschera, W, ed, Symposium on accelerator mass spectrometry, Proc: Argonne, Illinois, p 228–243.Google Scholar
Siegenthaler, U, Heimann, M, and Oeschger, H, 1980, 14C variations caused by changes in the global carbon cycle: in Stuiver, Minze and Kra, Renee, eds, Internatl radiocarbon conf, 10th, Proc: Radiocarbon, v 22, no. 2, p 177–191.CrossRefGoogle Scholar
Somayajulu, BLK, 1977, Analysis of causes for the beryllium-10 variations in deep sea sediments: Geochim et Cosmochim Acta, v 41, p 909–913.CrossRefGoogle Scholar
Stauffer, B, Neftel, A, Oeschger, H, and Schwander, J, 1982, CO2 concentration in air extracted from Greenland ice samples: Am Geophys Union mtg, Philadelphia, May 31 - June 14, 1982.Google Scholar
Stuiver, Minze, and Quay, PD, 1980, Changes in atmospheric carbon-14 attributed to a variable sun: Science, v 207, p 11–19.CrossRefGoogle ScholarPubMed
Stuiver, Minze, and Quay, PD, 1981, Atmospheric 14C changes resulting from fossil fuel CO2 release and cosmic ray flux variability: Earth Planetary Sci Letters, v 53, p 349–362.CrossRefGoogle Scholar
Suess, HE, 1980, The radiocarbon record in tree rings of the last 8000 years, in Stuiver, Minze and Kra, Renee, eds, Internatl radiocarbon conf, 10th, Proc: v 22, no. 2, p 200–209.Google Scholar
Woelfli, W, Bonani, G, Suter, M, Balzer, R, Nessi, M, and Stoller, Ch, 1982, Radioisotope dating with the ETHZ-EN-tandem accelerator, in Stuiver, Minze and Kra, Renee, eds, Internatl radiocarbon conf, 11th, Proc: Radiocarbon, v 25.Google Scholar