Hostname: page-component-cd9895bd7-gxg78 Total loading time: 0 Render date: 2024-12-26T04:39:58.330Z Has data issue: false hasContentIssue false

Solar Variability Traced by Cosmogenic Isotopes

Published online by Cambridge University Press:  12 April 2016

Jürg Beer
Affiliation:
Swiss Federal Institute for Environmental Science and Technology(EAWAG), CH-8600 Dübendorf, Switzerland
Stephan T. Baumgartner
Affiliation:
Swiss Federal Institute for Environmental Science and Technology(EAWAG), CH-8600 Dübendorf, Switzerland
Beate Dittrich-Hannen
Affiliation:
Institute of Particle Physics, ETH-Hönggerberg, CH-8093 Zürich, Switzerland
Jürg Hauenstein
Affiliation:
Physics Institute, University of Bern, CH-3012 Bern, Switzerland
Peter Kubik
Affiliation:
Paul Scherrer Institute, c/o Institute of Particle Physics, ETH-Hönggerberg, CH-8093 Zürich, Switzerland
Christian Lukasczyk
Affiliation:
Swiss Federal Institute for Environmental Science and Technology(EAWAG), CH-8600 Dübendorf, Switzerland
Werner Mende
Affiliation:
Institute of Meteorology, Freie Universität Berlin, Germany
Rita Stellmacher
Affiliation:
Institute of Meteorology, Freie Universität Berlin, Germany
Martin Suter
Affiliation:
Institute of Particle Physics, ETH-Hönggerberg, CH-8093 Zürich, Switzerland

Abstract

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 has been measured in a 300 m long ice core from Greenland. After a general analysis of the 10Be data the potential and the limitations of 10Be records in ice to reconstruct solar variability are discussed. Special emphasis is given to periods of low solar activity (Maunder Minimum etc.). The ‘clock problem’ is addressed, also the question whether the Schwabe cycle maintains its phase. Finally the question of what 10Be can tell us about changes of the solar irradiance in the past is explored.

Type
The Response of the Earth’s Atmosphere to Solar Irradiance Variations and Sun-Climate Connections
Copyright
Copyright © Kluwer 1994

References

Baliunas, S. & Jastrow, R. 1990 Evidence for long-term brightness changes of solar-type stars. Nature 348, 520523.Google Scholar
Beer, J., Blinov, A., Bonani, G., Finkel, R.C., Hofmann, H.J., Lehmann, B., Oeschger, H., Sigg, A., Schwander, J., Staffelbach, T., Stauffer, B., Suter, M. & Woelfli, W. 1990 Use of 10Be in polar ice to trace the 11-year cycle of solar activity. Nature 347, 164166.Google Scholar
Beer, J., Raisbeck, G.M. & Yiou, F. 1991 Time variations of 10Be and solar activity. In The Sun in Time (ed. Sonett, C.P., Giampapa, M.S. & Matthews, M.S.), pp. 343359. Univ. of Arizona Press.Google Scholar
Blinov, A. 1988 The dependence of cosmogenic isotope production rate on solar activitiy and geomagnetic field variations. In Secular Solar and Geomagnetic Variations in the last 10,000 Years (ed. Stephenson, F.R. & Wolfendale, A.W.), pp. 329340. Kluwer Academic Publishers.Google Scholar
Dicke, R.H. 1978 Is there a chronometer hidden deep in the Sun? Nature 276, 676680.Google Scholar
Eddy, J.A. 1976 The Maunder Minimum. Science 192, 11891201.Google Scholar
Friis-Christensen, E. & Lassen, K. 1991 Length of the solar cycle: An indicator of solar activity closely associated with climate. Nature 254, 698700.Google Scholar
Groveman, B.S. & Landsberg, H.E. 1979 Reconstruction of Northern hemisphere temperature. 1579 - 1880. University of Maryland, College Park, MD: Publication 79181.Google Scholar
Jones, P.D., Raper, S.C.B., Bradley, R.S., Diaz, H.F., Kelly, P.M. & Wigley, T.M.L. 1986 Northern Hemisphere surface air temperature variations, 1851-1984, J. Clim. Appl. Met. 25, 161179.Google Scholar
Kelly, P.M. & Wigley, T.M.L. 1992 Solar cycle length, greenhouse forcing and global climate. Nature 360, 328330.Google Scholar
Lal, D. & Peters, B. 1967 Cosmic ray produced radioactivity on the Earth. In Handbuch für Physik, 46/2 (ed. Flügge, S.), pp. 551612.Google Scholar
Lean, J. 1991 Variations in the Sun’s radiative output. Reviews of Geophysics 29/4, 505535.CrossRefGoogle Scholar
Lean, J., Hulburt, E.O., Skumanich, A. & White, O. 1992 Estimating the Sun’s radiative output during the Maunder Minimum. GRL 19, 15911594.CrossRefGoogle Scholar
Lockwood, G.W., Skiff, B.A., Baliunas, S.L. & Radick, R.R. 1992 Long-term solar brightness changes estimated from a survey of Sun-like stars. Nature 360, 653655.CrossRefGoogle Scholar
Newkirk, G. Jr. 1984 What accelerator mass spectrometry can do for solar physics. Nucl. Instrum. Meth. B5, 404410.Google Scholar
Raisbeck, G.M. & Yiou, F. 1980 10Be in polar ice cores as a record of solar activity. In Proc. Conf. on Ancient Sun (ed. Pepin, R.O., Eddy, J.A. & Merrill, R.B.), pp. 185190. Pergamon Press.Google Scholar
Schlesinger, M.E. & Ramankutty, N. 1992 Implications for global warming of intercycle solar irradiance variations. Nature 360, 330333.CrossRefGoogle Scholar
Siegenthaler, U. & Beer, J. 1988 Model comparison of 14C and 10Be isotope records. In Secular Solar and Geomagnetic Variations in the last 10,000 Years (ed. Stephenson, F.R. & Wolfendale, A.W.), pp. 315328. Kluwer Academic Publishers.Google Scholar
Stephenson, F.R. 1988 Solar variability from historical records. In Secular Solar and Geomagnetic Variations in the last 10,000 Years (ed. Stephenson, F.R. & Wolfendale, A.W.). pp. 109129. Kluwer Academic Publishers.Google Scholar
Stuiver, M., Brazunias, T.F., Becker, B. & Kromer, B. 1991 Climatic, solar, oceanic and geomagnetic influences on Late-Glacial and Holocene atmospheric 14C/12C change. Quot. Res. 35, 124.Google Scholar
Stuiver, M. & Quay, P.D. 1980 Changes in atmospheric Carbon-14 attributed to a variable Sun. Science 207, 1119.Google Scholar
Suter, M. 1990 Accelerator mass spectrometry: State of the art in 1990, Nucl. Instrum. Meth. B52, 211223.Google Scholar
Willson, R.C. & Hudson, H.S. 1988 Solar luminosity variations in solar cycle 21. Nature 332, 810812.Google Scholar