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The ‘Sterno-Etrussia’ Geomagnetic Excursion Around 2700 BP and Changes of Solar Activity, Cosmic Ray Intensity, and Climate

Published online by Cambridge University Press:  18 July 2016

V A Dergachev ,
O M Raspopov ,
B van Geel  and
G I Zaitseva
V A Dergachev
Affiliation:
Ioffe Physico-Technical Institute, St. Petersburg, Russia. Corresponding author. Email: [email protected]
O M Raspopov
Affiliation:
St. Petersburg Branch of IZMIRAN, St. Petersburg, Russia
B van Geel
Affiliation:
Institute for Biodiversity and Ecosystem Dynamics, University of Amsterdam, the Netherlands
G I Zaitseva
Affiliation:
The Institute for the History of Material Culture RAS, St. Petersburg, Russia
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Abstract

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The analysis of both paleo- and archeomagnetic data and magnetic properties of continental and marine sediments has shown that around 2700 BP, the geomagnetic Sterno-Etrussia excursion took place in 15 regions of the Northern Hemisphere. The study of magnetic properties of sediments of the Barents, Baltic, and White Seas demonstrates that the duration of this excursion was not more than 200–300 yr.

Paleoclimatic data provide extensive evidence for a sharp global cooling around 2700 B P. The causes of natural climate variation are discussed. Changes of the galactic cosmic ray intensity may play a key role as the causal mechanism of climate change. Since the cosmic ray intensity (reflected by the cosmogenic isotope level in the earth's atmosphere) is modulated by the solar wind and by the terrestrial magnetic field, this may be an important mechanism for long-term solar climate variability. The Sterno-Etrussia excursion may have amplified the climate shift, which, in the first place, was the effect of a decline of solar activity. During excursions and inversions, the magnetic moment decreases, which leads to an increased intensity of cosmic rays penetrating the upper atmosphere. Global changes in the electromagnetic field of the earth result in sharp changes in the climate-determining factors in the atmosphere, such as temperatures, total pressure field, moisture circulation, intensity of air flows, and thunderstorm activity. In addition, significant changes in the ocean circulation patterns and temperature regimes of oceans will have taken place.

Type
Part II
Information
Radiocarbon , Volume 46 , Issue 2: Proceedings of the 18th International Radiocarbon Conference (Part 2 of 2), Conference Editors: Nancy Beavan Athfield, Rodger J Sparks , 2004 , pp. 661 - 681
Copyright
Copyright © The Arizona Board of Regents on behalf of the University of Arizona 

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