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    The "Sterno-Etrussia" Geomagnetic Excursion around 2700 BP and Changes of Solar Activity, Cosmic Ray Intensity, and Climate

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    Author
    Dergachev, V. A.
    Raspopov, O. M.
    van Geel, B.
    Zaitseva, G. I.
    Issue Date
    2004-01-01
    Keywords
    Arctic Ocean
    Arctic region
    Atlantic Ocean
    Baltic Sea
    Barents Sea
    C 14
    carbon
    Cenozoic
    chronostratigraphy
    climate change
    concentration
    cosmic rays
    cyclic processes
    glaciation
    Holocene
    isotopes
    lake level changes
    magnetic declination
    magnetic field
    magnetic inclination
    magnetization
    marine sediments
    North Atlantic
    paleoclimatology
    paleoenvironment
    paleomagnetism
    Quaternary
    radioactive isotopes
    remanent magnetization
    sediments
    Sterno Etrussia geomagnetic excursion
    White Sea
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    Citation
    Dergachev, V. A., Raspopov, O. M., van Geel, B., & Zaitseva, G. I. (2004). The ‘Sterno-Etrussia’ geomagnetic excursion around 2700 BP and changes of solar activity, cosmic ray intensity, and climate. Radiocarbon, 46(2), 661-681.
    Publisher
    Department of Geosciences, The University of Arizona
    Journal
    Radiocarbon
    Description
    From the 18th International Radiocarbon Conference held in Wellington, New Zealand, September 1-5, 2003.
    URI
    http://hdl.handle.net/10150/654965
    DOI
    10.1017/S0033822200035724
    Additional Links
    http://radiocarbon.webhost.uits.arizona.edu/
    Abstract
    The analysis of both paleoand 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 BP. 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
    Proceedings
    text
    Language
    en
    ISSN
    0033-8222
    ae974a485f413a2113503eed53cd6c53
    10.1017/S0033822200035724
    Scopus Count
    Collections
    Radiocarbon, Volume 46, Number 2 (2004)

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