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9,400 years of cosmic radiation and solar activity from ice cores and tree rings

机译:来自冰芯和树环的9,400年宇宙辐射和太阳活动

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摘要

Understanding the temporal variation of cosmic radiation and solar activity during the Holocene is essential for studies of the solar-terrestrial relationship. Cosmic-ray produced radionuclides, such as 10Be and 14C which are stored in polar ice cores and tree rings, offer the unique opportunity to reconstruct the history of cosmic radiation and solar activity over many millennia. Although records from different archives basically agree, they also show some deviations during certain periods. So far most reconstructions were based on only one single radionuclide record, which makes detection and correction of these deviations impossible. Here we combine different 10Be ice core records from Greenland and Antarctica with the global 14C tree ring record using principal component analysis. This approach is only possible due to a new high-resolution 10Be record from Dronning Maud Land obtained within the European Project for Ice Coring in Antarctica in Antarctica. The new cosmic radiation record enables us to derive total solar irradi-ance, which is then used as a proxy of solar activity to identify the solar imprint in an Asian climate record. Though generally the agreement between solar forcing and Asian climate is good, there are also periods without any coherence, pointing to other forcings like volcanoes and greenhouse gases and their corresponding feedbacks. The newly derived records have the potential to improve our understanding of the solar dynamics and to quantify the solar influence on climate.
机译:了解全新世期间宇宙辐射和太阳活动的时间变化对于研究太阳与地球之间的关系至关重要。宇宙射线产生的放射性核素,例如10Be和14C,它们存储在极地冰芯和树环中,为重建数千年来的宇宙辐射和太阳活动的历史提供了独特的机会。尽管来自不同档案的记录基本上是一致的,但它们在某些时期也显示出一些偏差。迄今为止,大多数重建工作仅基于单个放射性核素记录,这使得无法检测和校正这些偏差。在这里,我们使用主成分分析将格陵兰岛和南极洲的不同10Be冰芯记录与全球14C年轮记录相结合。只有在Dronning Maud Land获得了新的高分辨率10Be记录后,这种方法才可行,该记录是在南极洲的南极欧洲取冰项目中获得的。新的宇宙辐射记录使我们能够得出太阳总辐照度,然后将其用作太阳活动的代理,以识别亚洲气候记录中的太阳烙印。尽管一般而言太阳强迫与亚洲气候之间的协议是好的,但也有一些时期没有任何连贯性,指向火山和温室气体等其他强迫及其相应的反馈。新近获得的记录有可能增进我们对太阳动力学的理解,并量化太阳对气候的影响。

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    Swiss Federal Institute of Aquatic Science and Technology, Eawag, Ueberlandstrasse 133, 8600 Dubendorf, Switzerland;

    Swiss Federal Institute of Aquatic Science and Technology, Eawag, Ueberlandstrasse 133, 8600 Dubendorf, Switzerland;

    Swiss Federal Institute of Aquatic Science and Technology, Eawag, Ueberlandstrasse 133, 8600 Dubendorf, Switzerland;

    Swiss Federal Institute of Aquatic Science and Technology, Eawag, Ueberlandstrasse 133, 8600 Dubendorf, Switzerland;

    Laboratory of Ion Beam Physics,Swiss Federal Institute of Technology Zurich, Schafmattstrasse 20, 8093 Zurich, Switzerland;

    Climate and Environmental Physics, Physics Institute and Oeschger Centre for Climate Change Research, University of Bern, Sidlerstrasse 5, 3012 Bern, Switzerland;

    Ulla Heikkila, Australian Nuclear Science and Technology Organisation (ANSTO), Lucas Heights, North South Wales 2234, Australia;

    Laboratory of Ion Beam Physics,Swiss Federal Institute of Technology Zurich, Schafmattstrasse 20, 8093 Zurich, Switzerland;

    Swiss Federal Institute of Aquatic Science and Technology, Eawag, Ueberlandstrasse 133, 8600 Dubendorf, Switzerland;

    Ken G. McCracken, Institute for Physical Science and Technology,University of Maryland, College Park, MD 20742;

    Alfred Wegener Institute for Polar and Marine Research, Am Handelshafen 12, 27568 Bremerhaven,Germany;

    Institute for Cosmic Ray Research, University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa 277-8582, Japan;

    Alfred Wegener Institute for Polar and Marine Research, Am Handelshafen 12, 27568 Bremerhaven,Germany;

    Alfred Wegener Institute for Polar and Marine Research, Am Handelshafen 12, 27568 Bremerhaven,Germany;

  • 收录信息 美国《科学引文索引》(SCI);美国《生物学医学文摘》(MEDLINE);美国《化学文摘》(CA);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    cosmogenic radionuclides; cosmic rays; solar modulation;

    机译:宇宙放射性核素;宇宙射线;太阳调制;

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