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DOI10.1073/pnas.1815725116
Multiradionuclide evidence for an extreme solar proton event around 2;610 B.P. (∼660 BC)
O’Hare P.; Mekhaldi F.; Adolphi F.; Raisbeck G.; Aldahan A.; Anderberg E.; Beer J.; Christl M.; Fahrni S.; Synal H.-A.; Park J.; Possnert G.; Southon J.; Bard E.; Muscheler R.
发表日期2019
ISSN0027-8424
起始页码5961
结束页码5966
卷号116期号:13
英文摘要Recently, it has been confirmed that extreme solar proton events can lead to significantly increased atmospheric production rates of cosmogenic radionuclides. Evidence of such events is recorded in annually resolved natural archives, such as tree rings [carbon-14 ( 14 C)] and ice cores [beryllium-10 ( 10 Be), chlorine-36 ( 36 Cl)]. Here, we show evidence for an extreme solar event around 2,610 years B.P. (∼660 BC) based on high-resolution 10 Be data from two Greenland ice cores. Our conclusions are supported by modeled 14 C production rates for the same period. Using existing 36 Cl ice core data in conjunction with 10 Be, we further show that this solar event was characterized by a very hard energy spectrum. These results indicate that the 2,610-years B.P. event was an order of magnitude stronger than any solar event recorded during the instrumental period and comparable with the solar proton event of AD 774/ 775, the largest solar event known to date. The results illustrate the importance of multiple ice core radionuclide measurements for the reliable identification of short-term production rate increases and the assessment of their origins. © 2019 National Academy of Sciences. All Rights Reserved.
英文关键词Ice cores; Radionuclides; Solar proton events; Solar storms
语种英语
scopus关键词beryllium 10; carbon 14; chlorine 36; multiradionuclide; proton; radioisotope; unclassified drug; Article; chemical analysis; chemical binding; controlled study; energy; energy resource; Greenland; ice core record; priority journal; solar energy; solar storm; spectrum; sun exposure; synthesis; weather
来源期刊Proceedings of the National Academy of Sciences of the United States of America
文献类型期刊论文
条目标识符http://gcip.llas.ac.cn/handle/2XKMVOVA/160400
作者单位O’Hare, P., Department of Geology—Quaternary Sciences, Lund University, Lund, 22362, Sweden; Mekhaldi, F., Department of Geology—Quaternary Sciences, Lund University, Lund, 22362, Sweden; Adolphi, F., Department of Geology—Quaternary Sciences, Lund University, Lund, 22362, Sweden, Climate and Environmental Physics and Oeschger Centre for Climate Change Research, Physics Institute, University of Bern, Bern, 3012, Switzerland; Raisbeck, G., Centre de Sciences Nucléaires et de Sciences de la Matière, CNRS, Université Paris-Saclay, Orsay, 91405, France; Aldahan, A., Department of Geology, United Arab Emirates University, Al Ain, United Arab Emirates; Anderberg, E., Department of Geology—Quaternary Sciences, Lund University, Lund, 22362, Sweden; Beer, J., Department of Surface Waters, Swiss Federal Institute of Aquatic Science and Technology, Dübendorf, 8600, Switzerland; Christl, M., Laboratory of Ion Beam Physics, Swiss Federal Institute of Technology, Zurich, 8093, Switzerland; Fahrni, S., Laboratory of Ion...
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O’Hare P.,Mekhaldi F.,Adolphi F.,et al. Multiradionuclide evidence for an extreme solar proton event around 2;610 B.P. (∼660 BC)[J],2019,116(13).
APA O’Hare P..,Mekhaldi F..,Adolphi F..,Raisbeck G..,Aldahan A..,...&Muscheler R..(2019).Multiradionuclide evidence for an extreme solar proton event around 2;610 B.P. (∼660 BC).Proceedings of the National Academy of Sciences of the United States of America,116(13).
MLA O’Hare P.,et al."Multiradionuclide evidence for an extreme solar proton event around 2;610 B.P. (∼660 BC)".Proceedings of the National Academy of Sciences of the United States of America 116.13(2019).
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