Multiradionuclide evidence for an extreme solar proton event around 2,610 B.P. (∼660 BC)

International audience 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 (C-14)] and i...

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Published in:Proceedings of the National Academy of Sciences
Main Authors: O’Hare, Paschal, Mekhaldi, Florian, Adolphi, Florian, Raisbeck, Grant, Aldahan, Ala, Anderberg, Emma, Beer, Jürg, Christl, Marcus, Fahrni, Simon, Synal, Hans-Arno, Park, Junghun, Possnert, Göran, Southon, John, Bard, Édouard, Muscheler, Raimund
Other Authors: Department of Geology Lund, Lund University Lund, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Swiss Federal Insitute of Aquatic Science and Technology Dübendorf (EAWAG), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology Zürich (ETH Zürich), Laboratory of Ion Beam Physics, Angström Laboratory, Uppsala University, Department of Earth System Science Irvine (ESS), University of California Irvine (UCI), University of California-University of California, Chaire Evolution du climat et de l'océan, Centre européen de recherche et d'enseignement des géosciences de l'environnement (CEREGE), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Collège de France (CdF (institution))-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Collège de France (CdF (institution))-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2019
Subjects:
Online Access:https://hal.archives-ouvertes.fr/hal-02476829
https://doi.org/10.1073/pnas.1815725116
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institution Open Polar
collection Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe)
op_collection_id ftccsdartic
language English
topic solar storms
ice cores
solar proton events
radionuclides
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
spellingShingle solar storms
ice cores
solar proton events
radionuclides
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
O’Hare, Paschal
Mekhaldi, Florian
Adolphi, Florian,
Raisbeck, Grant
Aldahan, Ala
Anderberg, Emma
Beer, Jürg
Christl, Marcus
Fahrni, Simon
Synal, Hans-Arno
Park, Junghun
Possnert, Göran
Southon, John,
Bard, Édouard
Muscheler, Raimund
Multiradionuclide evidence for an extreme solar proton event around 2,610 B.P. (∼660 BC)
topic_facet solar storms
ice cores
solar proton events
radionuclides
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
description International audience 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 (C-14)] and ice cores [beryllium-10 (Be-10), chlorine-36 (Cl-36)]. Here, we show evidence for an extreme solar event around 2,610 years B.P. (similar to 660 BC) based on high-resolution Be-10 data from two Greenland ice cores. Our conclusions are supported by modeled C-14 production rates for the same period. Using existing Cl-36 ice core data in conjunction with Be-10, 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.
author2 Department of Geology Lund
Lund University Lund
Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM)
Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Swiss Federal Insitute of Aquatic Science and Technology Dübendorf (EAWAG)
Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology Zürich (ETH Zürich)
Laboratory of Ion Beam Physics
Angström Laboratory
Uppsala University
Department of Earth System Science Irvine (ESS)
University of California Irvine (UCI)
University of California-University of California
Chaire Evolution du climat et de l'océan
Centre européen de recherche et d'enseignement des géosciences de l'environnement (CEREGE)
Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Collège de France (CdF (institution))-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Collège de France (CdF (institution))-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)
format Article in Journal/Newspaper
author O’Hare, Paschal
Mekhaldi, Florian
Adolphi, Florian,
Raisbeck, Grant
Aldahan, Ala
Anderberg, Emma
Beer, Jürg
Christl, Marcus
Fahrni, Simon
Synal, Hans-Arno
Park, Junghun
Possnert, Göran
Southon, John,
Bard, Édouard
Muscheler, Raimund
author_facet O’Hare, Paschal
Mekhaldi, Florian
Adolphi, Florian,
Raisbeck, Grant
Aldahan, Ala
Anderberg, Emma
Beer, Jürg
Christl, Marcus
Fahrni, Simon
Synal, Hans-Arno
Park, Junghun
Possnert, Göran
Southon, John,
Bard, Édouard
Muscheler, Raimund
author_sort O’Hare, Paschal
title Multiradionuclide evidence for an extreme solar proton event around 2,610 B.P. (∼660 BC)
title_short Multiradionuclide evidence for an extreme solar proton event around 2,610 B.P. (∼660 BC)
title_full Multiradionuclide evidence for an extreme solar proton event around 2,610 B.P. (∼660 BC)
title_fullStr Multiradionuclide evidence for an extreme solar proton event around 2,610 B.P. (∼660 BC)
title_full_unstemmed Multiradionuclide evidence for an extreme solar proton event around 2,610 B.P. (∼660 BC)
title_sort multiradionuclide evidence for an extreme solar proton event around 2,610 b.p. (∼660 bc)
publisher HAL CCSD
publishDate 2019
url https://hal.archives-ouvertes.fr/hal-02476829
https://doi.org/10.1073/pnas.1815725116
geographic Greenland
geographic_facet Greenland
genre Greenland
Greenland ice cores
ice core
genre_facet Greenland
Greenland ice cores
ice core
op_source ISSN: 0027-8424
EISSN: 1091-6490
Proceedings of the National Academy of Sciences of the United States of America
https://hal.archives-ouvertes.fr/hal-02476829
Proceedings of the National Academy of Sciences of the United States of America , National Academy of Sciences, 2019, 116 (13), pp.5961-5966. ⟨10.1073/pnas.1815725116⟩
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https://hal.archives-ouvertes.fr/hal-02476829
doi:10.1073/pnas.1815725116
PRODINRA: 476096
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WOS: 000462382800026
op_doi https://doi.org/10.1073/pnas.1815725116
container_title Proceedings of the National Academy of Sciences
container_volume 116
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container_start_page 5961
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spelling ftccsdartic:oai:HAL:hal-02476829v1 2023-05-15T16:29:29+02:00 Multiradionuclide evidence for an extreme solar proton event around 2,610 B.P. (∼660 BC) O’Hare, Paschal Mekhaldi, Florian Adolphi, Florian, Raisbeck, Grant Aldahan, Ala Anderberg, Emma Beer, Jürg Christl, Marcus Fahrni, Simon Synal, Hans-Arno Park, Junghun Possnert, Göran Southon, John, Bard, Édouard Muscheler, Raimund Department of Geology Lund Lund University Lund Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM) Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS) Swiss Federal Insitute of Aquatic Science and Technology Dübendorf (EAWAG) Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology Zürich (ETH Zürich) Laboratory of Ion Beam Physics Angström Laboratory Uppsala University Department of Earth System Science Irvine (ESS) University of California Irvine (UCI) University of California-University of California Chaire Evolution du climat et de l'océan Centre européen de recherche et d'enseignement des géosciences de l'environnement (CEREGE) Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Collège de France (CdF (institution))-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Collège de France (CdF (institution))-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE) 2019-03-26 https://hal.archives-ouvertes.fr/hal-02476829 https://doi.org/10.1073/pnas.1815725116 en eng HAL CCSD National Academy of Sciences info:eu-repo/semantics/altIdentifier/doi/10.1073/pnas.1815725116 info:eu-repo/semantics/altIdentifier/pmid/30858311 hal-02476829 https://hal.archives-ouvertes.fr/hal-02476829 doi:10.1073/pnas.1815725116 PRODINRA: 476096 PUBMED: 30858311 WOS: 000462382800026 ISSN: 0027-8424 EISSN: 1091-6490 Proceedings of the National Academy of Sciences of the United States of America https://hal.archives-ouvertes.fr/hal-02476829 Proceedings of the National Academy of Sciences of the United States of America , National Academy of Sciences, 2019, 116 (13), pp.5961-5966. ⟨10.1073/pnas.1815725116⟩ solar storms ice cores solar proton events radionuclides [SDU.STU]Sciences of the Universe [physics]/Earth Sciences info:eu-repo/semantics/article Journal articles 2019 ftccsdartic https://doi.org/10.1073/pnas.1815725116 2021-11-07T01:20:20Z International audience 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 (C-14)] and ice cores [beryllium-10 (Be-10), chlorine-36 (Cl-36)]. Here, we show evidence for an extreme solar event around 2,610 years B.P. (similar to 660 BC) based on high-resolution Be-10 data from two Greenland ice cores. Our conclusions are supported by modeled C-14 production rates for the same period. Using existing Cl-36 ice core data in conjunction with Be-10, 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. Article in Journal/Newspaper Greenland Greenland ice cores ice core Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) Greenland Proceedings of the National Academy of Sciences 116 13 5961 5966