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...
Published in: | Proceedings of the National Academy of Sciences |
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Main Authors: | , , , , , , , , , , , , , , |
Other Authors: | , , , , , , , , , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
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HAL CCSD
2019
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Online Access: | https://hal.science/hal-02476829 https://doi.org/10.1073/pnas.1815725116 |
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ftsorbonneuniv:oai:HAL:hal-02476829v1 |
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HAL Sorbonne Université |
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ftsorbonneuniv |
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, A Raisbeck, Grant Aldahan, Ala Anderberg, Emma Beer, Jürg Christl, Marcus Fahrni, Simon Synal, Hans-Arno Park, Junghun Possnert, Göran Southon, John, R. Bard, Edouard Muscheler, Raimund, R 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 Skane University Hospital 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 (UC Irvine) University of California (UC)-University of California (UC) Collège de France - 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, A Raisbeck, Grant Aldahan, Ala Anderberg, Emma Beer, Jürg Christl, Marcus Fahrni, Simon Synal, Hans-Arno Park, Junghun Possnert, Göran Southon, John, R. Bard, Edouard Muscheler, Raimund, R |
author_facet |
O’hare, Paschal Mekhaldi, Florian Adolphi, Florian, A Raisbeck, Grant Aldahan, Ala Anderberg, Emma Beer, Jürg Christl, Marcus Fahrni, Simon Synal, Hans-Arno Park, Junghun Possnert, Göran Southon, John, R. Bard, Edouard Muscheler, Raimund, R |
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.science/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.science/hal-02476829 Proceedings of the National Academy of Sciences of the United States of America, 2019, 116 (13), pp.5961-5966. ⟨10.1073/pnas.1815725116⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/doi/10.1073/pnas.1815725116 info:eu-repo/semantics/altIdentifier/pmid/30858311 hal-02476829 https://hal.science/hal-02476829 doi:10.1073/pnas.1815725116 INSPIRE: 1780896 PRODINRA: 476096 PUBMED: 30858311 PUBMEDCENTRAL: PMC6442557 WOS: 000462382800026 |
op_doi |
https://doi.org/10.1073/pnas.1815725116 |
container_title |
Proceedings of the National Academy of Sciences |
container_volume |
116 |
container_issue |
13 |
container_start_page |
5961 |
op_container_end_page |
5966 |
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1802644969083633664 |
spelling |
ftsorbonneuniv:oai:HAL:hal-02476829v1 2024-06-23T07:53:22+00:00 Multiradionuclide evidence for an extreme solar proton event around 2,610 B.P. (∼660 BC) O’hare, Paschal Mekhaldi, Florian Adolphi, Florian, A Raisbeck, Grant Aldahan, Ala Anderberg, Emma Beer, Jürg Christl, Marcus Fahrni, Simon Synal, Hans-Arno Park, Junghun Possnert, Göran Southon, John, R. Bard, Edouard Muscheler, Raimund, R Department of Geology Lund Skane University Hospital 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 (UC Irvine) University of California (UC)-University of California (UC) Collège de France - 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.science/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.science/hal-02476829 doi:10.1073/pnas.1815725116 INSPIRE: 1780896 PRODINRA: 476096 PUBMED: 30858311 PUBMEDCENTRAL: PMC6442557 WOS: 000462382800026 ISSN: 0027-8424 EISSN: 1091-6490 Proceedings of the National Academy of Sciences of the United States of America https://hal.science/hal-02476829 Proceedings of the National Academy of Sciences of the United States of America, 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 ftsorbonneuniv https://doi.org/10.1073/pnas.1815725116 2024-06-13T23:45:54Z 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 HAL Sorbonne Université Greenland Proceedings of the National Academy of Sciences 116 13 5961 5966 |