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Cosmogenic radionuclides reveal an extreme solar particle storm near a solar minimum 9125 years BP
During solar storms, the Sun expels large amounts of energetic particles (SEP) that can react with the Earth’s atmospheric constituents and produce cosmogenic radionuclides such as (14)C, (10)Be and (36)Cl. Here we present (10)Be and (36)Cl data measured in ice cores from Greenland and Antarctica. T...
Autores principales: | , , , , , , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
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Nature Publishing Group UK
2022
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8752676/ https://www.ncbi.nlm.nih.gov/pubmed/35017519 http://dx.doi.org/10.1038/s41467-021-27891-4 |
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author | Paleari, Chiara I. Mekhaldi, Florian Adolphi, Florian Christl, Marcus Vockenhuber, Christof Gautschi, Philip Beer, Jürg Brehm, Nicolas Erhardt, Tobias Synal, Hans-Arno Wacker, Lukas Wilhelms, Frank Muscheler, Raimund |
author_facet | Paleari, Chiara I. Mekhaldi, Florian Adolphi, Florian Christl, Marcus Vockenhuber, Christof Gautschi, Philip Beer, Jürg Brehm, Nicolas Erhardt, Tobias Synal, Hans-Arno Wacker, Lukas Wilhelms, Frank Muscheler, Raimund |
author_sort | Paleari, Chiara I. |
collection | PubMed |
description | During solar storms, the Sun expels large amounts of energetic particles (SEP) that can react with the Earth’s atmospheric constituents and produce cosmogenic radionuclides such as (14)C, (10)Be and (36)Cl. Here we present (10)Be and (36)Cl data measured in ice cores from Greenland and Antarctica. The data consistently show one of the largest (10)Be and (36)Cl production peaks detected so far, most likely produced by an extreme SEP event that hit Earth 9125 years BP (before present, i.e., before 1950 CE), i.e., 7176 BCE. Using the (36)Cl/(10)Be ratio, we demonstrate that this event was characterized by a very hard energy spectrum and was possibly up to two orders of magnitude larger than any SEP event during the instrumental period. Furthermore, we provide (10)Be-based evidence that, contrary to expectations, the SEP event occurred near a solar minimum. |
format | Online Article Text |
id | pubmed-8752676 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2022 |
publisher | Nature Publishing Group UK |
record_format | MEDLINE/PubMed |
spelling | pubmed-87526762022-01-20 Cosmogenic radionuclides reveal an extreme solar particle storm near a solar minimum 9125 years BP Paleari, Chiara I. Mekhaldi, Florian Adolphi, Florian Christl, Marcus Vockenhuber, Christof Gautschi, Philip Beer, Jürg Brehm, Nicolas Erhardt, Tobias Synal, Hans-Arno Wacker, Lukas Wilhelms, Frank Muscheler, Raimund Nat Commun Article During solar storms, the Sun expels large amounts of energetic particles (SEP) that can react with the Earth’s atmospheric constituents and produce cosmogenic radionuclides such as (14)C, (10)Be and (36)Cl. Here we present (10)Be and (36)Cl data measured in ice cores from Greenland and Antarctica. The data consistently show one of the largest (10)Be and (36)Cl production peaks detected so far, most likely produced by an extreme SEP event that hit Earth 9125 years BP (before present, i.e., before 1950 CE), i.e., 7176 BCE. Using the (36)Cl/(10)Be ratio, we demonstrate that this event was characterized by a very hard energy spectrum and was possibly up to two orders of magnitude larger than any SEP event during the instrumental period. Furthermore, we provide (10)Be-based evidence that, contrary to expectations, the SEP event occurred near a solar minimum. Nature Publishing Group UK 2022-01-11 /pmc/articles/PMC8752676/ /pubmed/35017519 http://dx.doi.org/10.1038/s41467-021-27891-4 Text en © The Author(s) 2022 https://creativecommons.org/licenses/by/4.0/Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) . |
spellingShingle | Article Paleari, Chiara I. Mekhaldi, Florian Adolphi, Florian Christl, Marcus Vockenhuber, Christof Gautschi, Philip Beer, Jürg Brehm, Nicolas Erhardt, Tobias Synal, Hans-Arno Wacker, Lukas Wilhelms, Frank Muscheler, Raimund Cosmogenic radionuclides reveal an extreme solar particle storm near a solar minimum 9125 years BP |
title | Cosmogenic radionuclides reveal an extreme solar particle storm near a solar minimum 9125 years BP |
title_full | Cosmogenic radionuclides reveal an extreme solar particle storm near a solar minimum 9125 years BP |
title_fullStr | Cosmogenic radionuclides reveal an extreme solar particle storm near a solar minimum 9125 years BP |
title_full_unstemmed | Cosmogenic radionuclides reveal an extreme solar particle storm near a solar minimum 9125 years BP |
title_short | Cosmogenic radionuclides reveal an extreme solar particle storm near a solar minimum 9125 years BP |
title_sort | cosmogenic radionuclides reveal an extreme solar particle storm near a solar minimum 9125 years bp |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8752676/ https://www.ncbi.nlm.nih.gov/pubmed/35017519 http://dx.doi.org/10.1038/s41467-021-27891-4 |
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