Use of 10Be to predict atmospheric 14C variations during the laschamp excursion: High sensitivity to cosmogenic isotope production calculations
International audience The Laschamp excursion is a period of reduced geomagnetic field intensity occurring 40.7 ± 1.0 kyr ago. As a consequence, cosmogenic isotope production increased dramatically and its sensitivity to solar activity was enhanced during this period. The latter occurs because a lar...
Published in: | Radiocarbon |
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Main Authors: | , , , |
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Format: | Article in Journal/Newspaper |
Language: | English |
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HAL CCSD
2014
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Online Access: | https://hal.science/hal-01088887 https://hal.science/hal-01088887/document https://hal.science/hal-01088887/file/USE%20OF%2010Be%20TO%20PREDICT%20ATMOSPHERIC.pdf https://doi.org/10.2458/56.16478 |
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Open Polar |
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Université de Nantes: HAL-UNIV-NANTES |
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ftunivnantes |
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English |
topic |
[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph] [PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph] |
spellingShingle |
[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph] [PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph] Cauquoin, Alexandre Raisbeck, G. Jouzel, Jean Paillard, D. Use of 10Be to predict atmospheric 14C variations during the laschamp excursion: High sensitivity to cosmogenic isotope production calculations |
topic_facet |
[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph] [PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph] |
description |
International audience The Laschamp excursion is a period of reduced geomagnetic field intensity occurring 40.7 ± 1.0 kyr ago. As a consequence, cosmogenic isotope production increased dramatically and its sensitivity to solar activity was enhanced during this period. The latter occurs because a larger fraction of the lower-energy interstellar galactic cosmic-ray particles, normally excluded by the geomagnetic field, is able to reach Earth's atmosphere. This produces a cosmogenic isotope production signal with a significant structure. As high-resolution 10Be profiles from both Antarctica (EDC) and Greenland (NGRIP-GRIP) during this crucial period are now available, one can use them as input into a box carbon cycle model in order to predict atmospheric 14C variations due to the Laschamp excursion. For this purpose, 10Be data are converted into 14C, using production calculations for the 10Be-14C conversion, after correction for the estimated difference of sensitivity between polar and global 10Be deposition. Several scenarios of carbon cycle state are simulated, from preindustrial to glacial conditions. Applying two recent cosmogenic isotope production calculations for the 10Be to 14C conversion, we found that the resulting atmospheric ?14C variations are very sensitive to which of these two are employed. For example, ?14C amplitude under glacial conditions varies from 260‰ (EDC) and 320‰ (Greenland) to 430‰ (EDC) and 510‰ (Greenland) depending on the formulation used for 10Be-14C conversion. ©2014 by the Arizona Board of Regents on behalf of the University of Arizona. |
author2 |
Laboratoire des Sciences du Climat et de l'Environnement Gif-sur-Yvette (LSCE) Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS) 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) Glaces et Continents, Climats et Isotopes Stables (GLACCIOS) Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS) Modélisation du climat (CLIM) |
format |
Article in Journal/Newspaper |
author |
Cauquoin, Alexandre Raisbeck, G. Jouzel, Jean Paillard, D. |
author_facet |
Cauquoin, Alexandre Raisbeck, G. Jouzel, Jean Paillard, D. |
author_sort |
Cauquoin, Alexandre |
title |
Use of 10Be to predict atmospheric 14C variations during the laschamp excursion: High sensitivity to cosmogenic isotope production calculations |
title_short |
Use of 10Be to predict atmospheric 14C variations during the laschamp excursion: High sensitivity to cosmogenic isotope production calculations |
title_full |
Use of 10Be to predict atmospheric 14C variations during the laschamp excursion: High sensitivity to cosmogenic isotope production calculations |
title_fullStr |
Use of 10Be to predict atmospheric 14C variations during the laschamp excursion: High sensitivity to cosmogenic isotope production calculations |
title_full_unstemmed |
Use of 10Be to predict atmospheric 14C variations during the laschamp excursion: High sensitivity to cosmogenic isotope production calculations |
title_sort |
use of 10be to predict atmospheric 14c variations during the laschamp excursion: high sensitivity to cosmogenic isotope production calculations |
publisher |
HAL CCSD |
publishDate |
2014 |
url |
https://hal.science/hal-01088887 https://hal.science/hal-01088887/document https://hal.science/hal-01088887/file/USE%20OF%2010Be%20TO%20PREDICT%20ATMOSPHERIC.pdf https://doi.org/10.2458/56.16478 |
geographic |
Greenland |
geographic_facet |
Greenland |
genre |
Antarc* Antarctica Greenland GRIP NGRIP |
genre_facet |
Antarc* Antarctica Greenland GRIP NGRIP |
op_source |
ISSN: 0033-8222 EISSN: 1945-5755 Radiocarbon https://hal.science/hal-01088887 Radiocarbon, 2014, 56 (1), pp.67-82. ⟨10.2458/56.16478⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/doi/10.2458/56.16478 hal-01088887 https://hal.science/hal-01088887 https://hal.science/hal-01088887/document https://hal.science/hal-01088887/file/USE%20OF%2010Be%20TO%20PREDICT%20ATMOSPHERIC.pdf doi:10.2458/56.16478 |
op_rights |
info:eu-repo/semantics/OpenAccess |
op_doi |
https://doi.org/10.2458/56.16478 |
container_title |
Radiocarbon |
container_volume |
56 |
container_issue |
1 |
container_start_page |
67 |
op_container_end_page |
82 |
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1766273791504154624 |
spelling |
ftunivnantes:oai:HAL:hal-01088887v1 2023-05-15T14:03:14+02:00 Use of 10Be to predict atmospheric 14C variations during the laschamp excursion: High sensitivity to cosmogenic isotope production calculations Cauquoin, Alexandre Raisbeck, G. Jouzel, Jean Paillard, D. Laboratoire des Sciences du Climat et de l'Environnement Gif-sur-Yvette (LSCE) Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS) 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) Glaces et Continents, Climats et Isotopes Stables (GLACCIOS) Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS) Modélisation du climat (CLIM) 2014 https://hal.science/hal-01088887 https://hal.science/hal-01088887/document https://hal.science/hal-01088887/file/USE%20OF%2010Be%20TO%20PREDICT%20ATMOSPHERIC.pdf https://doi.org/10.2458/56.16478 en eng HAL CCSD University of Arizona info:eu-repo/semantics/altIdentifier/doi/10.2458/56.16478 hal-01088887 https://hal.science/hal-01088887 https://hal.science/hal-01088887/document https://hal.science/hal-01088887/file/USE%20OF%2010Be%20TO%20PREDICT%20ATMOSPHERIC.pdf doi:10.2458/56.16478 info:eu-repo/semantics/OpenAccess ISSN: 0033-8222 EISSN: 1945-5755 Radiocarbon https://hal.science/hal-01088887 Radiocarbon, 2014, 56 (1), pp.67-82. ⟨10.2458/56.16478⟩ [SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph] [PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph] info:eu-repo/semantics/article Journal articles 2014 ftunivnantes https://doi.org/10.2458/56.16478 2023-03-08T02:56:14Z International audience The Laschamp excursion is a period of reduced geomagnetic field intensity occurring 40.7 ± 1.0 kyr ago. As a consequence, cosmogenic isotope production increased dramatically and its sensitivity to solar activity was enhanced during this period. The latter occurs because a larger fraction of the lower-energy interstellar galactic cosmic-ray particles, normally excluded by the geomagnetic field, is able to reach Earth's atmosphere. This produces a cosmogenic isotope production signal with a significant structure. As high-resolution 10Be profiles from both Antarctica (EDC) and Greenland (NGRIP-GRIP) during this crucial period are now available, one can use them as input into a box carbon cycle model in order to predict atmospheric 14C variations due to the Laschamp excursion. For this purpose, 10Be data are converted into 14C, using production calculations for the 10Be-14C conversion, after correction for the estimated difference of sensitivity between polar and global 10Be deposition. Several scenarios of carbon cycle state are simulated, from preindustrial to glacial conditions. Applying two recent cosmogenic isotope production calculations for the 10Be to 14C conversion, we found that the resulting atmospheric ?14C variations are very sensitive to which of these two are employed. For example, ?14C amplitude under glacial conditions varies from 260‰ (EDC) and 320‰ (Greenland) to 430‰ (EDC) and 510‰ (Greenland) depending on the formulation used for 10Be-14C conversion. ©2014 by the Arizona Board of Regents on behalf of the University of Arizona. Article in Journal/Newspaper Antarc* Antarctica Greenland GRIP NGRIP Université de Nantes: HAL-UNIV-NANTES Greenland Radiocarbon 56 1 67 82 |