How did the dipole axis vary during the first millennium BCE? New data from West Europe and analysis of the directional global database

International audience Despite progress in the knowledge of secular variation during the first millennium BCE in Europe, data coverage remains poor at the earliest periods, especially in some regions as in the Central Mediterranean area. This study presents three new directional and six new intensit...

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Published in:Physics of the Earth and Planetary Interiors
Main Authors: Hervé, Gwenaël, Chauvin, Annick, Lanos, Philippe, Lhuillier, Florian, Boulud-Gazo, Sylvie, Denti, Mario, Macario, Raphaël
Other Authors: IRAMAT-Centre de recherche en physique appliquée à l’archéologie (IRAMAT-CRP2A), Institut de Recherches sur les Archéomatériaux (IRAMAT), Université de Technologie de Belfort-Montbeliard (UTBM)-Université d'Orléans (UO)-Université Bordeaux Montaigne (UBM)-Centre National de la Recherche Scientifique (CNRS)-Université de Technologie de Belfort-Montbeliard (UTBM)-Université d'Orléans (UO)-Université Bordeaux Montaigne (UBM)-Centre National de la Recherche Scientifique (CNRS), Laboratoire des Sciences du Climat et de l'Environnement Gif-sur-Yvette (LSCE), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Climat et Magnétisme (CLIMAG), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Géosciences Rennes (GR), Université de Rennes (UR)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Rennes (OSUR), Université de Rennes (UR)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Rennes 2 (UR2)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Rennes 2 (UR2)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Centre National de la Recherche Scientifique (CNRS), Ludwig Maximilian University Munich = Ludwig Maximilians Universität München (LMU), Université de Nantes (UN), Centre de Recherche en Archéologie, Archéosciences, Histoire (CReAAH), Le Mans Université (UM)-Université de Rennes (UR)-Université de Rennes 2 (UR2)-Centre National de la Recherche Scientifique (CNRS)-Université de Nantes - UFR Histoire, Histoire de l'Art et Archéologie (UFR HHAA), Université de Nantes (UN)-Université de Nantes (UN)-Ministère de la Culture (MC), Université de Rennes 2 (UR2), Hadès - Bureau d'Investigations Archéologiques, German Research Foundation (DFG) HE7343/1-1, Campus France PRESTIGE program PRESTIGE-2017-1-0002, ANR-15-CE31-0011,SVPIntMex,Variation séculaire et Paléointensité au Mexique pendant le Plio-Quaternaire(2015), ANR-10-LABX-0052,LaScArBx,Using the world in ancient societies : processes and forms of appropriation of space in Long Time(2010)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2021
Subjects:
Online Access:https://insu.hal.science/insu-03203983
https://insu.hal.science/insu-03203983v2/document
https://insu.hal.science/insu-03203983v2/file/Herv%C3%A9%20et%20al.%20-%202021%20-%20How%20did%20the%20dipole%20axis%20vary%20during%20the%20first%20mill.pdf
https://doi.org/10.1016/j.pepi.2021.106712
id ftunivorleans:oai:HAL:insu-03203983v2
record_format openpolar
institution Open Polar
collection Université d'Orléans: HAL
op_collection_id ftunivorleans
language English
topic Archaeomagnetism
Archaeointensity
Geomagnetic secular variation
First millennium BCE
[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]
spellingShingle Archaeomagnetism
Archaeointensity
Geomagnetic secular variation
First millennium BCE
[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]
Hervé, Gwenaël
Chauvin, Annick
Lanos, Philippe
Lhuillier, Florian
Boulud-Gazo, Sylvie
Denti, Mario
Macario, Raphaël
How did the dipole axis vary during the first millennium BCE? New data from West Europe and analysis of the directional global database
topic_facet Archaeomagnetism
Archaeointensity
Geomagnetic secular variation
First millennium BCE
[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]
description International audience Despite progress in the knowledge of secular variation during the first millennium BCE in Europe, data coverage remains poor at the earliest periods, especially in some regions as in the Central Mediterranean area. This study presents three new directional and six new intensity data between the 13th and the 4th centuries BCE on archaeological kilns, pottery and baked clay fragments from South Italy and France. Archaeodirections were determined after thermal demagnetizations and archaeointensities using the Thellier-Thellier protocol with corrections for the anisotropy and cooling rate effects. The new data confirm the large deviation of the direction from a Geocentric Axial Dipole field, the high geomagnetic field strength and the fast secular variation observed in Europe during the earliest half of the first millennium BCE. Another characteristic of this period is a difference of ~25° between the longitudes of the virtual geomagnetic poles inferred from European and Middle East data. This unusual behaviour can be mainly related to the Levantine Iron Age anomaly (LIAA) and its expansion from the Middle East to Europe. However, the review of the global directional database shows that almost all virtual geomagnetic poles, 96% of them coming from Europe, the Middle East, East Asia, North America and Hawaii, are 10–25° away from the rotation axis towards North Russia between 1000 and 600 BCE. The calculation of a mean global VGP curve suggests that the North geomagnetic pole followed a clockwise motion during this period with a dipole tilt up to around 14°. This study shows that a dipole axis tilt may have played an important role in the rapid secular variation in western Eurasia, although part of this variation may also be related to non-dipole fields associated with the LIAA.
author2 IRAMAT-Centre de recherche en physique appliquée à l’archéologie (IRAMAT-CRP2A)
Institut de Recherches sur les Archéomatériaux (IRAMAT)
Université de Technologie de Belfort-Montbeliard (UTBM)-Université d'Orléans (UO)-Université Bordeaux Montaigne (UBM)-Centre National de la Recherche Scientifique (CNRS)-Université de Technologie de Belfort-Montbeliard (UTBM)-Université d'Orléans (UO)-Université Bordeaux Montaigne (UBM)-Centre National de la Recherche Scientifique (CNRS)
Laboratoire des Sciences du Climat et de l'Environnement Gif-sur-Yvette (LSCE)
Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Direction de Recherche Fondamentale (CEA) (DRF (CEA))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)
Climat et Magnétisme (CLIMAG)
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Direction de Recherche Fondamentale (CEA) (DRF (CEA))
Géosciences Rennes (GR)
Université de Rennes (UR)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Rennes (OSUR)
Université de Rennes (UR)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Rennes 2 (UR2)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Rennes 2 (UR2)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Centre National de la Recherche Scientifique (CNRS)
Ludwig Maximilian University Munich = Ludwig Maximilians Universität München (LMU)
Université de Nantes (UN)
Centre de Recherche en Archéologie, Archéosciences, Histoire (CReAAH)
Le Mans Université (UM)-Université de Rennes (UR)-Université de Rennes 2 (UR2)-Centre National de la Recherche Scientifique (CNRS)-Université de Nantes - UFR Histoire, Histoire de l'Art et Archéologie (UFR HHAA)
Université de Nantes (UN)-Université de Nantes (UN)-Ministère de la Culture (MC)
Université de Rennes 2 (UR2)
Hadès - Bureau d'Investigations Archéologiques
German Research Foundation (DFG) HE7343/1-1
Campus France PRESTIGE program PRESTIGE-2017-1-0002
ANR-15-CE31-0011,SVPIntMex,Variation séculaire et Paléointensité au Mexique pendant le Plio-Quaternaire(2015)
ANR-10-LABX-0052,LaScArBx,Using the world in ancient societies : processes and forms of appropriation of space in Long Time(2010)
format Article in Journal/Newspaper
author Hervé, Gwenaël
Chauvin, Annick
Lanos, Philippe
Lhuillier, Florian
Boulud-Gazo, Sylvie
Denti, Mario
Macario, Raphaël
author_facet Hervé, Gwenaël
Chauvin, Annick
Lanos, Philippe
Lhuillier, Florian
Boulud-Gazo, Sylvie
Denti, Mario
Macario, Raphaël
author_sort Hervé, Gwenaël
title How did the dipole axis vary during the first millennium BCE? New data from West Europe and analysis of the directional global database
title_short How did the dipole axis vary during the first millennium BCE? New data from West Europe and analysis of the directional global database
title_full How did the dipole axis vary during the first millennium BCE? New data from West Europe and analysis of the directional global database
title_fullStr How did the dipole axis vary during the first millennium BCE? New data from West Europe and analysis of the directional global database
title_full_unstemmed How did the dipole axis vary during the first millennium BCE? New data from West Europe and analysis of the directional global database
title_sort how did the dipole axis vary during the first millennium bce? new data from west europe and analysis of the directional global database
publisher HAL CCSD
publishDate 2021
url https://insu.hal.science/insu-03203983
https://insu.hal.science/insu-03203983v2/document
https://insu.hal.science/insu-03203983v2/file/Herv%C3%A9%20et%20al.%20-%202021%20-%20How%20did%20the%20dipole%20axis%20vary%20during%20the%20first%20mill.pdf
https://doi.org/10.1016/j.pepi.2021.106712
genre Geomagnetic Pole
genre_facet Geomagnetic Pole
op_source ISSN: 0031-9201
EISSN: 0031-9201
Physics of the Earth and Planetary Interiors
https://insu.hal.science/insu-03203983
Physics of the Earth and Planetary Interiors, 2021, 315, pp.106712. ⟨10.1016/j.pepi.2021.106712⟩
op_relation info:eu-repo/semantics/altIdentifier/doi/10.1016/j.pepi.2021.106712
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https://insu.hal.science/insu-03203983
https://insu.hal.science/insu-03203983v2/document
https://insu.hal.science/insu-03203983v2/file/Herv%C3%A9%20et%20al.%20-%202021%20-%20How%20did%20the%20dipole%20axis%20vary%20during%20the%20first%20mill.pdf
doi:10.1016/j.pepi.2021.106712
op_rights info:eu-repo/semantics/OpenAccess
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container_title Physics of the Earth and Planetary Interiors
container_volume 315
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spelling ftunivorleans:oai:HAL:insu-03203983v2 2024-09-15T18:07:27+00:00 How did the dipole axis vary during the first millennium BCE? New data from West Europe and analysis of the directional global database Hervé, Gwenaël Chauvin, Annick Lanos, Philippe Lhuillier, Florian Boulud-Gazo, Sylvie Denti, Mario Macario, Raphaël IRAMAT-Centre de recherche en physique appliquée à l’archéologie (IRAMAT-CRP2A) Institut de Recherches sur les Archéomatériaux (IRAMAT) Université de Technologie de Belfort-Montbeliard (UTBM)-Université d'Orléans (UO)-Université Bordeaux Montaigne (UBM)-Centre National de la Recherche Scientifique (CNRS)-Université de Technologie de Belfort-Montbeliard (UTBM)-Université d'Orléans (UO)-Université Bordeaux Montaigne (UBM)-Centre National de la Recherche Scientifique (CNRS) Laboratoire des Sciences du Climat et de l'Environnement Gif-sur-Yvette (LSCE) Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)) Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA) Climat et Magnétisme (CLIMAG) Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)) Géosciences Rennes (GR) Université de Rennes (UR)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Rennes (OSUR) Université de Rennes (UR)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Rennes 2 (UR2)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Rennes 2 (UR2)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Centre National de la Recherche Scientifique (CNRS) Ludwig Maximilian University Munich = Ludwig Maximilians Universität München (LMU) Université de Nantes (UN) Centre de Recherche en Archéologie, Archéosciences, Histoire (CReAAH) Le Mans Université (UM)-Université de Rennes (UR)-Université de Rennes 2 (UR2)-Centre National de la Recherche Scientifique (CNRS)-Université de Nantes - UFR Histoire, Histoire de l'Art et Archéologie (UFR HHAA) Université de Nantes (UN)-Université de Nantes (UN)-Ministère de la Culture (MC) Université de Rennes 2 (UR2) Hadès - Bureau d'Investigations Archéologiques German Research Foundation (DFG) HE7343/1-1 Campus France PRESTIGE program PRESTIGE-2017-1-0002 ANR-15-CE31-0011,SVPIntMex,Variation séculaire et Paléointensité au Mexique pendant le Plio-Quaternaire(2015) ANR-10-LABX-0052,LaScArBx,Using the world in ancient societies : processes and forms of appropriation of space in Long Time(2010) 2021-04 https://insu.hal.science/insu-03203983 https://insu.hal.science/insu-03203983v2/document https://insu.hal.science/insu-03203983v2/file/Herv%C3%A9%20et%20al.%20-%202021%20-%20How%20did%20the%20dipole%20axis%20vary%20during%20the%20first%20mill.pdf https://doi.org/10.1016/j.pepi.2021.106712 en eng HAL CCSD Elsevier info:eu-repo/semantics/altIdentifier/doi/10.1016/j.pepi.2021.106712 insu-03203983 https://insu.hal.science/insu-03203983 https://insu.hal.science/insu-03203983v2/document https://insu.hal.science/insu-03203983v2/file/Herv%C3%A9%20et%20al.%20-%202021%20-%20How%20did%20the%20dipole%20axis%20vary%20during%20the%20first%20mill.pdf doi:10.1016/j.pepi.2021.106712 info:eu-repo/semantics/OpenAccess ISSN: 0031-9201 EISSN: 0031-9201 Physics of the Earth and Planetary Interiors https://insu.hal.science/insu-03203983 Physics of the Earth and Planetary Interiors, 2021, 315, pp.106712. ⟨10.1016/j.pepi.2021.106712⟩ Archaeomagnetism Archaeointensity Geomagnetic secular variation First millennium BCE [SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph] info:eu-repo/semantics/article Journal articles 2021 ftunivorleans https://doi.org/10.1016/j.pepi.2021.106712 2024-07-22T23:39:59Z International audience Despite progress in the knowledge of secular variation during the first millennium BCE in Europe, data coverage remains poor at the earliest periods, especially in some regions as in the Central Mediterranean area. This study presents three new directional and six new intensity data between the 13th and the 4th centuries BCE on archaeological kilns, pottery and baked clay fragments from South Italy and France. Archaeodirections were determined after thermal demagnetizations and archaeointensities using the Thellier-Thellier protocol with corrections for the anisotropy and cooling rate effects. The new data confirm the large deviation of the direction from a Geocentric Axial Dipole field, the high geomagnetic field strength and the fast secular variation observed in Europe during the earliest half of the first millennium BCE. Another characteristic of this period is a difference of ~25° between the longitudes of the virtual geomagnetic poles inferred from European and Middle East data. This unusual behaviour can be mainly related to the Levantine Iron Age anomaly (LIAA) and its expansion from the Middle East to Europe. However, the review of the global directional database shows that almost all virtual geomagnetic poles, 96% of them coming from Europe, the Middle East, East Asia, North America and Hawaii, are 10–25° away from the rotation axis towards North Russia between 1000 and 600 BCE. The calculation of a mean global VGP curve suggests that the North geomagnetic pole followed a clockwise motion during this period with a dipole tilt up to around 14°. This study shows that a dipole axis tilt may have played an important role in the rapid secular variation in western Eurasia, although part of this variation may also be related to non-dipole fields associated with the LIAA. Article in Journal/Newspaper Geomagnetic Pole Université d'Orléans: HAL Physics of the Earth and Planetary Interiors 315 106712