Paleomagnetic records of excursions and reversals: possible biases caused by magnetization artefacts
Sedimentary and volcanic records of the Mono Lake (27 ka), Laschamp (42 ka), Blake (128 ka) and Cobb Mountain (1.1 Ma) geomagnetic excursions/events have been selected to test the coherency of the records and the hypothesis of preferred longitudes followed by the virtual geomagnetic pole (VGP) durin...
Published in: | Physics of the Earth and Planetary Interiors |
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ftccsdartic:oai:HAL:hal-03991335v1 2023-05-15T16:19:40+02:00 Paleomagnetic records of excursions and reversals: possible biases caused by magnetization artefacts Quidelleur, Xavier Valet, Jean-Pierre Institut de Physique du Globe de Paris (IPG Paris) 1994-01 https://hal.science/hal-03991335 https://doi.org/10.1016/0031-9201(94)90100-7 en eng HAL CCSD Elsevier info:eu-repo/semantics/altIdentifier/doi/10.1016/0031-9201(94)90100-7 hal-03991335 https://hal.science/hal-03991335 doi:10.1016/0031-9201(94)90100-7 ISSN: 0031-9201 EISSN: 0031-9201 Physics of the Earth and Planetary Interiors https://hal.science/hal-03991335 Physics of the Earth and Planetary Interiors, 1994, 82 (1), pp.27-48. ⟨10.1016/0031-9201(94)90100-7⟩ [SDU]Sciences of the Universe [physics] info:eu-repo/semantics/article Journal articles 1994 ftccsdartic https://doi.org/10.1016/0031-9201(94)90100-7 2023-02-19T00:22:10Z Sedimentary and volcanic records of the Mono Lake (27 ka), Laschamp (42 ka), Blake (128 ka) and Cobb Mountain (1.1 Ma) geomagnetic excursions/events have been selected to test the coherency of the records and the hypothesis of preferred longitudes followed by the virtual geomagnetic pole (VGP) during transitional periods. The distribution of the mean VGP longitudes (MVLs) for each individual event is not consistent with any simple pattern. The entire data set, including a total of six excursions, shows no preference for longitudinal sectors. The databases, one including both reversal and excursion records and another which contains only reversals, show that most of the MVLs with low dispersion values are at 90° from their site longitudes, with the majority lying over two preferred antipodal sectors of longitude. The other MVLs (with high dispersion values) are distributed in longitude around the globe. These two databases also show that the MVLs which do not lie at 90° from the site longitude are scattered around the globe, whereas the others are confined within two preferential bands of longitude. It is thus suggested that observations of two preferred sectors of longitude are the consequence of artefacts possibly linked to the acquisition of magnetization in sediments. We show that a shallowing of inclinations close to the horizontal plane, induced by the dominance of gravity forces in the presence of a very weak field, is compatible with these observations. Article in Journal/Newspaper Geomagnetic Pole Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) Physics of the Earth and Planetary Interiors 82 1 27 48 |
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Open Polar |
collection |
Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) |
op_collection_id |
ftccsdartic |
language |
English |
topic |
[SDU]Sciences of the Universe [physics] |
spellingShingle |
[SDU]Sciences of the Universe [physics] Quidelleur, Xavier Valet, Jean-Pierre Paleomagnetic records of excursions and reversals: possible biases caused by magnetization artefacts |
topic_facet |
[SDU]Sciences of the Universe [physics] |
description |
Sedimentary and volcanic records of the Mono Lake (27 ka), Laschamp (42 ka), Blake (128 ka) and Cobb Mountain (1.1 Ma) geomagnetic excursions/events have been selected to test the coherency of the records and the hypothesis of preferred longitudes followed by the virtual geomagnetic pole (VGP) during transitional periods. The distribution of the mean VGP longitudes (MVLs) for each individual event is not consistent with any simple pattern. The entire data set, including a total of six excursions, shows no preference for longitudinal sectors. The databases, one including both reversal and excursion records and another which contains only reversals, show that most of the MVLs with low dispersion values are at 90° from their site longitudes, with the majority lying over two preferred antipodal sectors of longitude. The other MVLs (with high dispersion values) are distributed in longitude around the globe. These two databases also show that the MVLs which do not lie at 90° from the site longitude are scattered around the globe, whereas the others are confined within two preferential bands of longitude. It is thus suggested that observations of two preferred sectors of longitude are the consequence of artefacts possibly linked to the acquisition of magnetization in sediments. We show that a shallowing of inclinations close to the horizontal plane, induced by the dominance of gravity forces in the presence of a very weak field, is compatible with these observations. |
author2 |
Institut de Physique du Globe de Paris (IPG Paris) |
format |
Article in Journal/Newspaper |
author |
Quidelleur, Xavier Valet, Jean-Pierre |
author_facet |
Quidelleur, Xavier Valet, Jean-Pierre |
author_sort |
Quidelleur, Xavier |
title |
Paleomagnetic records of excursions and reversals: possible biases caused by magnetization artefacts |
title_short |
Paleomagnetic records of excursions and reversals: possible biases caused by magnetization artefacts |
title_full |
Paleomagnetic records of excursions and reversals: possible biases caused by magnetization artefacts |
title_fullStr |
Paleomagnetic records of excursions and reversals: possible biases caused by magnetization artefacts |
title_full_unstemmed |
Paleomagnetic records of excursions and reversals: possible biases caused by magnetization artefacts |
title_sort |
paleomagnetic records of excursions and reversals: possible biases caused by magnetization artefacts |
publisher |
HAL CCSD |
publishDate |
1994 |
url |
https://hal.science/hal-03991335 https://doi.org/10.1016/0031-9201(94)90100-7 |
genre |
Geomagnetic Pole |
genre_facet |
Geomagnetic Pole |
op_source |
ISSN: 0031-9201 EISSN: 0031-9201 Physics of the Earth and Planetary Interiors https://hal.science/hal-03991335 Physics of the Earth and Planetary Interiors, 1994, 82 (1), pp.27-48. ⟨10.1016/0031-9201(94)90100-7⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/doi/10.1016/0031-9201(94)90100-7 hal-03991335 https://hal.science/hal-03991335 doi:10.1016/0031-9201(94)90100-7 |
op_doi |
https://doi.org/10.1016/0031-9201(94)90100-7 |
container_title |
Physics of the Earth and Planetary Interiors |
container_volume |
82 |
container_issue |
1 |
container_start_page |
27 |
op_container_end_page |
48 |
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1766006072470929408 |