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Evidence for a 3.45-billion-year-old magnetic remanence: Hints of an ancient geodynamo from conglomerates of South Africa
https://doi.org/10.24517/00067005
https://doi.org/10.24517/00067005eb9ec653-10a7-4e61-bcb5-7c7cfd97af20
名前 / ファイル | ライセンス | アクション |
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Item type | 学術雑誌論文 / Journal Article(1) | |||||||
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公開日 | 2022-09-01 | |||||||
タイトル | ||||||||
タイトル | Evidence for a 3.45-billion-year-old magnetic remanence: Hints of an ancient geodynamo from conglomerates of South Africa | |||||||
言語 | ||||||||
言語 | eng | |||||||
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資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||||
資源タイプ | journal article | |||||||
ID登録 | ||||||||
ID登録 | 10.24517/00067005 | |||||||
ID登録タイプ | JaLC | |||||||
著者 |
Usui, Yoichi
× Usui, Yoichi× Tarduno, John A.× Watkeys, Michael× Hofmann, Axel× Cottrell, Rory D. |
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著者別表示 |
臼井, 洋一
× 臼井, 洋一
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提供者所属 | ||||||||
内容記述タイプ | Other | |||||||
内容記述 | 金沢大学理工研究域地球社会基盤学系 | |||||||
書誌情報 |
Geochemistry, Geophysics, Geosystems 巻 10, 号 9, p. Q09Z07, 発行日 2009-09-24 |
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ISSN | ||||||||
収録物識別子タイプ | ISSN | |||||||
収録物識別子 | 1525-2027 | |||||||
DOI | ||||||||
関連タイプ | isIdenticalTo | |||||||
識別子タイプ | DOI | |||||||
関連識別子 | 10.1029/2009GC002496 | |||||||
出版者 | ||||||||
出版者 | American Geophysical Union, Geochemical Society / Wiley Open Access | |||||||
抄録 | ||||||||
内容記述タイプ | Abstract | |||||||
内容記述 | Paleomagnetic and rock magnetic analyses of ̃3445-million-year-old dacite conglomerate clasts and parent body rocks from the Barberton greenstone belt, South Africa, define two dominant components of magnetization. One component, unblocked at low temperature, is an overprint acquired ̃180 million years ago. The other component is unblocked at high temperatures and passes a conglomerate test, indicating that this component is older than the depositional age of the conglomerate (̃3416 Ma). The high unblocking temperature component shows scatter in the parent body rocks that can be explained by the effects of modern lightning strikes, Archean overprinting, and the presence of multidomain magnetic grains that are conducive to carrying secondary magnetizations. Alternatively, this scatter can be explained by exotic magnetization scenarios in the absence of a dynamo, including magnetization by an external field related to solar wind interaction with the atmosphere. Such exotic mechanisms can be tested with the acquisition of paleointensity data. While more scattered than paleomagnetic data recording the more recent geomagnetic field, the high unblocking temperature component in the dacite parent body shows some consistency, and the simplest explanation of the data is that they reflect a geodynamõ3445 million years ago. © 2009 by the American Geophysical Union. | |||||||
権利 | ||||||||
権利情報 | Copyright © 2009. American Geophysical Union. | |||||||
著者版フラグ | ||||||||
出版タイプ | VoR | |||||||
出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||||
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識別子タイプ | URI | |||||||
関連識別子 | https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2009GC002496 | |||||||
関連名称 | https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2009GC002496 | |||||||
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識別子タイプ | URI | |||||||
関連識別子 | https://agupubs.onlinelibrary.wiley.com/journal/15252027 | |||||||
関連名称 | https://agupubs.onlinelibrary.wiley.com/journal/15252027 | |||||||
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識別子タイプ | URI | |||||||
関連識別子 | http://sites.agu.org/ | |||||||
関連名称 | http://sites.agu.org/ | |||||||
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識別子タイプ | URI | |||||||
関連識別子 | https://authorservices.wiley.com/open-research/open-access/index.html | |||||||
関連名称 | https://authorservices.wiley.com/open-research/open-access/index.html |