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Magnetic Characteristics of Some Yamato Meteorites─Magnetic Classification of Stone Meteorites─
https://nipr.repo.nii.ac.jp/records/590
https://nipr.repo.nii.ac.jp/records/5902bf16ca0-1181-455f-b010-20a8daae5496
名前 / ファイル | ライセンス | アクション |
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KJ00000011278 (3.9 MB)
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Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||||||
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公開日 | 1976-12-01 | |||||||||
タイトル | ||||||||||
言語 | en | |||||||||
タイトル | Magnetic Characteristics of Some Yamato Meteorites─Magnetic Classification of Stone Meteorites─ | |||||||||
言語 | ||||||||||
言語 | eng | |||||||||
資源タイプ | ||||||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||||||
資源タイプ | departmental bulletin paper | |||||||||
ページ属性 | ||||||||||
内容記述タイプ | Other | |||||||||
内容記述 | P(論文) | |||||||||
著者名(英) |
Nagata, Takesi
× Nagata, Takesi
× Sugiura, Naoji
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著者所属(英) | ||||||||||
en | ||||||||||
National Institute of Polar Research | ||||||||||
著者所属(英) | ||||||||||
en | ||||||||||
Geophysical Institute, University of Tokyo | ||||||||||
抄録(英) | ||||||||||
内容記述タイプ | Other | |||||||||
内容記述 | 13 Yamato stone meteorites have been magnetically examined. They are one enstatite chondrite (E), 6 olivine-bronzite chondrites (H), 2 olivine-hypersthene chondrites (L), one carbonaceous chondrite (C) and 3 achondrites (aC). The intrinsic magnetic parameters of these stone meteorites obtained from their magnetic hysteresis curves and thermomagnetic curves, together with those of other 7 known chondritic meteorites, are specifically examined in terms of the compositional and petrographical classification of stone meteorites. The saturation magnetization (I_s) and major magnetic transition temperature (Θ_c) in the cooling process can be taken as the representative magnetic parameters in the proposed magnetic classification of stone meteorites. In the I_s versus Θ_c diagram, those examined stone meteorites, 25 in total, are separated into groups ; namely, I_s (E) > I_s (H) > I_s (L) > I_s (aC), Θ_c (H and L) < Θ_c (E and aC) ≃ 770℃, I_s (C) ≃ I_s (L) but Θ_c (C) < 600℃ < Θ_c (L). Although the boundary between the L-group and the H-group is not sharp enough in the I_s-Θ_c diagram, the L-group chondrites contain a distinctly larger amount of plessite phase which can be magnetically identified. | |||||||||
雑誌書誌ID | ||||||||||
収録物識別子タイプ | NCID | |||||||||
収録物識別子 | AA00733470 | |||||||||
書誌情報 |
Memoirs of National Institute of Polar Research. Ser. C, Earth sciences 巻 10, p. 30-58, 発行日 1976-12 |