Magnetic classification of meteorites (V) : Iron meteorites
P(論文) Sixteen iron meteorites are magnetically classified into three major classes; hexahedrite plus Ni-poor ataxite, octahedrite and Ni-rich ataxite on the basis of their thermomagnetic characteristics. Magnetic parameters for the classification scheme are ratio of saturation magnetization of kamac...
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ftnipr:oai:nipr.repo.nii.ac.jp:00001392 2024-09-09T19:51:58+00:00 Magnetic classification of meteorites (V) : Iron meteorites Nagata, Takesi 1982-12 application/pdf https://nipr.repo.nii.ac.jp/record/1392/files/KJ00000012026.pdf eng eng Memoirs of National Institute of Polar Research. Special issue 25 216 221 AA00733561 https://nipr.repo.nii.ac.jp/record/1392/files/KJ00000012026.pdf 1982 ftnipr 2024-06-17T04:00:33Z P(論文) Sixteen iron meteorites are magnetically classified into three major classes; hexahedrite plus Ni-poor ataxite, octahedrite and Ni-rich ataxite on the basis of their thermomagnetic characteristics. Magnetic parameters for the classification scheme are ratio of saturation magnetization of kamacite, I_s(α), to total saturation magnetization, I_s, namely I_s(α)/I_s, and transition temperature from γ-phase to α-phase of kamacite in the cooling process, Θ^*_<γ→α>. On an I_s(α)/I_s vs. Θ^*_<γ→α> diagram, the three major classes of iron meteorites are represented by their respective domains well separated from one another. departmental bulletin paper Other/Unknown Material Memoirs of National Institute of Polar Research Polar Research National Institute of Polar Research Repository, Japan |
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Open Polar |
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National Institute of Polar Research Repository, Japan |
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language |
English |
description |
P(論文) Sixteen iron meteorites are magnetically classified into three major classes; hexahedrite plus Ni-poor ataxite, octahedrite and Ni-rich ataxite on the basis of their thermomagnetic characteristics. Magnetic parameters for the classification scheme are ratio of saturation magnetization of kamacite, I_s(α), to total saturation magnetization, I_s, namely I_s(α)/I_s, and transition temperature from γ-phase to α-phase of kamacite in the cooling process, Θ^*_<γ→α>. On an I_s(α)/I_s vs. Θ^*_<γ→α> diagram, the three major classes of iron meteorites are represented by their respective domains well separated from one another. departmental bulletin paper |
author |
Nagata, Takesi |
spellingShingle |
Nagata, Takesi Magnetic classification of meteorites (V) : Iron meteorites |
author_facet |
Nagata, Takesi |
author_sort |
Nagata, Takesi |
title |
Magnetic classification of meteorites (V) : Iron meteorites |
title_short |
Magnetic classification of meteorites (V) : Iron meteorites |
title_full |
Magnetic classification of meteorites (V) : Iron meteorites |
title_fullStr |
Magnetic classification of meteorites (V) : Iron meteorites |
title_full_unstemmed |
Magnetic classification of meteorites (V) : Iron meteorites |
title_sort |
magnetic classification of meteorites (v) : iron meteorites |
publishDate |
1982 |
url |
https://nipr.repo.nii.ac.jp/record/1392/files/KJ00000012026.pdf |
genre |
Memoirs of National Institute of Polar Research Polar Research |
genre_facet |
Memoirs of National Institute of Polar Research Polar Research |
op_relation |
Memoirs of National Institute of Polar Research. Special issue 25 216 221 AA00733561 https://nipr.repo.nii.ac.jp/record/1392/files/KJ00000012026.pdf |
_version_ |
1809921308661645312 |