Supplementary Notes on the Magnetic Classification of Stony Meteorites
P(論文) A magnetic classification of stony meteorites on the basis of their saturation magnetization (I_s) and their major magnetic transition temperature (Θ_c) in the cooling process is revised by making use of recently reported chemical and petrographic data. The average values of (I_s in emu/gm, Θ_...
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ftnipr:oai:nipr.repo.nii.ac.jp:00000893 2024-09-09T19:51:58+00:00 Supplementary Notes on the Magnetic Classification of Stony Meteorites Nagata, Takesi 1978-02 application/pdf https://nipr.repo.nii.ac.jp/record/893/files/KJ00000011866.pdf eng eng Memoirs of National Institute of Polar Research. Special issue 8 233 239 AA00733561 https://nipr.repo.nii.ac.jp/record/893/files/KJ00000011866.pdf 1978 ftnipr 2024-06-17T04:04:30Z P(論文) A magnetic classification of stony meteorites on the basis of their saturation magnetization (I_s) and their major magnetic transition temperature (Θ_c) in the cooling process is revised by making use of recently reported chemical and petrographic data. The average values of (I_s in emu/gm, Θ_c in ℃) of enstatite chondrites (E), bronzite chondrites (H), hypersthene chondrites (L), carbonaceous chondrites (C) and achondrites (aC) are given by (48.0,764), (30.9,653), (12.5,656), (9.7,562) and (0.3,788) respectively. As either or both I_s and Θ_c values of each groups are distinctly separated from one another, stony meteorites can be classified reasonably well on the I_s∿Θ_c diagram. 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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National Institute of Polar Research Repository, Japan |
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English |
description |
P(論文) A magnetic classification of stony meteorites on the basis of their saturation magnetization (I_s) and their major magnetic transition temperature (Θ_c) in the cooling process is revised by making use of recently reported chemical and petrographic data. The average values of (I_s in emu/gm, Θ_c in ℃) of enstatite chondrites (E), bronzite chondrites (H), hypersthene chondrites (L), carbonaceous chondrites (C) and achondrites (aC) are given by (48.0,764), (30.9,653), (12.5,656), (9.7,562) and (0.3,788) respectively. As either or both I_s and Θ_c values of each groups are distinctly separated from one another, stony meteorites can be classified reasonably well on the I_s∿Θ_c diagram. departmental bulletin paper |
author |
Nagata, Takesi |
spellingShingle |
Nagata, Takesi Supplementary Notes on the Magnetic Classification of Stony Meteorites |
author_facet |
Nagata, Takesi |
author_sort |
Nagata, Takesi |
title |
Supplementary Notes on the Magnetic Classification of Stony Meteorites |
title_short |
Supplementary Notes on the Magnetic Classification of Stony Meteorites |
title_full |
Supplementary Notes on the Magnetic Classification of Stony Meteorites |
title_fullStr |
Supplementary Notes on the Magnetic Classification of Stony Meteorites |
title_full_unstemmed |
Supplementary Notes on the Magnetic Classification of Stony Meteorites |
title_sort |
supplementary notes on the magnetic classification of stony meteorites |
publishDate |
1978 |
url |
https://nipr.repo.nii.ac.jp/record/893/files/KJ00000011866.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 8 233 239 AA00733561 https://nipr.repo.nii.ac.jp/record/893/files/KJ00000011866.pdf |
_version_ |
1809921312800374784 |