Paleomagnetism of Stony Meteorites
P(論文) The paleointensity for a howardite, an ulerite and three diogenites has been determined. By referring to these five values of paleointensity, the paleointensity for 6 achondrites is determined by comparing their NRM with the saturation IRM (Fuller's method). The paleointensity (F_0) for a...
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| Language: | English |
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1979
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| Online Access: | https://nipr.repo.nii.ac.jp/record/1062/files/KJ00000011606.pdf |
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ftnipr:oai:nipr.repo.nii.ac.jp:00001062 |
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ftnipr:oai:nipr.repo.nii.ac.jp:00001062 2024-09-09T19:51:59+00:00 Paleomagnetism of Stony Meteorites Nagata, Takesi 1979-12 application/pdf https://nipr.repo.nii.ac.jp/record/1062/files/KJ00000011606.pdf eng eng Memoirs of National Institute of Polar Research. Special issue 15 280 293 AA00733561 https://nipr.repo.nii.ac.jp/record/1062/files/KJ00000011606.pdf 1979 ftnipr 2024-06-17T04:00:22Z P(論文) The paleointensity for a howardite, an ulerite and three diogenites has been determined. By referring to these five values of paleointensity, the paleointensity for 6 achondrites is determined by comparing their NRM with the saturation IRM (Fuller's method). The paleointensity (F_0) for achondrites thus determined is represented by F_0=(0.11±0.02) Oe. The paleointensity for Allende C_3-chondrite is examined from various standpoints. Four other C-chondrites having reasonably stable NRM also are paleomagnetically examined. The average paleointensity for the C-chondrites is F_0=(1.02±0.09) Oe. Ordinary chondrites have a less stable NRM so that the evaluated paleointensity for ordinary chondrites is less reliable. The paleointensity for comparatively stable ordinary chondrites ranges from 0.1 to 0.4 Oe. 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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ftnipr |
| language |
English |
| description |
P(論文) The paleointensity for a howardite, an ulerite and three diogenites has been determined. By referring to these five values of paleointensity, the paleointensity for 6 achondrites is determined by comparing their NRM with the saturation IRM (Fuller's method). The paleointensity (F_0) for achondrites thus determined is represented by F_0=(0.11±0.02) Oe. The paleointensity for Allende C_3-chondrite is examined from various standpoints. Four other C-chondrites having reasonably stable NRM also are paleomagnetically examined. The average paleointensity for the C-chondrites is F_0=(1.02±0.09) Oe. Ordinary chondrites have a less stable NRM so that the evaluated paleointensity for ordinary chondrites is less reliable. The paleointensity for comparatively stable ordinary chondrites ranges from 0.1 to 0.4 Oe. departmental bulletin paper |
| author |
Nagata, Takesi |
| spellingShingle |
Nagata, Takesi Paleomagnetism of Stony Meteorites |
| author_facet |
Nagata, Takesi |
| author_sort |
Nagata, Takesi |
| title |
Paleomagnetism of Stony Meteorites |
| title_short |
Paleomagnetism of Stony Meteorites |
| title_full |
Paleomagnetism of Stony Meteorites |
| title_fullStr |
Paleomagnetism of Stony Meteorites |
| title_full_unstemmed |
Paleomagnetism of Stony Meteorites |
| title_sort |
paleomagnetism of stony meteorites |
| publishDate |
1979 |
| url |
https://nipr.repo.nii.ac.jp/record/1062/files/KJ00000011606.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 15 280 293 AA00733561 https://nipr.repo.nii.ac.jp/record/1062/files/KJ00000011606.pdf |
| _version_ |
1809921349936742400 |