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Nondestructive characterization of Antarctic micrometeorites collected at the Dome Fuji Station by synchrotron radiation X-ray fluorescence analysis
https://doi.org/10.15094/00005984
https://doi.org/10.15094/00005984673cd306-7db8-4d57-8de2-495485d18a54
名前 / ファイル | ライセンス | アクション |
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KJ00000040976 (855.6 kB)
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Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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公開日 | 2000-03-01 | |||||
タイトル | ||||||
タイトル | Nondestructive characterization of Antarctic micrometeorites collected at the Dome Fuji Station by synchrotron radiation X-ray fluorescence analysis | |||||
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 | |||||
ID登録 | ||||||
ID登録 | 10.15094/00005984 | |||||
ID登録タイプ | JaLC | |||||
ページ属性 | ||||||
内容記述タイプ | Other | |||||
内容記述 | P(論文) | |||||
著者名(英) |
Nakai,Izumi
× Nakai,Izumi× Kondo,Nahoko× Itabashi,Masato× Sasaki,Miho× Terada,Yasuko× Terada,Kentaro× Noguchi ,Takaaki× Nakamura, Tomoki |
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著者所属(英) | ||||||
en | ||||||
Department of Applied Chemistry, Faculty of Science, Science University of Tokyo/Department of Applied Chemistry, Faculty of Science, Science University of Tokyo/Department of Applied Chemistry, Faculty of Science, Science University of Tokyo/Department of Applied Chemistry, Faculty of Science, Science University of Tokyo/Department of Applied Chemistry, Faculty of Science, Science University of Tokyo/Department of Earth and Planetary System Science, Faculty of Science, Hiroshima University/Department of Materials and Biological Science, Ibaraki University/Department of Earth and Planetary Science, Graduate School of Science, Kyushu University | ||||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The bulk trace element composition (Ca, Ti, Cr, Mn, Ni Cu, Zn, Ge, Se, Rb, Sr, Y, Zr, Mo) of eighty-three Antarctic micrometeorites was nondestructively analyzed using synchrotron radiation X-ray fluorescence analysis (SR-XRF), and these elements were characterized in terms of their abundance ratio relative to Murchison matrix composition. The relationship between heating history and chemical composition is also examined. We found a complementary relationship among I-type, S-type and unmelted AMMs in the micrometeorites' elemental abundance, which is consistent with the hypothesis that I-type and S-type spherules were separated from chondritic meteoroids. | |||||
雑誌書誌ID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA11182426 | |||||
書誌情報 |
Antarctic meteorite research 巻 13, p. 302-310, 発行日 2000-03 |
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出版者 | ||||||
出版者 | National Institute of Polar Research |