2025/06/09 更新

写真a

ザン ヨーユエ
張 友悦
Zhang Youyue
所属
先端研究院 地球深部ダイナミクス研究センター 助教
職名
助教
連絡先
メールアドレス
外部リンク

学位

  • 地球惑星物質科学専攻 博士(学術) ( 2022年3月   岡山大学 )

研究キーワード

  • 高圧実験

  • 惑星熱進化

研究分野

  • 自然科学一般 / 固体地球科学  / 高圧地球惑星科学

学歴

  • 岡山大学   地球惑星物質科学専攻

    2016年9月 - 2022年3月

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  • 中国科学技術大学   地球と空間科学学院

    2012年9月 - 2016年6月

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    国名: 中華人民共和国

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経歴

  • 愛媛大学   先端研究院 地球深部ダイナミクス研究センター   助教

    2025年1月 - 現在

  • 愛媛大学   地球深部ダイナミクス研究センター   研究員

    2024年1月 - 2024年12月

  • 岡山大学   惑星物質研究所   助教

    2023年4月 - 2023年12月

  • 岡山大学   惑星物質研究所   日本学術振興会特別研究員

    2022年4月 - 2023年3月

論文

  • Effect of water on seismic attenuation of the upper mantle: The origin of the sharp lithosphere–asthenosphere boundary

    Chao Liu, Takashi Yoshino, Daisuke Yamazaki, Noriyoshi Tsujino, Hitoshi Gomi, Moe Sakurai, Youyue Zhang, Ran Wang, Longli Guan, Kayan Lau, Yoshinori Tange, Yuji Higo

    Proceedings of the National Academy of Sciences   120 ( 32 )   2023年7月

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    掲載種別:研究論文(学術雑誌)   出版者・発行元:Proceedings of the National Academy of Sciences  

    Oceanic lithosphere moves over a mechanically weak layer (asthenosphere) characterized by low seismic velocity and high attenuation. Near mid-ocean ridges, partial melting can produce such conditions because of the high-temperature geotherm. However, seismic observations have also shown a large and sharp velocity reduction under oceanic plates at the lithosphere–asthenosphere boundary (LAB) far from mid-ocean ridges. Here, we report the effect of water on the seismic properties of olivine aggregates in water-undersaturated conditions at 3 GPa and 1,223 to 1,373 K via in-situ X-ray observation using cyclic loading. Our results show that water substantially enhances the energy dispersion and reduces the elastic moduli over a wide range of seismic frequencies (0.5 to 1,000 s). An attenuation peak that appears at higher frequencies (1 to 5 s) becomes more pronounced as the water content increases. If water exists only in the asthenosphere, this is consistent with the observation that the attenuation in the asthenosphere is almost constant over a wide frequency range. These sharp seismic changes at the oceanic LAB far from mid-ocean ridges could be explained by the difference in water content between the lithosphere and asthenosphere.

    DOI: 10.1073/pnas.2221770120

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  • Effect of Iron Content on Thermal Conductivity of Ferropericlase: Implications for Planetary Mantle Dynamics 査読

    Youyue Zhang, Takashi Yoshino, Masahiro Osako

    Geophysical Research Letters   50 ( 7 )   2023年3月

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    担当区分:筆頭著者, 責任著者   掲載種別:研究論文(学術雑誌)   出版者・発行元:American Geophysical Union (AGU)  

    DOI: 10.1029/2022gl101769

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  • High-pressure experimental study of tetragonal CaSiO3-perovskite to 200 GPa 査読

    Ningyu Sun, Hui Bian, Youyue Zhang, Jung-Fu Lin, Vitali B. Prakapenka, Zhu Mao

    American Mineralogist   107 ( 1 )   110 - 115   2022年1月

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    掲載種別:研究論文(学術雑誌)   出版者・発行元:Mineralogical Society of America  

    Abstract

    In this study, we have investigated the crystal structure and equation of state of tetragonal CaSiO3-perovskite up to 200 GPa using synchrotron X-ray diffraction in laser-heated diamond-anvil cells. X-ray diffraction patterns of the quenched CaSiO3-perovskite above 148 GPa clearly show that 200, 211, and 220 peaks of the cubic phase split into 004+220, 204+312, and 224+400 peak pairs, respectively, in the tetragonal structure, and their calculated full-width at half maximum (FWHM) exhibits a substantial increase with pressure. The distribution of diffraction peaks suggests that the tetragonal CaSiO3-perovskite most likely has an I4/mcm space group at 300 K between 148 and 199 GPa, although other possibilities might still exist. Using the Birch-Murnaghan equations, we have determined the equation of state of tetragonal CaSiO3-perovskite, yielding the bulk modulus K0T = 227(21) GPa with the pressure derivative of the bulk modulus, K0T′ = 4.0(3). Modeled sound velocities at 580 K and around 50 GPa using our results and literature values show the difference in the compressional (VP) and shear-wave velocity (VS) between the tetragonal and cubic phases to be 5.3 and 6.7%, respectively. At ~110 GPa and 1000 K, this phase transition leads to a 4.3 and 9.1% jump in VP and VS, respectively. Since the addition of Ti can elevate the transition temperature, the transition from the tetragonal to cubic phase may have a seismic signature compatible with the observed mid-lower mantle discontinuity around the cold subduction slabs, which needs to be explored in future studies.

    DOI: 10.2138/am-2021-7913

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  • Exploration of the best reference material on anelastic measurement by cyclic loading under high pressure 査読

    Chao Liu, Takashi Yoshino, Daisuke Yamazaki, Noriyoshi Tsujino, Hitoshi Gomi, Moe Sakurai, Youyue Zhang, Ran Wang, Longli Guan, Kayan Lau, Yoshinori Tange, Yuji Higo

    High Pressure Research   42 ( 1 )   14 - 28   2022年1月

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    記述言語:英語   掲載種別:研究論文(学術雑誌)   出版者・発行元:Informa UK Limited  

    Anelastic measurement by cyclic loading under high pressure has been developed by means of in situ X-ray observation at a synchrotron facility. In this method, the reference material is a key factor to precisely determine attenuation and moduli of unknown materials. We compared the performance of three types of reference materials (dense polycrystalline alumina, alumina single-crystal parallel to c-axis, and flexible graphite) under the pressure of 3 GPa and the temperature range between 1173 and 1373 K. The phase lags of strain between reference materials and samples show that the flexible graphite is less attenuated than dense polycrystalline alumina and alumina single crystal in various periods. The strain ratios show that the flexible graphite is much softer and can produce the measurable strain in the limited displacement. The flexible graphite, as reference material, is more excellent to detect the relatively lower energy dispersion of mantle minerals at high pressure.

    DOI: 10.1080/08957959.2021.2013834

    Web of Science

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  • Effect of iron content on thermal conductivity of olivine with implications for cooling history of rocky planets 査読

    Youyue Zhang, Takashi Yoshino, Akira Yoneda, Masahiro Osako

    Earth and Planetary Science Letters   519   109 - 119   2019年8月

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    担当区分:筆頭著者, 責任著者   掲載種別:研究論文(学術雑誌)   出版者・発行元:Elsevier BV  

    DOI: 10.1016/j.epsl.2019.04.048

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  • High-pressure generation in the Kawai-type multianvil apparatus equipped with tungsten-carbide anvils and sintered-diamond anvils, and X-ray observation on CaSnO3 and (Mg,Fe)SiO3 査読

    Daisuke Yamazaki, Eiji Ito, Takashi Yoshino, Noriyoshi Tsujino, Akira Yoneda, Hitoshi Gomi, Jaseem Vazhakuttiyakam, Moe Sakurai, Youyue Zhang, Yuji Higo, Yoshinori Tange

    Comptes Rendus Geoscience   351 ( 2-3 )   253 - 259   2019年2月

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    掲載種別:研究論文(学術雑誌)   出版者・発行元:Elsevier BV  

    DOI: 10.1016/j.crte.2018.07.004

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▼全件表示

講演・口頭発表等

  • Effect of iron on the lattice thermal conductivity of lower mantle minerals: implications for mantle dynamics 招待

    Youyue ZHANG, Takashi Yoshino, Masahiro Osako

    AGU Annual Meeting 2023  2023年12月 

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    開催年月日: 2023年12月

    記述言語:英語   会議種別:口頭発表(招待・特別)  

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  • 铁含量对铁方镁石热导率的影响与其对类地行星热进化及地幔动力学作用的探讨 招待

    張 友悦, 芳野 極, 大迫 正弘

    中国地球科学联合学术年会(CGU-2023)  2023年10月 

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    開催年月日: 2023年10月

    記述言語:中国語   会議種別:口頭発表(招待・特別)  

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共同研究・競争的資金等の研究課題

  • マントル遷移層とスラブの熱的特性に対する実験的制約:深発地震のメカニズムの解明

    2024年4月 - 2028年3月

    日本学術振興会  科学研究費助成事業  若手研究

    張 友悦

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    配分額:4680000円 ( 直接経費:3600000円 、 間接経費:1080000円 )

    マントル遷移層と沈み込むスラブの温度分布は、沈み込むスラブの相転移と浮力に強く影響し、さらに破壊挙動を制御し、深発地震の発生に影響を及ぼすと考えられている。本研究の目的は、川井型マルチアンビル高圧装置を用いて、パルス加熱法により、マントル遷移層と沈み込むスラブの主要相の圧力、温度、水分量に依存する熱伝導率と熱拡散率を現実の沈み込むスラブの条件で同時に測定することである。体系的な実験データに基づき、沈み込むスラブ内の温度プロファイルをシミュレートする。この研究により、マントル遷移層と沈み込むスラブの熱状態とダイナミクスが明らかになり、深発地震のメカニズム解明に新たな知見を与える。

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    CiNii Research

  • 惑星深部物質の熱伝導率に対する水と化学不純物の影響:地球型惑星の熱進化の探求

    2021年4月 - 2023年3月

    日本学術振興会  科学研究費助成事業  特別研究員奨励費

    Zhang Youyue

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    配分額:1500000円 ( 直接経費:1500000円 )

    The generation of observed magnetic field, surface geological activities and temperature distribution are all largely controlled by the core mantle boundary heat flux, which is governed by the heat transport properties of the lowermost mantle minerals. Accurate thermal conductivity values of exact compositions of planet-forming minerals are essential for good models of terrestrial planets, providing insights of thermal evolutions of these planets and helping us understand why the Earth is the only active and habitable terrestrial planet nowadays.
    The purpose of this study is to understand how impurities in minerals affect the thermal evolution of terrestrial planets and to achieve the following projects: (1) Determination of pressure dependence and temperature dependence of thermal conductivity of (Fe,Al)-bearing bridgmanite with different iron, aluminum content by pulse heating method. (2) Determination of pressure dependence and temperature dependence of thermal conductivity of anhydrous and hydrous Fe-rich ringwoodite by pulse heating method. In this fiscal year, we accomplished project (1). Simultaneous measurements of thermal conductivity and thermal diffusivity of post-spinel and bridgmanite with 5 different compositions were performed under high pressure up to 24 GPa. At 24 GPa, temperature dependence data were taken up to 1100 K. Based on present data, impurity effects on thermal properties of bridgmanite and its influence on slab dynamics and cooling history of terrestrial planets were identified.

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担当授業科目(学内)