Hugoniot equation of state of olivine and its geodynamic implications
Large olivine samples were hot-pressed synthesized for shock wave experiments. The shock wave experiments were carried out at pressure range between 11 and 42 GPa. Shock data on olivine sample yielded a linear relationship between shock wave velocity D and particle velocity u described by D=3.56（？0....
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| Veröffentlicht in: | Science China. Earth sciences 2016-03, Vol.59 (3), p.619-625 |
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| creator | Huang, XiaoGe Yuan, XianHao Chen, ZuAn Liu, FuSheng Bai, WuMing |
| description | Large olivine samples were hot-pressed synthesized for shock wave experiments. The shock wave experiments were carried out at pressure range between 11 and 42 GPa. Shock data on olivine sample yielded a linear relationship between shock wave velocity D and particle velocity u described by D=3.56（？0.13）＋2.57（？0.12）u. The shock temperature is determined by an energy relationship which is approximately 790°C at pressure 28 GPa. Due to low temperature and short experimental duration, we suggest that no phase change occurred in our sample below 30 GPa and olivine persisted well beyond its equilibrium boundary in metastable phase. The densities of metastable olivine are in agreement with the results of static compression. At the depth shallower than 410 km, the densities of metastable olivine are higher than those of the PREM model, facilitating cold slab to sink into the mantle transition zone. However, in entire mantle transition zone, the shock densities are lower than those of the PREM model, hampering cold slab to flow across the ＂660 km＂ phase boundary. |
| doi_str_mv | 10.1007/s11430-015-5231-2 |
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The shock wave experiments were carried out at pressure range between 11 and 42 GPa. Shock data on olivine sample yielded a linear relationship between shock wave velocity D and particle velocity u described by D=3.56（？0.13）＋2.57（？0.12）u. The shock temperature is determined by an energy relationship which is approximately 790°C at pressure 28 GPa. Due to low temperature and short experimental duration, we suggest that no phase change occurred in our sample below 30 GPa and olivine persisted well beyond its equilibrium boundary in metastable phase. The densities of metastable olivine are in agreement with the results of static compression. At the depth shallower than 410 km, the densities of metastable olivine are higher than those of the PREM model, facilitating cold slab to sink into the mantle transition zone. However, in entire mantle transition zone, the shock densities are lower than those of the PREM model, hampering cold slab to flow across the ＂660 km＂ phase boundary.</description><identifier>ISSN: 1674-7313</identifier><identifier>EISSN: 1869-1897</identifier><identifier>DOI: 10.1007/s11430-015-5231-2</identifier><language>eng</language><publisher>Beijing: Science China Press</publisher><subject>Earth and Environmental Science ; Earth Sciences ; Experiments ; Hugoniot ; Low temperature ; PREM模型 ; Research Paper ; Shock waves ; Temperature ; Transition zone ; Wave velocity ; 冲击波试验 ; 冲击波速度 ; 动力学意义 ; 地幔过渡带 ; 橄榄石 ; 状态方程</subject><ispartof>Science China. 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Earth sciences</title><addtitle>Sci. China Earth Sci</addtitle><addtitle>SCIENCE CHINA Earth Sciences</addtitle><description>Large olivine samples were hot-pressed synthesized for shock wave experiments. The shock wave experiments were carried out at pressure range between 11 and 42 GPa. Shock data on olivine sample yielded a linear relationship between shock wave velocity D and particle velocity u described by D=3.56（？0.13）＋2.57（？0.12）u. The shock temperature is determined by an energy relationship which is approximately 790°C at pressure 28 GPa. Due to low temperature and short experimental duration, we suggest that no phase change occurred in our sample below 30 GPa and olivine persisted well beyond its equilibrium boundary in metastable phase. The densities of metastable olivine are in agreement with the results of static compression. At the depth shallower than 410 km, the densities of metastable olivine are higher than those of the PREM model, facilitating cold slab to sink into the mantle transition zone. However, in entire mantle transition zone, the shock densities are lower than those of the PREM model, hampering cold slab to flow across the ＂660 km＂ phase boundary.</description><subject>Earth and Environmental Science</subject><subject>Earth Sciences</subject><subject>Experiments</subject><subject>Hugoniot</subject><subject>Low temperature</subject><subject>PREM模型</subject><subject>Research Paper</subject><subject>Shock waves</subject><subject>Temperature</subject><subject>Transition zone</subject><subject>Wave velocity</subject><subject>冲击波试验</subject><subject>冲击波速度</subject><subject>动力学意义</subject><subject>地幔过渡带</subject><subject>橄榄石</subject><subject>状态方程</subject><issn>1674-7313</issn><issn>1869-1897</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><recordid>eNp9kE1LxDAQhosoKLo_wFvRi5fqTL57FPELBC96DiVJa5Y22W1awX9v1oqIB-cyA3memfAWxSnCJQLIq4TIKFSAvOKEYkX2iiNUoq5Q1XI_z0KySlKkh8UqpTXkovmFyKPi9mHuYvBxKt12biYfQxnbMk3N5HZD7P27D65sgi39lMrORfsRmsGb0g-b3psvJZ0UB23TJ7f67sfF693ty81D9fR8_3hz_VQZxsRUudoabMExYrk1inBg1jIuDRBhgZvayBpqVFaiYApQctWKFi21CJaBosfFxbJ3M8bt7NKkB5-M6_smuDgnjVIKIThDkdHzP-g6zmPIv9tRSIFRXmcKF8qMMaXRtXoz-qEZPzSC3mWrl2x1zlbvstUkO2RxUmZD58Zfm_-Rzr4PvcXQbbP3c0kIhSA5UfQTfoiFbw</recordid><startdate>20160301</startdate><enddate>20160301</enddate><creator>Huang, XiaoGe</creator><creator>Yuan, XianHao</creator><creator>Chen, ZuAn</creator><creator>Liu, FuSheng</creator><creator>Bai, WuMing</creator><general>Science China Press</general><general>Springer Nature B.V</general><scope>2RA</scope><scope>92L</scope><scope>CQIGP</scope><scope>~WA</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7TG</scope><scope>7UA</scope><scope>7XB</scope><scope>88I</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>C1K</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>F1W</scope><scope>GNUQQ</scope><scope>H96</scope><scope>HCIFZ</scope><scope>KL.</scope><scope>L.G</scope><scope>M2P</scope><scope>PCBAR</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>Q9U</scope></search><sort><creationdate>20160301</creationdate><title>Hugoniot equation of state of olivine and its geodynamic implications</title><author>Huang, XiaoGe ; Yuan, XianHao ; Chen, ZuAn ; Liu, FuSheng ; Bai, WuMing</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c446t-e9dc1f0e42d5dc82504dd457c026d05c9c790918d7164801758f6f1d3d10d4083</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>Earth and Environmental Science</topic><topic>Earth Sciences</topic><topic>Experiments</topic><topic>Hugoniot</topic><topic>Low temperature</topic><topic>PREM模型</topic><topic>Research Paper</topic><topic>Shock waves</topic><topic>Temperature</topic><topic>Transition zone</topic><topic>Wave velocity</topic><topic>冲击波试验</topic><topic>冲击波速度</topic><topic>动力学意义</topic><topic>地幔过渡带</topic><topic>橄榄石</topic><topic>状态方程</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Huang, XiaoGe</creatorcontrib><creatorcontrib>Yuan, XianHao</creatorcontrib><creatorcontrib>Chen, ZuAn</creatorcontrib><creatorcontrib>Liu, FuSheng</creatorcontrib><creatorcontrib>Bai, WuMing</creatorcontrib><collection>中文科技期刊数据库</collection><collection>中文科技期刊数据库-CALIS站点</collection><collection>中文科技期刊数据库-7.0平台</collection><collection>中文科技期刊数据库- 镜像站点</collection><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Water Resources Abstracts</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest One Sustainability</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Natural Science Collection</collection><collection>Earth, Atmospheric & Aquatic Science Collection</collection><collection>Environmental Sciences and Pollution Management</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>ProQuest Central Student</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>SciTech Premium Collection</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><collection>Science Database</collection><collection>Earth, Atmospheric & Aquatic Science Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central Basic</collection><jtitle>Science China. Earth sciences</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Huang, XiaoGe</au><au>Yuan, XianHao</au><au>Chen, ZuAn</au><au>Liu, FuSheng</au><au>Bai, WuMing</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Hugoniot equation of state of olivine and its geodynamic implications</atitle><jtitle>Science China. Earth sciences</jtitle><stitle>Sci. China Earth Sci</stitle><addtitle>SCIENCE CHINA Earth Sciences</addtitle><date>2016-03-01</date><risdate>2016</risdate><volume>59</volume><issue>3</issue><spage>619</spage><epage>625</epage><pages>619-625</pages><issn>1674-7313</issn><eissn>1869-1897</eissn><abstract>Large olivine samples were hot-pressed synthesized for shock wave experiments. The shock wave experiments were carried out at pressure range between 11 and 42 GPa. Shock data on olivine sample yielded a linear relationship between shock wave velocity D and particle velocity u described by D=3.56（？0.13）＋2.57（？0.12）u. The shock temperature is determined by an energy relationship which is approximately 790°C at pressure 28 GPa. Due to low temperature and short experimental duration, we suggest that no phase change occurred in our sample below 30 GPa and olivine persisted well beyond its equilibrium boundary in metastable phase. The densities of metastable olivine are in agreement with the results of static compression. At the depth shallower than 410 km, the densities of metastable olivine are higher than those of the PREM model, facilitating cold slab to sink into the mantle transition zone. However, in entire mantle transition zone, the shock densities are lower than those of the PREM model, hampering cold slab to flow across the ＂660 km＂ phase boundary.</abstract><cop>Beijing</cop><pub>Science China Press</pub><doi>10.1007/s11430-015-5231-2</doi><tpages>7</tpages></addata></record> |
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| subjects | Earth and Environmental Science Earth Sciences Experiments Hugoniot Low temperature PREM模型 Research Paper Shock waves Temperature Transition zone Wave velocity 冲击波试验 冲击波速度 动力学意义 地幔过渡带 橄榄石 状态方程 |
| title | Hugoniot equation of state of olivine and its geodynamic implications |
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