{"@context":{"@vocab":"https://cir.nii.ac.jp/schema/1.0/","rdfs":"http://www.w3.org/2000/01/rdf-schema#","dc":"http://purl.org/dc/elements/1.1/","dcterms":"http://purl.org/dc/terms/","foaf":"http://xmlns.com/foaf/0.1/","prism":"http://prismstandard.org/namespaces/basic/2.0/","cinii":"http://ci.nii.ac.jp/ns/1.0/","datacite":"https://schema.datacite.org/meta/kernel-4/","ndl":"http://ndl.go.jp/dcndl/terms/","jpcoar":"https://github.com/JPCOAR/schema/blob/master/2.0/"},"@id":"https://cir.nii.ac.jp/crid/1360004232425661184.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1016/j.pepi.2017.11.001"}},{"identifier":{"@type":"URI","@value":"https://api.elsevier.com/content/article/PII:S003192011730239X?httpAccept=text/xml"}},{"identifier":{"@type":"URI","@value":"https://api.elsevier.com/content/article/PII:S003192011730239X?httpAccept=text/plain"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"Numerical experiments on thermal convection of highly compressible fluids with variable viscosity and thermal conductivity: Implications for mantle convection of super-Earths"}],"description":[{"notation":[{"@value":"Abstract   We conduct a series of numerical experiments of thermal convection of highly compressible fluids in a two-dimensional rectangular box, in order to study the mantle convection on super-Earths. The thermal conductivity and viscosity are assumed to exponentially depend on depth and temperature, respectively, while the variations in thermodynamic properties (thermal expansivity and reference density) with depth are taken to be relevant for the super-Earths with 10 times the Earth’s. From our experiments we identified a distinct regime of convecting flow patterns induced by the interplay between the adiabatic temperature change and the spatial variations in viscosity and thermal conductivity. That is, for the cases with strong temperature-dependent viscosity and depth-dependent thermal conductivity, a “deep stratosphere” of stable thermal stratification is formed at the base of the mantle, in addition to thick stagnant lids at their top surfaces. In the “deep stratosphere”, the fluid motion is insignificant particularly in the vertical direction in spite of smallest viscosity owing to its strong dependence on temperature. Our finding may further imply that some of super-Earths which are lacking in mobile tectonic plates on their top surfaces may have “deep stratospheres” at the base of their mantles."}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1420001326212654464","@type":"Researcher","personIdentifier":[{"@type":"KAKEN_RESEARCHERS","@value":"70344299"},{"@type":"NRID","@value":"1000070344299"},{"@type":"CINII_AUTHOR_ID","@value":"DA16198042"},{"@type":"URI","@value":"https://ci.nii.ac.jp/author/DA16198042#entity"},{"@type":"URI","@value":"https://viaf.org/viaf/NII%7CDA16198042"},{"@type":"NRID","@value":"9000386337311"},{"@type":"NRID","@value":"9000324661464"},{"@type":"NRID","@value":"9000356660861"},{"@type":"NRID","@value":"9000252453047"},{"@type":"RESEARCHMAP","@value":"https://researchmap.jp/read0141651"}],"foaf:name":[{"@value":"Masanori Kameyama"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004232425661184","@type":"Researcher","foaf:name":[{"@value":"Mayumi Yamamoto"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00319201"}],"prism:publicationName":[{"@value":"Physics of the Earth and Planetary Interiors"}],"dc:publisher":[{"@value":"Elsevier BV"}],"prism:publicationDate":"2018-01","prism:volume":"274","prism:startingPage":"23","prism:endingPage":"36"},"reviewed":"false","dc:rights":["https://www.elsevier.com/tdm/userlicense/1.0/"],"url":[{"@id":"https://api.elsevier.com/content/article/PII:S003192011730239X?httpAccept=text/xml"},{"@id":"https://api.elsevier.com/content/article/PII:S003192011730239X?httpAccept=text/plain"}],"createdAt":"2017-11-08","modifiedAt":"2019-10-05","project":[{"@id":"https://cir.nii.ac.jp/crid/1040282257274566528","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"26400457"},{"@type":"JGN","@value":"JP26400457"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-26400457/"}],"notation":[{"@language":"ja","@value":"『大きなマントルウェッジ』(BMW) 内の3次元マントル対流シミュレーション"},{"@language":"en","@value":"Numerical experiments of mantle convection in a Big Mantle Wedge associated with subducting plates"}]}],"relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050565162984274816","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Impurity Resistivity of fcc and hcp Fe-Based Alloys: Thermal Stratification at the Top of the Core of Super-Earths"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011144041861248","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Analyses of marginal stability, heat transfer and boundary layer properties for thermal convection in a compressible fluid with infinite Prandtl number"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011144946768128","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Dynamical consequences of depth-dependent thermal expansivity and viscosity on mantle circulations and thermal structure"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011145708848000","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Toward a Deterministic Model of Planetary Formation. 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