{"@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/1362262945413323264.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1029/rg002i004p00661"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2FRG002i004p00661"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/RG002i004p00661"}},{"identifier":{"@type":"NAID","@value":"30034662929"}}],"dc:title":[{"@value":"Tidal dissipation by solid friction and the resulting orbital evolution"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>Dissipation of tidal energy in the earth's mantle and the moon was calculated assuming a dissipation factor 1/<jats:italic>Q</jats:italic> constant throughout both bodies. In the mantle the dissipation varies from about 2 × 10<jats:sup>−6</jats:sup>/<jats:italic>Q</jats:italic> erg cm<jats:sup>−3</jats:sup> sec<jats:sup>−1</jats:sup> near the pole at the bottom of the mantle to about 0.02 × 10<jats:sup>−6</jats:sup>/<jats:italic>Q</jats:italic> erg cm<jats:sup>−3</jats:sup> sec<jats:sup>−1</jats:sup> near the surface. The effects of compressibility and inhomogeneity are less than 3%. In a homogeneous moon the dissipation varies from a maximum of about 0.03 × 10<jats:sup>−6</jats:sup>/<jats:italic>Q</jats:italic> erg cm<jats:sup>−3</jats:sup> sec<jats:sup>−1</jats:sup> near the center to a minimum of about 0.4 × 10<jats:sup>−9</jats:sup>/<jats:italic>Q</jats:italic> erg cm<jats:sup>−3</jats:sup> sec<jats:sup>−1</jats:sup> at the surface. A theory of orbital evolution is developed in which the disturbing function is expressed in a Fourier series with respect to time, so that the effects of variation of dissipation factor 1/<jats:italic>Q</jats:italic>, or lag angle ϵ, with amplitude and frequency can be examined. Comparisons with results of other authors are made.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1382262945413323264","@type":"Researcher","foaf:name":[{"@value":"William M. Kaula"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"87551209"},{"@type":"EISSN","@value":"19449208"}],"prism:publicationName":[{"@value":"Reviews of Geophysics"}],"dc:publisher":[{"@value":"American Geophysical Union (AGU)"}],"prism:publicationDate":"1964-11","prism:volume":"2","prism:number":"4","prism:startingPage":"661","prism:endingPage":"685"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2FRG002i004p00661"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/RG002i004p00661"}],"createdAt":"2008-02-06","modifiedAt":"2023-09-22","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050869456407986688","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Tidal deformation of Ganymede: Sensitivity of Love numbers on the interior structure"}]},{"@id":"https://cir.nii.ac.jp/crid/1360016864414104704","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Exploring the Recycling Model of Phobos Formation: Rubble-pile Satellites*"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857593698091136","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Tidal Evolution of the Eccentric Moon around Dwarf Planet (225088) Gonggong"}]},{"@id":"https://cir.nii.ac.jp/crid/1390001206234738176","@type":"Article","relationType":["isCitedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"A comparative study on the volcanism and tectonics of the terrestrial planets and satellites."},{"@language":"ja","@value":"地球型惑星,氷衛星の火山活動とテクトニクスの比較惑星学"},{"@value":"地球型惑星,氷衛星の火山活動とテクトニクスの比較惑星学〔英文〕"},{"@language":"ja-Kana","@value":"チキュウガタ ワクセイ ヒョウエイセイ ノ カザン カツドウ ト テクトニクス"}]},{"@id":"https://cir.nii.ac.jp/crid/2051996266990214656","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"MIRS : an imaging spectrometer for the MMX mission"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1029/rg002i004p00661"},{"@type":"CIA","@value":"30034662929"},{"@type":"CROSSREF","@value":"10.1186/s40623-021-01423-2_references_DOI_56nuduHAbAVSLzlDvnFFGh6qILx"},{"@type":"CROSSREF","@value":"10.3847/1538-3881/acbf53_references_DOI_56nuduHAbAVSLzlDvnFFGh6qILx"},{"@type":"CROSSREF","@value":"10.1002/2016je005071_references_DOI_56nuduHAbAVSLzlDvnFFGh6qILx"},{"@type":"CROSSREF","@value":"10.3847/1538-3881/ac1f91_references_DOI_56nuduHAbAVSLzlDvnFFGh6qILx"}]}