{"@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/1360011142938623488.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1029/2008je003134"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2008JE003134"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2008JE003134"}}],"dc:title":[{"@value":"Felsic highland crust on Venus suggested by Galileo Near‐Infrared Mapping Spectrometer data"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>We evaluated the spatial variation of Venusian surface emissivity at 1.18 <jats:italic>μ</jats:italic>m wavelength and that of near‐surface atmospheric temperature using multispectral images obtained by the Near‐Infrared Mapping Spectrometer (NIMS) on board the Galileo spacecraft. The Galileo NIMS observed the nightside thermal emission from the surface and the deep atmosphere of Venus, which is attenuated by scattering from the overlying clouds. To analyze the NIMS data, we used a radiative transfer model based on the adding method. Although there is still an uncertainty in the results owing to the not well known parameters of the atmosphere, our analysis revealed that the horizontal temperature variation in the near‐surface atmosphere is no more than ±2 K on the Venusian nightside and also suggests that the majority of lowlands likely has higher emissivity compared to the majority of highlands. One interpretation for the latter result is that highland materials are generally composed of felsic rocks. Since formation of a large body of granitic magmas requires water, the presence of granitic terrains would imply that Venus may have had an ocean and a mechanism to recycle water into the mantle in the past.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380011142938623492","@type":"Researcher","foaf:name":[{"@value":"George L. Hashimoto"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Earth and Planetary Atmospheric Science Organization of Advanced Science and Technology, Kobe University  Kobe Japan"}]},{"@id":"https://cir.nii.ac.jp/crid/1380861293027385216","@type":"Researcher","foaf:name":[{"@value":"Maarten Roos‐Serote"}],"jpcoar:affiliationName":[{"@value":"Lisbon Astronomical Observatory  Lisbon Portugal"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142938623494","@type":"Researcher","foaf:name":[{"@value":"Seiji Sugita"}],"jpcoar:affiliationName":[{"@value":"Department of Complexity Science and Engineering Graduate School of Frontier Science, University of Tokyo  Kashiwa Japan"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142938623491","@type":"Researcher","foaf:name":[{"@value":"Martha S. Gilmore"}],"jpcoar:affiliationName":[{"@value":"Department of Earth and Environmental Sciences Wesleyan University  Middletown Connecticut USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142938623489","@type":"Researcher","foaf:name":[{"@value":"Lucas W. Kamp"}],"jpcoar:affiliationName":[{"@value":"Jet Propulsion Laboratory California Institute of Technology  Pasadena California USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142938623493","@type":"Researcher","foaf:name":[{"@value":"Robert W. Carlson"}],"jpcoar:affiliationName":[{"@value":"Jet Propulsion Laboratory California Institute of Technology  Pasadena California USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142938623490","@type":"Researcher","foaf:name":[{"@value":"Kevin H. Baines"}],"jpcoar:affiliationName":[{"@value":"Jet Propulsion Laboratory California Institute of Technology  Pasadena California USA"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"01480227"}],"prism:publicationName":[{"@value":"Journal of Geophysical Research: Planets"}],"dc:publisher":[{"@value":"American Geophysical Union (AGU)"}],"prism:publicationDate":"2008-05","prism:volume":"113","prism:number":"E5","prism:startingPage":"E00B24"},"reviewed":"false","dcterms:accessRights":"http://purl.org/coar/access_right/c_abf2","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2008JE003134"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2008JE003134"}],"createdAt":"2008-12-30","modifiedAt":"2023-10-12","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360004234474605952","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Searching for Biosignatures in Exoplanetary Impact Ejecta"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285704781707648","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"The formation of the South Tharsis Ridge Belt: Basin and Range‐style extension on early Mars?"}]},{"@id":"https://cir.nii.ac.jp/crid/1360565170738047872","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Terrestrial Planet Formation: Constraining the Formation of Mercury"}]},{"@id":"https://cir.nii.ac.jp/crid/1361413119380635520","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Constraining the Formation of the Four Terrestrial Planets in the Solar System"}]},{"@id":"https://cir.nii.ac.jp/crid/1390582308084713856","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Radiative Effects on the Formation of the Stably Stratified Layer in the Lower Atmosphere of Venus"}]},{"@id":"https://cir.nii.ac.jp/crid/1523388080069817344","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Overview of Venus orbiter, Akatsuki"},{"@language":"ja-Kana","@value":"Overview of Venus orbiter Akatsuki"}]},{"@id":"https://cir.nii.ac.jp/crid/2050025942124908032","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Initial products of Akatsuki 1-μm camera"}]},{"@id":"https://cir.nii.ac.jp/crid/2051714792052822656","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"AKATSUKI returns to Venus"}]},{"@id":"https://cir.nii.ac.jp/crid/2051996267021864320","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Science requirements and description of the 1 μm camera onboard the Akatsuki Venus Orbiter"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1029/2008je003134"},{"@type":"OPENAIRE","@value":"doi_dedup___::c59ed37bf9e136e258bb571044739bc1"},{"@type":"CROSSREF","@value":"10.5047/eps.2011.03.007_references_DOI_RTIHYIAmYzohkq7Tf7RjiyYlBap"},{"@type":"CROSSREF","@value":"10.2151/jmsj.2024-025_references_DOI_RTIHYIAmYzohkq7Tf7RjiyYlBap"},{"@type":"CROSSREF","@value":"10.1186/s40623-017-0773-5_references_DOI_YYOCrPxDNMEU3xVk7QLO4c5V0Lw"},{"@type":"CROSSREF","@value":"10.1002/2015je004936_references_DOI_RTIHYIAmYzohkq7Tf7RjiyYlBap"},{"@type":"CROSSREF","@value":"10.1186/s40623-016-0457-6_references_DOI_RTIHYIAmYzohkq7Tf7RjiyYlBap"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/aa6544_references_DOI_RTIHYIAmYzohkq7Tf7RjiyYlBap"},{"@type":"CROSSREF","@value":"10.5047/eps.2011.02.009_references_DOI_RTIHYIAmYzohkq7Tf7RjiyYlBap"},{"@type":"CROSSREF","@value":"10.1089/ast.2015.1437_references_DOI_RTIHYIAmYzohkq7Tf7RjiyYlBap"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ab3b0a_references_DOI_RTIHYIAmYzohkq7Tf7RjiyYlBap"}]}