{"@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/1360011142937338752.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1175/1520-0469(1984)041<1901:zwitma>2.0.co;2"}},{"identifier":{"@type":"URI","@value":"http://journals.ametsoc.org/doi/pdf/abs/10.1175/1520-0469%281984%29041%3C1901%3AZWITMA%3E2.0.CO%3B2"}}],"dc:title":[{"@value":"Zonal Winds in the Middle Atmosphere of Venus from Pioneer Venus Radio Occultation Data"}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380011142937338752","@type":"Researcher","foaf:name":[{"@value":"Matthew Newman"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142937338755","@type":"Researcher","foaf:name":[{"@value":"Gerald Schubert"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142937338754","@type":"Researcher","foaf:name":[{"@value":"Arvydas J. Kliore"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011142937338753","@type":"Researcher","foaf:name":[{"@value":"Indu R. Patel"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00224928"},{"@type":"EISSN","@value":"15200469"}],"prism:publicationName":[{"@value":"Journal of the Atmospheric Sciences"}],"dc:publisher":[{"@value":"American Meteorological Society"}],"prism:publicationDate":"1984-06","prism:volume":"41","prism:number":"12","prism:startingPage":"1901","prism:endingPage":"1913"},"reviewed":"false","url":[{"@id":"http://journals.ametsoc.org/doi/pdf/abs/10.1175/1520-0469%281984%29041%3C1901%3AZWITMA%3E2.0.CO%3B2"}],"createdAt":"2002-07-27","modifiedAt":"2020-12-18","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050001335851969536","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Development of an ensemble Kalman filter data assimilation system for the Venusian atmosphere"}]},{"@id":"https://cir.nii.ac.jp/crid/1050856995323578240","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Initial performance of the radio occultation experiment in the Venus orbiter mission Akatsuki"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004229805014400","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"General circulation driven by baroclinic forcing due to cloud layer heating: Significance of planetary rotation and polar eddy heat transport"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004233436824448","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Equatorial jet in the lower to middle cloud layer of Venus revealed by Akatsuki"}]},{"@id":"https://cir.nii.ac.jp/crid/1360017280648680704","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Cold Collar Reproduced by a Venus GCM With the Akatsuki Horizontal Wind Assimilation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360283689327649920","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Vertical structure of the axi‐asymmetric temperature disturbance in the Venusian polar atmosphere: Comparison between radio occultation measurements and GCM results"}]},{"@id":"https://cir.nii.ac.jp/crid/1360283691778754560","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"The puzzling Venusian polar atmospheric structure reproduced by a general circulation model"}]},{"@id":"https://cir.nii.ac.jp/crid/1360290617864741632","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Superrotation in Planetary Atmospheres"}]},{"@id":"https://cir.nii.ac.jp/crid/1360298337072107520","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Dynamical Effect on Static Stability of the Venus Atmosphere Simulated Using a General Circulation Model: A Comparison With Radio Occultation Measurements"}]},{"@id":"https://cir.nii.ac.jp/crid/1360298757167570688","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A Sensitivity Study of the Thermal Tides in the Venusian Atmosphere: Structures and Dynamical Effects on the Superrotation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567182137648896","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Venusian middle-atmospheric dynamics in the presence of a strong planetary-scale 5.5-day wave"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567182137880448","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Dynamical relationship between wind speed magnitude and meridional temperature contrast: Application to an interannual oscillation in Venusian middle atmosphere GCM"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567182418875008","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Dynamics of polar vortices at cloud top and base on Venus inferred from a general circulation model: Case of a strong diurnal thermal tide"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567183246094848","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Local Time Dependence of the Thermal Structure in the Venusian Equatorial Upper Atmosphere: Comparison of Akatsuki Radio Occultation Measurements and GCM Results"}]},{"@id":"https://cir.nii.ac.jp/crid/1360846639279501568","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Baroclinic instability in the Venus atmosphere simulated by GCM"}]},{"@id":"https://cir.nii.ac.jp/crid/1360846639281846912","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Three‐Dimensional Structures of Thermal Tides Simulated by a Venus GCM"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848657114438272","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Inverse insolation dependence of Venus’ cloud-level convection"}]},{"@id":"https://cir.nii.ac.jp/crid/1360853567850553344","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Venusian Cloud Distribution Simulated by a General Circulation Model"}]},{"@id":"https://cir.nii.ac.jp/crid/1360861704764051968","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Vertical‐Wind‐Induced Cloud Opacity Variation in Low Latitudes Simulated by a Venus GCM"}]},{"@id":"https://cir.nii.ac.jp/crid/1361694366761317760","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Solar-locked and geographical atmospheric structures inferred from a Venus general circulation model with radiative transfer"}]},{"@id":"https://cir.nii.ac.jp/crid/1361975843215420800","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Thermal structure of the Venusian atmosphere from the sub-cloud region to the mesosphere as observed by radio occultation"}]},{"@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/2050588892138311424","@type":"Article","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Radio occultation experiment of the Venus atmosphere and ionosphere with the Venus orbiter Akatsuki"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1175/1520-0469(1984)041<1901:zwitma>2.0.co;2"},{"@type":"CROSSREF","@value":"10.1038/s41598-017-09461-1_references_DOI_YN8kckBJyiq2EelAqUljyypub55"},{"@type":"CROSSREF","@value":"10.1002/2015je004983_references_DOI_YN8kckBJyiq2EelAqUljyypub55"},{"@type":"CROSSREF","@value":"10.1038/ngeo3016_references_DOI_YN8kckBJyiq2EelAqUljyypub55"},{"@type":"CROSSREF","@value":"10.1029/2022je007689_references_DOI_PX8EvzxjQPGHV0oBR8E6p2VkOXH"},{"@type":"CROSSREF","@value":"10.1002/2016je005213_references_DOI_YN8kckBJyiq2EelAqUljyypub55"},{"@type":"CROSSREF","@value":"10.1038/ncomms10398_references_DOI_YN8kckBJyiq2EelAqUljyypub55"},{"@type":"CROSSREF","@value":"10.1016/j.icarus.2011.06.017_references_DOI_YN8kckBJyiq2EelAqUljyypub55"},{"@type":"CROSSREF","@value":"10.1007/s11214-020-00703-9_references_DOI_YN8kckBJyiq2EelAqUljyypub55"},{"@type":"CROSSREF","@value":"10.1029/2021je006957_references_DOI_YN8kckBJyiq2EelAqUljyypub55"},{"@type":"CROSSREF","@value":"10.1029/2022je007243_references_DOI_PX8EvzxjQPGHV0oBR8E6p2VkOXH"},{"@type":"CROSSREF","@value":"10.1029/2018je005640_references_DOI_YN8kckBJyiq2EelAqUljyypub55"},{"@type":"CROSSREF","@value":"10.5047/eps.2011.02.009_references_DOI_YN8kckBJyiq2EelAqUljyypub55"},{"@type":"CROSSREF","@value":"10.1016/j.icarus.2013.10.012_references_DOI_YN8kckBJyiq2EelAqUljyypub55"},{"@type":"CROSSREF","@value":"10.1016/j.icarus.2017.10.012_references_DOI_YN8kckBJyiq2EelAqUljyypub55"},{"@type":"CROSSREF","@value":"10.1002/2014je004624_references_DOI_YN8kckBJyiq2EelAqUljyypub55"},{"@type":"CROSSREF","@value":"10.1002/2017je005449_references_DOI_YN8kckBJyiq2EelAqUljyypub55"},{"@type":"CROSSREF","@value":"10.1186/s40623-017-0722-3_references_DOI_YN8kckBJyiq2EelAqUljyypub55"},{"@type":"CROSSREF","@value":"10.5047/eps.2011.03.009_references_DOI_YN8kckBJyiq2EelAqUljyypub55"},{"@type":"CROSSREF","@value":"10.1029/2019je006208_references_DOI_YN8kckBJyiq2EelAqUljyypub55"},{"@type":"CROSSREF","@value":"10.1029/2022je007595_references_DOI_YN8kckBJyiq2EelAqUljyypub55"},{"@type":"CROSSREF","@value":"10.1016/j.icarus.2018.11.015_references_DOI_YN8kckBJyiq2EelAqUljyypub55"},{"@type":"CROSSREF","@value":"10.1016/j.pss.2015.01.017_references_DOI_YN8kckBJyiq2EelAqUljyypub55"},{"@type":"CROSSREF","@value":"10.1038/s41598-020-59278-8_references_DOI_YN8kckBJyiq2EelAqUljyypub55"}]}