{"@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/1360576118699648256.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1007/s11214-022-00871-w"}},{"identifier":{"@type":"URI","@value":"https://link.springer.com/content/pdf/10.1007/s11214-022-00871-w.pdf"}},{"identifier":{"@type":"URI","@value":"https://link.springer.com/article/10.1007/s11214-022-00871-w/fulltext.html"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"Comparative Na and K Mercury and Moon Exospheres"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title><jats:p>Sodium and, in a lesser way, potassium atomic components of surface-bounded exospheres are among the brightest elements that can be observed from the Earth in our Solar System. Both species have been intensively observed around Mercury, the Moon and the Galilean Moons. During the last decade, new observations have been obtained thanks to space missions carrying remote and in situ instrumentation that provide a completely original view of these species in the exospheres of Mercury and the Moon. They challenged our understanding and modelling of these exospheres and opened new directions of research by suggesting the need to better take into account the relationship between the surface-exosphere and the magnetosphere. In this paper, we first review the large set of observations of Mercury and the Moon Sodium and Potassium exospheres. In the second part, we list what it tells us on the sources and sinks of these exospheres focusing in particular on the role of their magnetospheres of these objects and then discuss, in a third section, how these observations help us to understand and identify the key drivers of these exospheres.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380576118699648138","@type":"Researcher","foaf:name":[{"@value":"F. Leblanc"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699648778","@type":"Researcher","foaf:name":[{"@value":"C. Schmidt"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699647876","@type":"Researcher","foaf:name":[{"@value":"V. Mangano"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699648397","@type":"Researcher","foaf:name":[{"@value":"A. Mura"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699647896","@type":"Researcher","foaf:name":[{"@value":"G. Cremonese"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699648644","@type":"Researcher","foaf:name":[{"@value":"J. M. Raines"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699647889","@type":"Researcher","foaf:name":[{"@value":"J. M. Jasinski"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699648643","@type":"Researcher","foaf:name":[{"@value":"M. Sarantos"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699648005","@type":"Researcher","foaf:name":[{"@value":"A. Milillo"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699648152","@type":"Researcher","foaf:name":[{"@value":"R. M. Killen"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699648785","@type":"Researcher","foaf:name":[{"@value":"S. Massetti"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699648013","@type":"Researcher","foaf:name":[{"@value":"T. Cassidy"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699647890","@type":"Researcher","foaf:name":[{"@value":"R. J. Vervack"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699648404","@type":"Researcher","foaf:name":[{"@value":"S. Kameda"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699648263","@type":"Researcher","foaf:name":[{"@value":"M. T. Capria"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699648128","@type":"Researcher","foaf:name":[{"@value":"M. Horanyi"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699648260","@type":"Researcher","foaf:name":[{"@value":"D. Janches"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699648280","@type":"Researcher","foaf:name":[{"@value":"A. Berezhnoy"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699648776","@type":"Researcher","foaf:name":[{"@value":"A. Christou"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699648409","@type":"Researcher","foaf:name":[{"@value":"T. Hirai"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699648018","@type":"Researcher","foaf:name":[{"@value":"P. Lierle"}]},{"@id":"https://cir.nii.ac.jp/crid/1380576118699648782","@type":"Researcher","foaf:name":[{"@value":"J. Morgenthaler"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00386308"},{"@type":"EISSN","@value":"15729672"}],"prism:publicationName":[{"@value":"Space Science Reviews"}],"dc:publisher":[{"@value":"Springer Science and Business Media LLC"}],"prism:publicationDate":"2022-01-24","prism:volume":"218","prism:number":"1","prism:startingPage":"2"},"reviewed":"false","dc:rights":["https://creativecommons.org/licenses/by/4.0","https://creativecommons.org/licenses/by/4.0"],"url":[{"@id":"https://link.springer.com/content/pdf/10.1007/s11214-022-00871-w.pdf"},{"@id":"https://link.springer.com/article/10.1007/s11214-022-00871-w/fulltext.html"}],"createdAt":"2022-01-24","modifiedAt":"2023-11-16","project":[{"@id":"https://cir.nii.ac.jp/crid/1040000781975776896","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"17KK0097"},{"@type":"JGN","@value":"JP17KK0097"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-17KK0097/"}],"notation":[{"@language":"ja","@value":"太陽系外地球型惑星の水環境進化"},{"@language":"en","@value":"Aqueous environments of terrestrial exoplanets"}]},{"@id":"https://cir.nii.ac.jp/crid/1040000782013502848","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"19H00727"},{"@type":"JGN","@value":"JP19H00727"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-19H00727/"}],"notation":[{"@language":"ja","@value":"太陽系外地球型惑星の高層大気観測に向けた高感度紫外線検出器の開発"},{"@language":"en","@value":"Development of a high-sensitivity ultraviolet detector for observation of upper atmohspheres of terrestrial exoplanets"}]}],"relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360004233290081536","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Centrifugally stimulated exospheric ion escape at Mercury"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011143587338880","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"MESSENGER observations of Mercury's magnetosphere during northward 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Hunten FRSC who passed away in December 2010 after a very illustrious career."}]},{"@id":"https://cir.nii.ac.jp/crid/1360294647871171328","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Inhibition of solar wind impingement on mercury by planetary induction currents"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294647881154048","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Coronagraphic observations of the lunar sodium exosphere January–June, 2017"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294647902274048","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Asteroidal and cometary dust flux in the inner solar system"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294648055630592","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A transient enhancement of Mercury’s exosphere at extremely high altitudes inferred from pickup 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