{"@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/1362262944574068992.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1029/96gl01354"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F96GL01354"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/96GL01354"}},{"identifier":{"@type":"NAID","@value":"30013366782"}}],"dc:title":[{"@value":"The lunar wake at 6.8 R<sub>L</sub>: WIND magnetic field observations"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>We report on WIND magnetic field observations at ∼6.8 R<jats:sub>L</jats:sub> downstream of the moon on 27th December 1994. The moon was in the solar wind during the encounter. IMP‐8 observations are used to determine baseline IMF conditions, and therefore determine those features in the WIND data which are related to its proximity to the moon. Previous Explorer 35 observations suggest that the lunar wake is not detectable beyond a downstream distance of ∼4 R<jats:sub>L</jats:sub>. However, despite the distance of WIND from the moon, we observe a slight decrease in field intensity just prior to the spacecraft entering the optical shadow, a slight field strength enhancement whilst in shadow, and perhaps a weak depression once the spacecraft reemerges into sunlight. These signatures closely resemble, but are weaker than, the previous observations. We conclude that a lunar wake did extend to these distances at the time of this encounter. We also note a rotation in field direction some distance outside of the wake signature which may be attributed to the crossing of the lunar mach cone boundary. We discuss the observations in terms of simple models of the solar wind interaction with an insulating body.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1580009751480236416","@type":"Researcher","foaf:name":[{"@value":"C. J. Owen"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944574068994","@type":"Researcher","foaf:name":[{"@value":"R. P. Lepping"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944574068997","@type":"Researcher","foaf:name":[{"@value":"K. W. Ogilvie"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944574068992","@type":"Researcher","foaf:name":[{"@value":"J. A. Slavin"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944574068996","@type":"Researcher","foaf:name":[{"@value":"W. M. Farrell"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944574068995","@type":"Researcher","foaf:name":[{"@value":"J. B. Byrnes"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00948276"},{"@type":"EISSN","@value":"19448007"}],"prism:publicationName":[{"@value":"Geophysical Research Letters"}],"dc:publisher":[{"@value":"American Geophysical Union (AGU)"}],"prism:publicationDate":"1996-05-15","prism:volume":"23","prism:number":"10","prism:startingPage":"1263","prism:endingPage":"1266"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F96GL01354"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/96GL01354"}],"createdAt":"2004-02-04","modifiedAt":"2023-11-22","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360565166662412800","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Large‐amplitude monochromatic ULF waves detected by Kaguya at the Moon"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848657395512064","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Anomalous deformation of the Earth's bow shock in the lunar wake: Joint measurement by Chang’E-1 and SELENE"}]},{"@id":"https://cir.nii.ac.jp/crid/1390001206513659776","@type":"Article","relationType":["isReferencedBy","isCitedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"GEOTAIL observation of upstream ULF waves associated with lunar wake"}]},{"@id":"https://cir.nii.ac.jp/crid/1390282681488509056","@type":"Article","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Pitch angle diffusion of electrons at the boundary of the lunar wake"}]},{"@id":"https://cir.nii.ac.jp/crid/2050025942189449600","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"ELF magnetic fluctuations detected by Kaguya in deepest lunar wake associated with type-II protons"}]},{"@id":"https://cir.nii.ac.jp/crid/2051151842091721984","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Non-monochromatic whistler waves detected by Kaguya on the dayside surface of the moon"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1029/96gl01354"},{"@type":"CIA","@value":"30013366782"},{"@type":"CROSSREF","@value":"10.1186/s40623-015-0196-0_references_DOI_J9GHtUCC0NBZMDVzknS1RvIsGdF"},{"@type":"CROSSREF","@value":"10.1186/bf03351866_references_DOI_J9GHtUCC0NBZMDVzknS1RvIsGdF"},{"@type":"CROSSREF","@value":"10.5047/eps.2010.01.005_references_DOI_J9GHtUCC0NBZMDVzknS1RvIsGdF"},{"@type":"CROSSREF","@value":"10.1029/2011ja017249_references_DOI_J9GHtUCC0NBZMDVzknS1RvIsGdF"},{"@type":"CROSSREF","@value":"10.1186/bf03351789_references_DOI_J9GHtUCC0NBZMDVzknS1RvIsGdF"},{"@type":"CROSSREF","@value":"10.1016/j.pss.2011.01.002_references_DOI_J9GHtUCC0NBZMDVzknS1RvIsGdF"}]}