{"@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/1362825895240748672.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1029/2010ja015486"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2010JA015486"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2010JA015486"}}],"dc:title":[{"@value":"Backscattered solar wind protons by Phobos"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>We report Mars Express (MEX) measurements showing that the regolith‐covered Phobos surface backscatters 0.5%–10% of the impinging solar wind protons. Backscattered protons with an energy corresponding to 30%–40% of the solar wind energy injected in the flow are picked up by the solar wind and may cause field disturbances and wave activity. Since a similar backscattering of solar wind protons was observed and reported at the Moon, the backscattering of the solar wind particles is a typical physical process for regolith‐covered bodies in space, even though the regolith is highly porous and it has been thought that almost 100% of the solar wind protons are implanted.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380013168736810633","@type":"Researcher","foaf:name":[{"@value":"Y. Futaana"}],"jpcoar:affiliationName":[{"@value":"Swedish Institute of Space Physics  Kiruna Sweden"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895240748677","@type":"Researcher","foaf:name":[{"@value":"S. Barabash"}],"jpcoar:affiliationName":[{"@value":"Swedish Institute of Space Physics  Kiruna Sweden"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895240748674","@type":"Researcher","foaf:name":[{"@value":"M. Holmström"}],"jpcoar:affiliationName":[{"@value":"Swedish Institute of Space Physics  Kiruna Sweden"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895240748672","@type":"Researcher","foaf:name":[{"@value":"A. Fedorov"}],"jpcoar:affiliationName":[{"@value":"Centre d'Etude Spatiale des Rayonnements  Toulouse France"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895240748673","@type":"Researcher","foaf:name":[{"@value":"H. Nilsson"}],"jpcoar:affiliationName":[{"@value":"Swedish Institute of Space Physics  Kiruna Sweden"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895240748800","@type":"Researcher","foaf:name":[{"@value":"R. Lundin"}],"jpcoar:affiliationName":[{"@value":"Swedish Institute of Space Physics  Kiruna Sweden"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895240748801","@type":"Researcher","foaf:name":[{"@value":"E. Dubinin"}],"jpcoar:affiliationName":[{"@value":"Max‐Planck‐Institut für Sonnensystemforschung  Katlenburg‐Lindau Germany"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895240748675","@type":"Researcher","foaf:name":[{"@value":"M. Fränz"}],"jpcoar:affiliationName":[{"@value":"Max‐Planck‐Institut für Sonnensystemforschung  Katlenburg‐Lindau Germany"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"01480227"}],"prism:publicationName":[{"@value":"Journal of Geophysical Research: Space Physics"}],"dc:publisher":[{"@value":"American Geophysical Union (AGU)"}],"prism:publicationDate":"2010-10","prism:volume":"115","prism:number":"A10","prism:startingPage":"A10213"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2010JA015486"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2010JA015486"}],"createdAt":"2010-10-06","modifiedAt":"2023-11-02","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360285705151818368","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Statistical properties of planetary heavy‐ion precipitations toward the Martian ionosphere obtained from Mars Express"}]},{"@id":"https://cir.nii.ac.jp/crid/2050025942153241088","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"In situ observations of ions and magnetic field around Phobos : the mass spectrum analyzer (MSA) for the Martian Moons eXploration (MMX) mission"}]},{"@id":"https://cir.nii.ac.jp/crid/2051151842060090624","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Martian moons exploration MMX : sample return mission to Phobos elucidating formation processes of habitable planets"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1029/2010ja015486"},{"@type":"CROSSREF","@value":"10.1186/s40623-021-01452-x_references_DOI_VwTVraiw3MM0EYYSQfcwHIGkUSH"},{"@type":"CROSSREF","@value":"10.1002/jgra.50494_references_DOI_VwTVraiw3MM0EYYSQfcwHIGkUSH"},{"@type":"CROSSREF","@value":"10.1186/s40623-021-01545-7_references_DOI_VwTVraiw3MM0EYYSQfcwHIGkUSH"}]}