{"@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/1360848654734005248.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1002/2015gl065293"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2015GL065293"}},{"identifier":{"@type":"URI","@value":"https://onlinelibrary.wiley.com/doi/pdf/10.1002/2015GL065293"}},{"identifier":{"@type":"URI","@value":"https://onlinelibrary.wiley.com/doi/full-xml/10.1002/2015GL065293"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/am-pdf/10.1002/2015GL065293"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/2015GL065293"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"The spatial distribution of planetary ion fluxes near Mars observed by MAVEN"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title><jats:p>We present the results of an initial effort to statistically map the fluxes of planetary ions on a closed surface around Mars. Choosing a spherical shell ~1000 km above the planet, we map both outgoing and incoming ion fluxes (with energies >25 eV) over a 4 month period. The results show net escape of planetary ions behind Mars and strong fluxes of escaping ions from the northern hemisphere with respect to the solar wind convection electric field. Planetary ions also travel toward the planet, and return fluxes are particularly strong in the southern electric field hemisphere. We obtain a lower bound estimate for planetary ion escape of ~3 × 10<jats:sup>24</jats:sup> s<jats:sup>−1</jats:sup>, accounting for the ~10% of ions that return toward the planet and assuming that the ~70% of the surface covered so far is representative of the regions not yet visited by Mars Atmosphere and Volatile EvolutioN (MAVEN).</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380013168736810910","@type":"Researcher","foaf:name":[{"@value":"D. A. 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Eparvier"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado Boulder  Boulder Colorado USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380848654734005124","@type":"Researcher","foaf:name":[{"@value":"X. Fang"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado Boulder  Boulder Colorado USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380848654734005131","@type":"Researcher","foaf:name":[{"@value":"K. Fortier"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado Boulder  Boulder Colorado USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380848654734005377","@type":"Researcher","foaf:name":[{"@value":"T. Hara"}],"jpcoar:affiliationName":[{"@value":"Space Sciences Laboratory University of California  Berkeley, California USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380848654734005130","@type":"Researcher","foaf:name":[{"@value":"Y. Harada"}],"jpcoar:affiliationName":[{"@value":"Space Sciences Laboratory University of California  Berkeley, California USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380848654734004992","@type":"Researcher","foaf:name":[{"@value":"B. M. Jakosky"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado Boulder  Boulder Colorado USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380848654734005135","@type":"Researcher","foaf:name":[{"@value":"R. J. Lillis"}],"jpcoar:affiliationName":[{"@value":"Space Sciences Laboratory University of California  Berkeley, California USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380848654734004998","@type":"Researcher","foaf:name":[{"@value":"R. Livi"}],"jpcoar:affiliationName":[{"@value":"Space Sciences Laboratory University of California  Berkeley, California USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380848654734005138","@type":"Researcher","foaf:name":[{"@value":"J. G. 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Iowa"}]},{"@id":"https://cir.nii.ac.jp/crid/1890021791453854737","@type":"Researcher","foaf:name":[{"@value":"University of California Berkeley (UC Berkeley)"}]},{"@id":"https://cir.nii.ac.jp/crid/1890021791453854592","@type":"Researcher","foaf:name":[{"@value":"Institute of Geophysics and Planetary Physics Los Angeles (IGPP)"}]},{"@id":"https://cir.nii.ac.jp/crid/1890021791453854732","@type":"Researcher","foaf:name":[{"@value":"University of California Los Angeles (UCLA)"}]},{"@id":"https://cir.nii.ac.jp/crid/1890021791453854720","@type":"Researcher","foaf:name":[{"@value":"HELIOS - LATMOS"}]},{"@id":"https://cir.nii.ac.jp/crid/1890021791453854598","@type":"Researcher","foaf:name":[{"@value":"Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS)"}]},{"@id":"https://cir.nii.ac.jp/crid/1890021791453854723","@type":"Researcher","foaf:name":[{"@value":"Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national 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Michigan Ann Arbor"}]},{"@id":"https://cir.nii.ac.jp/crid/1890021791453854599","@type":"Researcher","foaf:name":[{"@value":"Cardon, Catherine"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00948276"},{"@type":"EISSN","@value":"19448007"}],"prism:publicationName":[{"@value":"Geophysical Research Letters"}],"dc:publisher":[{"@value":"American Geophysical Union 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