{"@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/1363670319140928768.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1002/2015gl063863"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2015GL063863"}},{"identifier":{"@type":"URI","@value":"https://onlinelibrary.wiley.com/doi/pdf/10.1002/2015GL063863"}},{"identifier":{"@type":"URI","@value":"https://onlinelibrary.wiley.com/doi/full-xml/10.1002/2015GL063863"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/2015GL063863"}}],"dc:title":[{"@value":"MAVEN IUVS observations of the aftermath of the Comet Siding Spring meteor shower on Mars"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title><jats:p>We report the detection of intense emission from magnesium and iron in Mars' atmosphere caused by a meteor shower following Comet Siding Spring's close encounter with Mars. The observations were made with the Imaging Ultraviolet Spectrograph, a remote sensing instrument on the Mars Atmosphere and Volatile EvolutioN spacecraft orbiting Mars. Ionized magnesium caused the brightest emission from the planet's atmosphere for many hours, resulting from resonant scattering of solar ultraviolet light. Modeling suggests a substantial fluence of low‐density dust particles 1–100 µm in size, with the large amount and small size contrary to predictions. The event created a temporary planet‐wide ionospheric layer below Mars' main dayside ionosphere. The dramatic meteor shower response at Mars is starkly different from the case at Earth, where a steady state metal layer is always observable but perturbations caused by even the strongest meteor showers are challenging to detect.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380857593819639168","@type":"Researcher","foaf:name":[{"@value":"N. M. Schneider"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado at Boulder  Boulder Colorado USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319140928899","@type":"Researcher","foaf:name":[{"@value":"J. I. Deighan"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado at Boulder  Boulder Colorado USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319140928771","@type":"Researcher","foaf:name":[{"@value":"A. I. F. Stewart"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado at Boulder  Boulder Colorado USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319140928900","@type":"Researcher","foaf:name":[{"@value":"W. E. McClintock"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado at Boulder  Boulder Colorado USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319140928897","@type":"Researcher","foaf:name":[{"@value":"S. K. Jain"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado at Boulder  Boulder Colorado USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319140928772","@type":"Researcher","foaf:name":[{"@value":"M. S. Chaffin"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado at Boulder  Boulder Colorado USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319140928770","@type":"Researcher","foaf:name":[{"@value":"A. Stiepen"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado at Boulder  Boulder Colorado USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319140928776","@type":"Researcher","foaf:name":[{"@value":"M. Crismani"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado at Boulder  Boulder Colorado USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319140928901","@type":"Researcher","foaf:name":[{"@value":"J. M. C. Plane"}],"jpcoar:affiliationName":[{"@value":"School of Chemistry University of Leeds  Leeds UK"}]},{"@id":"https://cir.nii.ac.jp/crid/1380298341931287168","@type":"Researcher","foaf:name":[{"@value":"J. D. Carrillo‐Sánchez"}],"jpcoar:affiliationName":[{"@value":"School of Chemistry University of Leeds  Leeds UK"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319140928775","@type":"Researcher","foaf:name":[{"@value":"J. S. Evans"}],"jpcoar:affiliationName":[{"@value":"Computational Physics, Inc.  Springfield Virginia USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319140928778","@type":"Researcher","foaf:name":[{"@value":"M. H. Stevens"}],"jpcoar:affiliationName":[{"@value":"Space Science Division Naval Research Laboratory  Washington District of Columbia USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319140928777","@type":"Researcher","foaf:name":[{"@value":"R. V. Yelle"}],"jpcoar:affiliationName":[{"@value":"Lunar and Planetary Laboratory University of Arizona  Tucson Arizona USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319140928773","@type":"Researcher","foaf:name":[{"@value":"J. T. Clarke"}],"jpcoar:affiliationName":[{"@value":"Center for Space Physics Boston University  Boston Massachusetts USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319140928769","@type":"Researcher","foaf:name":[{"@value":"G. M. Holsclaw"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado at Boulder  Boulder Colorado USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319140928898","@type":"Researcher","foaf:name":[{"@value":"F. Montmessin"}],"jpcoar:affiliationName":[{"@value":"LATMOS/IPSL  Guyancourt France"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319140928768","@type":"Researcher","foaf:name":[{"@value":"B. M. Jakosky"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado at Boulder  Boulder Colorado USA"}]}],"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":"2015-06-16","prism:volume":"42","prism:number":"12","prism:startingPage":"4755","prism:endingPage":"4761"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2015GL063863"},{"@id":"https://onlinelibrary.wiley.com/doi/pdf/10.1002/2015GL063863"},{"@id":"https://onlinelibrary.wiley.com/doi/full-xml/10.1002/2015GL063863"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/2015GL063863"}],"createdAt":"2015-06-16","modifiedAt":"2023-10-03","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360285704782389760","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Comparison of the Martian thermospheric density and temperature from IUVS/MAVEN data and general circulation modeling"}]},{"@id":"https://cir.nii.ac.jp/crid/1360853567612224128","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Martian Oxygen and Hydrogen Upper Atmospheres Responding to Solar and Dust Storm Drivers: Hisaki Space Telescope Observations"}]},{"@id":"https://cir.nii.ac.jp/crid/2051714792011282432","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Modelling cometary meteoroid stream traverses of the Martian Moons eXploration (MMX) spacecraft en route to Phobos"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1002/2015gl063863"},{"@type":"CROSSREF","@value":"10.1002/2016gl068388_references_DOI_KH5RaawkhsvBlmfEzXxS8H8a4n4"},{"@type":"CROSSREF","@value":"10.1029/2020je006500_references_DOI_KH5RaawkhsvBlmfEzXxS8H8a4n4"},{"@type":"CROSSREF","@value":"10.1186/s40623-021-01412-5_references_DOI_KH5RaawkhsvBlmfEzXxS8H8a4n4"}]}