{"@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/1363388845450910208.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1029/2009gl041814"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2009GL041814"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2009GL041814"}}],"dc:title":[{"@value":"Pumping out the atmosphere of Mars through solar wind pressure pulses"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>We study atmospheric escape from Mars during solar wind pressure pulses. During the solar minimum of 2007–08 we have observed 41 high pressure events, which are predominantly identified as corotating interaction regions (CIR) while a few are coronal mass ejections (CME), in data from the Advanced Composition Explorer (ACE) upstream of the Earth. 36 of these events are also identified using Mars Express (MEX) data at Mars. We use MEX measurements at Mars to compare the antisunward fluxes of heavy planetary ions during the passage of these pulses to the fluxes during quiet solar wind conditions. The ion fluxes are observed to increase by a factor of ∼2.5, on average. Hence, a third of the total outflow from Mars takes place during ∼15% of the time, when a solar wind pressure pulse impacts on the planet. This can have important consequences for the total time‐integrated outflow of plasma from Mars.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380576118725867527","@type":"Researcher","foaf:name":[{"@value":"N. J. T. Edberg"}],"jpcoar:affiliationName":[{"@value":"Department of Physics and Astronomy University of Leicester  Leicester UK"},{"@value":"Swedish Institute of Space Physics  Uppsala Sweden"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388845450910208","@type":"Researcher","foaf:name":[{"@value":"H. Nilsson"}],"jpcoar:affiliationName":[{"@value":"Swedish Institute of Space Physics  Kiruna Sweden"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388845450910212","@type":"Researcher","foaf:name":[{"@value":"A. O. Williams"}],"jpcoar:affiliationName":[{"@value":"Department of Physics and Astronomy University of Leicester  Leicester UK"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388845450910080","@type":"Researcher","foaf:name":[{"@value":"M. Lester"}],"jpcoar:affiliationName":[{"@value":"Department of Physics and Astronomy University of Leicester  Leicester UK"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388845450910081","@type":"Researcher","foaf:name":[{"@value":"S. E. Milan"}],"jpcoar:affiliationName":[{"@value":"Department of Physics and Astronomy University of Leicester  Leicester UK"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388845450910209","@type":"Researcher","foaf:name":[{"@value":"S. W. H. Cowley"}],"jpcoar:affiliationName":[{"@value":"Department of Physics and Astronomy University of Leicester  Leicester UK"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388845450910213","@type":"Researcher","foaf:name":[{"@value":"M. Fränz"}],"jpcoar:affiliationName":[{"@value":"Max Planck Institute for Solar System Research  Katlenburg‐Lindau Germany"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388845450910082","@type":"Researcher","foaf:name":[{"@value":"S. Barabash"}],"jpcoar:affiliationName":[{"@value":"Swedish Institute of Space Physics  Kiruna Sweden"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388845450910210","@type":"Researcher","foaf:name":[{"@value":"Y. Futaana"}],"jpcoar:affiliationName":[{"@value":"Swedish Institute of Space Physics  Kiruna Sweden"}]}],"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":"2010-02","prism:volume":"37","prism:number":"3","prism:startingPage":"L03107"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2009GL041814"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2009GL041814"}],"createdAt":"2010-02-15","modifiedAt":"2023-10-30","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050307746540945536","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"The Mars system revealed by the Martian Moons eXploration mission"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004233289579648","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A newly developed UHF radiotelescope for interplanetary scintillation observations: Solar Wind Imaging Facility"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285704778136064","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Inner heliosphere MHD modeling system applicable to space weather forecasting for the other planets"}]},{"@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/1360567180075629440","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Dependence of O<sup>+</sup> escape rate from the Venusian upper atmosphere on IMF directions"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848657114616832","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Loss of the Martian atmosphere to space: Present-day loss rates determined from MAVEN observations and integrated loss through time"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848660885719680","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"MAVEN observations of the response of Mars to an interplanetary coronal mass ejection"}]},{"@id":"https://cir.nii.ac.jp/crid/1360861707120239616","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Enhanced Ion Escape Rate During IMF Rotation Under Weak Intrinsic Magnetic Field Conditions on a Mars‐Like Planet"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1029/2009gl041814"},{"@type":"CROSSREF","@value":"10.1029/2011rs004694_references_DOI_8nNDLIf422NqqJAyYIHnBJbYjg1"},{"@type":"CROSSREF","@value":"10.1002/2013sw000989_references_DOI_8nNDLIf422NqqJAyYIHnBJbYjg1"},{"@type":"CROSSREF","@value":"10.1002/jgra.50494_references_DOI_8nNDLIf422NqqJAyYIHnBJbYjg1"},{"@type":"CROSSREF","@value":"10.1126/science.aad0210_references_DOI_8nNDLIf422NqqJAyYIHnBJbYjg1"},{"@type":"CROSSREF","@value":"10.1002/grl.50392_references_DOI_8nNDLIf422NqqJAyYIHnBJbYjg1"},{"@type":"CROSSREF","@value":"10.1016/j.icarus.2018.05.030_references_DOI_8nNDLIf422NqqJAyYIHnBJbYjg1"},{"@type":"CROSSREF","@value":"10.1186/s40623-021-01417-0_references_DOI_8nNDLIf422NqqJAyYIHnBJbYjg1"},{"@type":"CROSSREF","@value":"10.1029/2022ja030510_references_DOI_8nNDLIf422NqqJAyYIHnBJbYjg1"}]}