{"@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/1361137045189177088.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1029/2004ja010424"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2004JA010424"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2004JA010424"}}],"dc:title":[{"@value":"Dynamic coordinates for auroral ion outflow"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>The ionosphere provides a large and variable fraction of the plasma that makes up the Earth's magnetosphere. The sparseness of ion outflow observations and limitations of global magnetospheric models have limited progress in understanding how spatial and temporal variations in the ionospheric component of the magnetosphere affects magnetospheric processes such as storms and substorms. Moreover, because existing comprehensive ion outflow data sets are not organized in terms of large‐scale, dynamic, magnetospheric features, they cannot be used as boundary conditions or ground truth for large‐scale magnetospheric models. This paper presents a method to self‐consistently generate dynamic auroral zone boundaries from ion and electron data obtained on the same platform with mass‐resolved ion outflow observations. We show that this dynamic coordinate system can be used to organize the ion outflow observations so that they are compatible to use with large‐scale magnetospheric models.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380013168772453533","@type":"Researcher","foaf:name":[{"@value":"L. Andersson"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado  Boulder Colorado USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380861295177768065","@type":"Researcher","foaf:name":[{"@value":"W. K. Peterson"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado  Boulder Colorado USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380861295177768064","@type":"Researcher","foaf:name":[{"@value":"K. M. McBryde"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado  Boulder Colorado USA"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"01480227"}],"prism:publicationName":[{"@value":"Journal of Geophysical Research: Space Physics"}],"dc:publisher":[{"@value":"American Geophysical Union (AGU)"}],"prism:publicationDate":"2004-08","prism:volume":"109","prism:number":"A8","prism:startingPage":"A08201"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2004JA010424"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2004JA010424"}],"createdAt":"2004-08-05","modifiedAt":"2023-10-31","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360285704777305984","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Relationship between auroral substorm and ion upflow in the nightside polar ionosphere"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285708265409024","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Photoelectron flows in the polar wind during geomagnetically quiet periods"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567179757574784","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"An extensive survey of dayside diffuse aurora based on optical observations at Yellow River Station"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567180128519936","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Reduction of the field‐aligned potential drop in the polar cap during large geomagnetic storms"}]},{"@id":"https://cir.nii.ac.jp/crid/2051996266990212224","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"On the relationship between energy input to the ionosphere and the ion outflow flux under different solar zenith angles"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1029/2004ja010424"},{"@type":"CROSSREF","@value":"10.1186/s40623-021-01532-y_references_DOI_WDQ75EBva1qYMOb9R34w6Bvs8j0"},{"@type":"CROSSREF","@value":"10.1002/2013ja018965_references_DOI_WDQ75EBva1qYMOb9R34w6Bvs8j0"},{"@type":"CROSSREF","@value":"10.1029/2011ja017459_references_DOI_WDQ75EBva1qYMOb9R34w6Bvs8j0"},{"@type":"CROSSREF","@value":"10.1002/2015ja021699_references_DOI_WDQ75EBva1qYMOb9R34w6Bvs8j0"},{"@type":"CROSSREF","@value":"10.1002/jgra.50450_references_DOI_WDQ75EBva1qYMOb9R34w6Bvs8j0"}]}