{"@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/1361699996003300864.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1051/swsc/2018020"}},{"identifier":{"@type":"URI","@value":"https://www.swsc-journal.org/10.1051/swsc/2018020/pdf"}}],"dc:title":[{"@value":"EUHFORIA: European heliospheric forecasting information asset"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>The implementation and first results of the new space weather forecasting-targeted inner heliosphere model “European heliospheric forecasting information asset” (EUHFORIA) are presented. EUHFORIA consists of two major components: a coronal model and a heliosphere model including coronal mass ejections. The coronal model provides data-driven solar wind plasma parameters at 0.1 AU by constructing a magnetic field model of the coronal large-scale magnetic field and employing empirical relations to determine the plasma state such as the solar wind speed and mass density. These are then used as boundary conditions to drive a three-dimensional time-dependent magnetohydrodynamics model of the inner heliosphere up to 2 AU. CMEs are injected into the ambient solar wind modeled using the cone model, with their parameters obtained from fits to imaging observations. In addition to detailing the modeling methodology, an initial validation run is presented. The results feature a highly dynamic heliosphere that the model is able to capture in good agreement with in situ observations. Finally, future horizons for the model are outlined.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1381699996003300865","@type":"Researcher","foaf:name":[{"@value":"Jens Pomoell"}]},{"@id":"https://cir.nii.ac.jp/crid/1381699996003300864","@type":"Researcher","foaf:name":[{"@value":"S. Poedts"}]}],"publication":{"publicationIdentifier":[{"@type":"EISSN","@value":"21157251"}],"prism:publicationName":[{"@value":"Journal of Space Weather and Space Climate"}],"dc:publisher":[{"@value":"EDP Sciences"}],"prism:publicationDate":"2018","prism:volume":"8","prism:startingPage":"A35"},"reviewed":"false","dc:rights":["http://creativecommons.org/licenses/by/4.0"],"url":[{"@id":"https://www.swsc-journal.org/10.1051/swsc/2018020/pdf"}],"createdAt":"2018-06-26","modifiedAt":"2020-03-20","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360294643708714496","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"BepiColombo Science Investigations During Cruise and Flybys at the Earth, Venus and Mercury"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576118776686336","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"BepiColombo’s Cruise Phase: Unique Opportunity for Synergistic Observations"}]},{"@id":"https://cir.nii.ac.jp/crid/1360584341820448640","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Magnetohydrodynamic simulation of coronal mass ejections using interplanetary scintillation data observed from radio sites ISEE and LOFAR"}]},{"@id":"https://cir.nii.ac.jp/crid/2050025942148522496","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Validation of coronal mass ejection arrival-time forecasts by magnetohydrodynamic simulations based on interplanetary scintillation observations"}]},{"@id":"https://cir.nii.ac.jp/crid/2050870367078673408","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A review of the SCOSTEP’s 5-year scientific program VarSITI—Variability of the Sun and Its Terrestrial Impact"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1051/swsc/2018020"},{"@type":"CROSSREF","@value":"10.1186/s40645-021-00410-1_references_DOI_YyDuQ5NAAeDeqXoccr17UmRCbLw"},{"@type":"CROSSREF","@value":"10.1007/s11214-021-00797-9_references_DOI_YyDuQ5NAAeDeqXoccr17UmRCbLw"},{"@type":"CROSSREF","@value":"10.3389/fspas.2021.718024_references_DOI_YyDuQ5NAAeDeqXoccr17UmRCbLw"},{"@type":"CROSSREF","@value":"10.1016/j.asr.2022.09.028_references_DOI_YyDuQ5NAAeDeqXoccr17UmRCbLw"},{"@type":"CROSSREF","@value":"10.1186/s40623-020-01345-5_references_DOI_YyDuQ5NAAeDeqXoccr17UmRCbLw"}]}