{"@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/1362825894138224768.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1002/2014ja020239"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2014JA020239"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/2014JA020239"}},{"identifier":{"@type":"DOI","@value":"10.35099/aurora-570"}}],"dc:title":[{"@value":"The Comprehensive Inner Magnetosphere‐Ionosphere Model"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title><jats:p>Simulation studies of the Earth's radiation belts and ring current are very useful in understanding the acceleration, transport, and loss of energetic particles. Recently, the Comprehensive Ring Current Model (CRCM) and the Radiation Belt Environment (RBE) model were merged to form a Comprehensive Inner Magnetosphere‐Ionosphere (CIMI) model. CIMI solves for many essential quantities in the inner magnetosphere, including ion and electron distributions in the ring current and radiation belts, plasmaspheric density, Region 2 currents, convection potential, and precipitation in the ionosphere. It incorporates whistler mode chorus and hiss wave diffusion of energetic electrons in energy, pitch angle, and cross terms. CIMI thus represents a comprehensive model that considers the effects of the ring current and plasmasphere on the radiation belts. We have performed a CIMI simulation for the storm on 5–9 April 2010 and then compared our results with data from the Two Wide‐angle Imaging Neutral‐atom Spectrometers and Akebono satellites. We identify the dominant energization and loss processes for the ring current and radiation belts. We find that the interactions with the whistler mode chorus waves are the main cause of the flux increase of MeV electrons during the recovery phase of this particular storm. When a self‐consistent electric field from the CRCM is used, the enhancement of MeV electrons is higher than when an empirical convection model is applied. We also demonstrate how CIMI can be a powerful tool for analyzing and interpreting data from the new Van Allen Probes mission.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380579819466488321","@type":"Researcher","foaf:name":[{"@value":"M.‐C. Fok"}],"jpcoar:affiliationName":[{"@value":"NASA Goddard Space Flight Center  Greenbelt Maryland USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825894138224768","@type":"Researcher","foaf:name":[{"@value":"N. Y. Buzulukova"}],"jpcoar:affiliationName":[{"@value":"NASA Goddard Space Flight Center  Greenbelt Maryland USA"},{"@value":"Center for Research and Exploration in Space Science and Technology University of Maryland  College Park Maryland USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380579819466488320","@type":"Researcher","foaf:name":[{"@value":"S.‐H. Chen"}],"jpcoar:affiliationName":[{"@value":"NASA Goddard Space Flight Center  Greenbelt Maryland USA"},{"@value":"Center for Research and Exploration in Space Science and Technology Universities Space Research Association  Columbia Maryland USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825894138224774","@type":"Researcher","foaf:name":[{"@value":"A. Glocer"}],"jpcoar:affiliationName":[{"@value":"NASA Goddard Space Flight Center  Greenbelt Maryland USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825894138224770","@type":"Researcher","foaf:name":[{"@value":"T. Nagai"}],"jpcoar:affiliationName":[{"@value":"Department of Earth and Planetary Sciences Tokyo Institute of Technology  Tokyo Japan"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825894138224772","@type":"Researcher","foaf:name":[{"@value":"P. Valek"}],"jpcoar:affiliationName":[{"@value":"Southwest Research Institute  San Antonio Texas USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825894138224773","@type":"Researcher","foaf:name":[{"@value":"J. D. Perez"}],"jpcoar:affiliationName":[{"@value":"Physics Department Auburn University  Auburn Alabama USA"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"21699380"},{"@type":"EISSN","@value":"21699402"}],"prism:publicationName":[{"@value":"Journal of Geophysical Research: Space Physics"}],"dc:publisher":[{"@value":"American Geophysical Union (AGU)"}],"prism:publicationDate":"2014-09","prism:volume":"119","prism:number":"9","prism:startingPage":"7522","prism:endingPage":"7540"},"reviewed":"false","dcterms:accessRights":"http://purl.org/coar/access_right/c_abf2","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2014JA020239"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/2014JA020239"}],"createdAt":"2014-09-04","modifiedAt":"2023-10-03","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050009562087380864","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Nonlinear Wave Growth Analysis of Whistler‐Mode Chorus Generation Regions Based on Coupled MHD and Advection Simulation of the Inner Magnetosphere"}]},{"@id":"https://cir.nii.ac.jp/crid/1050564288161077632","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Theory, Modeling, and Integrated studies in the Arase (ERG) project"}]},{"@id":"https://cir.nii.ac.jp/crid/1050855345496386560","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Study of an Equatorward Detachment of Auroral Arc From the Oval Using Ground‐Space Observations and the BATS‐R‐US–CIMI Model"}]},{"@id":"https://cir.nii.ac.jp/crid/1360290617758485120","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Soft X‐ray and ENA Imaging of the Earth's Dayside Magnetosphere"}]},{"@id":"https://cir.nii.ac.jp/crid/1360298754807887232","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Excitation of Two Types of Storm‐Time Pc5 ULF Waves by Ring Current Ions Based on the Magnetosphere‐Ionosphere Coupled Model"}]},{"@id":"https://cir.nii.ac.jp/crid/1360580230583827712","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Thermospheric Density Perturbations Produced by Traveling Atmospheric Disturbances During August 2005 Storm"}]},{"@id":"https://cir.nii.ac.jp/crid/1360588379379003904","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Global validation of data-assimilative electron ring current nowcast for space weather applications"}]},{"@id":"https://cir.nii.ac.jp/crid/1360588380591389312","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Development of a Surface Charging Assessment System for the GEO Region by Combining Global Magnetosphere MHD and Spacecraft Charging Models"}]},{"@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":"10.1002/2014ja020239"},{"@type":"OPENAIRE","@value":"doi_dedup___::1b646d01231f7ca01e61f3c62711b136"},{"@type":"CROSSREF","@value":"10.1186/s40645-021-00410-1_references_DOI_FM7uwRvC0P2Cm6kLW2p4R35sk1L"},{"@type":"CROSSREF","@value":"10.1109/tps.2024.3519295_references_DOI_5OtZ79knFqRW77FfnQjppDF8QTx"},{"@type":"CROSSREF","@value":"10.1029/2020ja028816_references_DOI_FM7uwRvC0P2Cm6kLW2p4R35sk1L"},{"@type":"CROSSREF","@value":"10.1029/2020ja029080_references_DOI_FM7uwRvC0P2Cm6kLW2p4R35sk1L"},{"@type":"CROSSREF","@value":"10.1029/2022ja030486_references_DOI_FM7uwRvC0P2Cm6kLW2p4R35sk1L"},{"@type":"CROSSREF","@value":"10.1029/2021ja030071_references_DOI_FM7uwRvC0P2Cm6kLW2p4R35sk1L"},{"@type":"CROSSREF","@value":"10.1038/s41598-024-52187-0_references_DOI_FM7uwRvC0P2Cm6kLW2p4R35sk1L"},{"@type":"CROSSREF","@value":"10.1186/s40623-018-0785-9_references_DOI_FM7uwRvC0P2Cm6kLW2p4R35sk1L"},{"@type":"CROSSREF","@value":"10.1029/2019ja026951_references_DOI_FM7uwRvC0P2Cm6kLW2p4R35sk1L"}]}