{"@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/1362825896156855936.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1002/2017ja024178"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2017JA024178"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/2017JA024178"}}],"dc:title":[{"@value":"Generation of rising‐tone chorus in a two‐dimensional mirror field by using the general curvilinear PIC code"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title><jats:p>Recently, the generation of rising‐tone chorus has been implemented with one‐dimensional (1‐D) particle‐in‐cell (PIC) simulations in an inhomogeneous background magnetic field, where both the propagation of waves and motion of electrons are simply forced to be parallel to the background magnetic field. In this paper, we have developed a two‐dimensional (2‐D) general curvilinear PIC simulation code and successfully reproduced rising‐tone chorus waves excited from an anisotropic electron distribution in a 2‐D mirror field. Our simulation results show that whistler waves are mainly generated around the magnetic equator and continuously gain growth during their propagation toward higher‐latitude regions. The rising‐tone chorus waves are observed off the magnetic equator, which propagate quasi‐parallel to the background magnetic field with the wave normal angle smaller than 25°. Due to the propagating effect, the wave normal angle of chorus waves is increasing during their propagation toward higher‐latitude regions along an enough curved field line. The chirping rate of chorus waves is found to be larger along a field line with a smaller curvature.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1382825896156855937","@type":"Researcher","foaf:name":[{"@value":"Yangguang Ke"}],"jpcoar:affiliationName":[{"@value":"CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Science University of Science and Technology of China  Hefei China"},{"@value":"Collaborative Innovation Center of Astronautical Science and Technology  Harbin China"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825896156855936","@type":"Researcher","foaf:name":[{"@value":"Xinliang Gao"}],"jpcoar:affiliationName":[{"@value":"CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Science University of Science and Technology of China  Hefei China"},{"@value":"Collaborative Innovation Center of Astronautical Science and Technology  Harbin China"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825896156855940","@type":"Researcher","foaf:name":[{"@value":"Quanming Lu"}],"jpcoar:affiliationName":[{"@value":"CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Science University of Science and Technology of China  Hefei China"},{"@value":"Collaborative Innovation Center of Astronautical Science and Technology  Harbin China"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825896156855939","@type":"Researcher","foaf:name":[{"@value":"Xueyi Wang"}],"jpcoar:affiliationName":[{"@value":"Physics Department Auburn University  Auburn Alabama USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825896156855938","@type":"Researcher","foaf:name":[{"@value":"Shui Wang"}],"jpcoar:affiliationName":[{"@value":"CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Science University of Science and Technology of China  Hefei China"},{"@value":"Collaborative Innovation Center of Astronautical Science and Technology  Harbin China"}]}],"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":"2017-08","prism:volume":"122","prism:number":"8","prism:startingPage":"8154","prism:endingPage":"8165"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2017JA024178"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/2017JA024178"}],"createdAt":"2017-07-26","modifiedAt":"2023-10-02","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050282677835957376","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Cyclotron Acceleration of Relativistic Electrons Through Landau Resonance With Obliquely Propagating Whistler‐Mode Chorus Emissions"},{"@value":"Cyclotron acceleration of relativistic electrons through landau resonance with obliquely propagating whistler mode chorus emissions"}]},{"@id":"https://cir.nii.ac.jp/crid/1360290617718440960","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Observations of the Source Region of Whistler Mode Waves in Magnetosheath Mirror Structures"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857593671704704","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Measurability of the Nonlinear Response of Electron Distribution Function to Chorus Emissions in the Earth's Radiation Belt"}]},{"@id":"https://cir.nii.ac.jp/crid/1361131418080147072","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A Systematic Study in Characteristics of Lower Band Rising‐Tone Chorus Elements"}]},{"@id":"https://cir.nii.ac.jp/crid/2051433317034572672","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Nonlinear wave growth theory of whistler-mode chorus and hiss emissions in the magnetosphere"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1002/2017ja024178"},{"@type":"CROSSREF","@value":"10.1029/2019ja027488_references_DOI_3LPcyogNwmL7vTFH6ITfKykl6yB"},{"@type":"CROSSREF","@value":"10.1186/s40623-021-01380-w_references_DOI_3LPcyogNwmL7vTFH6ITfKykl6yB"},{"@type":"CROSSREF","@value":"10.1029/2018ja026374_references_DOI_3LPcyogNwmL7vTFH6ITfKykl6yB"},{"@type":"CROSSREF","@value":"10.1029/2021ja029624_references_DOI_3LPcyogNwmL7vTFH6ITfKykl6yB"},{"@type":"CROSSREF","@value":"10.1029/2019ja027368_references_DOI_3LPcyogNwmL7vTFH6ITfKykl6yB"}]}