{"@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/1361137045479513728.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.3847/1538-4365/ab05cf"}},{"identifier":{"@type":"URI","@value":"https://iopscience.iop.org/article/10.3847/1538-4365/ab05cf/pdf"}},{"identifier":{"@type":"URI","@value":"https://iopscience.iop.org/article/10.3847/1538-4365/ab05cf"}}],"dc:title":[{"@value":"CHIANTI—An Atomic Database for Emission Lines. XV. Version 9, Improvements for the X-Ray Satellite Lines"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title>\n               <jats:p>CHIANTI contains a large quantity of atomic data for the analysis of astrophysical spectra. Programs are available in IDL and Python to perform calculation of the expected emergent spectrum from these sources. The database includes atomic energy levels, wavelengths, radiative transition probabilities, rate coefficients for collisional excitation, ionization, and recombination, as well as data to calculate free–free, free–bound, and two-photon continuum emission. In Version 9, we improve the modeling of the satellite lines at X-ray wavelengths by explicitly including autoionization and dielectronic recombination processes in the calculation of level populations for select members of the lithium isoelectronic sequence and Fe <jats:sc>xviii–xxiii</jats:sc>. In addition, existing data sets are updated, new ions are added, and new total recombination rates for several Fe ions are included. All data and IDL programs are freely available at <jats:ext-link xmlns:xlink=\"http://www.w3.org/1999/xlink\" ext-link-type=\"uri\" xlink:href=\"http://www.chiantidatabase.org\" xlink:type=\"simple\">http://www.chiantidatabase.org</jats:ext-link> or through SolarSoft, and the Python code ChiantiPy is also freely available at <jats:ext-link xmlns:xlink=\"http://www.w3.org/1999/xlink\" ext-link-type=\"uri\" xlink:href=\"https://github.com/chianti-atomic/ChiantiPy\" xlink:type=\"simple\">https://github.com/chianti-atomic/ChiantiPy</jats:ext-link>.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380009142451590151","@type":"Researcher","foaf:name":[{"@value":"K. P. Dere"}]},{"@id":"https://cir.nii.ac.jp/crid/1381137045479513729","@type":"Researcher","foaf:name":[{"@value":"G. Del Zanna"}]},{"@id":"https://cir.nii.ac.jp/crid/1381137045479513732","@type":"Researcher","foaf:name":[{"@value":"P. R. Young"}]},{"@id":"https://cir.nii.ac.jp/crid/1381137045479513728","@type":"Researcher","foaf:name":[{"@value":"E. Landi"}]},{"@id":"https://cir.nii.ac.jp/crid/1381137045479513731","@type":"Researcher","foaf:name":[{"@value":"R. S. Sutherland"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00670049"},{"@type":"EISSN","@value":"15384365"}],"prism:publicationName":[{"@value":"The Astrophysical Journal Supplement Series"}],"dc:publisher":[{"@value":"American Astronomical Society"}],"prism:publicationDate":"2019-03-27","prism:volume":"241","prism:number":"2","prism:startingPage":"22"},"reviewed":"false","dc:rights":["https://iopscience.iop.org/page/copyright","https://iopscience.iop.org/info/page/text-and-data-mining"],"url":[{"@id":"https://iopscience.iop.org/article/10.3847/1538-4365/ab05cf/pdf"},{"@id":"https://iopscience.iop.org/article/10.3847/1538-4365/ab05cf"}],"createdAt":"2019-03-27","modifiedAt":"2024-01-17","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360013168774488064","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Evaluation of Fe XIV Intensity Ratio for Electron Density Diagnostics by Laboratory Measurements"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576118818048128","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"The Energy Conversion Rate of an Active Region Transient Brightening Estimated by Hinode Spectroscopic Observations"}]},{"@id":"https://cir.nii.ac.jp/crid/1360580229817817600","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Statistical analysis for EUV dynamic spectra and their impact on the ionosphere during solar flares"}]},{"@id":"https://cir.nii.ac.jp/crid/1360584341829762944","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A Comprehensive Simulation of Solar Wind Formation from the Solar Interior: Significant Cross-field Energy Transport by Interchange Reconnection near the Sun"}]},{"@id":"https://cir.nii.ac.jp/crid/2050588892101958144","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Validation of computed extreme ultraviolet emission spectra during solar flares"}]},{"@id":"https://cir.nii.ac.jp/crid/2050588892104440832","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Model-based reproduction and validation of the total spectra of a solar flare and their impact on the global environment at the X9.3 event of September 6, 2017"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.3847/1538-4365/ab05cf"},{"@type":"CROSSREF","@value":"10.1186/s40623-021-01376-6_references_DOI_9m6gL4skKix0lzYNha0GdBXuCf3"},{"@type":"CROSSREF","@value":"10.1186/s40623-021-01402-7_references_DOI_9m6gL4skKix0lzYNha0GdBXuCf3"},{"@type":"CROSSREF","@value":"10.3390/atoms9030060_references_DOI_9m6gL4skKix0lzYNha0GdBXuCf3"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ac09eb_references_DOI_9m6gL4skKix0lzYNha0GdBXuCf3"},{"@type":"CROSSREF","@value":"10.1186/s40623-023-01788-6_references_DOI_9m6gL4skKix0lzYNha0GdBXuCf3"},{"@type":"CROSSREF","@value":"10.3847/2041-8213/acdde0_references_DOI_9m6gL4skKix0lzYNha0GdBXuCf3"},{"@type":"CROSSREF","@value":"10.21203/rs.3.rs-2185113/v1_references_DOI_9m6gL4skKix0lzYNha0GdBXuCf3"}]}