{ "labelLang" : "hun", "responseDate" : "2024-03-28 21:42", "content" : { "otype" : "JournalArticle", "mtid" : 31057123, "status" : "VALIDATED", "published" : true, "comment" : "Funding Agency and Grant Number: JSPS KAKENHI [JP15H05816, JP18H04436, JP19K14756]; ISEE CICR International Workshop program; NASA\n Funding text: This work was supported by JSPS KAKENHI grant No. JP15H05816, JP18H04436, and JP19K14756. This work was also partially supported by ISEE CICR International Workshop program, and the authors would like to thank all the members of the workshop. Numerical computations were carried out in the Center for Integrated Data Science, Institute for SpaceEarth Environmental Research, Nagoya University through the joint research program. Wilcox Solar Observatory data used in this study were obtained via the website. http://wso.stanford.edu.The Wilcox Solar Observatory is currently supported by NASA. NSO/Kitt Peak data used here are produced cooperatively by NSF/NOAO, NASA/GSFC, and NOAA/SEL. Data were acquired by SOLIS instruments operated by NISP/NSO/AURA/NSF. Data storage was supported by the University of Colorado Boulder \"PetaLibrary.\"", "unhandledTickets" : 0, "deleted" : false, "lastRefresh" : "2023-04-24T10:31:21.252+0000", "lastModified" : "2020-01-09T01:14:54.956+0000", "created" : "2020-01-09T01:14:54.150+0000", "creator" : { "otype" : "Admin", "mtid" : 565, "link" : "/api/admin/565", "label" : "WoS import (admin)", "familyName" : "WoS", "givenName" : "import", "published" : true, "snippet" : true }, "lastDuplumSearch" : "2023-04-24T10:23:36.424+0000", "validated" : "2020-01-09T01:14:54.243+0000", "validator" : { "otype" : "Admin", "mtid" : 565, "link" : "/api/admin/565", "label" : "WoS import (admin)", "familyName" : "WoS", "givenName" : "import", "published" : true, "snippet" : true }, "core" : false, "citation" : true, "publicationPending" : false, "type" : { "otype" : "PublicationType", "mtid" : 24, "link" : "/api/publicationtype/24", "label" : "Folyóiratcikk", "code" : 24, "otypeName" : "JournalArticle", "listPosition" : 1, "published" : true, "oldId" : 24, "snippet" : true }, "subType" : { "otype" : "SubType", "mtid" : 10000059, "link" : "/api/subtype/10000059", "label" : "Szakcikk (Folyóiratcikk)", "name" : "Szakcikk", "nameEng" : "Article", "docType" : { "otype" : "PublicationType", "mtid" : 24, "link" : "/api/publicationtype/24", "label" : "Folyóiratcikk", "code" : 24, "otypeName" : "JournalArticle", "listPosition" : 1, "published" : true, "oldId" : 24, "snippet" : true }, "listPosition" : 101, "published" : true, "oldId" : 10000059, "snippet" : true }, "category" : { "otype" : "Category", "mtid" : 1, "link" : "/api/category/1", "label" : "Tudományos", "published" : true, "oldId" : 1, "snippet" : true }, "languages" : [ { "otype" : "Language", "mtid" : 10002, "link" : "/api/language/10002", "label" : "Angol", "name" : "Angol", "nameEng" : "English", "published" : true, "oldId" : 2, "snippet" : true } ], "firstAuthor" : "Iijima, H.", "authorships" : [ { "otype" : "PersonAuthorship", "mtid" : 89908011, "link" : "/api/authorship/89908011", "label" : "Iijima, H. ✉", "listPosition" : 1, "share" : 0.0, "first" : true, "last" : false, "corresponding" : true, "familyName" : "Iijima", "givenName" : "H.", "authorTyped" : true, "editorTyped" : false, "otherTyped" : false, "type" : { "otype" : "AuthorshipType", "mtid" : 1, "link" : "/api/authorshiptype/1", "label" : "Szerző", "code" : 0, "published" : true, "oldId" : 0, "snippet" : true }, "published" : false, "snippet" : true }, { "otype" : "PersonAuthorship", "mtid" : 89908012, "link" : "/api/authorship/89908012", "label" : "Hotta, H.", "listPosition" : 2, "share" : 0.0, "first" : false, "last" : false, "corresponding" : false, "familyName" : "Hotta", "givenName" : "H.", "authorTyped" : true, "editorTyped" : false, "otherTyped" : false, "type" : { "otype" : "AuthorshipType", "mtid" : 1, "link" : "/api/authorshiptype/1", "label" : "Szerző", "code" : 0, "published" : true, "oldId" : 0, "snippet" : true }, "published" : false, "snippet" : true }, { "otype" : "PersonAuthorship", "mtid" : 89908013, "link" : "/api/authorship/89908013", "label" : "Imada, S.", "listPosition" : 3, "share" : 0.0, "first" : false, "last" : true, "corresponding" : false, "familyName" : "Imada", "givenName" : "S.", "authorTyped" : true, "editorTyped" : false, "otherTyped" : false, "type" : { "otype" : "AuthorshipType", "mtid" : 1, "link" : "/api/authorshiptype/1", "label" : "Szerző", "code" : 0, "published" : true, "oldId" : 0, "snippet" : true }, "published" : false, "snippet" : true } ], "title" : "Effect of Morphological Asymmetry between Leading and Following Sunspots on the Prediction of Solar Cycle Activity", "identifiers" : [ { "otype" : "PublicationIdentifier", "mtid" : 16385525, "link" : "/api/publicationidentifier/16385525", "label" : "DOI: 10.3847/1538-4357/ab3b04", "source" : { "otype" : "PlainSource", "mtid" : 6, "link" : "/api/publicationsource/6", "label" : "DOI", "type" : { "otype" : "PublicationSourceType", "mtid" : 10001, "link" : "/api/publicationsourcetype/10001", "label" : "DOI", "mayHaveOa" : true, "published" : true, "snippet" : true }, "name" : "DOI", "nameEng" : "DOI", "linkPattern" : "https://doi.org/@@@", "publiclyVisible" : true, "published" : true, "oldId" : 6, "snippet" : true }, "validState" : "IDENTICAL", "idValue" : "10.3847/1538-4357/ab3b04", "realUrl" : "https://doi.org/10.3847/1538-4357/ab3b04", "published" : false, "snippet" : true }, { "otype" : "PublicationIdentifier", "mtid" : 16385524, "link" : "/api/publicationidentifier/16385524", "label" : "WoS: 000487689000002", "source" : { "otype" : "PlainSource", "mtid" : 1, "link" : "/api/publicationsource/1", "label" : "WoS", "type" : { "otype" : "PublicationSourceType", "mtid" : 10003, "link" : "/api/publicationsourcetype/10003", "label" : "Indexelő adatbázis", "mayHaveOa" : false, "published" : true, "snippet" : true }, "name" : "WoS", "nameEng" : "WoS", "linkPattern" : "https://www.webofscience.com/wos/woscc/full-record/@@@", "publiclyVisible" : true, "published" : true, "oldId" : 1, "snippet" : true }, "validState" : "IDENTICAL", "idValue" : "000487689000002", "realUrl" : "https://www.webofscience.com/wos/woscc/full-record/000487689000002", "published" : false, "snippet" : true }, { "otype" : "PublicationIdentifier", "mtid" : 21986582, "link" : "/api/publicationidentifier/21986582", "label" : "Scopus: 85073185564", "source" : { "otype" : "PlainSource", "mtid" : 3, "link" : "/api/publicationsource/3", "label" : "Scopus", "type" : { "otype" : "PublicationSourceType", "mtid" : 10003, "link" : "/api/publicationsourcetype/10003", "label" : "Indexelő adatbázis", "mayHaveOa" : false, "published" : true, "snippet" : true }, "name" : "Scopus", "linkPattern" : "http://www.scopus.com/record/display.url?origin=inward&eid=2-s2.0-@@@", "publiclyVisible" : true, "published" : true, "oldId" : 3, "snippet" : true }, "validState" : "IDENTICAL", "idValue" : "85073185564", "realUrl" : "http://www.scopus.com/record/display.url?origin=inward&eid=2-s2.0-85073185564", "published" : false, "snippet" : true } ], "journal" : { "otype" : "Journal", "mtid" : 559, "link" : "/api/journal/559", "label" : "ASTROPHYSICAL JOURNAL 1538-4357 0004-637X", "pIssn" : "1538-4357", "eIssn" : "0004-637X", "reviewType" : "REVIEWED", "noIF" : false, "sciIndexed" : true, "scopusIndexed" : true, "lang" : "FOREIGN", "hungarian" : false, "published" : true, "oldId" : 559, "snippet" : true }, "volume" : "883", "issue" : "1", "internalId" : "24", "firstPageOrInternalIdForSort" : "24", "pageLength" : 11, "publishedYear" : 2019, "abstractText" : "The morphological asymmetry of leading and following sunspots is a well-known characteristic of the solar surface. In the context of the large-scale evolution of the surface magnetic field, the asymmetry has been assumed to have only a negligible effect. Using the surface flux transport (SFT) model, we show that the morphological asymmetry of leading and following sunspots has a significant impact on the evolution of the large-scale magnetic field on the solar surface. By evaluating the effect of the morphological asymmetry of each bipolar magnetic region (BMR), we observe that the introduction of asymmetry to the BMR model significantly reduces the contribution to the polar magnetic field, especially for large and high-latitude BMRs. Strongly asymmetric BMRs can even reverse regular polar field formation. The SFT simulations based on the observed sunspot record show that the introduction of morphological asymmetry reduces the root-mean-square difference from the observed axial dipole strength by 30%-40%. These results indicate that the morphological asymmetry of leading and following sunspots has a significant effect on the solar cycle prediction.", "subjects" : [ { "otype" : "Classification", "mtid" : 10154, "link" : "/api/classification/10154", "label" : "Fizika", "published" : true, "snippet" : true } ], "keywords" : [ { "otype" : "Keyword", "mtid" : 1092108, "link" : "/api/keyword/1092108", "label" : "sunspots", "published" : true, "oldId" : 1092108, "snippet" : true }, { "otype" : "Keyword", "mtid" : 1092219, "link" : "/api/keyword/1092219", "label" : "Sun: activity", "published" : true, "oldId" : 1092219, "snippet" : true }, { "otype" : "Keyword", "mtid" : 1202329, "link" : "/api/keyword/1202329", "label" : "Sun: photosphere", "published" : true, "oldId" : 1202329, "snippet" : true } ], "digital" : null, "printed" : null, "sourceYear" : 2020, "foreignEdition" : true, "foreignLanguage" : true, "fullPublication" : true, "conferencePublication" : false, "nationalOrigin" : null, "missingAuthor" : false, "oaType" : "NONE", "oaCheckDate" : "2023-04-24", "oaFree" : false, "citationCount" : 0, "citationCountUnpublished" : 0, "citationCountWoOther" : 0, "independentCitCountWoOther" : 0, "doiCitationCount" : 0, "wosCitationCount" : 0, "scopusCitationCount" : 0, "independentCitationCount" : 0, "unhandledCitationCount" : 0, "citingPubCount" : 0, "independentCitingPubCount" : 0, "unhandledCitingPubCount" : 0, "citedPubCount" : 6, "citedCount" : 6, "ratings" : [ { "otype" : "SjrRating", "mtid" : 10748790, "link" : "/api/sjrrating/10748790", "label" : "sjr:Q1 (2019) Scopus - Astronomy and Astrophysics ASTROPHYSICAL JOURNAL 0004-637X 1538-4357", "listPos" : 11, "rankValue" : 0.24, "type" : "journal", "ratingType" : { "otype" : "RatingType", "mtid" : 10002, "link" : "/api/ratingtype/10002", "label" : "sjr", "code" : "sjr", "published" : true, "snippet" : true }, "subject" : { "otype" : "ClassificationExternal", "mtid" : 3103, "link" : "/api/classificationexternal/3103", "label" : "Scopus - Astronomy and Astrophysics", "published" : true, "oldId" : 3103, "snippet" : true }, "ranking" : "Q1", "calculation" : "DIRECT", "published" : true, "snippet" : true } ], "ratingsForSort" : "Q1", "hasCitationDuplums" : false, "directInstitutesForSort" : "", "ownerAuthorCount" : 5, "ownerInstituteCount" : 12, "directInstituteCount" : 0, "authorCount" : 3, "contributorCount" : 0, "hasQualityFactor" : true, "link" : "/api/publication/31057123", "label" : "Iijima H. et al. Effect of Morphological Asymmetry between Leading and Following Sunspots on the Prediction of Solar Cycle Activity. (2019) ASTROPHYSICAL JOURNAL 1538-4357 0004-637X 883 1", "template" : "