{"created":"2023-10-26T05:30:06.411369+00:00","id":2000162,"links":{},"metadata":{"_buckets":{"deposit":"4c6e77ed-cc32-40e1-93bf-9441fc7c7d11"},"_deposit":{"created_by":14,"id":"2000162","owner":"14","owners":[14],"pid":{"revision_id":0,"type":"depid","value":"2000162"},"status":"published"},"_oai":{"id":"oai:kyutech.repo.nii.ac.jp:02000162","sets":["8:9"]},"author_link":["35396","31407"],"control_number":"2000162","item_21_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2023-02-28","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"2","bibliographicPageStart":"229","bibliographicVolumeNumber":"944","bibliographic_titles":[{"bibliographic_title":"Astrophysical Journal","bibliographic_titleLang":"en"}]}]},"item_21_description_4":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"We report near-infrared polarization of the zodiacal light (ZL) measured from space by the Diffuse Infrared Background Experiment (DIRBE) on board the Cosmic Background Explorer in photometric bands centered at 1.25, 2.2, and 3.5 μm. To constrain the physical properties of interplanetary dust, we use DIRBE Weekly Sky Maps to investigate the solar elongation (epsilon), ecliptic latitude (β), and wavelength (λ) dependence of ZL polarization. We find that the polarization of the ZL varies as a function of epsilon and β, consistent with observed polarization at λ = 550 nm. While the polarization dependence on wavelength at (epsilon, β) = (90°, 0°) is modest (increasing from 17.7% ± 0.2% at 1.25% μm to 21.0% ± 0.3% at 3.5 μm), the variation is more pronounced at the north ecliptic pole (23.1% ± 1.6%, 35.1% ± 2.0%, and 39.3% ± 2.1% at 1.25, 2.2, and 3.5 μm, respectively). The variation in ZL polarization with wavelength is not explained by either Rayleigh scattering or absorptive particles larger than 10 μm.","subitem_description_language":"en","subitem_description_type":"Abstract"}]},"item_21_publisher_7":{"attribute_name":"出版社","attribute_value_mlt":[{"subitem_publisher":"IOP Publishing","subitem_publisher_language":"en"}]},"item_21_relation_12":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_type":"isIdenticalTo","subitem_relation_type_id":{"subitem_relation_type_id_text":"https://doi.org/10.3847/1538-4357/acb937","subitem_relation_type_select":"DOI"}}]},"item_21_rights_13":{"attribute_name":"著作権関連情報","attribute_value_mlt":[{"subitem_rights":"Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.","subitem_rights_resource":"http://creativecommons.org/licenses/by/4.0/"}]},"item_21_select_59":{"attribute_name":"査読の有無","attribute_value_mlt":[{"subitem_select_item":"yes"}]},"item_21_source_id_10":{"attribute_name":"NCID","attribute_value_mlt":[{"subitem_source_identifier":"0004-637X","subitem_source_identifier_type":"ISSN"}]},"item_21_source_id_8":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"1538-4357","subitem_source_identifier_type":"EISSN"},{"subitem_source_identifier":"0004-637X","subitem_source_identifier_type":"PISSN"}]},"item_21_version_type_58":{"attribute_name":"出版タイプ","attribute_value_mlt":[{"subitem_version_resource":"http://purl.org/coar/version/c_970fb48d4fbd8a85","subitem_version_type":"VoR"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"瀧本, 幸司","creatorNameLang":"ja"},{"creatorName":"Takimoto, Kohji","creatorNameLang":"en"}],"familyNames":[{},{}],"givenNames":[{},{}],"nameIdentifiers":[{"nameIdentifier":"35396","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"0000-0002-8405-9549","nameIdentifierScheme":"ORCiD","nameIdentifierURI":"https://orcid.org/0000-0002-8405-9549"}]},{"creatorNames":[{"creatorName":"Matsuura, Shuji","creatorNameLang":"en"}]},{"creatorNames":[{"creatorName":"Sano, Kei","creatorNameLang":"en"},{"creatorName":"佐野, 圭","creatorNameLang":"ja"}],"familyNames":[{},{}],"givenNames":[{},{}],"nameIdentifiers":[{"nameIdentifier":"31407","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"70802908","nameIdentifierScheme":"e-Rad","nameIdentifierURI":"https://nrid.nii.ac.jp/ja/nrid/1000070802908"},{"nameIdentifier":"56708069700","nameIdentifierScheme":"Scopus著者ID","nameIdentifierURI":"https://www.scopus.com/authid/detail.uri?authorId=56708069700"},{"nameIdentifier":"0000-0002-6468-8532","nameIdentifierScheme":"ORCiD","nameIdentifierURI":"https://orcid.org/0000-0002-6468-8532"},{"nameIdentifier":"100001400","nameIdentifierScheme":"九工大研究者情報","nameIdentifierURI":"https://hyokadb02.jimu.kyutech.ac.jp/html/##_ja.html"}]},{"creatorNames":[{"creatorName":"Feder, Richard M.","creatorNameLang":"en"}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_access","date":[{"dateType":"Available","dateValue":"2023-10-26"}],"filename":"LaSEINE-2022_025.pdf","filesize":[{"value":"8.5 MB"}],"format":"application/pdf","mimetype":"application/pdf","url":{"url":"https://kyutech.repo.nii.ac.jp/record/2000162/files/LaSEINE-2022_025.pdf"},"version_id":"788e64c0-73ac-401d-8f21-1321b65c4644"}]},"item_language":{"attribute_name":"言語","attribute_value_mlt":[{"subitem_language":"eng"}]},"item_resource_type":{"attribute_name":"資源タイプ","attribute_value_mlt":[{"resourcetype":"journal article","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"Near-infrared Polarization Charateristics of the Zodiacal Light Observed with DIRBE/COBE","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Near-infrared Polarization Charateristics of the Zodiacal Light Observed with DIRBE/COBE","subitem_title_language":"en"}]},"item_type_id":"21","owner":"14","path":["9"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2023-10-26"},"publish_date":"2023-10-26","publish_status":"0","recid":"2000162","relation_version_is_last":true,"title":["Near-infrared Polarization Charateristics of the Zodiacal Light Observed with DIRBE/COBE"],"weko_creator_id":"14","weko_shared_id":-1},"updated":"2024-04-02T08:43:20.020829+00:00"}