{"created":"2023-06-20T15:40:08.431686+00:00","id":215,"links":{},"metadata":{"_buckets":{"deposit":"b92c96a0-abb3-44d4-afc7-e1987149f280"},"_deposit":{"created_by":17,"id":"215","owners":[17],"pid":{"revision_id":0,"type":"depid","value":"215"},"status":"published"},"_oai":{"id":"oai:nagano-nct.repo.nii.ac.jp:00000215","sets":["3:14"]},"author_link":["368"],"item_2_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2002-06-28","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"80","bibliographicPageStart":"73","bibliographicVolumeNumber":"36","bibliographic_titles":[{"bibliographic_title":"長野工業高等専門学校紀要"}]}]},"item_2_description_19":{"attribute_name":"フォーマット","attribute_value_mlt":[{"subitem_description":"application","subitem_description_type":"Other"}]},"item_2_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"The cyclotron lines are affected by photon splitting in super-strong magnetized atmospheres(～4.4×10^9 T) into which the power-law-type flux is injected. Since photon splitting occurs in super-strong magnetic field regardless of the existence of the plasma, it will occur over the larger scale than the cyclotron resonant scattering, which is interaction with the electron. We considered the atmospheres consisted of cyclotron resonant scattering predominant and photon splitting predominant regions. The emergent spectra were calculated in the cases of the line formation regions located in the middle and top of the atmosphere. We found that the location of the line formation regions affect the depth of the line. Furthermore, we calculated the emergent spectra in several optical depths of cyclotron resonant scattering predominant region and found that the cyclotron absorption lines become unclear in the higher resonant energies than 200 keV.","subitem_description_type":"Abstract"}]},"item_2_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"長野工業高等専門学校"}]},"item_2_source_id_11":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AN00179170","subitem_source_identifier_type":"NCID"}]},"item_2_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0286-1909","subitem_source_identifier_type":"ISSN"}]},"item_2_version_type_20":{"attribute_name":"著者版フラグ","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":"NlSHIMURA, Osamu"}],"nameIdentifiers":[{"nameIdentifier":"368","nameIdentifierScheme":"WEKO"}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2013-02-19"}],"displaytype":"detail","filename":"nagano_nct-36-15.pdf","filesize":[{"value":"610.7 kB"}],"format":"application/pdf","licensetype":"license_11","mimetype":"application/pdf","url":{"label":"nagano_nct-36-15.pdf","url":"https://nagano-nct.repo.nii.ac.jp/record/215/files/nagano_nct-36-15.pdf"},"version_id":"d7610078-18c9-4f59-8314-70061b40d582"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"Cyclotron lines","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"photon splitting","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"super-strong magnetic field","subitem_subject_language":"en","subitem_subject_scheme":"Other"}]},"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":"departmental bulletin paper","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"The Influence of Photon Splitting on Cyclotron Line Formation in Atmospheres with Distinct Formation Regions","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"The Influence of Photon Splitting on Cyclotron Line Formation in Atmospheres with Distinct Formation Regions","subitem_title_language":"en"}]},"item_type_id":"2","owner":"17","path":["14"],"pubdate":{"attribute_name":"公開日","attribute_value":"2013-02-19"},"publish_date":"2013-02-19","publish_status":"0","recid":"215","relation_version_is_last":true,"title":["The Influence of Photon Splitting on Cyclotron Line Formation in Atmospheres with Distinct Formation Regions"],"weko_creator_id":"17","weko_shared_id":-1},"updated":"2023-06-20T16:14:59.442730+00:00"}