{"created":"2023-06-20T14:52:29.957140+00:00","id":20652,"links":{},"metadata":{"_buckets":{"deposit":"119991ba-15c6-4b93-a20c-be8645e113a5"},"_deposit":{"created_by":1,"id":"20652","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"20652"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00020652","sets":["1543:1778:1793","1887:1891"]},"author_link":["196957","196960","196955","196956","196959","196958"],"item_5_alternative_title_1":{"attribute_name":"その他のタイトル","attribute_value_mlt":[{"subitem_alternative_title":"T Tauri恒星の星周辺ディスクに対する非等方散乱を用いた放射平衡の計算"}]},"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2003-11","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"12","bibliographicPageStart":"9","bibliographic_titles":[{"bibliographic_title":"第36回月・惑星シンポジウム"},{"bibliographic_title":"Proceedings of the 36th ISAS Lunar and Planetary Symposium","bibliographic_titleLang":"en"}]}]},"item_5_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"T Tauri stars, consisting of central star and circumstellar disk, are thought to be progenitors of planetary systems like the solar system. Structure of T Tauri stars may determine the final state of the planetary system formed later. Because T Tauri stars are small and distant, it is hard to observe their structure directly. Instead, it has been deduced by calculating model spectral energy distributions (SEDs) and images and by comparing them with observed data. However, anisotropic scattering by small dust particles has not been incorporated adequately a previous work, though observed data at visible and infrared wavelengths are strongly dominated by anisotropically scattered radiation. Here, it was examined to what extent the anisotropic scattering (Mie scattering) may affect SEDs and images of T Tauri stars. It was found that the anisotropic scattering effect is not negligible and it should be taken into account faithfully in the radiative equilibrium calculations of T Tauri stars. Also, it is suggested that the radiative equilibrium calculations with anisotropic scattering model can be used to estimate the inclination of and the dust sizes in the disk.","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0046650003","subitem_description_type":"Other"}]},"item_5_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"宇宙航空研究開発機構宇宙科学研究本部"}]},"item_5_publisher_9":{"attribute_name":"出版者（英）","attribute_value_mlt":[{"subitem_publisher":"Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS)"}]},"item_5_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"東京大学 大学院理学系研究科"},{"subitem_text_value":"筑波大学 計算物理学研究センター"},{"subitem_text_value":"東京大学 大学院理学系研究科"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"University of Tokyo Graduate School of Science"},{"subitem_text_language":"en","subitem_text_value":"University of Tsukuba Center for Computational Physics"},{"subitem_text_language":"en","subitem_text_value":"University of Tokyo Graduate School of Science"}]},"item_access_right":{"attribute_name":"アクセス権","attribute_value_mlt":[{"subitem_access_right":"metadata only access","subitem_access_right_uri":"http://purl.org/coar/access_right/c_14cb"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"林, 和樹"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"中本, 泰史"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"五十嵐, 丈二"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Hayashi, Kazuki","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Nakamoto, Taishi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Igarashi, George","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"T Tauri星","subitem_subject_scheme":"Other"},{"subitem_subject":"Mie散乱","subitem_subject_scheme":"Other"},{"subitem_subject":"放射平衡","subitem_subject_scheme":"Other"},{"subitem_subject":"異方性散乱","subitem_subject_scheme":"Other"},{"subitem_subject":"惑星系","subitem_subject_scheme":"Other"},{"subitem_subject":"SED","subitem_subject_scheme":"Other"},{"subitem_subject":"赤外線放射","subitem_subject_scheme":"Other"},{"subitem_subject":"温度分布","subitem_subject_scheme":"Other"},{"subitem_subject":"T Tauri star","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Mie scattering","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"radiative equilibrium","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"anisotropic scattering","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"planetary system","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"SED","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"infrared radiation","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"temperature distribution","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":"conference paper","resourceuri":"http://purl.org/coar/resource_type/c_5794"}]},"item_title":"Radiative equilibrium calculations with anisotropic scattering for a circumstellar disk of a T Tauri star","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Radiative equilibrium calculations with anisotropic scattering for a circumstellar disk of a T Tauri star","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["1793","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"20652","relation_version_is_last":true,"title":["Radiative equilibrium calculations with anisotropic scattering for a circumstellar disk of a T Tauri star"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T03:47:12.441183+00:00"}