{"created":"2021-03-01T06:39:57.793472+00:00","id":34658,"links":{},"metadata":{"_buckets":{"deposit":"57eea401-0076-4605-87f5-23d4fc1a9ef3"},"_deposit":{"id":"34658","owners":[],"pid":{"revision_id":0,"type":"depid","value":"34658"},"status":"published"},"_oai":{"id":"oai:teapot.lib.ocha.ac.jp:00034658","sets":["347:359:675"]},"item_11_biblio_info_8":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2002-06","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"1","bibliographicPageEnd":"34","bibliographicPageStart":"31","bibliographicVolumeNumber":"53","bibliographic_titles":[{"bibliographic_title":"お茶の水女子大學自然科學報告"}]}]},"item_11_description_17":{"attribute_name":"フォーマット","attribute_value_mlt":[{"subitem_description":"application/pdf","subitem_description_type":"Other"}]},"item_11_description_46":{"attribute_name":"資源タイプ","attribute_value_mlt":[{"subitem_description":"紀要論文","subitem_description_type":"Other"}]},"item_11_description_7":{"attribute_name":"内容記述","attribute_value_mlt":[{"subitem_description":"In 2007, ACCESS (Advanced Cosmic ray Composition Experiment for the Space Station) on the International Space Station (ISS) detectors will measure the individual elemental composition of cosmic rays at energies a thousand times higher than any previous measurement of similar resolution-reaching to 10^<15> eV for understanding of the origin, source and acceleration mechanism of cosmic rays. We can determine the charge of cosmic rays using the silicon detector, one of the detectors in ACCESS. We simulate the reaction of very high energy heavy ions in silicon detector by Geant4 simulation tool. The simulation is carried out for one layer Si-detector and full ACCESS structure. The heavy ions (Z up to 28) with high energies from 10 GeV to 10 TeV penetrate one silicon layer with various thickness and the ions from 1 to 100 TeV penetrate the full detector. The results show that energy loss is linearly proportional to Z^2 and thickness. In full ACCESS simulation we can distinguish the backscattered particles originated in calorimeter from primaries. In order to determine the contamination of the backscattered particles in\\\nthe primaries in each pixel, the average distance distribution of the primary particles and the backscattered particles are calculated. Results show that the secondary particles do not affect so much for the identification of each element.","subitem_description_type":"Other"}]},"item_11_publisher_36":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"お茶の水女子大学"}]},"item_11_source_id_11":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AN00033958","subitem_source_identifier_type":"NCID"}]},"item_11_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"00298190","subitem_source_identifier_type":"ISSN"}]},"item_11_subject_20":{"attribute_name":"日本十進分類法","attribute_value_mlt":[{"subitem_subject":"400","subitem_subject_scheme":"NDC"}]},"item_11_text_18":{"attribute_name":"形態","attribute_value_mlt":[{"subitem_text_value":"266211 bytes"}]},"item_11_text_47":{"attribute_name":"資源タイプ・ローカル","attribute_value_mlt":[{"subitem_text_value":"紀要論文"}]},"item_11_text_48":{"attribute_name":"資源タイプ・NII","attribute_value_mlt":[{"subitem_text_value":"Departmental Bulletin Paper"}]},"item_11_text_49":{"attribute_name":"資源タイプ・DCMI","attribute_value_mlt":[{"subitem_text_value":"text"}]},"item_11_text_50":{"attribute_name":"資源タイプ・ローカル表示コード","attribute_value_mlt":[{"subitem_text_value":"03"}]},"item_11_text_79":{"attribute_name":"所属","attribute_value_mlt":[{"subitem_text_value":"Department of physics, Ewha Womans University"},{"subitem_text_value":"Center for High Energy Physics, Kyungpook Nat'l University"},{"subitem_text_value":"Department of physics, Seoul National University"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Choi, Min Jeong"}],"nameIdentifiers":[{"nameIdentifier":"70716","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Yang, Jongmann"}],"nameIdentifiers":[{"nameIdentifier":"70717","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Park, II Hung"}],"nameIdentifiers":[{"nameIdentifier":"70718","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":"2018-04-19"}],"displaytype":"detail","filename":"KJ00004830724.pdf","filesize":[{"value":"266.2 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"KJ00004830724.pdf","url":"https://teapot.lib.ocha.ac.jp/record/34658/files/KJ00004830724.pdf"},"version_id":"b3f4548b-b9d3-42b8-bdc4-a68a093412a0"}]},"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":"A Simulation of the Silicon Charge Detector on ISS","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"A Simulation of the Silicon Charge Detector on ISS"}]},"item_type_id":"11","owner":"1","path":["675"],"pubdate":{"attribute_name":"公開日","attribute_value":"2008-04-30"},"publish_date":"2008-04-30","publish_status":"0","recid":"34658","relation_version_is_last":true,"title":["A Simulation of the Silicon Charge Detector on ISS"],"weko_creator_id":"1","weko_shared_id":null},"updated":"2022-12-12T05:39:05.480530+00:00"}