{"created":"2023-05-15T14:43:10.082058+00:00","id":59142,"links":{},"metadata":{"_buckets":{"deposit":"d9692071-6f0f-427e-b8a0-265ac8fb1aab"},"_deposit":{"created_by":1,"id":"59142","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"59142"},"status":"published"},"_oai":{"id":"oai:repo.qst.go.jp:00059142","sets":["10:29"]},"author_link":["588960","588956","588958","588962","588961","588957","588959"],"item_10005_date_7":{"attribute_name":"発表年月日","attribute_value_mlt":[{"subitem_date_issued_datetime":"2002-03-15","subitem_date_issued_type":"Issued"}]},"item_10005_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"We present initial results from the first InterComparison for Cosmic-ray with Heavy Ion Beams At NIRS (ICCHIBAN) exposures made at HIMAC in Feb. 2002. The space radiation dosimetry community has long recognized the need to intercompare of spaceflight dosimeters and the Workshops on Radiation Monitoring for the International Space Station (WRMISS) has recommended that radiation instruments used aboard the ISS should be intercompared using well-known radiation fields on the ground. Following this recommendation, the HIMAC facility at the National Institute of Radiological Sciences has begun a series of exposures to intercompare radiation instruments designed for use in space as part of a newly initiated ICCHIBAN project. The initial series of measurements (1st ICCHIBAN run) was designed to establish the response of each detector to two well-characterized heavy ion beams; 400 MeV/nucleon 12C and 400 MeV/nucleon 56Fe. These beams are representative in charge and energy of two of the most significant heavy ion components present in the galactic cosmic radiation spectrum. The properties of the incident beam?such as intensity, profile, charge and total energy?were be characterized by several detectors, including silicon detectors, CR-39 plastic nuclear track detectors and plastic scintillation counters. Once the response of each detector to heavy ion beams of known composition is measured, the space radiation measurement instruments can be compared with one another, in future measurements at HIMAC and at other accelerators around the world. We conclude by discussing plans for future ICCHIBAN runs, including next 2nd ICCHIBAN run for passive detectors in early summer 2002.","subitem_description_type":"Abstract"}]},"item_10005_description_6":{"attribute_name":"会議概要（会議名, 開催地, 会期, 主催者等）","attribute_value_mlt":[{"subitem_description":"2nd Workshop","subitem_description_type":"Other"}]},"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":"Uchihori, Yukio"}],"nameIdentifiers":[{"nameIdentifier":"588956","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Fujitaka, Kazunobu"}],"nameIdentifiers":[{"nameIdentifier":"588957","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Yasuda, Nakahiro"}],"nameIdentifiers":[{"nameIdentifier":"588958","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Benton, Eric"}],"nameIdentifiers":[{"nameIdentifier":"588959","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"内堀 幸夫","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"588960","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"藤高 和信","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"588961","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"安田 仲宏","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"588962","nameIdentifierScheme":"WEKO"}]}]},"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 object","resourceuri":"http://purl.org/coar/resource_type/c_c94f"}]},"item_title":"INTERCOMPARISON OF RADIATION ISNTRUMENTS FOR COSMIC-RAY WITH HEAVY ION BEAMS AT NIRS (ICCHIBAN PROJECT)","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"INTERCOMPARISON OF RADIATION ISNTRUMENTS FOR COSMIC-RAY WITH HEAVY ION BEAMS AT NIRS (ICCHIBAN PROJECT)"}]},"item_type_id":"10005","owner":"1","path":["29"],"pubdate":{"attribute_name":"公開日","attribute_value":"2002-06-10"},"publish_date":"2002-06-10","publish_status":"0","recid":"59142","relation_version_is_last":true,"title":["INTERCOMPARISON OF RADIATION ISNTRUMENTS FOR COSMIC-RAY WITH HEAVY ION BEAMS AT NIRS (ICCHIBAN PROJECT)"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-05-15T22:08:13.129628+00:00"}