{"created":"2023-06-20T15:17:34.048563+00:00","id":11478,"links":{},"metadata":{"_buckets":{"deposit":"dc4db5bc-466d-4936-a354-0c654e75843e"},"_deposit":{"created_by":20,"id":"11478","owners":[20],"pid":{"revision_id":0,"type":"depid","value":"11478"},"status":"published"},"_oai":{"id":"oai:nifs-repository.repo.nii.ac.jp:00011478","sets":["6:7"]},"author_link":["127786","127787","126050","127788","123133","126865"],"item_10001_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2022-06-27","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":" June 2022","bibliographicPageStart":"P06034","bibliographicVolumeNumber":"17","bibliographic_titles":[{"bibliographic_title":"Journal of Instrumentation"}]}]},"item_10001_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"Imaging bolometers have been studied for ITER to serve as a complementary diagnostic to the resistive bolometers for the measurement of radiated power. Two tangentially viewing InfraRed imaging Video Bolometers (IRVB) could be proposed for an ITER equatorial port, one having a view of the entire plasma cross-section (core viewing) and one tilted down 43 degrees from the horizontal to view the divertor (divertor viewing). The IRVBs have 7 cm (horizontal) by 9 cm (vertical) Pt sensor foils, 6 mm × 6 mm apertures, 15 × 20 pixels and focal lengths of 7.8 cm and 21 cm, respectively. Using SANCO and SOLPS models for a 840 m3 plasma radiating 67.3 MW, synthetic images from the IRVBs are calculated to estimate the maximum signal strengths to be 246 W/m2 and 62 W/m2, respectively. We propagate the X-ray energy spectra from the models through the synthetic diagnostics to give the photon energy spectrum for each IRVB pixel, which are used to calculate the fraction of the power absorbed by the foil as a function of foil thickness. Using a criteria of >95% absorbed power fraction, we selected foil thicknesses of 30 μm and 10 μm, respectively. We used these thicknesses and assumed IR systems having 105 fps, 1024×1280 pixels and sensitivities of 15 mK, to calculate the IRVB sensitivities of 3.19 W/m2 and 1.05 W/m2, and signal to noise ratios of 77 and 59, respectively. Using the Monte Carlo Nuclear Particle code we calculated for the core viewing IRVB the foil heating by neutrons to be 1.0 W/m2 and by gammas to be 117 W/m2. This indicates that countermeasures may be needed to remove the nuclear heating signal.","subitem_description_type":"Abstract"}]},"item_10001_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"IOP Publishing "}]},"item_10001_relation_14":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_type":"isIdenticalTo","subitem_relation_type_id":{"subitem_relation_type_id_text":"https://doi.org/10.1088/1748-0221/17/06/P06034","subitem_relation_type_select":"DOI"}}]},"item_10001_relation_16":{"attribute_name":"情報源","attribute_value_mlt":[{"subitem_relation_name":[{"subitem_relation_name_text":"B.J. Peterson et al 2022 JINST 17 P06034"}]}]},"item_10001_relation_17":{"attribute_name":"関連サイト","attribute_value_mlt":[{"subitem_relation_name":[{"subitem_relation_name_text":"Publisher version"}],"subitem_relation_type_id":{"subitem_relation_type_id_text":"https://doi.org/10.1088/1748-0221/17/06/P06034","subitem_relation_type_select":"DOI"}}]},"item_10001_rights_15":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"© 2022 The Author(s)"},{"subitem_rights":"Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. "},{"subitem_rights":"Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI."}]},"item_10001_source_id_11":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA12456425 ","subitem_source_identifier_type":"NCID"}]},"item_10001_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"1748-0221","subitem_source_identifier_type":"ISSN"}]},"item_10001_text_23":{"attribute_name":"NAIS","attribute_value_mlt":[{"subitem_text_value":"13432"}]},"item_10001_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":"PETERSON, Byron J."}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"NISHITANI, Takeo"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"REICHLE, Roger"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"MUNECHIKA, K."}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"O'MULLANE, M.G."}],"nameIdentifiers":[{}]},{"creatorAffiliations":[{"affiliationNameIdentifiers":[{"affiliationNameIdentifier":""}],"affiliationNames":[{"affiliationName":""}]}],"creatorNames":[{"creatorName":"MUKAI, Kiyofumi"}],"familyNames":[{}],"givenNames":[{}],"nameIdentifiers":[{}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2022-07-21"}],"displaytype":"detail","filename":"13432_J.Inst.pdf","filesize":[{"value":"3.6 MB"}],"format":"application/pdf","licensetype":"license_6","mimetype":"application/pdf","url":{"label":"13432_J.Inst","url":"https://nifs-repository.repo.nii.ac.jp/record/11478/files/13432_J.Inst.pdf"},"version_id":"0dee093a-559d-4ce1-9139-acb92424b7a7"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"Plasma diagnostics - interferometry","subitem_subject_scheme":"Other"},{"subitem_subject":"spectroscopy and imaging","subitem_subject_scheme":"Other"},{"subitem_subject":"Nuclear instruments and methods for hot plasma diagnostics","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":"journal article","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"Estimates of foil thickness, signal, noise, and nuclear heating of imaging bolometers for ITER","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Estimates of foil thickness, signal, noise, and nuclear heating of imaging bolometers for ITER"}]},"item_type_id":"10001","owner":"20","path":["7"],"pubdate":{"attribute_name":"公開日","attribute_value":"2022-07-21"},"publish_date":"2022-07-21","publish_status":"0","recid":"11478","relation_version_is_last":true,"title":["Estimates of foil thickness, signal, noise, and nuclear heating of imaging bolometers for ITER"],"weko_creator_id":"20","weko_shared_id":-1},"updated":"2023-09-26T03:36:27.473237+00:00"}