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  1. 学会・会議発表論文
  2. 学会・会議発表論文

Space Dust Impacts Detector Development for the Evaluation of Ejecta

http://hdl.handle.net/10228/00007225
http://hdl.handle.net/10228/00007225
a417bb5f-d2ce-44a2-83e0-9ea1eec9c1d4
名前 / ファイル ライセンス アクション
LaSEINE-2018_add02.pdf LaSEINE-2018_add02.pdf (1.7 MB)
Item type 会議発表論文 = Conference Paper(1)
公開日 2019-06-18
資源タイプ
資源タイプ識別子 http://purl.org/coar/resource_type/c_5794
資源タイプ conference paper
タイトル
タイトル Space Dust Impacts Detector Development for the Evaluation of Ejecta
言語 en
言語
言語 eng
著者 Faure, Pauline

× Faure, Pauline

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en Faure, Pauline

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Masuyama, Shingo

× Masuyama, Shingo

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en Masuyama, Shingo

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Nakamoto, Hiroshi

× Nakamoto, Hiroshi

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en Nakamoto, Hiroshi

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赤星, 保浩

× 赤星, 保浩

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e-Rad_Researcher 60222519
Scopus著者ID 7003586539
九工大研究者情報 14

en Akahoshi, Yasuhiro

ja 赤星, 保浩

ja-Kana アカホシ, ヤスヒロ

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Kitazawa, Yukihito

× Kitazawa, Yukihito

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en Kitazawa, Yukihito

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Koura, Takao

× Koura, Takao

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en Koura, Takao

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抄録
内容記述タイプ Abstract
内容記述 This paper aims at a) introducing the space dust impacts detector developed at Kyushu Institute of Technology (KIT), b) presenting the detector utility for the evaluation of ejecta, and c) raising awareness of the space community regarding the risk represented by orbital debris. The space dust impacts detector introduced into this paper belongs to the in-situ detection systems and has for purposes to be a) light, 30 g, b) low cost, about EUR200, c) low power consuming, 0.01W, d) easily adaptable on-board of spacecraft, and e) able to detect impacts of debris with a diameter ranging from 100 μm to 600 μm. The detector is mounted on the nano-satellite, Horyu-II, developed at KIT and launched on May 18, 2012. The data received will be very helpful to identify the detector's strengths and weaknesses to improve it and create a second version that will aim at evaluating ejecta fragments produced during hypervelocity impact testing. An accurate evaluation of ejecta is critical for orbital debris risk assessment and mitigation. If all space activities were stopped, debris will still be created by chain reaction. The number of debris could then become so large, that the access to certain LEOs will be quasi-impossible, which will jeopardize the space exploration as well as scientific, educational, and security missions that benefit to all mankind. Debris is therefore a serious issue that should be taken into consideration at every step of the development of a small or large spacecraft.
備考
内容記述タイプ Other
内容記述 2012 Hypervelocity Impact Symposium (HVIS 2012), September 16-20, 2012, Baltimore, Maryland
書誌情報 Procedia Engineering

巻 58, p. 594-600, 発行日 2012-09
出版社
出版社 Elsevier
DOI
関連タイプ isIdenticalTo
識別子タイプ DOI
関連識別子 https://doi.org/10.1016/j.proeng.2013.05.068
ISSN
収録物識別子タイプ EISSN
収録物識別子 1877-7058
著作権関連情報
権利情報 Copyright (c) 2013 The Authors. Published by Elsevier Ltd. Open access under CC BY-NC-ND license.
著作権関連情報
権利情報 http://creativecommons.org/licenses/by-nc-nd/3.0/
キーワード
主題Scheme Other
主題 Space environment
キーワード
主題Scheme Other
主題 Debris
キーワード
主題Scheme Other
主題 Hypervelocity impact
キーワード
主題Scheme Other
主題 Modeling
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
査読の有無
値 yes
連携ID
値 7726
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