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Plasma-Surface Interaction Modeling Utilizing Particle-In-Cell Code for Solar wind in the Solar Corona Region
https://jaxa.repo.nii.ac.jp/records/48379
https://jaxa.repo.nii.ac.jp/records/4837900ea56eb-f499-4514-8326-a0f66d751698
名前 / ファイル | ライセンス | アクション |
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AA2130027006.pdf (2.0 MB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2022-02-14 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Plasma-Surface Interaction Modeling Utilizing Particle-In-Cell Code for Solar wind in the Solar Corona Region | |||||
言語 | ||||||
言語 | eng | |||||
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 | |||||
その他のタイトル | ||||||
その他のタイトル | Particle-In-Cell法を用いた太陽コロナ中の太陽風におけるプラズマと衛星表面の干渉モデルに関する研究 | |||||
著者 |
ガルシア ペレス, ホルヘ
× ガルシア ペレス, ホルヘ× 鈴木, 宏二郎× GARCIA PEREZ, Jorge Alberto× SUZUKI, Kojiro |
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著者所属 | ||||||
東京大学 | ||||||
著者所属 | ||||||
東京大学 | ||||||
著者所属(英) | ||||||
en | ||||||
The University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
The University of Tokyo | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構(JAXA) | |||||
出版者(英) | ||||||
出版者 | Japan Aerospace Exploration Agency (JAXA) | |||||
書誌情報 |
宇宙航空研究開発機構特別資料: 第53回流体力学講演会/第39回航空宇宙数値シミュレーション技術シンポジウム論文集 en : JAXA Special Publication: Proceedings of the 53rd Fluid Dynamics Conference / the 39th Aerospace Numerical Simulation Symposium 巻 JAXA-SP-21-008, p. 101-108, 発行日 2022-02-14 |
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会議概要(会議名, 開催地, 会期, 主催者等) | ||||||
内容記述タイプ | Other | |||||
内容記述 | 第53回流体力学講演会/第39回航空宇宙数値シミュレーション技術シンポジウム (2021年6月30日-7月2日. 日本航空宇宙学会 : 宇宙航空研究開発機構(JAXA)オンライン会議) | |||||
会議概要(会議名, 開催地, 会期, 主催者等)(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The 53rd Fluid Dynamics Conference / the 39th Aerospace Numerical Simulation Symposium (June 30 - July 2, 2021. The Japan Society for Aeronautical and Space Sciences : Japan Aerospace Exploration Agency (JAXA), Online meeting) | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | With the intention of studying the heat up process in the Solar Corona, current scientific efforts involve in-situ measurements with Solar Probes, such as PSP (Parker Solar Probe) mission. In this study, a new Particle-In-Cell code, SCSI (Solar Corona-Satellite Interaction), is developed and tested, with the intention of exploring the phenomena involved in the interaction between the solar wind present in the Solar Corona and the surface of a spacecraft. SCSI is developed with an Object-Oriented approach, allowing features such as several numerical schemes in a single domain, and multigrid meshes. The present program probed successful in replicating the spatial distribution of the species involved and the electric currents present in the system, among other parameters. The floating potential calculated on the probe surface as well as the electric barrier generated around it also show similarities with previous studies on the subject. | |||||
内容記述 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 形態: カラー図版あり | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Physical characteristics: Original contains color illustrations | |||||
ISSNONLINE | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 2433-2232 | |||||
著者版フラグ | ||||||
出版タイプ | VoR | |||||
出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA2130027006 | |||||
レポート番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | レポート番号: JAXA-SP-21-008 |