@inproceedings{oai:jaxa.repo.nii.ac.jp:00048379,
 author = {ガルシア ペレス, ホルヘ and 鈴木, 宏二郎 and GARCIA PEREZ, Jorge Alberto and SUZUKI, Kojiro},
 book = {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, JAXA Special Publication: Proceedings of the 53rd Fluid Dynamics Conference / the 39th Aerospace Numerical Simulation Symposium},
 month = {Feb},
 note = {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), 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), 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., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA2130027006, レポート番号: JAXA-SP-21-008},
 pages = {101--108},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {Plasma-Surface Interaction Modeling Utilizing Particle-In-Cell Code for Solar wind in the Solar Corona Region},
 volume = {JAXA-SP-21-008},
 year = {2022}
}