@inproceedings{oai:jaxa.repo.nii.ac.jp:00003213,
 author = {Orger, Necmi Cihan and CordovaAlarcon, J. Rodrigo and 豊田, 和弘 and 趙, 孟佑 and Orger, Necmi Cihan and CordovaAlarcon, J. Rodrigo and Toyoda, Kazuhiro and Cho, Mengu},
 book = {宇宙航空研究開発機構特別資料: 第14回「宇宙環境シンポジウム」講演論文集, JAXA Special Publication: Proceedings of the 14th Spacecraft Environment Symposium},
 month = {Jan},
 note = {第14回宇宙環境シンポジウム (2017年11月6日-8日. 神戸大学先端融合研究環統合研究拠点コンベンションホール), 神戸市, 兵庫県, Recent studies have shown that dust grains can be transported in the laboratory experiments due to charging within micro-cavities between the particles. Therefore, electrostatic forces acting on the dust grains can be described as the repulsive Coulomb force between charged grains and the force resulting from the surface electric field due to the plasma sheath above the surface. In this study, we investigate different ambient plasma conditions to understand how the lunar dust particles are mobilized under the variation of surface potential, dust potential, electric field and the plasma sheath above the lunar terminator. In addition, electrostatic forces are compared to the gravity force and the contact forces for the micron and submicron sized dust particles, and it has been seen that the repulsive force between the charged dust grains can be stronger than the other forces. Finally, the current level of the experimental work is presented, which is prior to investigation of the impact modification on the electrostatic lofting of the silica dust grains in the vacuum chamber., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730013008, レポート番号: JAXA-SP-17-006},
 pages = {59--62},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {Investigation of Electrostatic Transportation of Lunar Dust Grains due to Ambient Plasma Conditions},
 volume = {JAXA-SP-17-006},
 year = {2018}
}