@inproceedings{oai:jaxa.repo.nii.ac.jp:00020454,
 author = {佐藤, 毅彦 and Connerney, Jack and 徳丸, 宗利 and 林, 啓志 and Sato, Takehiko and Connerney, Jack and Tokumaru, Munetoshi and Hayashi, Keiji},
 book = {第40回月・惑星シンポジウム, Proceedings of the 40th ISAS Lunar and Planetary Symposium},
 month = {Jul},
 note = {We have compared time history of integrated flux of Jupiter's H3(+) aurora, acquired in 1998-2000, with the sola-wind database. The solar wind at Jupiter is simulated based on the MHD (MagnetoHydroDynamic) tomography analysis of InterPlanetary Scintillation (IPS). The auroral flux is found to be affected by the solar-wind dynamic pressure and by the polarity of Interplanetary Magnetic Field (IMF), indicating that reconnection with IMF has influences on particle precipitation in the Jovian magnetosphere., 資料番号: AA0063723034},
 pages = {147--150},
 publisher = {宇宙航空研究開発機構宇宙科学研究本部, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS)},
 title = {Magnetic reconnection signature in Jupiter's H3(+) auroral activity},
 year = {2007}
}