@inproceedings{oai:jaxa.repo.nii.ac.jp:00020474,
 author = {河原木, 皓 and 森岡, 昭 and 三澤, 浩昭 and 土屋, 史紀 and Kawaragi, Ko and Morioka, Akira and Misawa, Hiroaki and Tsuchiya, Fuminori},
 book = {第39回月・惑星シンポジウム, Proceedings of the 39th ISAS Lunar and Planetary Symposium},
 month = {Aug},
 note = {Saturn's outer magnetosphere is considered to be one of sources of auroral particles, inducing the complex interaction between magnetospheric particles and Titan. In 1980s, Voyager 1 and 2 had revealed the existence of high energy (approximately keV) electrons with non-Maxwellian distribution in this region, although the source of these electrons has not been clear. We investigated the possibility that the source of high energy electrons is resulted by the electron acceleration accompanied by aurora in the polar region. Then we analyzed the electron flux and radio wave data observed by Cassini spacecraft. Analyzed results showed correspondence between emission power of SKR (Saturn Kilometric Radiation), index of auroral activity, and magnetospheric electron flux., 資料番号: AA0063505012},
 pages = {45--48},
 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 = {Source of high energy electrons in Saturn's outer magnetosphere},
 year = {2006}
}