@inproceedings{oai:jaxa.repo.nii.ac.jp:00020621,
 author = {土屋, 史紀 and 三澤, 浩昭 and 渡邉, 拓男 and 野村, 詩穂 and 森岡, 昭 and 三好, 由純 and 近藤, 哲朗 and Tsuchiya, Fuminori and Misawa, Hiroaki and Watanabe, Takuo and Nomura, Shiho and Morioka, Akira and Miyoshi, Yoshizumi and Kondo, Tetsuro},
 book = {第37回月・惑星シンポジウム, Proceedings of the 37th ISAS Lunar and Planetary Symposium},
 month = {Feb},
 note = {Jovian synchrotron radiations (JSR) which are emitted from relativistic electrons trapped in the Jupiter's radiation belt were observed during a rarely strong solar event occurred on October 28 and 29, 2003. The observation was made by the Iitate Planetary Radio Telescope (IPRT) at Iitate Observatory in Japan during the period from October 16 to November 20 in 2003. Variations of the JSR intensity were compared with the solar F10.7 flux and it was found that the intensity of the JSR showed unusual increase of its magnitude by about 50 percent and the subsequent rapid decrease after the solar event with the decay rate of about 0.3 Jy/day. Comparing with the previous observations of the short term variation of the JSR, an unusual response of Jupiter's radiation belt associated with the rarely strong solar activity is supposed., 資料番号: AA0047898043},
 pages = {167--170},
 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 = {The response of the Jovian synchrotron radiation at 325 MHz associated with the strong solar activity during October to November 2003},
 year = {2004}
}