| Project/Area Number |
19340142
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| Research Category |
Grant-in-Aid for Scientific Research (B)
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| Allocation Type | Single-year Grants |
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| Section | 一般 |
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| Research Field |
Space and upper atmospheric physics
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| Research Institution | Kochi National College of Technology |
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Principal Investigator |
IMAI Kazumasa Kochi National College of Technology, 電気情報工学科, 教授 (20132657)
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| Co-Investigator(Kenkyū-buntansha) |
KONDO Tetsuro 独立行政法人情報通信研究機構, 新世代ワイヤレス研究センター鹿島宇宙技術センター, センター長 (10359052)
MISAWA Hiroaki 東北大学, 理学(系)研究科(研究院), 准教授 (90219618)
TSUCHIYA Fuminori 東北大学, 理学(系)研究科(研究院), 助教 (10302077)
NAKAJO Tomoyuki 福井工業大学, 工学部, 講師 (00367509)
KAWANO Nobuyuki 国立天文台, RISE推進室, 教授 (10186116)
NODA Hirotomo 国立天文台, RISE推進室, 助教 (10353426)
IWATA Takahiro 独立行政法人宇宙航空研究開発機構, 宇宙科学研究所, 准教授 (20201949)
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| Project Period (FY) |
2007 – 2009
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| Project Status |
Completed (Fiscal Year 2009)
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| Budget Amount *help |
¥15,860,000 (Direct Cost: ¥12,200,000、Indirect Cost: ¥3,660,000)
Fiscal Year 2009: ¥3,640,000 (Direct Cost: ¥2,800,000、Indirect Cost: ¥840,000)
Fiscal Year 2008: ¥5,330,000 (Direct Cost: ¥4,100,000、Indirect Cost: ¥1,230,000)
Fiscal Year 2007: ¥6,890,000 (Direct Cost: ¥5,300,000、Indirect Cost: ¥1,590,000)
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| Keywords | 超高層物理学 / 電波天文学 / 惑星電波 / 月探査 / 磁気圏・電離圏 |
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| Research Abstract |
The radiation mechanism of the Jupiter's decametric radio emissions has not been fully understood. We developed a Jupiter radio e-VLBI system over the Internet. We successfully received Jupiter radio emissions by using this e-VLBI system. The micro structures of Jupiter radio source are also considered by the model of Jupiter radio searchlight beam. This study is very important step toward the moon-earth baseline VLBI to investigate the Jupiter radio source in detail.
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