| Project/Area Number |
24501041
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| Research Category |
Grant-in-Aid for Scientific Research (C)
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| Allocation Type | Multi-year Fund |
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| Section | 一般 |
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| Research Field |
Science education
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| Research Institution | The University of Tokyo |
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Principal Investigator |
YOSHIDA Hideto 東京大学, 大学院理学系研究科(理学部), 技術専門員 (30376553)
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| Co-Investigator(Renkei-kenkyūsha) |
TERASAWA Toshio 理化学研究所, 階層縦断型基礎物理学研究グループ, 研究員 (30134662)
YOSHIKAWA Ichiro 東京大学, 新領域創成科学研究科, 教授 (10311169)
NAKAMURA Takuji 国立極地研究所, 研究教育系, 教授 (40217857)
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| Research Collaborator |
MIYAMOTO Hideaki 巣鴨高等学校, 教諭
USUI Takashi 日本流星研究会
YAGUCHI Noriyuki 日本流星研究会
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| Project Period (FY) |
2012-04-01 – 2017-03-31
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| Project Status |
Completed (Fiscal Year 2016)
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| Budget Amount *help |
¥5,460,000 (Direct Cost: ¥4,200,000、Indirect Cost: ¥1,260,000)
Fiscal Year 2015: ¥650,000 (Direct Cost: ¥500,000、Indirect Cost: ¥150,000)
Fiscal Year 2014: ¥910,000 (Direct Cost: ¥700,000、Indirect Cost: ¥210,000)
Fiscal Year 2013: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2012: ¥2,860,000 (Direct Cost: ¥2,200,000、Indirect Cost: ¥660,000)
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| Keywords | 流星電波観測 / 多地点観測 / 前方散乱レーダー / 自然科学教育 / GPS / 超高層大気 / 実習教材 / フィールドワーク / 多地点電波観測 / 電波干渉計 |
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| Outline of Final Research Achievements |
This study developed the teaching aids for experiment of observation which do not have similar methods in the world. The novel observation methods can determine meteor parameters (radiant, velocity) using forward scattering radio waves from meteor trail. A meteor orbit can be determined from this obtained meteor parameters. The feature of the developed observation methods can determine a meteor trail without large professional observation facility. These developed teaching aids can be felt familiar about upper atmosphere, plasma and small solar system bodies. This may also fit active learning. Furthermore, in this study also developed the observation method suitable for outreach activities. As for this, many people may get interested.
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