粒子加速過程の直接計測による惑星放射線帯生成モデルの実証

Research Project

Project/Area Number	18H03727
Research Category	Grant-in-Aid for Scientific Research (A)
Allocation Type	Single-year Grants
Section	一般
Review Section	Medium-sized Section 17:Earth and planetary science and related fields
Research Institution	Tohoku University
Principal Investigator	加藤雄人東北大学, 理学研究科, 教授 (60378982)
Co-Investigator(Kenkyū-buntansha)	笠原慧東京大学, 大学院理学系研究科(理学部), 准教授 (00550500)
Project Period (FY)	2018-04-01 – 2023-03-31
Project Status	Granted (Fiscal Year 2020)
Budget Amount *help	¥43,940,000 (Direct Cost: ¥33,800,000、Indirect Cost: ¥10,140,000) Fiscal Year 2020: ¥8,970,000 (Direct Cost: ¥6,900,000、Indirect Cost: ¥2,070,000) Fiscal Year 2019: ¥8,970,000 (Direct Cost: ¥6,900,000、Indirect Cost: ¥2,070,000) Fiscal Year 2018: ¥15,080,000 (Direct Cost: ¥11,600,000、Indirect Cost: ¥3,480,000)
Keywords	宇宙プラズマ・プラズマ波動 / 地球惑星磁気圏 / 太陽地球システム・宇宙天気 / オーロラ・磁気嵐