Basic Physical Processes of Weakly Ionized Plasma and Planet Formation
| Project/Area Number |
18540238
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| Research Category |
Grant-in-Aid for Scientific Research (C)
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| Allocation Type | Single-year Grants |
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| Section | 一般 |
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| Research Field |
Astronomy
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| Research Institution | Kyoto University |
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Principal Investigator |
INUTSUKA Shu-ichiro Kyoto University, 大学院・理学研究科, 教授 (80270453)
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| Project Period (FY) |
2006 – 2009
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| Project Status |
Completed (Fiscal Year 2009)
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| Budget Amount *help |
¥4,060,000 (Direct Cost: ¥3,400,000、Indirect Cost: ¥660,000)
Fiscal Year 2009: ¥780,000 (Direct Cost: ¥600,000、Indirect Cost: ¥180,000)
Fiscal Year 2008: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2007: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2006: ¥1,200,000 (Direct Cost: ¥1,200,000)
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| Keywords | 星形成 / 惑星形成 / 系外惑星系 / 原始惑星系円盤 / MHD / 弱電離プラズマ / 太陽風 / 乱流 / 惑星起源・進化 / 理論天文学 / 微惑星 / 重力不安定性 / 磁気流体力学 / 電離度 / 系外惑星 / 塵粒子 / プラズマ / 摩擦電離 / 磁気乱流 / 磁気回転不安定性 / SPH |
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| Research Abstract |
I investigate the various physical processes in weakly ionized protoplanetary disks and clarified the important processes for the disk evolution and planet formation. According to these developments, I have proposed a new scenario for planet formation, called "Hybrid Scenario of Planet Formation."
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Report
(6 results)
Research Products
(123 results)
