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無限解析研究部門（竹広 真一）
Showing the original Japanese · View translation
地球や惑星の大気・マントル・中心核の流れを、流体力学で調べる研究室。
AboutAbout the lab
惑星規模の流れを、単純なモデルで理解する。
竹広研究室は、
惑星の
惑星大気や
研究グループの
Key terms
- 密度成層
- 重い流体が
下、 軽い流体が 上と いうように、 高さや 深さに よって 流体の 密度が 層状に 変わっている 状態 - 数値実験
- 現象を
単純化した モデルの 方程式を、 コンピュータで 解いて 流れの 様子を 調べる 方法 - 熱対流
- 下から
温められた 流体が 上昇し、 冷えて 下降する ことで できる 流れ - シアー流
- 速度の
違う 流れが 平行に 並んでいる 流れ。 乱流に 変わる きっかけと なる 不安定が 起こる
ResearchResearch themes
地球や
*Illustrative image回転球殻内の熱対流と帯状流
回転の
*Illustrative imageシアー流の不安定と波の過剰反射
速度差の
*Illustrative image研究のための計算機環境の開発
地球
MembersFaculty
- Associate Professor竹広 真一
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Report an errorAbout the images
The top and research theme images are illustrative and were not taken at the lab. They are cropped from Wikimedia Commons images. Cropped CC BY-SA images are provided under the same CC BY-SA license as the original (version shown on each line).
- Top image: “A Close-Up Look at Jupiter’s Dynamic Atmosphere ( )” European Space Agency / CC BY 2.0 (cropped)
- 回転球殻内の
熱対流と 帯状流: “Lower Mantle Superplume” Brews ohare / CC BY-SA 3.0 (cropped) - シアー流の
不安定と 波の 過剰反射: “Kelvin–Helmholtz instability clouds” fdecomite / CC BY 2.0 (cropped) - 研究の
ための 計算機環境の 開発: “Kraken Supercomputer ( )” Oak Ridge National Laboratory / CC BY 2.0 (cropped) - Related lab (無限解析研究部門
（緒方 芳子） ): “Thousands of Atoms Swap 'Spins' with Partners in Quantum Square Dance ( )” National Institute of Standards and Technology / Public domain (cropped) - Related lab (無限解析研究部門
（玉川 安騎男） ): “Klein-map” PSL27 / CC BY-SA 4.0 (cropped) - Related lab (無限解析研究部門
（望月 新一） ): “Kyoto University RIMS” KATSURA Roen / CC BY 3.0 (cropped) - Related lab (無限解析研究部門
（並河 良典） ): “Consani-Scholten” Ursulageorges / CC BY 4.0 (cropped)
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