Numerical Modeling of Moist Convection in Jupiter's Atmosphere
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- Sugiyama,Ko-ichiro
- Dep. of Cosmosciences, Hokkaido Univ.
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- Odaka,Masatsugu
- Dep. of Cosmosciences, Hokkaido Univ.
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- Nakajima,Kensuke
- Dep. of Earth and Planetary Sciences, Kyushu Univ.
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- Hayashi,Yoshi-Yuki
- Dep. of Earth and Planetary Sciences, Kobe Univ.
Bibliographic Information
- Other Title
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- 木星大気雲対流の直接数値計算(大気・海洋・惑星の流れ(3),一般講演)
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Abstract
We develop a two-dimensional fluid dynamical model that incorporates condensation of H_2O and NH_3 and the production reaction of NH_4SH. We run the model for a long simulation time in order to examine the structure of moist convection layer in Jupiter's atmosphere that establishes through a large number of life cycles of convective clouds. Our results show that H_2O and NH_4SH cloud particles are advected to the altitudes above the NH_3 condensation level. The convective motion and the distribution of condensible species depend on the deep tropospheric mixing ratios of condensible volatiles.
Journal
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- 日本流体力学会年会講演論文集
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日本流体力学会年会講演論文集 2007 247-, 2007-08-06
日本流体力学会
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Details 詳細情報について
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- CRID
- 1540291245378906880
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- NII Article ID
- 110008459222
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- NII Book ID
- AA11567941
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- Text Lang
- ja
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- Data Source
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- NDL-Digital
- CiNii Articles