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)

書誌事項

タイトル別名
  • Numerical Modeling of Moist Convection in Jupiter's Atmosphere

この論文をさがす

抄録

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.

収録刊行物

詳細情報 詳細情報について

問題の指摘

ページトップへ