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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  • Numerical Modeling of Moist Convection in Jupiter's Atmosphere

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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.

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