Modeling the disequilibrium species for Jupiter and Saturn: Implications for Juno and Saturn entry probe
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- 作者：Dong Wang ; a ; dw459@cornell.edu" class="auth_mail" title="E-mail the corresponding author ; wangdong8500@gmail.com" class="auth_mail" title="E-mail the corresponding author ; Jonathan I. Luninea ; jlunine@astro.cornell.edu" class="auth_mail" title="E-mail the corresponding author ; Olivier Mousisb
- 关键词：Abundances ; atmospheres ; Atmospheres ; chemistry ; Jupiter ; atmosphere ; Saturn ; atmosphere
- 刊名：Icarus
- 出版年：2016
- 出版时间：15 September 2016
- 年：2016
- 卷：276
- 期：Complete
- 页码：21-38
- 全文大小：2751 K
文摘
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A diffusion-kinetics code is applied to Jupiter and Saturn’s atmospheres.
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Chemistry for species containing H, C, N, O, P, Si, Ge, and As is investigated.
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Tropospheric C2H6 is predicted to be a tracer for the deep eddy diffusion coefficient.
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Latitudinal variations for CO and GeH4 abundances are predicted.
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Implications for constraining deep oxygen via Juno and a Saturn entry probe are discussed.