Super-adiabatic temperature gradient at Jupiter's equatorial zone and implications for the water abundance-Reference-Cited by-同舟云学术

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Super-adiabatic temperature gradient at Jupiter's equatorial zone and implications for the water abundance

Published:2024-05 Issue: Volume:414 Page:116028
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Li Cheng,Allison Michael,Atreya Sushil,Brueshaber Shawn,Fletcher Leigh N.,Guillot Tristan,Li Liming,Lunine Jonathan,Miguel Yamila,Orton Glenn,Steffes Paul,Waite J. Hunter,Wong Michael H.,Levin Steven,Bolton Scott

Funder

Horizon 2020

NASA Marshall Space Flight Center

National Aeronautics and Space Administration

Southwest Research Institute

European Research Council

Publisher

Elsevier BV

Reference62 articles.

1. Interaction of a cumulus cloud ensemble with the large-scale environment, Part I;Arakawa;J. Atmos. Sci.,1974

2. The chemical composition of the sun;Asplund;Annu. Rev. Astron. Astrophys.,2009

3. Laboratory measurements of the 5–20 cm wavelength opacity of ammonia, water vapor, and methane under simulated conditions for the deep jovian atmosphere;Bellotti;Icarus,2016

4. The Betts-Miller scheme;Betts,1993

5. Highly Depleted Alkali Metals in Jupiter’s Deep Atmosphere;Bhattacharya;ApJL,2023

Cited by 3 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. GASTLI;Astronomy & Astrophysics;2024-08

2. The Metallicity and Carbon-to-oxygen Ratio of the Ultrahot Jupiter WASP-76b from Gemini-S/IGRINS;The Astronomical Journal;2024-06-18

3. Recipes for Forming a Carbon–Rich Giant Planet;Space Science Reviews;2024-06

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