The Deep Atmospheric Composition of Jupiter from Thermochemical Calculations Based on Galileo and Juno Data
The deep atmosphere of Jupiter is obscured beneath thick clouds. This causes direct observations to be difficult, and thermochemical equilibrium models fill in the observational gaps. This research uses <i>Galileo</i> and <i>Juno</i> data together with the Gibbs free energy m...
Hlavní autoři: | , , , , , , |
---|---|
Médium: | Článek |
Jazyk: | English |
Vydáno: |
MDPI AG
2023-02-01
|
Edice: | Remote Sensing |
Témata: | |
On-line přístup: | https://www.mdpi.com/2072-4292/15/3/841 |