Radiative Transfer model of Jupiter’s atmosphere in ASIMUT-ALVL

Key Points

• Modeling of Jupiter's atmosphere focused on radiative transfer dynamics and thermal radiation phenomena.
• The study reveals key interactions of thermal radiation, enhancing spectral analysis capabilities within planetary science.
• Assessment using advanced modeling techniques in the ASIMUT-ALVL framework, which enables detailed atmospheric simulations.
• This approach may enable greater insight into Jupiter’s atmospheric processes and potential climate dynamics.