Global Chemical Transport on Hot Jupiters: Insights from the 2D VULCAN Photochemical Model

Global Chemical Transport on Hot Jupiters: Insights from the 2D VULCAN Photochemical Model

The atmospheric dynamics of tidally locked hot Jupiters is characterized by strong equatorial winds. Understanding the interaction between global circulation and chemistry is crucial in atmospheric studies and interpreting observations. Two-dimensional (2D) photochemical transport models shed light...

Full description

Bibliographic Details
Main Authors: Shang-Min Tsai, Vivien Parmentier, João M. Mendonça, Xianyu Tan, Russell Deitrick, Mark Hammond, Arjun B. Savel, Xi Zhang, Raymond T. Pierrehumbert, Edward W. Schwieterman
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Exoplanet atmospheres
Exoplanet atmospheric composition
Exoplanet atmospheric dynamics
Planetary atmospheres
Online Access:https://doi.org/10.3847/1538-4357/ad1600

Internet

https://doi.org/10.3847/1538-4357/ad1600

Similar Items