Radiatively Active Clouds and Magnetic Effects Explored in a Grid of Hot Jupiter GCMs

Documenti analoghi

• Comparative Planetology of Magnetic Effects in Ultrahot Jupiters: Trends in High Resolution Spectroscopy
  di: Beltz, Hayley, et al.
  Pubblicazione: (2024)
• A Direct Comparison between the use of Double Gray and Multiwavelength Radiative Transfer in a General Circulation Model with and without Radiatively Active Clouds
  di: Malsky, Isaac, et al.
  Pubblicazione: (2023)
• Up, Up, and Away: Winds and Dynamical Structure as a Function of Altitude in the Ultra-Hot Jupiter WASP-76b
  di: Kesseli, Aurora Y., et al.
  Pubblicazione: (2024)
• Exploring the Impact of Tilted Magnetic Dipoles on the Atmospheric Dynamics of Hot Jupiters: Towards an Improved Magnetohydrodynamic Framework
  di: Fecanin, James, et al.
  Pubblicazione: (2026)
• Assessing robustness and bias in 1D retrievals of 3D Global Circulation Models at high spectral resolution: a WASP-76 b simulation case study in emission
  di: van Sluijs, Lennart, et al.
  Pubblicazione: (2025)