Clouds in Partial Atmospheres of Lava Planets and Where to Find Them
Authors: T. Giang Nguyen, Nicolas B. Cowan, Lisa Dang
T. Giang Nguyen et al
2024 The Astronomical Journal168.
Provider: AAS Journals
Caption: Figure 7.
Radiative cooling as a function of pressure and temperature: we calculate the radiative cooling and separate the fluxes into three channels: UV (left), visible (middle), and IR (right).