MARCS 1D Archives

Diagram of the MSG model algorithm for cloudy substellar atmospheres. The boxes with a dashed outline indicate parameters that are inputs to the model. The boxes with a dotted outline indicate control processes within the workflow. For a detailed explanation of the cloud formation process, see section 2. For a detailed explanation of the control process, see section 4.3. For the convergence criteria considered under the control process see section 4.1 -- astro-ph.EP

Astronomy & Telescopes, Atmospheres, Climate, Weather, Brown Dwarfs, Exoplanets, -moons, -comets, Imaging & Spectroscopy, Status Report

The MSG Model For Cloudy Substellar Atmospheres: A Grid Of Self-consistent Substellar Atmosphere Models With Microphysical Cloud Formation

by Keith CowingJanuary 22, 2025January 22, 2025

State-of-the-art JWST observations are unveiling unprecedented views into the atmospheres of substellar objects in the infrared, further highlighting the importance of clouds. Current forward models struggle to fit the silicate […]

MARCS 1D

The MSG Model For Cloudy Substellar Atmospheres: A Grid Of Self-consistent Substellar Atmosphere Models With Microphysical Cloud Formation

Gullies In The Equatorial Region of Mars

Orbital Biosignature Assay: Watching Forests Grow From Space

Signs And Signatures Of Intelligence

CO Snow Lines Are Stabilised By The Vertical Transport Of Volatiles

Multi-year Ground-Based Survey Photometry of Active Comet 103P/Hartley 2 and Centaur (2060) Chiron: A Tale of Two Comets in the Pre-LSST Era