Opendata

ATMO

ATMO is a 1D-2D atmospheric code for the study of the atmosphere of brown dwarfs and exoplanets. The code has originally been developed at the University of Exeter (http://exoclimatology.com) and is currently a collaboration between different groups across the globe. The main developers are:

      • 1D and 2D newton solver: P. Tremblin
      • Radiative transfer: D. Amundsen, P. Tremblin
      • Opacities: D. Amundsen, M. Phillips, R. Ridgway, J. Goyal
      • Equilibrium chemistry: P. Tremblin, B. Drummond, J. Goyal
      • Condensation and rainouts: P. Tremblin, J. Goyal
      • Out-of-equilibrium chemistry: O. Venot, E. Hebrard, B. Drummond
      • Convection: P. Tremblin, M. Phillips
      • Retrieval: D. Sing

Several grids have been developed with the code:

 


ARK

ARK is a 3D hydrodynamics code for the study of convective problems. The code is freely available at https://gitlab.erc-atmo.eu/erc-atmo/ark. It has been used in several studies:

 


DYNAMICO

DYNAMICO is a general circulation model (GCM) currently developed at IPSL available at http://forge.ipsl.jussieu.fr/dynamico. We have developed a patch available at https://gitlab.erc-atmo.eu/erc-atmo/dynamico_hj to adapt the code to the study of the atmospheric circulation of hot Jupiters showing that the long timescale deep circulation (“paleoclimate” like study) is responsible for the inflated radius of these planets.