Figure 3 from HELIOS: AN OPEN-SOURCE, GPU-ACCELERATED RADIATIVE TRANSFER CODE FOR SELF-CONSISTENT EXOPLANETARY ATMOSPHERES

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

HELIOS: AN OPEN-SOURCE, GPU-ACCELERATED RADIATIVE TRANSFER CODE FOR SELF-CONSISTENT EXOPLANETARY ATMOSPHERES

Authors: Matej Malik, Luc Grosheintz, João M. Mendonça, Simon L. Grimm, Baptiste Lavie, Daniel Kitzmann, Shang-Min Tsai, Adam Burrows, Laura Kreidberg, Megan Bedell, Jacob L. Bean, Kevin B. Stevenson, and Kevin Heng

2017 The Astronomical Journal 153 56.

Provider: AAS Journals

Caption: Figure 3.

Opacities, as functions of wavelength, for all of the opacity sources used in the current study, computed using HELIOS-K (Grimm & Heng 2015). For illustration, we set T = 1500 K and P = 1 bar. Each opacity is weighted by its mass mixing ratio. We include only Rayleigh scattering by molecular hydrogen, but CIA associated with both H₂–H₂ and H₂–He pairs.

Other Images in This Article

Copyright and Terms & Conditions