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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 8.

Consistency check of HELIOS by examining the temperature–pressure profiles (left panel) and synthetic spectra (right panel) in the idealized limits of scattering: ﹩{g}_{0}=0﹩ (isotropic scattering), ﹩{g}_{0}=0.5﹩ (forward scattering), and ﹩{g}_{0}=-0.5﹩ (backward scattering). For illustration, we set ﹩{\omega }_{0}=0.5﹩. Both the single-scattering albedo (﹩{\omega }_{0}﹩) and scattering asymmetry factor (g0) are assumed to be constant across wavelength, but we note that the two-stream solutions we implemented allow for them to generally be specified as functions of wavelength, temperature, and pressure. The qualitative trends associated with the temperature–pressure profiles and synthetic spectra are consistent with physical expectations (see text).

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