Spherical Radiative Transfer in C++ (SRTC++): A Parallel Monte-Carlo Radiative Transfer Model for Titan: A Parallel Monte Carlo Radiative Transfer Model for Titan

  • Brian K. Jackson
  • , Jason W. Barnes
  • , Shannon M. Mackenzie
  • , Eliot F. Young
  • , Laura E. Trouille
  • , Sèbastien Rodriguez
  • , Thomas Cornet
  • , Máté Ádámkovics
  • , Christophe Sotin
  • , Jason M. Soderblom

Research output: Contribution to journalArticlepeer-review

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Abstract

We present a new computer program, SRTC++, to solve spatial problems associated with explorations of Saturn’s moon Titan. The program implements a three-dimensional structure well-suited to addressing shortcomings arising from plane-parallel radiative transfer approaches. SRTC++’s design uses parallel processing in an object-oriented, compiled computer language (C++) leading to a flexible and fast architecture. We validate SRTC++ using analytical results, semianalytical radiative transfer expressions, and an existing Titan plane-parallel model. SRTC++ complements existing approaches, addressing spatial problems like near-limb and near-terminator geometries, non-Lambertian surface phase functions (including specular reflections), and surface albedo nonuniformity.

Original languageAmerican English
Article number264
JournalThe Astronomical Journal
Volume155
Issue number6
DOIs
StatePublished - 1 Jun 2018

Keywords

  • planets and satellites: individual (Titan)
  • radiative transfer

EGS Disciplines

  • Physics

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