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Data_README.md

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Base Titan Atmosphere

All molecules are compared to this in analysis files

  • Atmosphere: Base Titan atmosphere: 96% N2 & 1 scalar CH4 (standard Titan object CH4 scalar vertical profile ~3.13%)
  • Aerosols: Khare Haze: 6.325ppb abundance & .15um Radius with standard Titan object haze vertical profile
  • Surface: 100% Titan USGS surface

Lakes & Ices

  • Atmosphere: Base Titan atmosphere: 96% N2 & 1 scalar CH4 (standard Titan object CH4 scalar vertical profile ~3.13%)
  • Aerosols: Khare Haze: 6.325ppb abundance & .15um Radius with standard Titan object haze vertical profile
  • Surface: 80% Titan USGS surface 20% Lake component with thickness 10um if OPTIC type

Hazes

  • Atmosphere: Base Titan atmosphere: 96% N2 & 1 scalar CH4 (standard Titan object CH4 scalar vertical profile ~3.13%)
  • Aerosols: Haze Type: 6.325ppb abundance & change radius with standard Titan object haze vertical profile
  • Surface: 100% Titan USGS surface

Atmosphere

  • Atmosphere: Base Titan atmosphere: 96% N2 & 1 scalar CH4 (standard Titan object CH4 scalar vertical profile ~3.13%) with added molecule at 10ppmv with a width of 0.7 if source is from JPL
  • Aerosols: Khare Haze: 6.325ppb abundance & .15um Radius with standard Titan object haze vertical profile
  • Surface: 100% Titan USGS surface

Isotopes

CO:

  • Atmosphere: Titan atmosphere: 96% N2 & 1 scalar CH4 (standard Titan object CH4 scalar vertical profile ~3.13%) with CO isotopes varied +-0.05 scalar increments
  • 12C16O .987 scalar
  • 13C16O .011 scalar
  • 12C18O .002 scalar
  • Aerosols: Khare Haze: 6.325ppb abundance & .15um Radius with standard Titan object haze vertical profile
  • Surface: 100% Titan USGS surface CH4:
  • Atmosphere: Titan atmosphere: 96% N2 & 1 scalar CH4 (standard Titan object CH4 scalar vertical profile ~3.13%) with CH4 isotopes (12CH4, 13CH4) varied at 1 +-0.05 scalar increments
  • Aerosols: Khare Haze: 6.325ppb abundance & .15um Radius with standard Titan object haze vertical profile
  • Surface: 100% Titan USGS surface