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intercomparisons:a2_lambert

Case A2: Rayleigh atmosphere with Lambertian surface

Setup:

  • similar to case A1, with small modifications
  • surface albedo: 0.3
  • optical thickness: 0.1
  • Rayleigh depolarization factor: 0.03
  • transmittance at bottom and reflectance at top of layer
  • solar zenith angle sza: 50°
  • solar azimuth angle saa: 0°
  • viewing zenith angles
    • at bottom: vza: 0° - 80°, 5° increment
    • at top: vza: 100° - 180°, 5° increment
  • viewing azimuth angle vaa: 0° - 180°, 5° increment

Output format:

Results

Difference plots between the models IPOL, 3DMCPOL, SPARTA (previously named TROPOS), SHDOM, PSTAR and MYSTIC for the full radiation field:
3DMCPOL
IPOL
SPARTA
SHDOM
PSTAR

Data of all models (MYSTIC and 3DMCPOL include also standard deviation):
MYSTIC
3DMCPOL
IPOL
SPARTA
SHDOM
PSTAR

intercomparisons/a2_lambert.txt · Last modified: 2015/03/10 16:41 (external edit)