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A hierarchial set of energy balance models parameterized for the Earth system using the Rapid Radiative Transfer Model for GCMs (RRTM-G).

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Mihir-DG/earth-EBMs

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earth-EBMs

A hierarchial set of energy balance models parameterized for the Earth system using the Rapid Radiative Transfer Model for GCMs (RRTM-G) as implemented in climt using Python. Convection is modeled in the RCE setup as a secondary adjustive mechanism that is activated in regions of radiative instability.

Models:

  1. 0D Radiative Equilibrium
  2. 1D Radiative Equilibrium (RE)
  3. 1D Radiative-Convective Equilibrium (RCE)

0-D Model Initial Conditions:

  • Planetary Albedo: 0.29
  • Emissivity Coefficient: 0.619 +/- 0.000425

1-D Model Initial Conditions:

  • Surface Type: Aquaplanet
  • Zenith angle: 75 deg.
  • Surface Direct SW Albedo: 0.3
  • Surface Diffuse SW Albedo: 0.259 (0.3 sin(60))
  • Surface Direct Near-Infrared Albedo: 0.45
  • Ocean Mixed Layer Depth: 40 m
  • Solar variation: None; Uniform flux of 1367.6
  • Error margin in energy budget: 5 W/m^2.
  • RE Energetics
    • Surface temperature: 250 K
    • Air Temperature: Isothermal; 230 K.
  • RCE Energetics
    • Surface Temperature: 275 K
    • Air Temperature: Isothermal; 250 K

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A hierarchial set of energy balance models parameterized for the Earth system using the Rapid Radiative Transfer Model for GCMs (RRTM-G).

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