The method for computing the surface turbulent heat and radiative exchange, evaporative flux, and surface drag is integrally coupled with the formulation of heat transfer through the sea ice and snow. The equation governing vertical heat transfer in the ice and snow, which allows for internal absorption of penetrating solar radiation, is
The boundary condition for the heat equation at the surface is
Snow melt and accumulation is computed from
When CAM 3.0 is coupled to the mixed layer ocean and the sea ice is snow-free, sea ice surface melt is computed from
Parameterizations of albedo, surface fluxes, brine pockets, and shortwave radiative transfer within the sea ice are given next. Finally, the numerical solution to Eq. 6.1 is described. Numerical methods for Eqs. 6.2 -6.6 are straight-forward and hence are not described here.
Symbol | Description | Value |
Density of snow | 330 kg m | |
Density of ice | 917 kg m | |
Density of surface ocean water | 1026 kg m | |
Specific heat of atmosphere dry | 1005 J kg K | |
Specific heat of atmosphere water | 1810 J kg K | |
Specific heat of ocean water | 3996 J kg K | |
Specific heat of snow | 0 J kg K | |
Specific heat of fresh ice | 2054 J kg K | |
Aerodynamic roughness of ice | 5.0x10 m | |
Reference height for bulk fluxes | 10 m | |
saturation specific humidity constant | 11637800 | |
saturation specific humidity constant | 5897.8 | |
Thermal conductivity of snow | 0.31 W m K | |
Thermal conductivity of fresh ice | 2.0340 W m K | |
Thermal conductivity ice constant | 0.1172 W m ppt | |
Latent heat of fusion of ice | 3.340x10 J kg | |
Latent heat of vaporization | 2.501x10 J kg | |
Melting temperature of top surface | 0 C | |
Ocean freezing temperature constant | 0.054 C ppt | |
Stefan-Boltzmann constant | 5.67x10 W m K | |
Ice emissivity | 0.95 | |
Ice SW visible extinction coefficient | 1.4 m | |
Ice SW near-ir extinction coefficient | 17.6 m |