Piomass is a fairly simple model it uses wind speed, wind direction, surface air temperature, cloud cover and with the latest update sea surface temperatures. Cloud cover and time of year are used to calculate solar and longwave radiation. Using air temperature and energy input modified by currents, wind and SST’s along with ice thicknesses, concentration and extent are used to calculate ice growth. Currents (from unnamed ocean model) and wind can move ice when the ice is mobile and SST energy. From what I read that is the basics
Piomas concerns:
*There is currently no funding to maintain or upgrade Piomas
*Most of the validation data is older 6 years or older
http://psc.apl.uw.edu/sea_ice_cdr/data tables.html Exceptions:
BGEP, which is only 4 moored buoys in Beaufort sea.
icebridge quicklook, that prerelease data has a stated accuracy of +/- 1 meter of thickness. The final versions is much more accurate but not the quicklook data.
Cryostat volume is 23% lower than Piomass while this is not thickness it the extent is the similar.
*Piomass shows thin ice in Greenland Sea where none exists.
Piomas more info:
*Piomas uses NSIDC ice concentration and snow extent NISE near real time snow and ice extent 25 km
*Reynalds Sea surface temperatures for NCEP/NCAR on ice free areas
*Atmospheric wind, surface air and cloud cover to compute solar and longwave radiation
*Unnamed forced ocean circulation model with input at its open boundaries located at 45 north
*Stated piomas uncertainty +/- 1.35x10^3 km^3 areas in sea of Okhotsk and Gulf of St Lawrence are
excluded
*spatial coverage 45 N to 90 N grid size 360 x 120 generalized curvilinear coordinate system (Grid shape irregular
Focus only on ice growth
Hycom uses hybrid coordinates layered in the open stratified ocean and smoothly transition to terrain following in shallow areas with specific coordinates for mixed layers or unstratified seas. It’s a global ocean model coupled with a global atmospheric model.
It includes such physical processes as background internal wave breaking, shear instability mixing, double diffusion salt fingering and diffusive instability are parameterized. In the surface boundary layer wind driven mixing, surface buoyancy fluxes and convective instabilities are parameterized. Other factors include nonlocal mixing of temperature and salinity which permits counter gradient fluxes. The Kraus-Turner slab model the dynamical instability model of Price and the MellorYamada level 2.5 turbulence closure of the Prineton ocen model.
Hycom algorithms
advdiff.pdf (horizontal advection/diffusion)
boundary.pdf (boundary conditions)
diapycnal.pdf (three interior diapycnal mixing algorithms)
float.pdf (synthetic floats/drifters/moorings)
hybrid.pdf (hybrid vertical coordinate adjustment)
ice.pdf (energy loan ice model)
KPP.pdf (K-Profile Parameterization vertical mixing)
KT.pdf (three Kraus-Turner mixed layer models)
mesh.pdf (horizontal mesh)
momentum.pdf (momentum equation, including pressure gradient force)
MY.pdf (Mellor-Yamada level 2.5 turbulence closure vertical mixing)
PWP.pdf (Price-Weller-Pinkel dynamical instability vertical mixing)
state.pdf (equation of state, including cabbeling and thermobaricity)
surface.pdf (surface fluxes, including penetrating shortwave radiation)
vdiff.pdf (solution of vertical diffusion equation)
Other algorithms used from MICOM (HYCOM’s precursor) include continuity equation barotropic
momentum equation advection algorithm and vertical mode splitting
https://www.hycom.org/attachments/067_overview.pdfHycom does an 8 day run every day.
0.08 degree resolution from 40 N to 40 S and 0.04 degree resolution poleward.
Focus on entire ocean atmosphere with parameterization of many physical interactions.