Snow, forest and lake aspects in the HIRLAM surface scheme Stefan Gollvik, SMHI, Patrick Samuelsson, RC, SMHI.

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Presentation transcript:

Snow, forest and lake aspects in the HIRLAM surface scheme Stefan Gollvik, SMHI, Patrick Samuelsson, RC, SMHI

Totally 7 tiles: sea, ice, open land, low veg., forest, open land snow, forest snow For all land tiles: 3 prognostic tempereatures, soil depths of 1, 7.2 and 43.2 cm. Heat conduction dependent on soil type, soil water and (parameterized) soil ice. Climatological forcing below third layer. The forest tile has a common (prognostic) canopy temperature and separate temperatures for the snow free and snow covered forest floor. Two separate snow covers with separate evolutions of temperature, snow amount, liquid water, density and albedo Sea ice has 2 layers, the deepest 92 cm for oceans and 42 cm in the Baltic. Heat flux at the bottom, from the water. At present no lake model, work is going on here. A new surface scheme for HIRLAM including snow and canopy temperature

The snow tiles The surface analysis, SPAN (Navasques et.al.) is performing an OI analysis of snow depth. The first guess is relaxed towards climatology. Using the first guess snow density, the snow depth is transformed to the model variable, snow water equivalent. The analysis increment (for the open land snow) is also added to the ice tile and the forest tile multiplied with an ad hoc factor of 1 and 0.5 respectively. The snow fractions are simply estimated as: At present an ad hoc sncrit as a function of latitude and time of the year Idea: Estimate sncrit by also analysing the snow fraction (satellite ?)

Now slightly reduced value of this resistance (tuning)

Snow density calculations The snow density is calculated by a weighted value of three components: dry snow water in the snow ice due to frozen water in the snow, and rain freezing on cold snow (at present not stored as a separate variable) The dry snow is, in turn, composed of old snow, with gradually increasing density (Douville et.al.,1995), and newly fallen snow with density ρ min (=100kg/m3). The amount of water which can be suspended in the snow, before going to the soil, wsat, (fraction) is a function of the snow density: wsat= 0.12 – 0.08 (ρ sn - ρ min ) / (550 - ρ min ) The snow density is thus influencing the heat capacity of the thermally active layer.

Phase shift of water in the snow The total energy available for the snow per unit time is: If > 0, the timestep is divided into two parts, first the time it takes to increase the temperature to melting point, and then the rest of the timestep, the energy goes to melting, and the heat conduction is done with the temperature of the melting snow as upper boundary condition If < 0, the timestep can be divided into freezing, followed by cooling. It is assumed that the water is suspended in the snow, and the freezing can penetrate down to a typical depth Sn freeze (0.03m). How much of the timestep, that is used for freezing (freezefrac), before the cooling takes place, is parameterized as a function of Sn freeze, the amount of water in the snow, wsat, snow depth and density.

T scn2 T sc2 T dsn TdTd T clim T Low tree heat capacity The forest tile Canopy air temperature and humidity q ca Calculations of r b and r d follows Choudbury and Monteith, 1988 Canopy water

Radiation in the forest We define a view factor viewfs, defined as how much of the incoming SW radiation is passing the canopy and reaching the forest floor. This parameter is a function of LAI, solar angle and total cloudcover. The corresponding factor for long wave radiation, viewfl, is only a function of LAI. Then we calculate the radiation as usual between soil and atmosphere, but also between the canopy and the forest floor, both for snow covered and snow free parts, separately.

Heat conduction in the soil. Dependent on the fractions of clay, silt and sand the soil is classified in 11 classes: Dependent on the class, the porosity and amount of quartz is estimated, and the heat conductivity is calculated, taking into account the amount of soil water and the soil ice, at present estimated as a function of temperature (Viterbo). This parameterization follows Peters-Lidard et.al., 1998

March 2006

T2m bias at 12 UTC +48H, left=new surface scheme, right=ref. March 2006

T2m bias at 00 UTC +48H, left=new surface scheme, right=ref. March 2006

Some remaining bias problems in summer, June 2005

Something about lake plans in HIRLAM

FLake A lake model based on two-layer parametric representation of the temperature profile and self-similarity concept. Thus, it is not a 1D multi-layer model (like SMHI-PROBE), which makes it numerically efficient. FLake is fully coupled to RCA3 (at each time step): RCA3 provides: u,v,q,T,SW,LW, psurf,(Rain & Snow not used at the moment) FLake provides: turbulent fluxes (HIRLAM concept), albedo + prognostic variables…

Prognostic variables in FLake Surface temperatures (water, ice, snow ) Ice (and snow) depth Mixed layer depth Shape factor Bottom temperature (Extreme temperature of bottom sediment) (Depth of the sediment extreme temperature)

RCA3/FLake results RCA3/FLake: ERA40 lateral and SST boundary conditions Resolution: 0.44° x 0.44° horizontal 24 vert. levels 30 min time step Spin up: Sep 1 –Dec Analysed period: Jan 1 –Dec

FLake results Due to limitations of information (depth) in lake data base most lakes are set to standard depth =10 m.

HIRLAM surface plans Tuning of the surface scheme, in connection with the other physical parameterizations. Start the work of externalization Compare this scheme with SURFEX Start work of interaction between the surface analysis and 4D-var Improve the changes of surface temperatures in Span, to better fit the T2m-analysis (idea from Balsamo ?) Work is under way, to implement Flake in HIRLAM Add snow on sea ice, and urban area (Aladin)

Thank you