Parameterisation of Lakes in NWP and Climate Models COSMO/CLM Training Course Langen, Germany, March 2009 Erdmann Heise, Bodo Ritter (German Weather Service,

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Presentation transcript:

Parameterisation of Lakes in NWP and Climate Models COSMO/CLM Training Course Langen, Germany, March 2009 Erdmann Heise, Bodo Ritter (German Weather Service, Offenbach am Main, Germany) Georgy Kirillin (Leibniz Institute of Freshwater Ecology and Inland Fisheries, Berlin, Germany) Ekaterina Kourzeneva (Russian State Hydrometeorological University, St. Petersburg, Russia) Natalia Schneider (University of Kiel, Kiel, Germany) Arkady Terzhevik (Northern Water Problems Institute, Petrozavodsk, Russia) Dmitrii V. Mironov German Weather Service, Offenbach am Main, Germany

Outline Parameterisation of lakes in NWP and climate models – the problem The lake model “FLake” FLake in the COSMO model COSMO-FLake performance Conclusions and outlook

Parameterisation of Lakes in NWP and Climate Models A Twofold Problem (1a) The interaction of the atmosphere with the underlying surface is strongly dependent on the surface temperature and its time-rate-of-change. (Most) NWP systems assume that the water surface temperature can be kept constant over the forecast period. The assumption is doubtful for small-to-medium size relatively shallow lakes, where the diurnal variations of the surface temperature reach several degrees. A large number of such lakes will become resolved-scale features as the horizontal resolution is increased. (1b) Apart from forecasting the lake surface temperature, its initialisation is also an issue. (2) Lakes strongly modify the structure and the transport properties of the atmospheric surface layer. A major outstanding question is the parameterisation of the roughness of the water surface with respect to wind (e.g. limited fetch) and to scalar quantities.

Lake Regions: Finland, Karelia

Lake Regions: Khanty-Mansiisk Region (middle Ob’ river) Lake Regions: Canada

Lake Parameterisation Schemes for NWP and Climate Models (e.g. Hostetler and Bartlein 1990, Hostetler et al. 1993, 1994, Bates et al. 1993, Ljungemir et al. 1996, Goyette et al. 2000, Tsuang et al. 2001, Song et al. 2004, Leon et al. 2005, Mackay 2005, Stepanenko and Lykosov 2005, Stepanenko 2007) One-layer models, complete mixing down to the bottom Neglect stratification  large errors in the surface temperature Turbulence closure models, multi-layer (finite-difference) Describe the lake thermocline better  expensive computationally A compromise between physical realism and computational economy is required A two layer-model with a parameterised vertical temperature structure

The Concept Put forward by Kitaigorodskii and Miropolsky (1970) to describe the temperature structure of the oceanic seasonal thermocline. The essence of the concept is that the temperature profile in the thermocline can be fairly accurately parameterised through a “universal” function of dimensionless depth, using the temperature difference across the thermocline,  =  s -  b, and its thickness,  h, as appropriate scales of temperature and depth:

Analogy with the Mixed-Layer Concept Using  s (t) and h(t) as appropriate scales of temperature and depth, the temperature profile in the upper mixed layer is represented as Since the layer is well mixed, the “universal” function  (  ) is simply a constant equal to 1. Then, integrating the heat transfer equation (partial differential equation in z, t) over z from 0 to h(t), reduces the problem to the solution of an ordinary differential equation for  s (t),

The Lake Model “FLake” the surface temperature, the bottom temperature, the mixed-layer depth, the shape factor with respect to the temperature profile in the thermocline, the depth within bottom sediments penetrated by the thermal wave, and the temperature at that depth. The model is based on the idea of self-similarity (assumed shape) of the evolving temperature profile. That is, instead of solving partial differential equations (in z, t) for the temperature and turbulence quantities (e.g. TKE), the problems is reduced to solving ordinary differential equations for time-dependent parameters (variables) that specify the temperature profile. These are (optional, modules can be switched off) In case of ice-covered lake, additional prognostic variables are the ice depth, the temperature at the ice upper surface, the snow depth, and the temperature at the snow upper surface. Important! The model does not require (re-)tuning.

Schematic representation of the evolving temperature profile (a) The evolving temperature profile is characterised by a number of time-dependent variables, namely, the temperature  s (t) of the mixed layer, its depth h(t), the bottom temperature  b (t), and the temperature-profile shape factor C  (t). Optionally, the depth H(t) within bottom sediments penetrated by the thermal wave and the temperature  H (t) at that depth can be computed. C  (t)

(b) In winter, additional variables are computed, namely, the temperature  I (t) at the ice upper surface and the ice thickness H I (t). Optionally, the temperature  S (t) at the snow upper surface and the snow thickness H S (t) are computed. C  (t)

FLake in NWP and Climate Models: External Parameters geographical latitude (easy) lake fraction of the NWP model grid-box (not so easy) lake depth (not easy at all, e.g. for lack of data) typical wind fetch optical characteristics of lake water (extinction coefficients with respect to solar radiation) depth of the thermally active layer of bottom sediments, temperature at that depth (cf. soil model parameters) Default values of the last three parameters can be used.

Lake Fraction Lake-fraction external-parameter field for the LM1 numerical domain (DWD) of the COSMO model based on the GLCC data set ( with 30 arc sec resolution, that is ca. 1 km at the equator.

Lake Depth Lake depths for the LM1 numerical domain of the COSMO model. The field is developed using various data sets. Each lake is characterised by its mean depth.

FLake in the COSMO Model: Configuration bottom sediment module is switched off (heat flux through the water-bottom sediment interface is zero) snow above the lake ice is not considered explicitly, the effect of snow is accounted for implicitly through the temperature dependence of the ice surface albedo (cf. Mironov and Ritter 2003, 2004) turbulent fluxes at the surface are computed with the current COSMO-model surface-layer scheme (Raschendorfer 2001); optionally, the new surface-layer scheme (Mironov et al. 2003) can be used no tile approach: lakes are the COSMO-model grid-boxes with FR_LAKE>0.5, otherwise land or sea water 2D fields of lake fraction and of lake depth based on data (GLCC, lake-depth data set developed at DWD), default values of other lake-specific parameters

FLake in the COSMO Model: Parallel Experiment COSMO-model parallel experiment over one year, 1 January through 31 December 2006, using the LM1 numerical domain of DWD The entire COSMO-model data assimilation cycle except that the lake surface temperature is not re-initialised through the SST analysis but is predicted by FLake “artificial” initial conditions at the cold start, where the lake surface temperature is equal to the COSMO-model SST from the analysis

FLake in COSMO: Results from Parallel Experiment January – 31 December 2006 Lake Hjälmaren, Sweden (mean depth = 6.1 m) Black – lake surface temperature from the COSMO SST analysis Green – lake surface temperature computed with FLake

FLake in COSMO: Results from Parallel Experiment January – 31 December 2006 Lake Hjälmaren, Sweden (mean depth = 6.1 m) Ice thickness (left) and ice surface temperature (right) computed with COSMO-FLake

FLake in COSMO: Results from Parallel Experiment January – 31 December 2006 Lake Balaton, Hungary (mean depth = 3.3 m) Black – lake surface temperature from the COSMO SST analysis Green – lake surface temperature computed with FLake

FLake in COSMO: Results from Parallel Experiment January – 31 December 2006 Lake Balaton, Hungary (mean depth = 3.3 m). Ice thickness computed with COSMO-FLake. Ice melting: very beginning of March Freeze-up: 10 January

FLake in COSMO: Results from Parallel Experiment January – 31 December 2006 Neisiedlersee, Austria-Hungary (mean depth = 0.8 m) Black – lake surface temperature from the COSMO SST analysis Green – lake surface temperature computed with FLake

FLake in COSMO: Results from Parallel Experiment January – 31 December 2006 Lake Vänern, Sweden (mean depth = 27 m) Black – lake surface temperature from the COSMO SST analysis Green – lake surface temperature computed with FLake

FLake in COSMO: Results from Parallel Experiment January – 31 December 2006 Lough Neagth, UK (mean depth = 8.9 m) Black – lake surface temperature from the COSMO SST analysis Green – lake surface temperature computed with FLake

Conclusions FLake is implemented into the COSMO model (setting the logical switch llake=.FALSE. makes the lake scheme invisible as if it were not present in the COSMO model) Scientific documentation and the synopsis of FLake routines are ready Results from test runs are promising Outlook Testing within COSMO-EU of DWD (work is underway at DWD, c/o Hermann Asensio and Dmitrii Mironov) A comprehensive lake-depth data set, European and eventually global (a prototype data set is available; further work is underway, c/o Ekaterina Kourzeneva, RSHU, Meteo France) FLake Web Page (or its mirror c/o Arkady Terzhevik and Georgiy Kirillin

Thanks for your attention! Acknowledgements. Frank Beyrich, Michael Buchhold, Günther Doms, Thomas Hanisch, Peter Meyring, Van Tan Nguyen, Ulrich Schättler, Christoph Schraff (DWD), Sergey Golosov (IL), Burkhardt Rockel (GKSS), Patrick Samuelsson, Anders Ullerstig (SMHI). EU Commissions, Projects INTAS and INTAS