Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison...

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Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and Oleg Evteev Hydrometcentre of Russia

Transcript of Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison...

Page 1: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.

Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison

with profilers and radiosondes data

Veniamin Perov and Oleg Evteev

Hydrometcentre of Russia

Page 2: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.
Page 3: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.

z

TKE

Schematic view of a turbulent length scale (mixing length)scheme based on a parcel displacement (BL89) for a boundary layer scheme of the

COSMO model

Page 4: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.

)()()( '' zEdzzzg

vv

lz

z ref

up

)()()( '' zEdzzzg

vv

lz

z ref

up

,2/1downup llL Lkzl

111

Blackadar formula, local l

.m 200,76.0,40.0,111

2/1

lCeC

N

lzl NN

Turbulent length scale based on a parcel displacement scheme

Page 5: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.
Page 6: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.
Page 7: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.
Page 8: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.

Potential temperature profiles for local L (blue) and nonlocal L(red),Moscow 12h, 17.07.09

Page 9: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.
Page 10: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.
Page 11: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.
Page 12: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.
Page 13: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.
Page 14: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.

Difference of T2M fields (new – ref), COSMO-RU, 19.07.2009

Page 15: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.

Differences for T2M fields (nonlocal L minus local L), 12h, 170709,Full area

Page 16: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.

Differences for T2M fields (nonlocal L minus local L), 12h, 17072009,Moscow area

Page 17: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.

Differences for T2M fields (nonlocal L minus local L), left and total cloud cover,

right , Black Sea coastal region

Page 18: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.

Differences for TD2M fields (nonlocal L minus local L), 12h, 17072009,Moscow area

Page 19: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.

Differences for U10M fields (nonlocal L minus local L), 12h, 17072009,Moscow area

Page 20: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.

• Mesoscale modeling in mountain area should include simulations of main processes in this domain. These are formation of the regional slope winds, blocked flow, deviated flow, sheltering effect after obstacle, generation of turbulence by wind shear at the lower part of flow.

• In the upper part of flow it will be generation of turbulence by roughness, mountain waves and generation of turbulence by mountain wave breaking.

• For high mountains we need also to take into account a tropopause perturbation. All these processes require the use of three-dimensional turbulence and the non-use of simple diagnostic formulas for turbulence length scale (mixing length).

• In this case, together with the equation for the turbulent kinetic energy (TKE) will have to use the equation for mixing length or equation for the dissipation of TKE.

Mesoscale modeling in mountain region

Page 21: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.

Turbulence and convection in mountain region

Page 22: Testing of the non-local turbulent length-scale formulation within 3D COSMO-RU model, comparison with profilers and radiosondes data Veniamin Perov and.

Main results

• Algorithm for computing the nonlinear turbulence length scale based on displacement method of air parcel (BL89) was developed. A new algorithm for calculation turbulence length scale has a more rigorous physical basis in comparison with the algorithm currently used (Blackadar formulae).

• Algorithm was impact in module TUBDIFF of main COSMO program • Calculations were performed for convective situations (July 2009) by full

3-D COSMO model. Results showed differences in fields of temperature, humidity, clouds and wind between variants with local (reference) and nonlocal turbulence length scales.

• An article for publication is prepared base on the current work.