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Observation and simulation of flow in vegetation canopies Roger H. Shaw University of California, Davis.

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Presentation on theme: "Observation and simulation of flow in vegetation canopies Roger H. Shaw University of California, Davis."— Presentation transcript:

1 Observation and simulation of flow in vegetation canopies Roger H. Shaw University of California, Davis

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3 Kinetic energy spectral densities that are strongly peaked Strong correlations between streamwise and vertical velocities Large velocity skewness (Sk u >0; Sk w <0) Transport dominated by organized structures Larger contributions from sweep motions than ejections Canopy turbulence

4 “We will understand the movement of the stars long before we understand canopy turbulence” Galileo Galilei

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7 Time traces of velocity components

8 Z=2.4h

9 Z=0.9h

10 Scalar ‘ramps’ correlated through the depth of the canopy show wholesale ‘ flushing’ of the canopy airspace by large scale gusts.

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13 Scalar

14 Vertical velocity

15 Streamwise velocity

16 Turbulent kinetic energy budget determined from LES

17 Large-eddy simulation of surface and canopy layers Based on NCAR code developed by Moeng (1984) Modified to include drag effects on both the resolved-scale flow and SGS motions An experimental tool and framework for investigation of observed phenomena

18 22 Resolved- and subgrid-scales in large-eddy simulation (LES)

19 LES resolved- and subgrid-scales

20 canopy periodic horizontal boundary conditions frictionless lid at upper boundary (no flux) uniform force to drive the flow scalar source through depth of canopy

21 Canopy specification: Represented at each grid point by element area density a (m 2 /m 3 ) Area density horizontally uniform but a(z) Canopy elements rigid Volume occupied by solid elements is considered to be negligible

22 Static pressure perturbation

23 22 Resolved- subgrid- and wake-scales

24 Mean flow KE Resolved- scale TKE Subgrid-scale TKE Internal energy 12 3

25 Mean flow KE Resolved- scale TKE Subgrid-scale TKE Wake- scale TKE Internal energy Viscous drag Form drag 12 3 45 6 7 8 910

26 Drag parameterization: Blasius solution for flow parallel to a flat plate:

27 inertial cascade form drag SGS energy pool 

28 inertial cascade form drag SGS energywake energy ww  sgs

29 Subgrid-scale energy equation where

30 Wake-scale energy equation where

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34 Additional variable e w to represent kinetic energy associated with wake motions Dissipation of e w controlled by dimension of canopy elements

35 Additional variable e w to represent kinetic energy associated with wake motions Dissipation of e w controlled by dimension of canopy elements Rate of conversion of kinetic energy from resolved scales to wake scales is large Effective diffusivity of wake-scale turbulence can be ignored

36 Additional variable e w to represent kinetic energy associated with wake motions Dissipation of e w controlled by dimension of canopy elements Rate of conversion of kinetic energy from resolved scales to wake scales is large Effective diffusivity of wake-scale turbulence can be ignored Important to include the conversion of resolved and SGS energy to wake-scale kinetic energy

37 Additional variable e w to represent kinetic energy associated with wake motions Dissipation of e w controlled by dimension of canopy elements Rate of conversion of kinetic energy from resolved scales to wake scales is large Effective diffusivity of wake-scale turbulence can be ignored Important to include the conversion of resolved and SGS energy to wake-scale kinetic energy Viscous drag and direct dissipation in viscous boundary layers of leaves is of little consequence

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40 Conditional sampling of LES output and composite averaging of flow structures 1.Pressure signal at z/h=1 used as detection function 2.Structures aligned according to peak in pressure signal 3.Composite averages of various elements of the structures Approximately 1,600 events extracted from one 30-minute time series (but not all independent)

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45 270 seconds (17 frames)

46 y/h x/h

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50 The structure of the large-eddy motion as a solution to the eigenvalue problem: Where  ij is the spectral density tensor  i is the eigenvector is the associated eigenvalue

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