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Observation and simulation of flow in vegetation canopies

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Kinetic energy spectral densities that are strongly peaked ... Galileo Galilei. Time traces of velocity components. Z=2.4h. Z=0.9h ... – PowerPoint PPT presentation

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Title: Observation and simulation of flow in vegetation canopies


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Observation and simulation of flow in vegetation
canopies Roger H. Shaw University of California,
Davis
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Canopy turbulence
  • Kinetic energy spectral densities that are
    strongly peaked
  • Strong correlations between streamwise and
    vertical velocities
  • Large velocity skewness (Skugt0 Skwlt0)
  • Transport dominated by organized structures
  • Larger contributions from sweep motions than
    ejections

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We will understand the movement of the stars
long before we understand canopy
turbulence Galileo Galilei
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Time traces of velocity components
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Z2.4h
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Z0.9h
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Scalar ramps correlated through the depth of
the canopy show wholesale flushing of the
canopy airspace by large scale gusts.
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Scalar
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Vertical velocity
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Streamwise velocity
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Turbulent kinetic energy budget determined from
LES
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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

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Resolved- and subgrid-scales in large-eddy
simulation (LES)
2?
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LES resolved- and subgrid-scales
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  • periodic horizontal boundary conditions
  • frictionless lid at upper boundary (no flux)
  • uniform force to drive the flow
  • scalar source through depth of canopy

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  • Canopy specification
  • Represented at each grid point by element
  • area density a (m2/m3)
  • Area density horizontally uniform but a(z)
  • Canopy elements rigid
  • Volume occupied by solid elements is
  • considered to be negligible

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Static pressure perturbation
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Resolved- subgrid- and wake-scales
2?
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Internal energy
Mean flow KE
Resolved-scale TKE
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Subgrid-scale TKE
1
2
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Viscous drag
Internal energy
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9
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Mean flow KE
Resolved-scale TKE
3
Subgrid-scale TKE
1
2
Wake-scale TKE
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Form drag
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Drag parameterization
Blasius solution for flow parallel to a flat
plate
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inertial cascade
form drag
?
SGS energy pool
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inertial cascade
form drag
?sgs
?w
SGS energy
wake energy
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Subgrid-scale energy equation
where
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Wake-scale energy equation
where
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  • Additional variable ew to represent kinetic
    energy
  • associated with wake motions
  • Dissipation of ew controlled by dimension of
  • canopy elements

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  • Additional variable ew to represent kinetic
    energy
  • associated with wake motions
  • Dissipation of ew 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

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  • Additional variable ew to represent kinetic
    energy
  • associated with wake motions
  • Dissipation of ew 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

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  • Additional variable ew to represent kinetic
    energy
  • associated with wake motions
  • Dissipation of ew 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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Conditional sampling of LES output and composite
averaging of flow structures
  1. Pressure signal at z/h1 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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270 seconds (17 frames)
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The structure of the large-eddy motion as a
solution to the eigenvalue problem
Where Fij is the spectral density tensor fi is
the eigenvector l is the associated eigenvalue
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