Turbulence in Fluid Dynamics: A Comprehensive Exploration

Turbulence
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U
 
(
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r
-
S
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)
 
:
Coriolis
acceleration
pressure-gradient
acceleration
gravity
viscous dissipation
 
local momentum source/sink terms
inertial acceleration
Reynolds number Re
Transition from laminar (smooth) to turbulent (chaotic) flow at Re ~10
3
-10
4
In atmosphere, 
U ~ 
10
 
m s
-1
, 
L ~ 
1 km, 
ν
 = 0.15 cm
2
 s
-1   
 → Re ~ 10
9 
fully turbulent
Dealing with subgrid transport
Atmospheric flow is turbulent down to mm scale where viscous dissipation
(molecular diffusion) takes over
Typical observations of surface wind (10 Hz)
Advection in models must cut off the subgrid scales:   
                             
                                                
u
      =       
<
 
u 
>         +             
u’
instantaneous      grid average           fluctuating
                              resolved                unresolved (turbulent) 
                            deterministic            stochastic   
Brasseur and Jacob, chap. 8.2
turbulent eddies
vertical
wind 
w
T
CO
2 
(
n
)
Importance of subgrid scales for mean transport 
Observations from Harvard Forest tower on a typical summer day
(Bill Munger, Harvard)
tower
Time-averaged vertical flux <
F
> = <
nw> = <n
><
w
>  + <
n’w’
>
w 
= <
w
> + 
w’         n 
= <
n
> + 
n’
resolved    turbulent
  (small)       (large)
.
.
.
.
.
.
.
.
n’
w’
Turbulent flux is covariance between fluctuating components
.
Brasseur and Jacob, chap. 10.2.4
Turbulent diffusion parameterization for small-scale eddies
California fire plumes, Oct 2004
Industrial plumes
In 1-D (vertical)
      resolved        turbulent
Generalized continuity equation in 3-D (Eulerian):
K
z
 is a turbulent diffusion coefficient, 
same for all species 
(similarity assumption)
implies Gaussian plumes for point sources
with
Brasseur and Jacob, chap.8.4.1
Lagrangian treatment of small-scale eddies

x,
Δ
y,
 Δ
z)
T
 
p
o
s
i
t
i
o
n
t
o
p
o
s
i
t
i
o
n
t
o
+
t
Treat turbulent component as Markov chain:
 
where the 
Δξ
 random components have expected value of
zero and standard deviation 
Δ
t
Brasseur and Jacob, chap. 4.11.2
Gaussian plume modeling of point source dispersion
Transport in cross-wind direction is parameterized as diffusive process:
Turbulent diffusion coefficients
for steady wind, inert plume
Steady state solution with suitable boundary conditions:
Point source 
with emission rate 
q
Brasseur and Jacob, chap. 4.12.1
Deep convection
Convective cloud
(0.1-100 km)
Model grid scale
Model
vertical
levels
updraft
entrainment
downdraft
detrainment
 Subgrid in horizontal but organized in vertical
 Requires non-local parameterization of mass transport
Large-scale
subsidence
“C-shaped” profile
for species with surface
source
z
C
Brasseur and Jacob, chap. 8.8
Question 1. Somewhat counterintuitively, representation of subgrid turbulent diffusion
is more important in fine-resolution models than in coarse-resolution models. Why?
 
That’s because the turbulent diffusion parameterization (like molecular diffusion) is
most efficient on small spatial scales.
 
Consider a model grid cell:
 
Δ
x
 
Rate constant for ventilation by
advection: 
k
A
 = u/
Δ
x
 
Rate constant for ventilation by
turbulent diffusion: 
k
D
 =2K/(
Δ
x)
2
 
Typical horizontal values 
u 
 = 5 m s
-1
, 
K
 = 10 m
2
 s
-1
Horizontal advection = turbulent diffusion for 
Δ
x 
= 4 km
Typical vertical values 
w
 = 1 cm s
-1
, 
K
 = 10 m
2
 s
-1
Turbulent diffusion dominates on any grid
 
But fine-resolution models can resolve large eddies (like deep convection) that are not
amenable to turbulent diffusion parameterization. So coarse models are more in need of
non-local 
turbulence parameterizations
Question 2. Satellites aim to quantify emissions from point sources by measuring
concentrations in the plumes. Can these plume data be interpreted with a Gaussian
plume model to infer the emissions?
 
No, unless they are very large. Problem is that the observed plumes are instantaneous,
i.e., a single realization of turbulence, whereas the Gaussian plume model assumes
averaging over many realizations. Very large plumes experience these many
realizations but small plumes don’t.
 
Instantaneous methane plumes
seen by GHGSat over Turkmenistan
 
So we have to use different methods
    [Varon et al., AMT 2018]
The same problem arises when predicting the
downwind impacts of an instantaneous event
(such as an explosion)
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Exploring the complexities of turbulence in fluid dynamics, from the Navier-Stokes equations to subgrid transport and turbulent diffusion. Insights into the transition from laminar to turbulent flow, subgrid scale importance, and treatment of small-scale eddies are discussed. The impact of turbulence on atmospheric phenomena and the parameterization of turbulent diffusion for small-scale eddies are also highlighted.

  • Fluid Dynamics
  • Turbulence
  • Navier-Stokes
  • Subgrid Transport
  • Turbulent Diffusion

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  1. Turbulence Chaos in the solution of the continuity equation for momentum U (Navier-Stokes): pressure-gradient acceleration inertial acceleration viscous dissipation U t 1 = U + p + 2 U 2 Coriolis acceleration U g U gravity a local momentum source/sink terms 2 inertial acceleration viscous dissipation U U U / / U U L L UL = = ~ Reynolds number Re 2 2 Transition from laminar (smooth) to turbulent (chaotic) flow at Re ~103-104 In atmosphere, U ~ 10m s-1, L ~ 1 km, = 0.15 cm2 s-1 Re ~ 109 fully turbulent

  2. Dealing with subgrid transport Atmospheric flow is turbulent down to mm scale where viscous dissipation (molecular diffusion) takes over Typical observations of surface wind (10 Hz) turbulent eddies Advection in models must cut off the subgrid scales: u = <u > + u instantaneous grid average fluctuating resolved unresolved (turbulent) deterministic stochastic Brasseur and Jacob, chap. 8.2

  3. Importance of subgrid scales for mean transport Observations from Harvard Forest tower on a typical summer day tower (Bill Munger, Harvard) forest vertical wind w T CO2 (n) w = <w> + w n = <n> + n n Time-averaged vertical flux <F> = <nw> = <n><w> + <n w > ... . resolved turbulent (small) (large) .... w Turbulent flux is covariance between fluctuating components . Brasseur and Jacob, chap. 10.2.4

  4. Turbulent diffusion parameterization for small-scale eddies = resolved turbulent implies Gaussian plumes for point sources C z F nw K n In 1-D (vertical) Kz is a turbulent diffusion coefficient, same for all species (similarity assumption) z z a California fire plumes, Oct 2004 Industrial plumes Generalized continuity equation in 3-D (Eulerian): K 0 0 0 x n t = + + n n C P L U K i = ( ) K K 0 0 with i a i i i y K 0 z Brasseur and Jacob, chap.8.4.1

  5. Lagrangian treatment of small-scale eddies Treat turbulent component as Markov chain: = + 2 x u t K x x = + 2 y v t K y y position to+ t = w t + 2 z K z z where the random components have expected value of zero and standard deviation t ( ( x, y, z)T position to Brasseur and Jacob, chap. 4.11.2

  6. Gaussian plume modeling of point source dispersion Point source with emission rate q Transport in cross-wind direction is parameterized as diffusive process: 2 2 C t C x C y C z = + + u K K for steady wind, inert plume y z 2 2 Turbulent diffusion coefficients Steady state solution with suitable boundary conditions: 2 2 q u y z K = + ( , , ) C x y z exp[ ( )] 4 ( 1/2 ) 4 K K x x K y z y z Brasseur and Jacob, chap. 4.12.1

  7. Deep convection Subgrid in horizontal but organized in vertical Requires non-local parameterization of mass transport Convective cloud (0.1-100 km) z detrainment C-shaped profile for species with surface source Model vertical levels Large-scale subsidence downdraft updraft entrainment C Model grid scale Brasseur and Jacob, chap. 8.8

  8. Question 1. Somewhat counterintuitively, representation of subgrid turbulent diffusion is more important in fine-resolution models than in coarse-resolution models. Why? That s because the turbulent diffusion parameterization (like molecular diffusion) is most efficient on small spatial scales. Consider a model grid cell: Rate constant for ventilation by advection: kA = u/ x Rate constant for ventilation by turbulent diffusion: kD =2K/( x)2 x advection turbulent diffusion k k u x K = = A Typical horizontal values u = 5 m s-1, K = 10 m2 s-1 2 Horizontal advection = turbulent diffusion for x = 4 km Typical vertical values w = 1 cm s-1, K = 10 m2 s-1 Turbulent diffusion dominates on any grid D But fine-resolution models can resolve large eddies (like deep convection) that are not amenable to turbulent diffusion parameterization. So coarse models are more in need of non-local turbulence parameterizations

  9. Question 2. Satellites aim to quantify emissions from point sources by measuring concentrations in the plumes. Can these plume data be interpreted with a Gaussian plume model to infer the emissions? No, unless they are very large. Problem is that the observed plumes are instantaneous, i.e., a single realization of turbulence, whereas the Gaussian plume model assumes averaging over many realizations. Very large plumes experience these many realizations but small plumes don t. So we have to use different methods [Varon et al., AMT 2018] The same problem arises when predicting the downwind impacts of an instantaneous event (such as an explosion) Instantaneous methane plumes seen by GHGSat over Turkmenistan

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