- Source: Stokes number
The Stokes number (Stk), named after George Gabriel Stokes, is a dimensionless number characterising the behavior of particles suspended in a fluid flow. The Stokes number is defined as the ratio of the characteristic time of a particle (or droplet) to a characteristic time of the flow or of an obstacle, or
S
t
k
=
t
0
u
0
l
0
{\displaystyle \mathrm {Stk} ={\frac {t_{0}\,u_{0}}{l_{0}}}}
where
t
0
{\displaystyle t_{0}}
is the relaxation time of the particle (the time constant in the exponential decay of the particle velocity due to drag),
u
0
{\displaystyle u_{0}}
is the fluid velocity of the flow well away from the obstacle, and
l
0
{\displaystyle l_{0}}
is the characteristic dimension of the obstacle (typically its diameter) or a characteristic length scale in the flow (like boundary layer thickness). A particle with a low Stokes number follows fluid streamlines (perfect advection), while a particle with a large Stokes number is dominated by its inertia and continues along its initial trajectory.
In the case of Stokes flow, which is when the particle (or droplet) Reynolds number is less than about one, the particle drag coefficient is inversely proportional to the Reynolds number itself. In that case, the characteristic time of the particle can be written as
t
0
=
ρ
p
d
p
2
18
μ
g
{\displaystyle t_{0}={\frac {\rho _{p}d_{p}^{2}}{18\mu _{g}}}}
where
ρ
p
{\displaystyle \rho _{p}}
is the particle density,
d
p
{\displaystyle d_{p}}
is the particle diameter and
μ
g
{\displaystyle \mu _{g}}
is the fluid dynamic viscosity.
In experimental fluid dynamics, the Stokes number is a measure of flow tracer fidelity in particle image velocimetry (PIV) experiments where very small particles are entrained in turbulent flows and optically observed to determine the speed and direction of fluid movement (also known as the velocity field of the fluid). For acceptable tracing accuracy, the particle response time should be faster than the smallest time scale of the flow. Smaller Stokes numbers represent better tracing accuracy; for
S
t
k
≫
1
{\displaystyle \mathrm {Stk} \gg 1}
, particles will detach from a flow especially where the flow decelerates abruptly. For
S
t
k
≪
1
{\displaystyle \mathrm {Stk} \ll 1}
, particles follow fluid streamlines closely. If
S
t
k
<
0.1
{\displaystyle \mathrm {Stk} <0.1}
, tracing accuracy errors are below 1%.
Relaxation time and tracking error in particle image velocimetry (PIV)
The Stokes number provides a means of estimating the quality of PIV data sets, as previously discussed. However, a definition of a characteristic velocity or length scale may not be evident in all applications. Thus, a deeper insight of how a tracking delay arises could be drawn by simply defining the differential equations of a particle in the Stokes regime. A particle moving with the fluid at some velocity
v
p
(
t
)
{\displaystyle v_{p}(t)}
will encounter a variable fluid velocity field as it advects. Let's assume the velocity of the fluid, in the Lagrangian frame of reference of the particle, is
v
f
(
t
)
{\displaystyle v_{f}(t)}
. It is the difference between these velocities that will generate the drag force necessary to correct the particle path:
Δ
v
(
t
)
=
v
f
(
t
)
−
v
p
(
t
)
{\displaystyle \Delta v(t)=v_{f}(t)-v_{p}(t)}
The stokes drag force is then:
F
D
=
3
π
μ
d
p
Δ
v
{\displaystyle F_{D}=3\pi \mu d_{p}\Delta v}
The particle mass is:
m
p
=
ρ
p
4
3
π
(
d
p
2
)
3
=
ρ
p
π
d
p
3
6
{\displaystyle m_{p}=\rho _{p}{\frac {4}{3}}\pi {\bigg (}{\frac {d_{p}}{2}}{\bigg )}^{3}=\rho _{p}{\frac {\pi d_{p}^{3}}{6}}}
Thus, the particle acceleration can be found through Newton's second law:
d
v
p
(
t
)
d
t
=
F
D
m
p
=
18
μ
d
p
2
ρ
p
Δ
v
(
t
)
{\displaystyle {\frac {dv_{p}(t)}{dt}}={\frac {F_{D}}{m_{p}}}={\frac {18\mu }{{d_{p}}^{2}\rho _{p}}}\Delta v(t)}
Note the relaxation time
t
0
=
ρ
p
d
p
2
18
μ
g
{\displaystyle t_{0}={\frac {\rho _{p}d_{p}^{2}}{18\mu _{g}}}}
can be replaced to yield:
d
v
p
(
t
)
d
t
=
1
t
0
Δ
v
(
t
)
{\displaystyle {\frac {dv_{p}(t)}{dt}}={\frac {1}{t_{0}}}\Delta v(t)}
The first-order differential equation above can be solved through the Laplace transform method:
t
0
s
v
p
(
s
)
=
v
f
−
v
p
(
s
)
{\displaystyle t_{0}sv_{p}(s)=v_{f}-v_{p}(s)}
v
p
(
s
)
v
f
(
s
)
=
1
t
0
s
+
1
{\displaystyle {\frac {v_{p}(s)}{v_{f}(s)}}={\frac {1}{t_{0}s+1}}}
The solution above, in the frequency domain, characterizes a first-order system with a characteristic time of
t
0
{\displaystyle t_{0}}
. Thus, the −3 dB gain (cut-off) frequency will be:
f
−
3
dB
=
1
2
π
t
0
{\displaystyle f_{-3{\text{ dB}}}={\frac {1}{2\pi t_{0}}}}
The cut-off frequency and the particle transfer function, plotted on the side panel, allows for the assessment of PIV error in unsteady flow applications and its effect on turbulence spectral quantities and kinetic energy.
Particles through a shock wave
The bias error in particle tracking discussed in the previous section is evident in the frequency domain, but it can be difficult to appreciate in cases where the particle motion is being tracked to perform flow field measurements (like in particle image velocimetry). A simple but insightful solution to the above-mentioned differential equation is possible when the forcing function
v
f
(
t
)
=
V
u
−
Δ
V
H
(
t
)
{\displaystyle v_{f}(t)=V_{u}-\Delta VH(t)}
is a Heaviside step function; representing particles going through a shockwave. In this case,
V
u
{\displaystyle V_{u}}
is the flow velocity upstream of the shock; whereas
Δ
V
{\displaystyle \Delta V}
is the velocity drop across the shock.
The step response for a particle is a simple exponential:
v
p
(
t
)
=
(
V
u
−
Δ
V
)
+
Δ
V
e
−
t
/
t
0
{\displaystyle v_{p}(t)=(V_{u}-\Delta V)+\Delta Ve^{-t/t_{0}}}
To convert the velocity as a function of time to a particle velocity distribution as a function of distance, let's assume a 1-dimensional velocity jump in the
x
{\displaystyle x}
direction. Let's assume
x
=
0
{\displaystyle x=0}
is positioned where the shock wave is, and then integrate the previous equation to get:
x
particle
=
∫
0
Δ
t
v
p
(
t
)
d
t
=
∫
0
Δ
t
(
V
u
−
Δ
V
)
d
t
+
∫
0
Δ
t
Δ
V
e
−
t
/
t
0
d
t
{\displaystyle x_{\text{particle}}=\int _{0}^{\Delta t}v_{p}(t)dt=\int _{0}^{\Delta t}(V_{u}-\Delta V)dt+\int _{0}^{\Delta t}\Delta Ve^{-t/t_{0}}dt}
x
particle
=
Δ
t
(
V
u
−
Δ
V
)
+
Δ
t
Δ
V
(
1
−
e
−
Δ
t
/
t
0
)
{\displaystyle x_{\text{particle}}=\Delta t(V_{u}-\Delta V)+\Delta t\Delta V(1-e^{-\Delta t/t_{0}})}
Considering a relaxation time of
Δ
t
=
3
t
0
{\displaystyle \Delta t=3t_{0}}
(time to 95% velocity change), we have:
x
particle
,
95
%
=
3
t
0
(
V
u
−
Δ
V
)
+
3
t
0
Δ
V
(
1
−
e
−
3
)
{\displaystyle x_{{\text{particle}},95\%}=3t_{0}(V_{u}-\Delta V)+3t_{0}\Delta V(1-e^{-3})}
x
particle
,
95
%
=
3
t
0
(
V
u
−
0.05
Δ
V
)
{\displaystyle x_{{\text{particle}},95\%}=3t_{0}(V_{u}-0.05\Delta V)}
This means the particle velocity would be settled to within 5% of the downstream velocity at
x
particle
,
95
%
{\displaystyle x_{{\text{particle}},95\%}}
from the shock. In practice, this means a shock wave would look, to a PIV system, blurred by approximately this
x
particle
,
95
%
{\displaystyle x_{{\text{particle}},95\%}}
distance.
For example, consider a normal shock wave of Mach number
M
=
2
{\displaystyle M=2}
at a stagnation temperature of 298 K. A propylene glycol particle of
d
p
=
1
μ
m
{\displaystyle d_{p}=1~\mu {\text{m}}}
would blur the flow by
x
particle
,
95
%
=
5
mm
{\displaystyle x_{{\text{particle}},95\%}=5{\text{ mm}}}
; whereas a
d
p
=
10
μ
m
{\displaystyle d_{p}=10~\mu {\text{m}}}
would blur the flow by
x
particle
,
95
%
=
500
mm
{\displaystyle x_{{\text{particle}},95\%}=500{\text{ mm}}}
(which would, in most cases, yield unacceptable PIV results).
Although a shock wave is the worst-case scenario of abrupt deceleration of a flow, it illustrates the effect of particle tracking error in PIV, which results in a blurring of the velocity fields acquired at the length scales of order
x
particle
,
95
%
{\displaystyle x_{{\text{particle}},95\%}}
.
Non-Stokesian drag regime
The preceding analysis will not be accurate in the ultra-Stokesian regime. i.e. if the particle Reynolds number is much greater than unity. Assuming a Mach number much less than unity, a generalized form of the Stokes number was demonstrated by Israel & Rosner.
Stk
e
=
Stk
24
Re
o
∫
0
Re
o
d
Re
′
C
D
(
Re
′
)
Re
′
{\displaystyle {\text{Stk}}_{\text{e}}={\text{Stk}}{\frac {24}{{\text{Re}}_{o}}}\int _{0}^{{\text{Re}}_{o}}{\frac {d{\text{Re}}^{\prime }}{C_{D}({\text{Re}}^{\prime }){\text{Re}}^{\prime }}}}
Where
Re
o
{\displaystyle {\text{Re}}_{o}}
is the "particle free-stream Reynolds number",
Re
o
=
ρ
g
|
u
|
d
p
μ
g
{\displaystyle {\text{Re}}_{o}={\frac {\rho _{g}|\mathbf {u} |d_{p}}{\mu _{g}}}}
An additional function
ψ
(
Re
o
)
{\displaystyle \psi ({\text{Re}}_{o})}
was defined by; this describes the non-Stokesian drag correction factor,
Stk
e
=
Stk
⋅
ψ
(
Re
o
)
{\displaystyle {\text{Stk}}_{e}={\text{Stk}}\cdot \psi ({\text{Re}}_{o})}
It follows that this function is defined by,
ψ
(
Re
o
)
=
24
Re
o
∫
0
Re
o
d
Re
′
C
D
(
Re
′
)
Re
′
{\displaystyle \psi ({\text{Re}}_{o})={\frac {24}{{\text{Re}}_{o}}}\int _{0}^{{\text{Re}}_{o}}{\frac {d{\text{Re}}^{\prime }}{C_{D}({\text{Re}}^{\prime }){\text{Re}}^{\prime }}}}
Considering the limiting particle free-stream Reynolds numbers, as
Re
o
→
0
{\displaystyle {\text{Re}}_{o}\to 0}
then
C
D
(
Re
o
)
→
24
/
Re
o
{\displaystyle C_{D}({\text{Re}}_{o})\to 24/{\text{Re}}_{o}}
and therefore
ψ
→
1
{\displaystyle \psi \to 1}
. Thus as expected there correction factor is unity in the Stokesian drag regime. Wessel & Righi evaluated
ψ
{\displaystyle \psi }
for
C
D
(
Re
)
{\displaystyle C_{D}({\text{Re}})}
from the empirical correlation for drag on a sphere from Schiller & Naumann.
ψ
(
Re
o
)
=
3
(
c
Re
o
1
/
3
−
arctan
(
c
Re
o
1
/
3
)
)
c
3
/
2
Re
o
{\displaystyle \psi ({\text{Re}}_{o})={\frac {3({\sqrt {c}}{\text{Re}}_{o}^{1/3}-\arctan({\sqrt {c}}{\text{Re}}_{o}^{1/3}))}{c^{3/2}{\text{Re}}_{o}}}}
Where the constant
c
=
0.158
{\displaystyle c=0.158}
. The conventional Stokes number will significantly underestimate the drag force for large particle free-stream Reynolds numbers. Thus overestimating the tendency for particles to depart from the fluid flow direction. This will lead to errors in subsequent calculations or experimental comparisons.
Application to anisokinetic sampling of particles
For example, the selective capture of particles by an aligned, thin-walled circular nozzle is given by Belyaev and Levin as:
c
/
c
0
=
1
+
(
u
0
/
u
−
1
)
(
1
−
1
1
+
S
t
k
(
2
+
0.617
u
/
u
0
)
)
{\displaystyle c/c_{0}=1+(u_{0}/u-1)\left(1-{\frac {1}{1+\mathrm {Stk} (2+0.617u/u_{0})}}\right)}
where
c
{\displaystyle c}
is particle concentration,
u
{\displaystyle u}
is speed, and the subscript 0 indicates conditions far upstream of the nozzle. The characteristic distance is the diameter of the nozzle. Here the Stokes number is calculated,
S
t
k
=
u
0
V
s
d
g
{\displaystyle \mathrm {Stk} ={\frac {u_{0}V_{s}}{dg}}}
where
V
s
{\displaystyle V_{s}}
is the particle's settling velocity,
d
{\displaystyle d}
is the sampling tube's inner diameter, and
g
{\displaystyle g}
is the acceleration of gravity.
See also
Stokes' law – For the drag force in fluids on particles whose Reynolds number is less than one
References
Further reading
Fuchs, N. A. (1989). The mechanics of aerosols. New York: Dover Publications. ISBN 978-0-486-66055-4.
Hinds, William C. (1999). Aerosol technology: properties, behavior, and measurement of airborne particles. New York: Wiley. ISBN 978-0-471-19410-1.
Snyder, WH; Lumley, JL (1971). "Some Measurements of Particle Velocity Autocorrelation Functions in a Turbulent Flow". Journal of Fluid Mechanics. 48: 41–71. Bibcode:1971JFM....48...41S. doi:10.1017/S0022112071001460. S2CID 122731370.
Collins, LR; Keswani, A (2004). "Reynolds number scaling of particle clustering in turbulent aerosols". New Journal of Physics. 6 (119): 119. Bibcode:2004NJPh....6..119C. doi:10.1088/1367-2630/6/1/119.
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