Proudman
[536]
, using Lighthill’s
acoustic analogy, derived a formula for acoustic power generated by
isotropic turbulence without mean flow. More recently, Lilley
[375]
re-derived the formula by accounting for the
retarded time difference that was neglected in Proudman’s original
derivation. Both derivations yield acoustic power due to the unit
volume of isotropic turbulence (in
) as
(11–16) |
where
and
are the turbulence velocity and length
scales, respectively, and
is the speed
of sound.
in
Equation 11–16
is
a model constant. In terms of
and
,
Equation 11–16
can
be rewritten as
(11–17) |
where
(11–18) |
The rescaled constant,
, is set to 0.1 in Ansys Fluent based
on the calibration of Sarkar and Hussaini
[567]
in using direct numerical simulation of isotropic
turbulence.
Ansys Fluent can also report the acoustic power in dB, which is computed from
(11–19) |
where
is
the reference acoustic power (
=10
–12
W/m
3
by default).
The Proudman’s formula gives an approximate measure of the local contribution to total acoustic power per unit volume in a given turbulence field. Proper caution, however, should be taken when interpreting the results in view of the assumptions made in the derivation, such as high Reynolds number, small Mach number, isotropy of turbulence, and zero mean motion.
This source model for axisymmetric jets is based on the works of Goldstein [210] who modified the model originally proposed by Ribner [555] to better account for anisotropy of turbulence in axisymmetric turbulent jets.
In Goldstein’s model, the total acoustic power emitted by the unit volume of a turbulent jet is computed from
(11–20) |
where
and
are the radial and angular coordinates
of the receiver location, and
is the
directional acoustic intensity per unit volume of a jet defined by
(11–21) |
in
Equation 11–21
is the modified convection factor defined by
(11–22) |
and
(11–23) |
(11–24) |
The remaining parameters are defined as
(11–25) |
(11–26) |
(11–27) |
(11–28) |
(11–29) |
(11–30) |
where
and
are computed differently depending on the turbulence
model chosen for the computation. When the RSM is selected, they are
computed from the corresponding normal stresses. For all other two-equation
turbulence models, they are obtained from
(11–31) |
(11–32) |
Ansys Fluent reports the acoustic power both in the dimensional units (W/m 3 ) and in dB computed from
(11–33) |
where
is
the reference acoustic power (
=10
–12
W/m
3
by default).
Far-field sound generated by turbulent boundary layer flow over a solid body at low Mach numbers is often of practical interest. The Curle’s integral [128] based on acoustic analogy can be used to approximate the local contribution from the body surface to the total acoustic power. To that end, one can start with the Curle’s integral
(11–34) |
where
denotes the emission time (
), and
the integration surface.
Using this, the sound intensity in the far field can then be approximated by
(11–35) |
where
is
the correlation area,
, and
is the angle between
and the wall-normal direction
.
The total acoustic power emitted from the entire body surface can be computed from
(11–36) |
where
(11–37) |
which can be interpreted as the local contribution per unit surface area of the body surface to the total acoustic power. The mean-square time derivative of the surface pressure and the correlation area are further approximated in terms of turbulent quantities like turbulent kinetic energy, dissipation rate, and wall shear.
Ansys Fluent reports the acoustic surface power defined by Equation 11–37 both in physical (W/m 2 ) and dB units.
The linearized Euler equations (LEE) can be derived from the Navier-Stokes equations starting from decompositions of the flow variables into mean, turbulent, and acoustic components, and by assuming that the acoustic components are much smaller than the mean and turbulent components. The resulting linearized Euler equations for the acoustic velocity components can be written as
(11–38) |
where the subscript "
" refers to the corresponding
acoustic components, and the prime superscript refers to the turbulent
components.
The right side of
Equation 11–38
can be considered as effective source terms responsible for sound
generation. Among them, the first three terms involving turbulence
are the main contributors. The first two terms denoted by
are often referred to as "shear-noise"
source terms, since they involve the mean shear. The third term denoted
by
is often called
the "self-noise" source term, as it involves turbulent
velocity components only.
The turbulent velocity field needed to compute the LEE source
terms is obtained using the method of stochastic noise generation
and radiation (SNGR)
[55]
. In this
method, the turbulent velocity field and its derivatives are computed
from a sum of
Fourier modes.
(11–39) |
where
,
,
are the amplitude, phase, and directional (unit)
vector of the
Fourier mode
associated with the wave-number vector
.
Note that the source terms in the LEE are vector quantities, having two or three components depending on the dimension of the problem at hand.
Lilley’s equation is a third-order wave equation that can be derived by combining the conservation of mass and momentum of compressible fluids. When the viscous terms are omitted, it can be written in the following form:
(11–40) |
where
.
Lilley’s equation can be linearized about the underlying steady flow as
(11–41) |
where
is the turbulent velocity component.
Substituting Equation 11–41 into the source term of Equation 11–40 , we have
(11–42) |
The resulting source terms in Equation 11–42 are evaluated using the mean velocity field and the turbulent (fluctuating) velocity components synthesized by the SNGR method. As with the LEE source terms, the source terms in Equation 11–42 are grouped depending on whether the mean velocity gradients are involved ( shear noise or self noise ), and reported separately in Ansys Fluent.