The echo
r(
t) from a collection of scatterers in two dimensions can be modeled as
where
h(
x, z, t) is the pulse-echo response to a point scatterer at (
x, z), and
γ(
x, z) is the object function, which describes the scattering properties as a function of position [
12]. Here the scatterers are taken to be in the
xz plane; ultrasound propagation is in the +
z direction. Although
h(
x, z, t) is spatially varying in general, in the far field of an unfocused transducer, local spatial invariance can be assumed, and the impulse response modeled as
where
he is the pulse envelope,
ωl the ultrasound radian frequency, and
cl the acoustic wave speed. This model implies that displacement of a point target in the ±
z direction induces a proportional change in echo arrival time but does not otherwise change the echo. The envelope signal
he(
x, t) is taken to be centered around
t = 0, i.e., pulse emission occurs at
t = 0. The envelope
he is assumed to vary slowly relative to the ultrasound frequency.
With this assumption, the effect of a small displacement in the
z direction, Δ
z, can be modeled as a phase shift of the echo signal. A point target at location (
x, z + Δ
z) yields echo
If the displacement Δ
z is small, such that the extra delay 2Δ
z/c induces a negligible change in the envelope signal, then the effect of the displacement is just a phase shift of the echo of the undisturbed target,
An elastic medium supports shear wave propagation, in addition to the longitudinal ultrasound waves. Such a shear wave in the target object displaces scattering centers. A
z-polarized plane shear wave of frequency
ωs propagating in the +
x direction induces a displacement of the scatterers in the ±
z direction of
where
a is the displacement amplitude, and
ks the wave-number of the shear wave. The phase of the shear wave source with respect to the ultrasound pulse emission is denoted by
ϕ. The passage of the shear wave moves a point at
z to position
z + Δ
z. As described in [
13], when
ωsa/c
l ![[double less-than sign]](/corehtml/pmc/pmcents/x226A.gif)
1, and the pulse duration is short compared with the shear wave frequency, the value of
t at the time of pulse-scatterer interaction is well approximated by
z/c
l, where
z is the undisturbed scatterer range. In the present case,
ωsa/cl is on the order of 10
−4. Using the approximation of (
4), (
1) can be written to include the effect of the shear wave as
where
β = 2
akl and
![[gamma with circumflex]](/corehtml/pmc/pmcents/x03B3x0302.gif)
(
x, t) represents the object function convolved in the
z direction with the impulse response, and shaded in the
x direction by
h. That is,
![[gamma with circumflex]](/corehtml/pmc/pmcents/x03B3x0302.gif)
is the object function blurred in the range direction and illuminated but unblurred in the lateral direction.
r(
t, ks,
ϕ) represents the complete echo as a function of time, modulated by the shear wave displacement of the scatterers. In the absence of any shear-wave-induced motion, (
1) and (
7) are equivalent.
Eq. (7) is a phase-modulated version of (
1). For small values of
β, i.e., |
β|
π, we can make the approximation
e−jβ cos(ωsz/cl−ksx−ϕ) ≈ 1 −
jβ cos (
ωs z/
cl −
ksx −
ϕ). Using this approximation and the identity cos(
x −
π/2) = sin(
x) we can write
and
Define
I and
Q as
and
Note that neither
I nor
Q is necessarily real. Then
that is, the sum
I(
ks) +
jQ(
ks) is the Fourier transform of
![[gamma with circumflex]](/corehtml/pmc/pmcents/x03B3x0302.gif)
(
x, t) scaled by 2
jβejcrzks, where
cr is the ratio of shear wave speed to longitudinal wave speed and
crzks =
ωsz/
cl. The term
ejcrzks represents the phase shift of the shear wave caused by the propagation delay of the ultrasound pulse from the transducer to depth
z. The inverse Fourier transform may be applied, then, to recover
![[gamma with circumflex]](/corehtml/pmc/pmcents/x03B3x0302.gif)
(
x) from the signals
I(
t, ks) and
Q(
t, ks),
Recovery of
![[gamma with circumflex]](/corehtml/pmc/pmcents/x03B3x0302.gif)
, then, yields an image of the object
γ blurred by the axial (time) component of the impulse response, and shaded laterally by the extent of
he. For typical imaging depths and wave speed ratios, the term
e−jcrz|ks| is negligible.
This development assumed that the vibration amplitude
a, and therefore
β, is independent of shear wave frequency and position. It is straightforward to show that variation in
β with shear wave frequency introduces a lateral blurring, whereas variation with
x introduces a lateral shading. Treating
β as a separable function of space and shear wavenumber,
β =
βx(
x)
βks(
ks), we can write (
13) to include both effects as
where *
x indicates convolution with respect to
x and
B(
x) is the inverse Fourier transform of
βks,
Here we have used the Fourier transform property that multiplication in one domain is equivalent to convolution in the other. Thus, the convolution on the left-hand side of (
14) clears the
βks term on the right-hand side. The
βx term, being independent of
ks is simply cleared by multiplication. Taking the right-hand side of (
14) as the reconstructed image, it is clear that
βx shades the image as a function of lateral position, whereas the convolution with
B(
x) introduces a lateral blurring.
Several effects may be anticipated from (
14). As the shear wave propagates from its source, any attenuation with distance will lead to decreased image brightness. A laterally varying gain, similar to time-gain compensation in B-mode imaging, could be applied to eliminate this shading. If
βk is a rectangular window function, such that
βks(
ks) =
β0 for |
ks| less than some maximum value and zero otherwise, the effect is to convolve the ideal image with a scaled sinc, similar to the effect of a unapodized phased array. The strong lateral side lobes which result are undesirable for image contrast. A smoother
βks function may be used to reduce ringing. Because the effect of
βks on
I and
Q is multiplicative, actual scaling of vibration amplitude with wavenumber or scaling of
I and
Q after echo collection are equivalent.
Because
B(
x) represents the lateral blurring function, it is straightforward to predict lateral resolution by calculating the Fourier transform in (
15) and applying a suitable resolution metric. For instance, we may consider the full-width at half-maximum (FWHM) size of
B(
x) as representative of point target resolution. In the case of a uniform weighting of shear wave frequency data up to a maximum spatial frequency
kmax,
B(
x) = sin(
kmaxx)/
πx.
B(
x) has a maximum at
x = 0 of
k/
π. Solving
B(
x)/
B(0) = 1/2 for
x yields the FWHM value. Computing this expression numerically yields
Again, this resolution result is independent of the ultrasound wavelength and aperture size. For comparison, the FWHM beamwidth of a rectangular aperture of width
ω focused at depth
z is 1.21
λz/
ω.
Sampling of
I(
ks) +
jQ(
ks) at discrete values of
ks allows image reconstruction over a limited field of view. In this case,
ks must be sampled densely enough to avoid aliasing (wrap-around) artifacts in the reconstructed image. Given a wavenumber step size of Δ
k, the inverse discrete-time Fourier transform of
R(
kn),
is periodic with a period of 2
π/Δ
k. To avoid wrap-around aliasing of the image, Δ
k must be small enough to ensure that the entire illuminated extent of the object is less than
π / Δ
k. If the illuminated object is of lateral extent
L, then the Nyquist sampling requirement is satisfied if Δ
k ≤ 2
π /
L. This inequality may be expressed in terms of the vibration frequency
ω through the identity
k =
ω /
c as
In those cases where the term e−jcrz|ks| is negligible, the need to collect echoes for both positive and negative values of ks is eliminated. This is so because, when e−jcrz|ks| is one, I(ks) = I(−ks) and Q(ks) = −Q(−ks). In this case, the echo data generated from backward-going shear waves is redundant, and reconstruction from only forward-going waves is possible.