
Imaging Methodologies 221
projections of f (x, y) are finally converted into nonattenuated projections
p(x
r
, φ) by a translation in Fourier space given by the relation
F
1
{p}(ν
x
r
, φ) = F
1
{p
μ
0
}
⎛
⎝
ν
2
x
r
+
μ
0
2φ
2
, φ +i sinh
−1
μ
0
ν
x
r
⎞
⎠
, (6.9)
where F
1
is the one-dimensional Fourier transform with regard to x
r
of the
operand function. With this equation, and executing a Fourier series expan-
sion to compute the complex angles which are the arguments of the Fourier
transform of p
μ
0
(x
r
, φ), we obtain the nonattenuated projections that will be
used in the analytical image reconstruction process.
For the iterative correction methods, the attenuation correction is included
in the iterative image reconstruction process itself. This is currently the most
widely used correction method in clinical practice today [21,22], operating
at the level of constructing the activity projections too. In each iteration, the
attenuation map is employed via Equation 6.6 to calculate the attenuated
projections from the activity distribution estimate proposed in that iteration.
Those attenuated projections are compared with the measured projections,
and the estimated activity distribution is updated according to the result of
that comparison. Image reconstruction, thus, follows the usual course of iter-
ative methods, with the single difference being in the model of formation of
the parallel projections from the activity distribution estimates.
6.2.2.1.4 Correction of Scattered Radiation
Correcting scattered radiation in SPECT involves determining the number of
γ photons detected along each direction in space that has not suffered any
Compton scattering interaction. The products of this type of interaction, as
referred to in Chapter 5 (see Figure 5.6), are one electron and one γ photon
that share the energy of the incident photon. The scattered photon is emitted
along a direction θ relative to the incident photon and carries an energy given
by Equation 5.5.
The energy E
carried by the scattered photon is always smaller than the
energy of the incident photon, and this fact can be used to distinguish photons
that have undergone Compton scattering from those that have not, by simply
measuring the energy of the detected photons. The correction of scattered
radiation must be performed before the attenuation correction, so that the
latter will solely operate on the nonscattered photons, which are the only
ones whose direction bears a causality relation with their emission points.
Executing the energy discrimination of the detected photons is, therefore,
the simplest way of estimating the number S of scattered photons, a value
that can then be subtracted from the total number of detected photons C to
obtain the number of nonscattered photons T in each direction of the parallel
projections:
T = C −S. (6.10)