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Lecture 14: Emission Tomography III
Shahid Younas
NUCLEAR IMAGING
Emission Tomography III
Single Photon Emission Computed Tomography (SPECT)
Attenuation correction
Lecture 14: Emission Tomography III
X- or gamma rays that must traverse long paths through the patient produce
fewer counts, due to attenuation, than those from activity closer to the near
surface of the patient.
Introduction-Attenuation correction
Lecture 14: Emission Tomography III
 Images acquired with SPECT has,
 Poor spatial resolution
 Apparent decrease in activity
Introduction-Attenuation correction
Lecture 14: Emission Tomography III
 Transverse image slices of a phantom with a
uniform activity distribution will show a
gradual decrease in activity toward the center.
Introduction-Attenuation correction
Lecture 14: Emission Tomography III
 The primary mechanism for attenuation in tissue is Compton
Scattering.
 This changes photon direction with loss of energy.
 The change of direction results in missed count.
Introduction-Attenuation correction
Lecture 14: Emission Tomography III
The effects of attenuation
are more intense at lower
energies but are still
significant at the highest
energy value.
Introduction-Attenuation correction
Lecture 14: Emission Tomography III
Summing two planar
projection images
separated by 180.
Introduction-Attenuation correction
Lecture 14: Emission Tomography III
The magnitude of
attenuation effect depends
on the tissue type.
Attenuation correction
Lecture 14: Emission Tomography III
Thus, to accurately represent the activity distribution measured with SPECT,
it is necessary to accurately correct for the effects of attenuation.
Attenuation correction Techniques
Lecture 14: Emission Tomography III
 Approximate methods are available for attenuation correction.
 Change Method, assumes a constant attenuation coefficient
throughout the patient.
 Over-undercompensate-as attenuation is not uniform
Attenuation correction Techniques
Lecture 14: Emission Tomography III
Constant Attenuation Coefficient
A1 A1 A1
A1 A1 A1
A1 A1 A1
Attenuation correction Techniques
Lecture 14: Emission Tomography III
 Some SPECT cameras have radioactive sources to measure the
attenuation through the patient,
 After acquisition, the transmission projection data are reconstructed
to provide maps of tissue attenuation characteristics across transverse
sections of the patient, similar to x-ray CT images.
Attenuation correction Techniques
Lecture 14: Emission Tomography III
 Some SPECT cameras have radioactive sources to measure the
attenuation through the patient,
 Finally these attenuation maps are used during SPECT image
reconstruction to provide attenuation-corrected SPECT images.
Attenuation correction Techniques
Lecture 14: Emission Tomography III
 Transmission sources are available in several configurations,
 Scanning Collimated Line Sources
 Fixed Line Sources
Attenuation correction Techniques
Lecture 14: Emission Tomography III
 Transmission data usually acquired simultaneously with the
acquisition of the emission projection data,
 Performing the two separately poses significant problems in
the spatial alignment of the two data sets.
Attenuation correction Techniques
Lecture 14: Emission Tomography III
 Radionuclide used for transmission measurements is chosen to have
primary gamma-ray emissions that differ significantly in energy from
those of the radiopharmaceuticals.
 Separate energy windows are used
Attenuation correction Techniques
Lecture 14: Emission Tomography III
 Scattering of the higher energy photons in the patient and in the
detector causes some cross-talk in the lower energy window.
 AC using transmission sources is used Myocardial perfusion
imaging.
 AC using transmission sources is promising but it is still under
development.
SPECT Collimator
Lecture 14: Emission Tomography III
Most commonly used is the high-resolution parallel-hole collimator
 Fan-beam collimators mainly used for brain SPECT
 FOV decreases with distance from collimator
Multihead SPECT Cameras
Lecture 14: Emission Tomography III
 Two or three scintillation camera heads reduce limitations imposed
by collimation and limited time per view.
 Y-offsets and X- and Y-magnification factors of all heads must be
precisely matched throughout rotation.
SPECT Performance
Lecture 14: Emission Tomography III
 Spatial resolution
 X- and Y-magnification factors and multi-energy spatial registration
 Alignment of projection images to axis-of-rotation
 Uniformity
 Camera head tilt
SPECT Spatial resolution
Lecture 14: Emission Tomography III
 Can be measured by acquiring a SPECT study of a line source
(capillary tube filled with a solution of Tc-99m, placed parallel to
axis of rotation).
 FWHM of the line sources are determined from the reconstructed
transverse images (ramp filter).
SPECT Spatial resolution
Lecture 14: Emission Tomography III
 National Electrical
Manufacturers
Association (NEMA)
specifies a cylindrical
plastic water-filled
phantom, 22 cm in
diameter, containing 3
line sources
SPECT Spatial resolution
Lecture 14: Emission Tomography III
 NEMA spatial resolution measurements are primarily determined by
the collimator used.
 Tangential resolution 7 to 8 mm FWHM for LEHR
 central resolution 9.5 to 12 mm
 radial resolution 9.4 to 12 mm
SPECT Spatial resolution
Lecture 14: Emission Tomography III
 NEMA measurements not necessarily representative of clinical
performance
 Studies can be acquired using longer imaging times and closer orbits
than would be possible in a patient.
SPECT Spatial resolution
Lecture 14: Emission Tomography III
 NEMA measurements not necessarily representative of clinical
performance
 Studies can be acquired using longer imaging times and closer orbits
than would be possible in a patient.
SPECT Spatial resolution
Lecture 14: Emission Tomography III
 NEMA measurements not necessarily representative of clinical
performance
 Studies can be acquired using longer imaging times and closer orbits
than would be possible in a patient.
 Filters used for clinical studies have lower spatial frequency cutoffs
than the ramp filters used in NEMA measurements.
Comparison with conventional planar scintillation camera imaging
Lecture 14: Emission Tomography III
 In theory, SPECT should produce spatial resolution similar to that of
planar scintillation camera imaging.
 In clinical imaging, its resolution is usually slightly worse.
 Camera head is closer to patient in conventional planar imaging than
in SPECT.
Comparison with conventional planar scintillation camera imaging
Lecture 14: Emission Tomography III
 Short time per view of SPECT may mandate use of lower resolution
collimator to obtain adequate number of counts.
 In planar imaging, radioactivity in tissues in front of and behind an
organ of interest causes a reduction in contrast.
Comparison with conventional planar scintillation camera imaging
Lecture 14: Emission Tomography III
 Main advantage of SPECT is markedly improved contrast and
reduced structural noise produced by eliminating the activity in
overlapping structures.
 SPECT also offers promise of partial correction for effects of
attenuation and scattering of photons in the patient
Magnification factors
Lecture 14: Emission Tomography III
The X- and Y-magnification factors, often called X and Y gains,
related distances in the object being imaged, in the x and y directions, to
the numbers of pixels between the corresponding points in the resultant
image.
Magnification factors
Lecture 14: Emission Tomography III
 Magnification factors determined from a digital image of two point
sources placed against the camera’s collimator
If X- and Y-magnification factors are unequal, the projection images will
be distorted in shape, as will coronal, sagittal, and oblique images.
COR calibration
Lecture 14: Emission Tomography III
 The axis of rotation (AOR) is an imaginary reference line about
which the head or heads of a SPECT camera rotate.
 If a radioactive line source were placed on the AOR, each projection
image would depict a vertical straight line near the center of the
image.
COR calibration
Lecture 14: Emission Tomography III
 This projection of the AOR into the image is called the center of
rotation (COR).
 Ideally, the COR is aligned with the center, in the x-direction, of each
projection image.
COR calibration
Lecture 14: Emission Tomography III
 Misalignment may be mechanical or electronic.
 Camera head may not be exactly centered in the gantry.
COR calibration
Lecture 14: Emission Tomography III
COR Degradation and Sinogram
COR calibration
Lecture 14: Emission Tomography III
 COR misalignment causes a loss of spatial resolution in the resultant
transverse images.
 Large misalignment cause a point source to appear as “doughnut”.
 Doughnut are not centered in the image so can be distinguished from
“ring” artifacts produced by non-uniformities.
COR calibration
Lecture 14: Emission Tomography III
 COR alignment is assessed by placing a point source or line source in
the camera field of view.
 Projected imaged and or sinogram is analyzed by the camera’s
computer.
COR calibration
Lecture 14: Emission Tomography III
 Misalignment may be corrected by shifting each image in the x-
direction by the proper number of pixels prior to filtered back-
projection
 If COR misalignment varies with camera head angle, it can only be
corrected if computer permits angle-by-angle corrections.
Uniformity
Lecture 14: Emission Tomography III
 Nonuniformities that are not apparent in low-count daily uniformity
studies can cause significant artifacts in SPECT.
 Artifact appears in transverse images as a ring centered about the
AOR.
Uniformity
Lecture 14: Emission Tomography III
Cylinder filled with a uniform
radionuclide solution showing
a ring artifact due to non-
uniformity.
Uniformity
Lecture 14: Emission Tomography III
 Primary intrinsic causes of non-uniformity are,
a. Spatial non-linearities
 stretch the image in some areas
 reducing the local count density
 compress other areas of the images
 Increasing the count density
a. Local variation in the light collection efficiency
Uniformity
Lecture 14: Emission Tomography III
 Lookup table can not correct,
 Local variations in detection efficiency such as dents or
manufacturing defects in the collimators.
Uniformity
Lecture 14: Emission Tomography III
 High-count uniformity images used to determine pixel correction
factors,
 At least 30 million counts for 64 x 64 images
 At least 120 million counts for 128 x 128 images
 Collected every 1 or 2 weeks; separate images for each camera head
Camera head tilt
Lecture 14: Emission Tomography III
 Camera head or heads must be exactly parallel to the AOR.

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Medical Physics Imaging PET CT SPECT CT Lecture

  • 1. Lecture 14: Emission Tomography III Shahid Younas NUCLEAR IMAGING Emission Tomography III Single Photon Emission Computed Tomography (SPECT)
  • 2. Attenuation correction Lecture 14: Emission Tomography III X- or gamma rays that must traverse long paths through the patient produce fewer counts, due to attenuation, than those from activity closer to the near surface of the patient.
  • 3. Introduction-Attenuation correction Lecture 14: Emission Tomography III  Images acquired with SPECT has,  Poor spatial resolution  Apparent decrease in activity
  • 4. Introduction-Attenuation correction Lecture 14: Emission Tomography III  Transverse image slices of a phantom with a uniform activity distribution will show a gradual decrease in activity toward the center.
  • 5. Introduction-Attenuation correction Lecture 14: Emission Tomography III  The primary mechanism for attenuation in tissue is Compton Scattering.  This changes photon direction with loss of energy.  The change of direction results in missed count.
  • 6. Introduction-Attenuation correction Lecture 14: Emission Tomography III The effects of attenuation are more intense at lower energies but are still significant at the highest energy value.
  • 7. Introduction-Attenuation correction Lecture 14: Emission Tomography III Summing two planar projection images separated by 180.
  • 8. Introduction-Attenuation correction Lecture 14: Emission Tomography III The magnitude of attenuation effect depends on the tissue type.
  • 9. Attenuation correction Lecture 14: Emission Tomography III Thus, to accurately represent the activity distribution measured with SPECT, it is necessary to accurately correct for the effects of attenuation.
  • 10. Attenuation correction Techniques Lecture 14: Emission Tomography III  Approximate methods are available for attenuation correction.  Change Method, assumes a constant attenuation coefficient throughout the patient.  Over-undercompensate-as attenuation is not uniform
  • 11. Attenuation correction Techniques Lecture 14: Emission Tomography III Constant Attenuation Coefficient A1 A1 A1 A1 A1 A1 A1 A1 A1
  • 12. Attenuation correction Techniques Lecture 14: Emission Tomography III  Some SPECT cameras have radioactive sources to measure the attenuation through the patient,  After acquisition, the transmission projection data are reconstructed to provide maps of tissue attenuation characteristics across transverse sections of the patient, similar to x-ray CT images.
  • 13. Attenuation correction Techniques Lecture 14: Emission Tomography III  Some SPECT cameras have radioactive sources to measure the attenuation through the patient,  Finally these attenuation maps are used during SPECT image reconstruction to provide attenuation-corrected SPECT images.
  • 14. Attenuation correction Techniques Lecture 14: Emission Tomography III  Transmission sources are available in several configurations,  Scanning Collimated Line Sources  Fixed Line Sources
  • 15. Attenuation correction Techniques Lecture 14: Emission Tomography III  Transmission data usually acquired simultaneously with the acquisition of the emission projection data,  Performing the two separately poses significant problems in the spatial alignment of the two data sets.
  • 16. Attenuation correction Techniques Lecture 14: Emission Tomography III  Radionuclide used for transmission measurements is chosen to have primary gamma-ray emissions that differ significantly in energy from those of the radiopharmaceuticals.  Separate energy windows are used
  • 17. Attenuation correction Techniques Lecture 14: Emission Tomography III  Scattering of the higher energy photons in the patient and in the detector causes some cross-talk in the lower energy window.  AC using transmission sources is used Myocardial perfusion imaging.  AC using transmission sources is promising but it is still under development.
  • 18. SPECT Collimator Lecture 14: Emission Tomography III Most commonly used is the high-resolution parallel-hole collimator  Fan-beam collimators mainly used for brain SPECT  FOV decreases with distance from collimator
  • 19. Multihead SPECT Cameras Lecture 14: Emission Tomography III  Two or three scintillation camera heads reduce limitations imposed by collimation and limited time per view.  Y-offsets and X- and Y-magnification factors of all heads must be precisely matched throughout rotation.
  • 20. SPECT Performance Lecture 14: Emission Tomography III  Spatial resolution  X- and Y-magnification factors and multi-energy spatial registration  Alignment of projection images to axis-of-rotation  Uniformity  Camera head tilt
  • 21. SPECT Spatial resolution Lecture 14: Emission Tomography III  Can be measured by acquiring a SPECT study of a line source (capillary tube filled with a solution of Tc-99m, placed parallel to axis of rotation).  FWHM of the line sources are determined from the reconstructed transverse images (ramp filter).
  • 22. SPECT Spatial resolution Lecture 14: Emission Tomography III  National Electrical Manufacturers Association (NEMA) specifies a cylindrical plastic water-filled phantom, 22 cm in diameter, containing 3 line sources
  • 23. SPECT Spatial resolution Lecture 14: Emission Tomography III  NEMA spatial resolution measurements are primarily determined by the collimator used.  Tangential resolution 7 to 8 mm FWHM for LEHR  central resolution 9.5 to 12 mm  radial resolution 9.4 to 12 mm
  • 24. SPECT Spatial resolution Lecture 14: Emission Tomography III  NEMA measurements not necessarily representative of clinical performance  Studies can be acquired using longer imaging times and closer orbits than would be possible in a patient.
  • 25. SPECT Spatial resolution Lecture 14: Emission Tomography III  NEMA measurements not necessarily representative of clinical performance  Studies can be acquired using longer imaging times and closer orbits than would be possible in a patient.
  • 26. SPECT Spatial resolution Lecture 14: Emission Tomography III  NEMA measurements not necessarily representative of clinical performance  Studies can be acquired using longer imaging times and closer orbits than would be possible in a patient.  Filters used for clinical studies have lower spatial frequency cutoffs than the ramp filters used in NEMA measurements.
  • 27. Comparison with conventional planar scintillation camera imaging Lecture 14: Emission Tomography III  In theory, SPECT should produce spatial resolution similar to that of planar scintillation camera imaging.  In clinical imaging, its resolution is usually slightly worse.  Camera head is closer to patient in conventional planar imaging than in SPECT.
  • 28. Comparison with conventional planar scintillation camera imaging Lecture 14: Emission Tomography III  Short time per view of SPECT may mandate use of lower resolution collimator to obtain adequate number of counts.  In planar imaging, radioactivity in tissues in front of and behind an organ of interest causes a reduction in contrast.
  • 29. Comparison with conventional planar scintillation camera imaging Lecture 14: Emission Tomography III  Main advantage of SPECT is markedly improved contrast and reduced structural noise produced by eliminating the activity in overlapping structures.  SPECT also offers promise of partial correction for effects of attenuation and scattering of photons in the patient
  • 30. Magnification factors Lecture 14: Emission Tomography III The X- and Y-magnification factors, often called X and Y gains, related distances in the object being imaged, in the x and y directions, to the numbers of pixels between the corresponding points in the resultant image.
  • 31. Magnification factors Lecture 14: Emission Tomography III  Magnification factors determined from a digital image of two point sources placed against the camera’s collimator If X- and Y-magnification factors are unequal, the projection images will be distorted in shape, as will coronal, sagittal, and oblique images.
  • 32. COR calibration Lecture 14: Emission Tomography III  The axis of rotation (AOR) is an imaginary reference line about which the head or heads of a SPECT camera rotate.  If a radioactive line source were placed on the AOR, each projection image would depict a vertical straight line near the center of the image.
  • 33. COR calibration Lecture 14: Emission Tomography III  This projection of the AOR into the image is called the center of rotation (COR).  Ideally, the COR is aligned with the center, in the x-direction, of each projection image.
  • 34. COR calibration Lecture 14: Emission Tomography III  Misalignment may be mechanical or electronic.  Camera head may not be exactly centered in the gantry.
  • 35. COR calibration Lecture 14: Emission Tomography III COR Degradation and Sinogram
  • 36. COR calibration Lecture 14: Emission Tomography III  COR misalignment causes a loss of spatial resolution in the resultant transverse images.  Large misalignment cause a point source to appear as “doughnut”.  Doughnut are not centered in the image so can be distinguished from “ring” artifacts produced by non-uniformities.
  • 37. COR calibration Lecture 14: Emission Tomography III  COR alignment is assessed by placing a point source or line source in the camera field of view.  Projected imaged and or sinogram is analyzed by the camera’s computer.
  • 38. COR calibration Lecture 14: Emission Tomography III  Misalignment may be corrected by shifting each image in the x- direction by the proper number of pixels prior to filtered back- projection  If COR misalignment varies with camera head angle, it can only be corrected if computer permits angle-by-angle corrections.
  • 39. Uniformity Lecture 14: Emission Tomography III  Nonuniformities that are not apparent in low-count daily uniformity studies can cause significant artifacts in SPECT.  Artifact appears in transverse images as a ring centered about the AOR.
  • 40. Uniformity Lecture 14: Emission Tomography III Cylinder filled with a uniform radionuclide solution showing a ring artifact due to non- uniformity.
  • 41. Uniformity Lecture 14: Emission Tomography III  Primary intrinsic causes of non-uniformity are, a. Spatial non-linearities  stretch the image in some areas  reducing the local count density  compress other areas of the images  Increasing the count density a. Local variation in the light collection efficiency
  • 42. Uniformity Lecture 14: Emission Tomography III  Lookup table can not correct,  Local variations in detection efficiency such as dents or manufacturing defects in the collimators.
  • 43. Uniformity Lecture 14: Emission Tomography III  High-count uniformity images used to determine pixel correction factors,  At least 30 million counts for 64 x 64 images  At least 120 million counts for 128 x 128 images  Collected every 1 or 2 weeks; separate images for each camera head
  • 44. Camera head tilt Lecture 14: Emission Tomography III  Camera head or heads must be exactly parallel to the AOR.