instrumentation final - slides

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494 Terms

1
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What is required during SPECT acceptance testing?

All planar gamma camera tests plus SPECT-specific acceptance tests.

2
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Why must multihead camera calibration factors match closely?

Because differences between heads can create artifacts and non-uniform reconstructions.

3
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What is the maximum allowed difference between calibration factors on multihead cameras?

0.5 percent.

4
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What is the maximum allowed difference between acceptance test results on multihead cameras?

10 percent.

5
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Why is QC more important in SPECT than in planar imaging?

Because any projection error becomes amplified during reconstruction.

6
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What happens when camera rotation is inaccurate in SPECT?

Errors appear in the reconstructed slices and degrade image quality.

7
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What should corrected uniformity be for SPECT?

3 percent or better.

8
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How much variation should be present in a flood source used for SPECT QC?

Less than 1 percent variation in activity.

9
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Why is pixel size accuracy important in SPECT?

Incorrect pixel dimensions distort reconstruction and attenuation correction.

10
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How often must pixel size calibration be performed?

Quarterly.

11
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What does the axis of rotation represent?

The physical line around which the gamma camera rotates.

12
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What does the center of rotation represent?

The center point of the 3D reconstruction matrix.

13
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What indicates correct rotational alignment during COR testing?

Projection midpoints crossing at the same point.

14
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What does the COR analysis program calculate?

The difference between the AOR and COR and the necessary offset.

15
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What source is used for COR testing?

A 1 mCi Tc-99m point source.

16
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Why are 32 stops used in a COR test?

To fully evaluate the camera over a 360-degree rotation.

17
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How many counts per projection are required for COR?

Between 5000 and 20000.

18
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What matrix size is typically used for COR?

128 by 128.

19
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What must be done if the COR X-offset exceeds 0.5 pixel?

Erase the stored correction and generate a new one.

20
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What artifact appears in 360-degree SPECT when COR is incorrect?

A doughnut artifact.

21
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What artifact appears in 180-degree SPECT when COR is incorrect?

A pitchfork artifact.

22
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How does incorrect COR appear in clinical images?

As subtle blurring or distortion due to misplaced activity.

23
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How often should COR be checked?

Weekly until stable, then at regular intervals.

24
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What does the reference scan measure?

Attenuation of gamma rays in air for systems using attenuation correction.

25
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How long does a reference scan require?

Two minutes.

26
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How many counts are needed for a reference scan?

At least 1.8 million counts.

27
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How do you test stability of detector heads?

Acquire images at 0, 90, 180, and 270 degrees using a sheet source.

28
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What should detector head stability images look like when subtracted?

They should contain only noise.

29
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What is collimator hole angulation error?

A collimator hole has a different angle than the rest, causing mispositioning.

30
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How does a 1 percent hole angulation relate to offset error?

It corresponds to approximately 3.5 mm of positioning error.

31
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When should collimator hole angulation be evaluated?

During acceptance testing or when collimator damage is suspected.

32
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What does the Jaszczak phantom test?

Resolution, contrast, and uniformity in SPECT.

33
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What do rods in the Jaszczak phantom measure?

Spatial resolution.

34
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What do spheres in the Jaszczak phantom measure?

Contrast resolution.

35
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Why are SPECT artifacts more severe than planar artifacts?

Reconstruction amplifies small projection errors.

36
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What causes ray artifacts in SPECT?

Filtered backprojection, especially in the presence of hot areas.

37
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What causes ring artifacts in SPECT?

Flood nonuniformity, COR errors, or collimator defects.

38
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How do ring artifacts appear?

As circular alternating bright and dark rings.

39
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What causes motion artifacts in SPECT?

Patient movement between projections.

40
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How do motion artifacts appear?

As blurring or double structures.

41
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What causes truncation artifacts in attenuation-corrected SPECT?

Part of the patient is outside the field of view during transmission imaging.

42
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What does the energy window select?

It selects the range of photon energies around the photopeak that the detector will accept.

43
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Why is a narrow energy window used for calibration?

To precisely locate the exact photopeak.

44
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Why is a wide energy window used for imaging?

To increase counts and improve statistics during patient studies.

45
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What is peak broadening?

The spreading of the energy peak that prevents two close photon energies from being separated.

46
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What does energy resolution measure?

How well a detector can distinguish between gamma rays of different energies.

47
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How is percent energy resolution calculated?

FWHM divided by the photopeak energy times 100.

48
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Why is Cs-137 used to measure energy resolution?

Because it produces a stable 662 keV photopeak.

49
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What does the height of the photopeak represent?

The maximum number of detected events at the true photon energy.

50
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What does FWHM represent?

The width of the peak at half its maximum height.

51
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What does poor energy resolution indicate?

A decline in detector performance that may require servicing.

52
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Why is tracking energy resolution over time important?

It detects gradual degradation in detector function.

53
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How often is energy resolution typically measured?

Quarterly or annually depending on manufacturer guidelines.

54
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What is background in SPECT imaging?

Nonspecific activity seen from all angles that appears more prominent due to multiple projections.

55
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What improves image quality regarding background?

A cleaner target-to-background ratio.

56
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What is structured background in FBP?

Counts from high-uptake areas spread across the matrix during filtered backprojection.

57
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How is structured background reduced?

By using a ramp filter or iterative reconstruction.

58
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Why is noise a larger issue in SPECT?

Because each projection has fewer counts due to short acquisition times.

59
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Why must noise be evaluated per projection?

Because noise varies from angle to angle, not just overall.

60
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How does FBP affect noise?

It amplifies noise and spreads it into nearby voxels.

61
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What happens when projections are noisy?

Artificial hot or cold spots may appear in reconstructed slices.

62
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What part of the frequency spectrum contains noise?

The high-frequency region.

63
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Why must noise filtering be balanced?

Filtering removes noise but also removes fine detail.

64
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How do iterative reconstruction algorithms treat counts?

They treat them as Poisson data and estimate the most likely distribution.

65
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What is the downside of increasing iterations in iterative reconstruction?

It increases noise.

66
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Why does increasing camera-to-patient distance worsen resolution?

Because gamma rays diverge and the collimator blurs more with distance.

67
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How is resolution loss from distance reduced?

Using body-contour orbits or long-bore collimators.

68
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How does attenuation affect SPECT images?

It reduces detected photons, increases noise, and distorts activity distribution.

69
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Why does Compton scatter reduce image quality?

It adds photons to the wrong locations, decreasing contrast.

70
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Why is patient motion critical in SPECT?

Because motion projects the same structure into different locations.

71
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How is motion detected?

By reviewing projection cine loops or sinograms.

72
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What do discontinuities in a sinogram indicate?

Motion between projections.

73
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What is the partial volume effect?

Loss of accurate activity representation due to voxel averaging.

74
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When does PVE cause major problems?

When the object is smaller than twice the system FWHM.

75
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What is spillover in PVE?

Activity from one region contributing to neighboring voxels.

76
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What does spillover do to hot or cold areas?

It enlarges them and decreases contrast.

77
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What determines contrast in SPECT?

The visibility of differences in uptake between normal and abnormal tissue.

78
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Why are cold lesions hard to detect?

They have low contrast in hot backgrounds.

79
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How is uniformity measured in SPECT?

From transaxial slices of a cylindrical phantom.

80
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Why is SPECT uniformity worse than planar?

Reconstruction amplifies small nonuniformities.

81
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What factors determine spatial resolution in SPECT?

Intrinsic resolution, collimator resolution, matrix size, and angular sampling.

82
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How does noise affect resolution?

More noise degrades resolution.

83
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How can iterative reconstruction improve resolution?

By modeling system geometry and resolution recovery.

84
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Why is collimator choice more important in SPECT?

Because SPECT suffers greater loss of sensitivity and resolution than planar imaging.

85
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Why do longer collimator bores improve resolution?

They restrict accepted angles more effectively.

86
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How do fan-beam and cone-beam collimators improve sensitivity?

They magnify small organs and use the detector area efficiently.

87
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What energy window width is commonly used in SPECT?

A 20 percent window centered on the photopeak.

88
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Why might multiple energy peaks be included in SPECT?

To increase total counts when radionuclides emit several usable energies.

89
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What tradeoff occurs when increasing matrix size?

Resolution improves, but counts per pixel decrease, increasing noise.

90
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How does zoom affect pixel size?

It reduces pixel size and improves effective resolution.

91
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What is continuous rotation?

The camera rotates without stopping for each projection.

92
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What is the downside of continuous rotation?

Motion blur within each projection.

93
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What is step-and-shoot acquisition?

The camera stops for each projection before acquiring counts.

94
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Why is step-and-shoot preferred?

There is less motion blur and better image quality.

95
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What is a circular orbit?

An orbit where the radius remains constant.

96
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Why is an elliptical orbit better than circular?

It fits the patient more closely and improves resolution.

97
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What is a body-contour orbit?

An orbit that follows the patient’s outline for the smallest possible radius.

98
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What happens when too few stops are used in SPECT?

Streak artifacts and reconstruction errors occur.

99
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What rule links matrix size to number of stops?

Use as many stops as pixels per row: 64 stops for 64×64, 128 stops for 128×128.

100
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What is the maximum practical imaging time for SPECT?

About 30 to 45 minutes.