Limitations to X-ray quality Flashcards

(37 cards)

1
Q

Limitations to X-ray image quality

A

Unsharpness
Scatter
Noise

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2
Q

Types of Unsharpness

A

Geometric
Movement
Detector

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3
Q

Main causes of unsharpness

A
Focal spot size
Focus-object-film distance
Detector design (pixel size) 
Screen-film system
Movement
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4
Q

Effect of focal spot size (1), FFD (2),Focus-Obj Dist (3) and Compression (4)

A

(1) Inc spot size = Inc penumbra
(2) Dec FFD = Inc Mag, Inc unsharpness
(3) Dec FOD = Inc unsharpness
(4) Compression brings structures together, inc sharpness

Mag mammo uses fine focus to decrease penumbra

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5
Q

Calculating Geo unsharp

A

Blur b = yf/x = f(M-1)

Unsharpness = Ug = f(M-1)/M = yf/(x+y)

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6
Q

Reducing Geo unsharpness

A
  • Small focal spot
  • Long source-Im dist
  • Short obj-im dist
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7
Q

Causes of Receptor Unsharpness

A

Digital: Detector design / Mat pixel size

- CR: laser spot size

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8
Q

Calculating receptor unsharp

A

Ur = F/M

F = intrinsic unsharp for zero thickness object on receptor.

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9
Q

Total Unsharpness

A

U = sqrt(Ug^2 + Ur^2)

= 1/M sqrt(f^2(M-1)^2 + F^2)

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10
Q

Movement Unsharpness and minimising it

A

Internal movement: Breathing, heartbeat

Min: Use short as poss exposure time

Reduce mag: Long FFD, short FOD

Use compression in mammo

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11
Q

Define scatter

A

Detected photons with no spatial information

Acts like fog on an image

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12
Q

Contrast with and without scatter

A

Without scatter: C = 1 - e ^ x(μ1 - μ2)

With scatter:

C = 1 - e ^ x(μ1 - μ2) / 1 + R

R = scatter to primary ratio

1/1+R C degradation factor

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13
Q

Grid structure calculations

A

Lines per mm N = 1/(D+d)
Grid ratio r = h/D

d= septa width D = low atten width

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14
Q

Grid impact and designs

A

Inc patient dose

Grid moves to avoid artefacts

Complex design: HTC, complex movement

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15
Q

Grid parameters

A

Primary transmission: ideal 1 real 0.6

Scatter trans fact: ideal 0 real 0.05-0.2

Bucky factor: inc in dose due to grid, kV, patient thickness. Grid ratio is factor 3-8

Contrast imp factor: ratio of contrast deg factor with and without grid

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16
Q

Air gap

A

Gap betw patient exit surface and detector

Photons scatter out of primary area

Cause magnification

1/r effect due to atten of scatter

17
Q

Scatter reduction

A
  • Use collimation
  • Use a low kV
  • Use a grid
  • Use an air gap
  • Use compression
18
Q

Types of noise

A
  • Quantum noise (Recap)
  • Fixed pattern (structure) noise
  • Electronic noise
  • Anatomical noise
19
Q

Impact of Counts on SNR

A

Noise = sqrt N

SNR = N / sqrt N = sqrt N

4 x N -> 2 x SNR

20
Q

Define quantum noise

A

Caused by statistical fluctuations in the number of photons per unit area
absorbed in detector

Dominant source of image noise

21
Q

Define fixed pattern noise

A

Variations in pixel sensitivity, filter thickness, table
top attenuation etc

Equivalent to a signal prop to dose

Reduce by using flat-fielding in DR

22
Q

Define electronic noise

A

• Arises from detector and detector electronics / thermal effects

Assumed to be constant

Significant at lower doses

23
Q

Fluoro noise and its reduction

A

Quantum dominates

Use temporal averaging to reduce effects

All types of noise are present

24
Q

How to combine noise

A

nt = sqrt(n1 ^2 + n2^2 ….

25
Noise component analysis
For a given detector air kerma (AK) • Quantum noise: sq = a(AK)1/2 • Fixed pattern (structure) noise: ss = b(AK) • Electronic noise se = c • Total noise st = √ a2(AK) + b2(AK)2 + c2 st = std lin. pixel value
26
Define Anatomical Noise
Noise due to a normal tissue structure in image task dependent Anatomy masks detail in mammo can reduce with compression and tomo
27
Ways of measuring image quality
* Spatial frequency * Modulation transfer function * Limiting spatial resolution * Signal-to-noise ratio and contrast-to-noise ratio * Noise power spectrum * Receiver Operating Characteristics Tests
28
Measures of resolution
Point, line and edge spread functions show degree of blurring present in imaging system
29
Modulation Transfer function
MTF = Image modulation / Object Modulation
30
Nyquist limit
The reciprocal of 1/(2 x sampling distance)
31
Comparing MTF of DR and CR
MTF for DR is much higher than for standard CR DR MTF also higher at nyquist Higher theoretical limiting spatial resolution for standard CR but not much signal
32
MTF from edge spread function
1) Differentiate to get LSF from ESF | 2) FT ESF to get MTF
33
Limiting spatial resolution & its measurement
Describes the ability of a system to record fine detail. High res = poss to record high detail Measure with bar pattern test - count groups of lines less useful than mtf but easier to measure
34
SNR and CNR limits of SNR
SNR relates signal amp to noise SNR = pv / stdpv pv = lin pixel value ``` CNR the difference in pixel value between the object and background, divided by the standard deviation ``` CNR = M1 - M2 / sqrt(std1^2 + std2^2 / 2) std not necessarily a good measure of im quality
35
Define noise power Spectrum
A plot of the amount of noise at each spatial frequency Grid can appear as a spike at the grid spacing freq
36
Define ROC testing and limits
1) Statistical approach 2) Review of a large no, clinical images 3) Use a panel of observers and compare their opinion to a ground truth. Difficult to coord and costly
37
Producing an ROC curve
Plot TPP and FPP based on a range of decision thresholds. TPP = No. TP / TP + FN