Before the analysis is done in EPIQA, measured images may be processed by applying a Gaussian convolution. This "blurs" the EPID images. The degree of blurring is controlled with a Sigma parameter (given in [mm]).
Gaussian convolution is not possible in Varian Portal Dosimetry.
In the following example, the impact of Gaussian convolution shall be demonstrated. An IMRT plan with 6 Gantry angles, 12 fields, beam energy 15MV, was evaluated with EPIQA in the MIX setup (no additional buildup). Eclipse algorithm was AAA 8.6.14 (with our 0.125 cm3 chamber beam data). According to MIX setup, depth of dose matrices in Eclipse was 3 cm.
The Gamma Agreement Index (GAI) in percent gives the fraction of pixels within the evaluation area that pass the Gamma criterion (i.e., where Gamma < 1). Ideally, it is 100%.
The following table shows the GAI for multiple evaluations of the same plan using different degrees of blurring. For the Gaussian convolution, the Sigma setting was varied between zero (no Gaussian convolution) and 4 mm. Each link goes to a screenshot of the respective EPIQA screen:
Field | No Convolution | Sigma = 2 mm | Sigma = 3 mm | Sigma = 3.5 mm | Sigma = 4 mm |
---|---|---|---|---|---|
140 IMRTani _1 | 92.10% | 96.28% | 97.73% | 98.45% | 99.25% |
140 IMRTani _2 | 89.67% | 95.46% | 97.40% | 98.10% | 98.48% |
25 IMRTani _1 | 73.59% | 91.07% | 97.79% | 99.21% | 98.59% |
25 IMRTani _2 | 96.79% | 98.60% | 99.33% | 99.58% | 99.69% |
270 IMRTani _1 | 91.66% | 97.66% | 99.36% | 99.48% | 99.45% |
270 IMRTani _2 | 87.15% | 92.80% | 95.76% | 96.46% | 96.91% |
90 IMRTani _1 | 92.49% | 96.75% | 97.70% | 98.38% | 99.32% |
90 IMRTani _2 | 91.32% | 96.48% | 98.83% | 99.01% | 99.01% |
220 IMRTani _1 | 91.60% | 98.32% | 99.47% | 99.99% | 99.96% |
220 IMRTani _2 | 93.71% | 97.37% | 98.61% | 99.10% | 99.38% |
335 IMRTani _1 | 96.03% | 98.35% | 99.10% | 99.58% | 99.59% |
335 IMRTani _2 | 69.43% | 88.46% | 95.29% | 96.59% | 96.76% |
The effect of Gaussian convolution on the GAI is clearer when plotted:
GAI improves with increasing Sigma (=more blurring). Around Sigma = 4 mm, GAI starts to decrease again, because EPID images are blurred more than the Eclipse "images". However, the Sigma value for which the GAI is at maximum is not the same for all fields.
At first glance, Gaussian convolution is a nice tool to improve your results!
Although Gaussian convolution should not be used unreflectedly (in other words: simply to improve the evaluation results), a point can be made that some blurring may be justified, especially for higher photon energies: