A practical method for measuring planar spatial resolution with scatter on a CZT gamma camera.

IF 3 2区 医学 Q2 RADIOLOGY, NUCLEAR MEDICINE & MEDICAL IMAGING EJNMMI Physics Pub Date : 2024-07-01 DOI:10.1186/s40658-024-00656-w
Corinne Barrau, Perrine Tylski
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Abstract

Purpose: This study proposes a practical method for evaluating 2D spatial resolution with scatter on a CZT planar detector gamma camera, which is simpler and faster than the NEMA method. It is used to characterize the influence of distance on spatial resolution FWHM on a CZT camera equipped with a WEHR collimator.

Methods: The practical method uses linear sources tilted with respect to the detector axes. The spatial resolution full width at half maximum (FWHM) with four tilt angles was compared to the FWHM evaluated using the NEMA NU1-2018 method. Spatial resolution FWHM was also assessed with tilted sources acquired at distances of 0 to 20 cm using a single angle, with and without the post-processing image enhancement proposed by the manufacturer.

Results: Estimated spatial resolution FWHM with tilted sources was close to the spatial resolution FWHM estimated at 7.63 mm by the NEMA method, with deviations ranging from - 5.62 to 4.59% at 10 cm depending on the angle considered. The study of spatial resolution FWHM dependence on distance indicates that, for distances less than 3 cm, the FWHM no longer decreases with distance. The manufacturer's post-processing reduces the FWHM by an average of 15%.

Conclusion: The practical method is quicker to implement and gives comparable results to the NEMA reference method for spatial resolution FWHM. Evaluation of spatial resolution with linear sources at short distances from the collimator is limited by the collimator effect and signal digitization. The tilted source method can be used to measure spatial resolution quickly and easily under clinical conditions for CZT planar cameras.

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利用 CZT 伽玛相机的散射测量平面空间分辨率的实用方法。
目的:本研究提出了一种评估 CZT 平面探测器伽马相机散射二维空间分辨率的实用方法,它比 NEMA 方法更简单、更快捷。这种方法比 NEMA 方法更简单、更快捷,可用于描述配备 WEHR 准直器的 CZT 伽玛相机上距离对空间分辨率 FWHM 的影响:该实用方法使用相对于探测器轴线倾斜的线性光源。将四个倾斜角度的空间分辨率半最大全宽(FWHM)与使用 NEMA NU1-2018 方法评估的 FWHM 进行了比较。此外,还评估了使用单个角度在 0 至 20 厘米距离处获取的倾斜光源的空间分辨率半最大值,以及是否使用了制造商建议的后处理图像增强技术:使用倾斜光源估计的空间分辨率 FWHM 接近 NEMA 方法估计的空间分辨率 FWHM(7.63 毫米),根据考虑的角度不同,10 厘米处的偏差在-5.62% 到 4.59% 之间。对空间分辨率 FWHM 与距离关系的研究表明,当距离小于 3 厘米时,FWHM 不再随距离的增加而减小。制造商的后处理可将 FWHM 平均降低 15%:结论:实用方法实施起来更快,其结果与 NEMA 空间分辨率 FWHM 参考方法相当。在距离准直器很近的地方使用线性光源评估空间分辨率,会受到准直器效应和信号数字化的限制。倾斜光源法可用于在临床条件下快速、轻松地测量 CZT 平面相机的空间分辨率。
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来源期刊
EJNMMI Physics
EJNMMI Physics Physics and Astronomy-Radiation
CiteScore
6.70
自引率
10.00%
发文量
78
审稿时长
13 weeks
期刊介绍: EJNMMI Physics is an international platform for scientists, users and adopters of nuclear medicine with a particular interest in physics matters. As a companion journal to the European Journal of Nuclear Medicine and Molecular Imaging, this journal has a multi-disciplinary approach and welcomes original materials and studies with a focus on applied physics and mathematics as well as imaging systems engineering and prototyping in nuclear medicine. This includes physics-driven approaches or algorithms supported by physics that foster early clinical adoption of nuclear medicine imaging and therapy.
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