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Full correction for spatially distributed speed-of-sound in echo ultrasound based on measuring aberration delays via transmit beam steering

机译:基于通过发射束转向测量像差延迟的回声超声中空间分布声速的完全校正

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摘要

Aberrations of the acoustic wave front, caused by spatial variations of the speed-of-sound, are a main limiting factor to the diagnostic power of medical ultrasound imaging. If not accounted for, aberrations result in low resolution and increased side lobe level, over all reducing contrast in deep tissue imaging. Various techniques have been proposed for quantifying aberrations by analysing the arrival time of coherent echoes from so-called guide stars or beacons. In situations where a guide star is missing, aperture-based techniques may give ambiguous results. Moreover, they are conceptually focused on aberrators that can be approximated as a phase screen in front of the probe. We propose a novel technique, where the effect of aberration is detected in the reconstructed image as opposed to the aperture data. The varying local echo phase when changing the transmit beam steering angle directly reflects the varying arrival time of the transmit wave front. This allows sensing the angle-dependent aberration delay in a spatially resolved way, and thus aberration correction for a spatially distributed volume aberrator. In phantoms containing a cylindrical aberrator, we achieved location-independent diffraction-limited resolution as well as accurate display of echo location based on reconstructing the speed-of-sound spatially resolved. First successful volunteer results confirm the clinical potential of the proposed technique.
机译:由声速的空间变化引起的声波阵面像差是限制医学超声成像诊断能力的主要因素。如果不加以考虑,像差会导致分辨率降低和旁瓣水平升高,总体上会降低深部组织成像的对比度。已经提出了各种技术,用于通过分析来自所谓的引导星或信标的相干回波的到达时间来量化像差。在缺少引导星的情况下,基于光圈的技术可能会产生含糊的结果。而且,它们在概念上集中在可以作为探头前面的相位屏近似的像差器上。我们提出了一种新颖的技术,其中在与孔径数据相反的重建图像中检测像差的影响。当改变发射束转向角时,改变的局部回波相位直接反映了发射波前的变化到达时间。这允许以空间分辨的方式感测与角度有关的像差延迟,并因此对空间分布的体积像差器进行像差校正。在包含圆柱形像差的幻像中,我们通过重建空间分辨的声速,获得了与位置无关的衍射极限分辨率以及对回波位置的精确显示。首次成功的志愿者结果证实了该技术的临床潜力。

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