Abstract

The prerequisites, mechanisms and principles of motion artifacts in AMBER radiographs were analysed. The experiments were performed using metronomes, a moving conventional mammography phantom, and arrangements of oscillating coil spring, spheroid and grid elements. A diagnostic dosimeter and TLDs, respectively, were used to measure exposure times and doses. The degree of distortion in AMBER radiographs depends on the direction of the object movement relative to the AMBER fan beam in a complex manner. The size of the motion artifacts depends on the local exposure time. The maximum value of this time is 75 ms and thus 1.5 times higher than specified by the manufacturer. To interpret AMBER radiographs possible system specific artifacts have to be considered to avoid misinterpretations of potentially significant details.

Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call