Volume 81, Issue 1 pp. 247-257
FULL PAPER

Effect of k-space-weighted image contrast and ultrasound focus size on the accuracy of proton resonance frequency thermometry

Bryant T. Svedin

Corresponding Author

Bryant T. Svedin

Utah Center for Advanced Imaging Research, University of Utah, Salt Lake City, Utah

Correspondence Bryant T. Svedin, Utah Center for Advanced Imaging Research, Department of Radiology and Imaging Sciences, 729 Arapeen Drive, Salt Lake City, UT 84108. Email: [email protected]Search for more papers by this author
Christopher R. Dillon

Christopher R. Dillon

Utah Center for Advanced Imaging Research, University of Utah, Salt Lake City, Utah

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Dennis L. Parker

Dennis L. Parker

Utah Center for Advanced Imaging Research, University of Utah, Salt Lake City, Utah

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First published: 29 July 2018
Citations: 8

Funding information: NIH R01 CA172787, R01 EB013433, and S10OD018482; Siemens Medical Solutions

Abstract

Purpose

To construct a predictive model that describes how the duration and symmetry of a k-space-weighted image contrast (KWIC) window affects the temporal resolution of differently sized ultrasound foci when using a pseudo-golden angle stack-of-stars acquisition.

Methods

We performed a modulation analysis of proton resonance frequency temperature measurements to create the temporal modulation transfer function for KWIC windows of different symmetry and temporal duration. We reconstructed simulated ultrasound heating trajectories and stack-of-stars k-space data as well as experimental phantom data using the same trajectories. Images were reconstructed using symmetric and asymmetric KWIC windows of 3 different temporal durations. Simulated results were compared against temporal modulation transfer function predictions, experimental results, and the original simulated temperatures.

Results

The temporal modulation transfer function shows that temporal resolution with KWIC reconstructions depend on the object size. The KWIC window duration affected SNR and severity of undersampling artifacts. Accuracy and response delay improved as the KWIC window duration decreased or the size of the heated region within the KWIC plane increased. Precision worsened as the window duration decreased. Using a symmetric window eliminated the response delay to heated region size but introduced a large reconstruction delay.

Conclusion

The accuracy and precision of proton resonance frequency temperature measurements from a stack-of-stars acquisition using a sliding KWIC window reconstruction are dependent on the size of the KWIC window and the size and shape of the heated region. The temporal modulation transfer function of KWIC reconstructions for any object size can predict the temporal response to changes in signal being acquired, such as temperature and contrast enhancement.

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