Efficient implementation for spherical flux computation and its application to vascular segmentation.

IEEE Trans Image Process

Lo Kwee-Seong Medical Image Analysis Laboratory, Department of Computer Science and Engineering, The Hong Kong University of Science and Technology, Clear Water Bay, Hong Kong.

Published: March 2009

AI Article Synopsis

  • Spherical flux is crucial for analyzing tubular structures in medical imaging, but traditional calculation methods become slow for larger spheres.
  • The authors propose a new method to compute spherical flux in the Fourier domain, improving efficiency by reformulating calculations with the divergence theorem and convolution operations.
  • Experimental results show that this new approach is more computationally efficient while maintaining accuracy, especially advantageous for multiscale analyses that don’t depend on sphere size.

Article Abstract

Spherical flux is the flux inside a spherical region, and it is very useful in the analysis of tubular structures in magnetic resonance angiography and computed tomographic angiography. The conventional approach is to estimate the spherical flux in the spatial domain. Its running time depends on the sphere radius quadratically, which leads to very slow spherical flux computation when the sphere size is large. This paper proposes a more efficient implementation for spherical flux computation in the Fourier domain. Our implementation is based on the reformulation of the spherical flux calculation using the divergence theorem, spherical step function, and the convolution operation. With this reformulation, most of the calculations are performed in the Fourier domain. We show how to select the frequency subband so that the computation accuracy can be maintained. It is experimentally demonstrated that, using the synthetic and clinical phase contrast magnetic resonance angiographic volumes, our implementation is more computationally efficient than the conventional spatial implementation. The accuracies of our implementation and that of the conventional spatial implementation are comparable. Finally, the proposed implementation can definitely benefit the computation of the multiscale spherical flux with a set of radii because, unlike the conventional spatial implementation, the time complexity of the proposed implementation does not depend on the sphere radius.

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http://dx.doi.org/10.1109/TIP.2008.2010073DOI Listing

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