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A geometric based preprocessing for weighted ray transforms with applications in SPECT

  • Fedor Goncharov ORCID logo EMAIL logo

Abstract

In this work we investigate numerically the reconstruction approach proposed in [F. O. Goncharov and R. G. Novikov, An analog of Chang inversion formula for weighted Radon transforms in multidimensions, Eurasian J. Math. Comput. Appl. 4 2016, 2, 23–32] for weighted ray transforms (weighted Radon transforms along oriented straight lines) in 3D. In particular, the approach is based on a geometric reduction of the data modeled by weighted ray transforms to new data modeled by weighted Radon transforms along two-dimensional planes in 3D. Such reduction could be seen as a preprocessing procedure which could be further completed by any preferred reconstruction algorithm. In a series of numerical tests on modelized and real SPECT (single photon emission computed tomography) data we demonstrate that such procedure can significantly reduce the impact of noise on reconstructions.

MSC 2010: 44A12; 35R30; 49N45

A A few remarks on implementations

There were only two crucial steps for our numerical implementations:[1]

  1. Numerical implementation of formulas (2.5) and (2.6) for reduction of PWaf to Rwf. This issue was already commented in Section 2.1. We used quadratic and spline interpolations in variables z,s, respectively, to sample PWaf for missing rays. By doing so we were obtaining the data which did not belong to the image of operator PWa. To our knowledge, efficient interpolation of data even for Pf, where P is the classical ray transform, is still an open question.

  2. Inversion of classical Radon transform R for d=3. The reconstruction methods from Section 3.7 are based on inversion of the classical Radon transform in dimension d=3. There exist many open-access libraries for efficient computations of R-1 for d=2 (for example, in MATLAB/Octave, C/C++ or Python), but for d=3 we did not find any. Because of that we have implemented our own numerical version of R-1 for d=3, based on the well-known Projection Theorem (see [36, Chapter 2, Theorem 1.1]) and using a very nice NUFFT library (i.e., Non-uniform Fast Fourier Transform) for MATLAB/Octave developed in TU Chemnitz [30].

Acknowledgements

The materials for the present work were obtained in the framework of research conducted under the direction of Professor R. G. Novikov. I am also very grateful for the comments and remarks of professor L. Kunyansky during the conference AIP-2019 and also during the author’s thesis defense procedure. Also I would like to express my gratitude to J.-P. Guillement from Université de Nantes for providing codes for SPECT reconstructions in 2D and for related discussions on numerical methods in SPECT.

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Received: 2020-02-11
Accepted: 2020-03-17
Published Online: 2020-04-22
Published in Print: 2021-06-01

© 2020 Walter de Gruyter GmbH, Berlin/Boston

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