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Efficient and accurate computation of spherical mean values at scattered center points. (English) Zbl 1263.65138

From a mathematical point of view (it means without any connection to a practical use described in the summary), the authors consider spherical means defined by \[ f:\mathbb R^d \rightarrow \mathbb R,\quad Mf(y,r)=\frac 1 {\omega_{d-1}} \int_{S^{d-1}}f(y+r\xi)d\sigma(\xi) \] (centerpoint \(y\in \mathbb R^d\), radius \(r>0\), \(\sigma\) denotes the surface measure on the sphere and \(\omega_{d-1}=\sigma(S^{d-1})\)) and use iterative methods for their computation. A spectral discretization via trigonometric polynomials in such a way that computations can be done via a nonequispaced fast Fourier transform (FFT), however, the sparse FFT is used in the three-dimensional case. The studied theory is illustrated numerically.

MSC:

65T40 Numerical methods for trigonometric approximation and interpolation
65R10 Numerical methods for integral transforms
65T50 Numerical methods for discrete and fast Fourier transforms
44A12 Radon transform
92C55 Biomedical imaging and signal processing
42A10 Trigonometric approximation