Core Concepts
This article presents the numerical verification and validation of several inversion algorithms for recovering symmetric 2-tensor fields in the plane from various combinations of V-line transforms, their corresponding first moments, and the star transform.
Abstract
The paper examines the performance of the proposed inversion algorithms in different settings and illustrates the results with numerical simulations on smooth and non-smooth phantoms.
The key highlights and insights are:
Reconstruction of special tensor fields:
Tensor field f = d^2φ can be recovered from the knowledge of either Lf or Mf, where φ is a function.
Tensor field f = (d⊥)^2φ can be recovered from the knowledge of either Tf or Mf, where φ is a function.
Tensor field f = dd⊥φ can be recovered from the knowledge of either Lf, Tf or Mf, where φ is a function.
Tensor field f = dg can be recovered from the knowledge of Lf and Mf, where g is a vector field.
Tensor field f = d⊥g can be recovered from the knowledge of Lf and Tf, where g is a vector field.
Recovery of a general symmetric 2-tensor field f:
f can be recovered from the combination of Lf, Tf and Mf.
When u1 ≠ u2, f can be recovered from any of the following combinations: (a) Lf, L^1f and Tf, (b) Tf, T^1f and Lf, (c) Mf, M^1f and Lf, (d) Mf, M^1f and Tf.
f can be recovered either from the combination of Lf, L^1f, Mf or Tf, T^1f, Mf.
f can be reconstructed from the star transform Sf.
The numerical simulations demonstrate the effectiveness of the proposed inversion algorithms in accurately recovering the tensor fields, even in the presence of noise.
Stats
The relative errors in the reconstructions are provided in the corresponding figures and tables.