Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group

3D optical tomography in the presence of void regions

Open Access Open Access

Abstract

We present an investigation of the effect of a 3D non-scattering gap region on image reconstruction in diffuse optical tomography. The void gap is modelled by the Radiosity-Diffusion method and the inverse problem is solved using the adjoint field method. The case of a sphere with concentric spherical gap is used as an example.

©2000 Optical Society of America

Full Article  |  PDF Article
More Like This
Optical tomography in the presence of void regions

Hamid Dehghani, Simon R. Arridge, Martin Schweiger, and David T. Delpy
J. Opt. Soc. Am. A 17(9) 1659-1670 (2000)

Linear single-step image reconstruction in the presence of nonscattering regions

H. Dehghani and D. T. Delpy
J. Opt. Soc. Am. A 19(6) 1162-1171 (2002)

Influence investigation of a void region on modeling light propagation in a heterogeneous medium

Defu Yang, Xueli Chen, Shenghan Ren, Xiaochao Qu, Jie Tian, and Jimin Liang
Appl. Opt. 52(3) 400-408 (2013)

Supplementary Material (2)

Media 1: MOV (3751 KB)     
Media 2: MOV (3760 KB)     

Cited By

Optica participates in Crossref's Cited-By Linking service. Citing articles from Optica Publishing Group journals and other participating publishers are listed here.

Alert me when this article is cited.


Figures (4)

Fig. 1.
Fig. 1. Left : cutaway of spherical mesh. Right : location of sources and detectors on the sphere surface
Fig. 2.
Fig. 2. distribution of photon density, photons/mm3 (top row) and mean time of photon flight, picoseconds (bottom row) over sphere surface. Left to right, solid sphere (no gap), gap widths 3mm, 4mm, 5mm.
Fig. 3.
Fig. 3. Sensitivity functions for the 3mm gap case. Left intensity (photons/mm2), right mean time(picoseconds mm). The functions plotted are cross-sections through the equatorial plane of the sphere. Also available as a QuickTime movie, pmdf.mov. (3.8MB)
Fig. 4.
Fig. 4. Target images (top row) and reconstructions (bottom row) for the 3mm gap case. The images are transverse, sagittal and coronal slices through the true centre of the blob, orientated according to the diagram in the top right panel. Bottom right shows a profile along the equatorial diameter through the blob centre. A movie showing a rotating orthographic view is attached rotating3d.mov (3.8MB).

Equations (14)

Equations on this page are rendered with MathJax. Learn more.

· κ ( r ) Φ ( r ; ω ) + ( µ a ( r ) + i ω c ) Φ ( r ; ω ) = 0 r Ω d ( Ξ d Ω d )
Φ ( m ; ω ) + 2 A κ ( m ) Φ ( m ; ω ) ν = η ( m ; ω ) m Ω 1 +
Φ ( m ; ω ) + 2 A κ Φ ( m ; ω ) ν = 1 π Ξ cos θ cos θ Φ ( m ; ω ) 2 A h ( m , m ) ×
exp [ ( μ a + i ω c ) m m ] m m 2 d m m , m Ξ
cos θ = ν ̂ ( m ) · m m m m , cos θ = ν ̂ ( m ) · m m m m
y η ( m ; ω ) = 𝓟 η ( μ a κ ) κ ( m ) Φ η ( m ; ω ) ν , m Ω 1 +
C = 1 2 j = 1 s g j 𝓟 j μ a κ , g j 𝓟 j ( μ a κ ) L 2 ( Ω )
( α β ) = ( Re ( Φ j - Ψ j ) Re ( Φ j - · Ψ j ) )
· κ ( r ) Ψ j ( r ; ω ) + ( μ a ( r ) i ω c ) Ψ j ( r ; ω ) = 0 r Ω d \ ( Ξ d Ω d )
Ψ j ( m ; ω ) + 2 A κ ( m ) Ψ j ( m ; ω ) ν = g j ( m ; ω ) 𝓟 j ( μ a κ ) m Ω 1 +
Ψ j ( m ; ω ) + 2 A κ Ψ j ( m ; ω ) ν = 1 π Ξ cos θ cos θ ' Ψ j ( m ; ω ) 2 A h ( m , m ) x
exp [ ( μ a i ω c ) m m ] m m 2 d m m , m Ξ
f ( m , m ) = cos θ ( m ) cos θ ( m ) π m m 2
f τ α , τ α ( m , m ) = k = 1 N k = 1 N u n ( k ) ( m ) u n ( k ) ( m ) cos θ n ( k ) cos θ n ( k ) π N n ( k ) N n ( k ) 2
Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All rights reserved, including rights for text and data mining and training of artificial technologies or similar technologies.