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  • Editor: Alan E. Willner
  • Vol. 37, Iss. 24 — Dec. 15, 2012
  • pp: 5220–5222
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Structural length-scale sensitivities of reflectance measurements in continuous random media under the Born approximation

Andrew J. Radosevich, Ji Yi, Jeremy D. Rogers, and Vadim Backman  »View Author Affiliations


Optics Letters, Vol. 37, Issue 24, pp. 5220-5222 (2012)
http://dx.doi.org/10.1364/OL.37.005220


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Abstract

Which range of structures contributes to light scattering in a continuous random media, such as biological tissue? In this Letter, we present a model to study the structural length-scale sensitivity of scattering in continuous random media under the Born approximation. The scattering coefficient μs, backscattering coefficient μb, anisotropy factor g, and reduced scattering coefficient μs* as well as the shape of the spatial reflectance profile are calculated under this model. For media with a biologically relevant Henyey–Greenstein phase function with g0.93 at wavelength λ=633nm, we report that μs* is sensitive to structural length-scales from 46.9 nm to 2.07 μm (i.e., λ/13 to 3λ), μb is sensitive from 26.7 to 320 nm (i.e., λ/24 to λ/2), and the spatial reflectance profile is sensitive from 30.8 nm to 2.71 μm (i.e., λ/21 to 4λ).

© 2012 Optical Society of America

Elastic light scattering provides a valuable tool to detect and quantify subdiffractional structures even if they cannot be resolved by a conventional imaging system. However, the limits of the sensitivity of light scattering to different structural length-scales in a continuous random media (e.g., biological tissue) have not yet been fully studied. In this Letter, we present the methodologies used to study the length-scale sensitivities of the scattering parameters μs, μ b, g, and μ s * as well as the diffuse reflectance profile in continuous random media.

Consider a statistically homogeneous random medium composed of a continuous distribution of fluctuating refractive index, n(r⃗). We define the excess refractive index which contributes to scattering as n Δ(r⃗)=n(r⃗)/ n o1, where n o is the mean refractive index. Since n Δ(r⃗) is a random process, it is mathematically useful to describe the distribution of refractive index through its statistical autocorrelation function B n( r d)= n Δ(r⃗) n Δ(r⃗ r d)dr⃗.

One versatile model for Bn( rd) employs the Whittle–Matérn family of correlation functions [1

P. Guttorp and T. Gneiting, “On the Whittle–Matérn correlation family ,” National Research Center for Statistics and the Environment, Technical Report Series (2005).

,2

J. D. Rogers, İ. R. Çapoğlu, and V. Backman, Opt. Lett. 34, 1891 (2009). [CrossRef]

]:
B n( r d)= A n· ( r d l c) D3 2· K D3 2 ( r d l c),
(1)
where K ν(·) is the modified Bessel function of the second kind with order ν, l c is the characteristic length of heterogeneity, A n is the fluctuation strength, and D determines the shape of the distribution (e.g., Gaussian as D, decaying exponential for D=4, and power law for D<3). Importantly, when D=3 this model predicts a scattering phase function that is identical to the commonly used Henyey–Greenstein model.

All light scattering characteristics can be expressed through the power spectral density Φ s. Under the Born approximation, Φ s is the Fourier transform of B n [2

J. D. Rogers, İ. R. Çapoğlu, and V. Backman, Opt. Lett. 34, 1891 (2009). [CrossRef]

,3

A. Ishimaru, Wave Propagation and Scattering in Random Media (IEEE, 1997).

]:
Φ s( k s)= A n l c 3Γ ( D 2) π 3/2 2 (5D)/2· (1+ k s 2 l c 2) D/2,
(2)
where k s=2ksin(θ/2) and k is the wavenumber.

In order to study the sensitivity of scattering to short length-scales (lower length-scale analysis), we perturb n Δ(r⃗) by convolving with a three-dimensional Gaussian:
G(r⃗)= ( 16πln(2) W 2) 3/2·exp ( 4ln(2) W 2 r⃗ 2),
(3)
where W is the FWHM. Conceptually, G(r⃗) represents a process that modifies the original medium by removing “particles” smaller than W. Using the convolution theorem, this modified medium can be expressed as n Δ l(r⃗)= F 1 [F[ n Δ(r⃗)]·F[G(r⃗)]], where F indicates the Fourier transform operation and the superscript l indicates that lower frequencies are retained.

The autocorrelation of n Δ l(r⃗) can then be found as
B n l( r d)= F 1 [ |F[ n Δ(r⃗)]| 2· |F[G(r⃗)]| 2] =4π 0 Φ s l( k s) k ssin( k sr) rd k s,
(4)
where Φ s l( k s) is the power spectral density for n Δ l(r⃗) and can be computed as
Φ s l( k s)= A n l c 3Γ( D 2) π 3/2 2 (5D)/2· exp ( k s 2 W l 2 8ln(2)) (1+ k s 2 l c 2) D/2.
(5)
We note that Eq. (4) has no closed form solution, but can be evaluated numerically.

Figure 1 demonstrates the functions described by Eqs. (4) and (5) for varying values of Wl using a B n l( r d) with D=3, l c=1μm, and wavelength λ=633nm. This corresponds to a biologically relevant Henyey–Greenstein function with anisotropy factor g0.93. For increasing W l, B n l( r d) shows a decreasing value at short length-scales [Fig. 1(a)]. The point at which B n l( r d) deviates from the original B n( r d) corresponds roughly to the value of W l. The lower value of Bnl( rd) at short length-scales corresponds to decreased intensity of Φ s l( k s) at higher spatial frequencies after Fourier transformation [Fig. 1(b)]. To study the sensitivity of scattering to large length-scales (upper length-scale analysis), we employ the same model as above but filter larger particles by evaluating n Δ h(r⃗)= F 1 [F[ n Δ(r⃗)]·(1F[G(r⃗)])], where the superscript h indicates that higher frequencies are retained. The autocorrelation of n Δ h(r⃗) can then be found as
B n h( r d)= F 1 [ |F[ n Δ(r⃗)]| 2· |1F[G(r⃗)]| 2] =4π 0 Φ s h( k s) k ssin( k sr) rd k s,
(6)
where
Φ s h( k s)= A n l c 3Γ( D 2) π 3/2 2 (5D)/2· (1exp ( k s 2 W h 2 16ln(2))) 2 (1+ k s 2 l c 2) D/2.
(7)

Fig. 1. Lower length-scale analysis for W l=0, 10, 50, and 100 nm with D=3, l c=1μm, and λ=633nm. The normalized (a)  Bnl( rd) and (b)  Φ s l( k s). In each panel the arrow indicates increasing W l.

Figure 2 shows the functions described by Eqs. (6) and (7). For decreasing Wh, B n h( r d) exhibits a decrease at larger length-scales [Fig. 2(a)]. These alterations lead to a decreased intensity of Φ s h( k s) at lower spatial frequencies [Fig. 2(b)].

As a way to visualize the continuous media represented by the above equations, Fig. 3 provides example cross-sectional slices through n Δ(r⃗), n Δ l(r⃗), and n Δ h(r⃗) for D=3, l c=1μm, and W l= W h=100nm.

Fig. 2. Upper length-scale analysis for W h=, 10, 5, and 1 μm with D=3, l c=1μm, and λ=633nm. (a)  Bnh( rd) where the dashed curves indicate locations in which the curve is negative. (b)  Φ s h( k s). In each panel the arrow indicates decreasing Wh.
Fig. 3. Example media with D=3 and l c=1μm. (a)  n Δ(r⃗), (b)  n Δ l(r⃗), and (c)  n Δ h(r⃗) for W l= W h=100nm.

Implementing the above methods, we now define a number of measurable scattering quantities. First, the differential scattering cross section per unit volume for unpolarized light σ(θ), can be found by incorporating the dipole scattering pattern into Φ s( k s):
σ(θ)=2π k 4 (1+ cos 2θ) Φ s( k s).
(8)
The shape of σ(θ) can be parameterized by the scattering coefficient μ s, the backscattering coefficient μ b, and g [4

C. F. Bohren and D. R. Huffman, Absorption and Scattering of Light by Small Particles (Wiley, 1983).

]:
μ s=2π 1 1σ(cosθ)dcosθ,
(9)
μb=4π·σ(θ=π),
(10)
g= 2π μ s 1 1cosθ·σ(cosθ)dcosθ.
(11)
Conceptually, μs is the total scattered power per unit volume, μ b represents the power scattered in the backward direction per unit volume, and g describes how forward directed the scattering is. Finally, the effective transport in a multiple scattering medium is expressed by the reduced scattering coefficient μ s *= μ s·(1g).

Figure 4(a) shows percent changes in the above scattering parameters under the lower length-scale analysis for a Bnl( rd) with D=3, l c=1μm, and λ=633nm. With increasing Wl, each parameter decreases from its original value. For μ s, the decrease occurs because scattering material is removed from the medium. For 1g and μb, the decrease occurs as a result of reduced backscattering [see Fig. 1(b)]. For μ s *, the decrease is a combination of the previous two effects.

Fig. 4. Percent change in scattering parameters with varying values of Wl and W h for D=3, l c=1μm, and λ=633nm. (a) Lower and (b) upper length-scale percent changes. The dotted line indicates the ±5% threshold.

To provide specific length-scale sensitivity quantification, we focus on the parameters most relevant to reflectance measurements: μ s * for samples within the multiple scattering regime and μ b for samples within the single scattering regime. Defining a 5% threshold (a common significance level in statistics) the minimum length-scale sensitivity ( r min) of μ s * and μb equals 46.9 nm ( λ/13) and 26.7 nm ( λ/24), respectively. Thus, measurements of μs* and μ b provide sensitivity to structures much smaller than the diffraction limit. Interestingly, r min is smaller for μ b than μ s *. This can be understood by noting that k s is maximized in the backscattering direction (i.e., θ=π) and so provides the most sensitivity to alterations of B n( r d) at small length-scales (see Fig. 1).

Figure 4(b) shows percent changes in the scattering parameters under the upper length-scale analysis. With decreasing W h, μs decreases because scattering material is removed from the medium. For 1g, an increase occurs due to a reduction in the forward scattering component. Combining these two opposing effects, the maximum length-scale sensitivity ( r max) for μs* equals 2.07 μm ( 3λ). For μ b, a very small value of W h is needed in order to alter backscattering. As a result, r max for μ b is only 320 nm ( λ/2).

In order to study the length-scale sensitivity of the spatial reflectance profile we performed electric field Monte Carlo simulations of continuous random medium as described in [5

A. J. Radosevich, J. D. Rogers, İ. R. Çapoğlu, N. N. Mutyal, P. Pradhan, and V. Backman, J. Biomed. Opt. 17, 115001 (2012). [CrossRef]

]. Here, we display the distribution measured with unpolarized illumination and collection, P oo(r). P oo(r) is the distribution of light that exits a semi-infinite medium antiparallel to the incident beam and within an annulus of radius r from the entrance point. It is normalized such that 0 P oo(r)dr=1.

Figure 5(a) shows P oo under the lower length-scale analysis for a B n( r d) with D=3, l c=1μm, and λ=633nm. With increasing Wl, the value of P oo is decreased within the subdiffusion regime (i.e., r· μ s *<1). This decrease can be attributed in part to the decreased intensity of the phase function in the backscattering direction [see Fig. 1(b)]. For r· μ s *>1, a range that is essentially insensitive to the shape of the phase function, P oo remains largely unchanged. Figure 5(b) shows similar results for the upper length-scale analysis. In order to perform a sensitivity analysis, we calculate the maximum percent error at any position on P oo relative to the original case. Applying a 5% threshold once again, we find that r min=30.8nm ( λ/21) and r max=2.71μm ( 4λ).

Fig. 5. Monte Carlo simulations of P oo with D=3, l c=1μm, and λ=633nm. (a) Lower length-scale analysis for W l=0, 30, 60, and 90 nm. Arrow indicates increasing Wl. (b) Upper length-scale analysis for W h=, 10, 2, 0.5 μm. Arrows indicate decreasing Wh.

Finally, we note that the exact values of r min and r max depend on the shape of B n( r d). The values given above provide an estimate assuming a correlation function shape that is widely used and accepted for modeling of biological tissue (Henyey–Greenstein). Figure 6 illustrates the dependence of r min and r max on the shape of Bn( rd), assuming the Whittle–Matérn model and using μs* as an example. As either D or l c increases, Bn( rd) shifts relatively more weight to larger length-scales and away from smaller length-scales. As a result, both r min and r max increase monotonically with D and lc.

Fig. 6. (a)  r min and (b)  r max for μ s * with different shapes of B n( r d) and λ=633nm.

Acknowledgments

This study was supported by National Institutes of Health grants RO1CA128641 and R01EB003682. A.J. Radosevich is supported by a National Science Foundation Graduate Research Fellowship under Grant DGE-0824162.

References

1.

P. Guttorp and T. Gneiting, “On the Whittle–Matérn correlation family ,” National Research Center for Statistics and the Environment, Technical Report Series (2005).

2.

J. D. Rogers, İ. R. Çapoğlu, and V. Backman, Opt. Lett. 34, 1891 (2009). [CrossRef]

3.

A. Ishimaru, Wave Propagation and Scattering in Random Media (IEEE, 1997).

4.

C. F. Bohren and D. R. Huffman, Absorption and Scattering of Light by Small Particles (Wiley, 1983).

5.

A. J. Radosevich, J. D. Rogers, İ. R. Çapoğlu, N. N. Mutyal, P. Pradhan, and V. Backman, J. Biomed. Opt. 17, 115001 (2012). [CrossRef]

OCIS Codes
(170.3660) Medical optics and biotechnology : Light propagation in tissues
(290.7050) Scattering : Turbid media
(290.5825) Scattering : Scattering theory

ToC Category:
Scattering

History
Original Manuscript: October 11, 2012
Manuscript Accepted: November 14, 2012
Published: December 13, 2012

Virtual Issues
Vol. 8, Iss. 1 Virtual Journal for Biomedical Optics

Citation
Andrew J. Radosevich, Ji Yi, Jeremy D. Rogers, and Vadim Backman, "Structural length-scale sensitivities of reflectance measurements in continuous random media under the Born approximation," Opt. Lett. 37, 5220-5222 (2012)
http://www.opticsinfobase.org/ol/abstract.cfm?URI=ol-37-24-5220


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References

  1. P. Guttorp and T. Gneiting, “On the Whittle–Matérn correlation family,” National Research Center for Statistics and the Environment, Technical Report Series (2005).
  2. J. D. Rogers, İ. R. Çapoğlu, and V. Backman, Opt. Lett. 34, 1891 (2009). [CrossRef]
  3. A. Ishimaru, Wave Propagation and Scattering in Random Media (IEEE, 1997).
  4. C. F. Bohren and D. R. Huffman, Absorption and Scattering of Light by Small Particles (Wiley, 1983).
  5. A. J. Radosevich, J. D. Rogers, İ. R. Çapoğlu, N. N. Mutyal, P. Pradhan, and V. Backman, J. Biomed. Opt. 17, 115001 (2012). [CrossRef]

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