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Multiple scattering in optical
coherence tomography signal: Monte
Carlo modeling and experimental
study
Gang Yao, Lihong V. Wang
Gang Yao, Lihong V. Wang, "Multiple scattering in optical coherence
tomography signal: Monte Carlo modeling and experimental study," Proc.
SPIE 3598, Coherence Domain Optical Methods in Biomedical Science and
Clinical Applications III, (30 April 1999); doi: 10.1117/12.347489
Event: BiOS '99 International Biomedical Optics Symposium, 1999, San Jose,
CA, United States
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Multiple Scattering in Optical Coherence Tomography Signal:
Monte Carlo Modeling and Experimental Study
Gang Yao, Lihong Wang*
Optical Imaging Laboratory, Biomedical Engineering Program, Texas A&M University
233 Zachry Engineering Center, College Station, TX 77843-3120
ABSTRACT
The angle biased Monte Carlo technique is applied to simulate the OCT signal from homogeneous turbid medium. The OCT
signal is divided into two categories: one is from a specific imaging target layer in the turbid medium (Class I photon); the
other is from the other background medium (Class II photon). The Class II signal has wider spatial and angular distribution
than the Class I signal. And it experiences more scattering events. The multiple scattered photons will decrease the contrast
of the OCT image and their contributions become dominant at larger depths. The average number of scattering events
increases with the probing depth for both Class I and Class II lights. Experimental study is conducted by measuring the
depth-resolved degree of polarization (DOP) of the back-scattered signal from the turbid media. The DOP is derived from
the Stokes vector measurements. The incident light is linear polarized and could be depolarize by the multiple scattering.
The DOP decreases to 0.5
when
Class I signal is equal to the Class II signal. Experiments in the Intralipid solution with
different scattering coefficient show the imaging depth is limited to 3 -
4
optical depths.
Keywords: Optical coherence tomography, Monte Carlo, multiple scattering, depolarization, stokes vector
1. INTRODUCTORY
Because of its high spatial resolution and high dynamic range, optical coherence tomography (OCT)' has drawn much
attention recently. Unfortunately, its applications in highly scattering biological tissue are limited by its penetration depth
unlike its successful applications in transparent tissues such as the ocular organs.23 It is believed that multiple scattering that
becomes dominant at large depths is the fundamental limitation for OCT to achieve a large probing depth in turbid media.4
In order to understand the governing physical process and better interpret the OCT signal in highly scattering media, a
couple of theoretical models have been developed. Pan et at5 established the relationship between the path-length resolved
reflectance signal with the OCT signal using linear system theory. They used Monte Carlo technique to simulate the path-
length resolved reflectance but did not separate the effects of the singly scattered light and the multiply scattered light.
Recently, Schmitt et al 6
described
an OCT model based on the Huygens-Fresnel diffraction optics. They split the OCT
signal as the summation of singly back-scattered light (coherent) and multiply scattered light (partially coherent). The effect
of multiple scattering on the formation of speckle patterns and the degradation of image contrast were demonstrated.
In reality, light scattering in turbid media is a complex process, and it is only an approximation to assume that the OCT
signal is from single back-scattering alone. A photon still contributes to the OCT signal after a limited number of scattering
events. A more realistic model is needed to study the OCT signal from the turbid media.
In this paper, we simulate the light scattering process in homogeneous turbid media by Monte Carlo method.7 The OCT
signal is divided into two classes: one is the light coming from the target layer in the medium; and the other is the light
coming from the background other than the target layer. Angle biasing technique8 is applied to speed up the simulation and
reduce the statistical variance. A polarization sensitive OCT is used to measure the depth resolved degree of polarization
(DOP) of back-scattering signal from turbid media. The DOP is derived from the Stokes vector of the back-scattered signal.
Because the multiple scattering will depolarize the incident light, the change of polarization degree is a sensitive indication
ofthe dominance ofthe multiple scattering events.
Correspondence: Email: 1wangtamu.edu, Tel: (409)847-9040, Fax: (409)845-4450
Part
of the SPIE Conference on Coherence Domain Optical Methods in Biomedical
10
Science and Clinical Applications Ill • San Jose, California • January 1999
SPIE Vol. 3598 • 0277-786X/99/$10.00
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2. THEORETICAL STUDY
2.1 OCT model
An OCT system is a Michelson interferometer illuminated by a low-coherence light source. The light from the reference
arm and the sampling arm can interfere at the detector only when the difference of their optical path-lengths is within the
coherence length of the light source. The interference signal is used to construct a tomographic image of the sample.
Therefore, the spatial resolution of OCT is determined by the coherence length of the light source.
In the simulation, it is assumed that the probing fiber is in direct contact with the
turbid medium. For simplicity, the fiber is assumed to emit a pencil beam. The
radius of the probing fiber is 10 rim, and the receiving angle is 5°. The light
back-scattered from the sample is divided into two different classes: Class I and
Class II (Fig. 1).
The Class I light is the light scattered from a specific layer whose central depth
corresponds to the path-length of the reference arm and whose thickness is
determined by
\ItJ
11
(1)
Fig.1. Composition of the OCT signal,
where I represents the light from the
specified target layer (Class I), and H
represents the light from the rest of the
medium (Class II).
where n is the refractive index of the medium, l is the coherence length of the
light source in vacuum, and Az is the thickness of the layer. Because the photons
scattered from this layer contain information about the local optical properties,
the Class I light is considered the useful signal that provides direct imaging
information. The Class II light is the light scattered from the rest of the medium whose optical path-length is within the
range of [p—4/2, p+l!2], where p is the path-length of the reference arm. Because the path-length difference between this
part of the light and the reference light is within the coherence length, the Class II light affects the OCT signal. The Class Ii
light may be from anywhere above the specific layer in the turbid medium, i.e., it does not contain information about the
specific probing depth in the medium. Therefore, this part of the light is responsible for the degradation of the contrast of
OCT images and may overwhelm the Class I signal at large probing depths.
The OCT signal can be written as:5
Jd(r) =
1s 'r +2(JsIr)1I2 Re[Vrnc(r)],
(2)
where t is the time delay between the reference arm and the sampling arm; i. and I. are the ensemble averaged light
intensities from the reference arm and the sampling arm, respectively; and Vmc i5 the mutual coherence function of the light
from the two arms and is assumed to be rectangular for simplicity. Equation (2) indicates that the OCT signal is proportional
to the square root ofthe diffuse reflectance h. In our model, I. is the summation ofthe Class I light (li) and the Class II light
(12):
Is = Ii + '2
(3)
The light whose path-length difference with the reference path-length is beyond the coherence length is simply discarded
because it does not contribute to the OCT signal.
2.2 Angle biased Monte Carlo simulation
Monte Carlo simulation has been proved to be an accurate method to study photon-tissue interaction. Because biological
tissues usually have very large anisotropy factors, light undergoes highly forward scattering and has a small chance to be
back-scattered. However, OCT modeling requires very high spatial resolution (of the order of the coherence length).
Therefore, it would be a very time consuming task to use the conventional Monte Carlo algorithm. In order to accelerate the
computation, we applied a variance reduction technique called "angle biased" sampling.8 The basic idea is to use an
artificial scattering phase function to replace the true phase function when sampling the scattering angle and then update the
photon weight according to:
11
2nAz=l,
I_AZ
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