Open Access
1 October 2003 Small-volume frequency-domain oximetry: phantom experiments and first in vivo results
Stefan Willmann, Albert Terenji, Jens Osterholtz, Joerg Meister, Peter Hering, Hans-Joachim Schwarzmaier M.D.
Author Affiliations +

1.

Introduction

Tissue oximetry based on optical techniques has been performed since 1942.1 2 The spectral range between 600 and 1000 nm is well suited for optical tissue oximetry because at these wavelengths, the absorption spectrum of hemoglobin is closely related to its oxygenation state.2 3 Moreover, the penetration depth of biological tissues is high in this spectral range. Usually, the light attenuation ratio at two different wavelengths is measured. Measurements are performed in either transmission or reflection geometry depending on the part of the body accessible to the sensor of the pulse oximeter.4 5 6 From these data, the oxygen saturation S[O 2] can be derived. However, the measurement of a simple attenuation ratio does not account for the contributions of photon losses due to scattering within biological tissues. Thus, these systems do not provide absolute absorption data. Therefore, all systems available so far must be calibrated to account for scattering. To this end, the pulse-oximeter readings are usually compared with ex vivo blood samples measured by conventional blood gas analyzers.6 7 8 Moreover, other absorbers such as melanin in the epidermal skin layer contribute to the background absorption and affect the measured quantities. Therefore, the latter cannot be taken into account without further calibration of the pulse oximeter. As a consequence, simple pulse oximetry reveals substantial errors when applied to different skin colors, for example, to Afro-Caribbean fetuses as reported by D’Antona et al.;9

To overcome the need for calibration, quantitative methods have been developed to determine the absorption coefficient of a turbid medium in vivo absolutely such as, for example, the frequency-domain multi-distance (FDMD) method.10 11 12 This technique is based on spatially resolved phase and intensity measurements using photon density waves in the frequency range of 10 to 100 MHz.13 14 15 16 17 To derive the absorption coefficients from the measured quantities, the diffusion approximation of radiative transport theory is often employed.15 16 17 Unfortunately, the diffusion approximation is only valid at large distances from the source (typically >20 mm in biological tissues).18 Consequently, the applicators used in the framework of this technique are comparatively bulky and, therefore, are not suited for minimally invasive monitoring such as, e.g., that required for measuring fetal blood oxygen saturation sub partu. To describe the photon transport in areas close to the light source quantitatively, the Monte-Carlo technique has been employed17 to extract the absorption coefficients from the measured quantities. However, Monte-Carlo simulations of photon transport in turbid media are currently still too time consuming to allow on-line processing of the measured data, although considerable progress has recently been made to accelerate the calculations.19 20

In this study, we propose to use the modified microscopic Beer-Lambert law (MBL) for the determination of the oxygen saturation and the total hemoglobin content for the first time. The modified MBL has been described previously21 and is the first technique that allows for an absolute determination of the absorption coefficient of turbid media at small source-detector separations on-line. Thus, the MBL can overcome the disadvantages of the techniques described above.

The aim of this study was to show that the MBL can be used to absolutely determine the oxygen saturation (S[O 2]) and total hemoglobin content (THC) on-line and in vivo at source detector separations suitable for minimally invasive applications such as the measurement of fetal oxygen saturation sub partu. To this end, a frequency-domain device was designed that was used in combination with the MBL for data processing. The system was evaluated in vitro using a series of solid scattering and absorbing phantoms with known optical properties mimicking those of neonate skin in the red and near-infrared spectral range. In addition, the influence of the layered skin structure and various contents of background absorber (e.g., melanin) on the oximeter readings has been investigated using the Monte-Carlo technique. Finally, a first in vivo feasibility test was performed to measure S[O 2] and THC of blood in human tissue on the forearm of a healthy adult volunteer.

2.

Theory

To determine the absorption coefficient of biological tissue, we applied the microscopic Beer-Lambert law (MBL) first introduced by Tsuchiya and Urakami22 23 in its modified time-integrated version.21 The basic idea of the MBL is to apply the well-known Beer-Lambert law to the individual pathlengths of a photon that is multiply scattered in a turbid medium. The temporal impulse response function R(μas,t) 22 depends on the scattering coefficient μs and the absorption coefficient μa and can be written as

Eq. (1)

R(μs,μa,t)=s(μs,t)exp{μacnt}
where s(μs,t) represents the probability of a scattered photon reaching the detector in the case of a non-absorbing medium a=0). The term exp{−μacnt} accounts for the losses due to absorption (cn=c0/n is the phase velocity in the medium with refractive index n).

If the time-integrated intensity I DC (in the following referred to as DC intensity)

Eq. (2)

IDC(μs,μa)=0R(μs,μa,t)dt
and the mean time of flight 〈t〉

Eq. (3)

t=0tR(μs,μa,t)dt0R(μs,μa,t)dt
of the photons are determined at two or more source detector separations, the absolute absorption coefficient μa can be derived from the slope of a ln{I DC } vs. 〈t〉 plot21:

Eq. (4)

μa=1cn Δ ln{IDC}Δt.
As discussed in detail in Ref. 21, Eq. (4) can be applied to turbid media with absorption coefficients between approximately 5×10−4 and 2 mm−1 and reduced scattering coefficients μs between 0.2 and 2 mm−1, a range typically found in biological tissues.24 25 26 27 28 29 30 Outside this range of optical properties, the linear behavior of ln{I DC } as a function of 〈t〉 should no longer be assumed because of a weak dependence of I DC and 〈t〉 on the scattering coefficient of the medium.

In the frequency domain, the mean time of flight can be determined from the slope of the phase (Φ) as a function of the frequency (f)16:

Eq. (5)

t=ΔΦ2πΔf.
As an analytical model, the MBL is suited to process the measured data on-line. Unlike the diffusion approximation, it is not limited to large source-detector separations. In addition, it has been shown to be insensitive to the measurement geometry.31 32

3.

Experimental Methods

3.1.

Frequency-Domain Setup

Frequency-domain measurements were performed using a setup similar to that described by Madsen et al.;33 A schematic drawing of the device is shown in Fig. 1. As light sources, three laser diodes were used [SDL 7432-H1 (λ=678 nm), SDL 2352-H1 (λ=808 nm), and SDL 5432-H1 (λ=835 nm), all from Spectra Diode Labs, San Jose, California]. The laser diodes were selectively bias-modulated in the frequency range between 300 kHz and 200 MHz by a vector network analyzer (HP 8712C, Hewlett Packard, Palo Alto, California) in combination with a high-frequency multiplexer (7016, Keithley, Cleveland, Ohio) and three bias tees (5580, Picosecond Labs, Boulder, Colorado). The modulated laser light was delivered to the sample via quartz/quartz optical fibers with a core diameter of 600 μm and a numerical aperture of 0.2. An identical fiber was used to collect the remitted photons at several source-detector separations ρ (between 3 and 9 mm). A high-speed avalenche-photodiode receiver (APD S90302C, EG&G Electrooptics, Boudreuil, Canada) with a spectral bandwidth of 800 MHz was used as optical detector. All measurements were performed with a frequency resolution of 4 MHz (51 data points) and a spectral bandwidth of 3.7 kHz. Phase and intensity data were averaged 16 times. The multiplexer and the network analyzer were controlled by a personal computer that was also used to record the measured data. The acquisition time for a single frequency sweep was approximately 400 ms.

Figure 1

Experimental setup of the frequency-domain spectrometer: LDD1–LDD3, laser diode drivers; LD1–LD3, laser diodes; S1–S3, shutters; FC1–FC3, fiber couplers; APD, avalanche photodiode; MPX, multiplexer.

010304j.1.jpg

3.2.

Scattering and Absorbing Phantoms

Tissue phantoms were designed to perform an evaluation of the new technique. Several recipes have been published to manufacture solid phantoms with defined scattering and absorption properties.34 We embedded TiO 2 particles (TiPure 960, DuPont, Mechelen, Belgium) into clear polyester resin (Norpol 340-500, Reichhold, Hamburg, Germany) as described in Ref. 35. A stock solution of 800 mg TiO 2 in 20 ml ethanol was used. The effective diameter of the TiO 2 particles was 350 nm. In order to determine the volume filling fraction of the scatterers (f sca ), we performed integrating-sphere measurements21 for a series of thin phantoms with various amounts of TiO 2 particles. We found that a volume filling fraction of f sca =3 of the stock solution resulting in reduced scattering coefficients of 1.03 mm−1 at 678 nm, 0.71 mm−1 at 808 nm, and 0.71 mm−1 at 835 nm, respectively (see Table 1), was best suited to mimic the scattering properties of neonatal skin (∼1 mm−1 in the NIR-wavelength range24).

Table 1

Optical properties of the phantoms for the three different wavelengths of the laser diodes determined by frequency-domain spectroscopy and integrating spheres measurements (mean±standard error).
Wavelength (nm) 678 808 835
Volume filling fraction
absorber ()
Absorption coefficient (mm−1)
0.000 0.027 ± 0.002 0.030 ± 0.004 0.038 ± 0.003
0.656 0.056 ± 0.004 0.102 ± 0.004 0.080 ± 0.002
1.303 0.072 ± 0.003 0.158 ± 0.009 0.109 ± 0.006
1.942 0.101 ± 0.005 0.219 ± 0.010 0.130 ± 0.004
2.572 0.107 ± 0.006 0.255 ± 0.014 0.167 ± 0.019
3.195 0.134 ± 0.016 0.289 ± 0.009 0.193 ± 0.024
Volume filling fraction
scatterer ()
Reduced scattering coefficient (mm−1)
3.0 1.03 ± 0.10 0.71 ± 0.06 0.71 ± 0.06

The absorption properties of the phantoms were adjusted with regard to the absorption coefficients of human skin at the wavelengths of interest. The respective data have been calculated using Eq. (8) (see below) from the known extinction spectra of Hb and HbO 2 (Ref. 3) for a total hemoglobin content of 190 g/l, which is typical for fetal blood.36 The volume fraction occupied by blood vessels was assumed to be 5.37 The resulting absorption coefficients at the wavelengths of interest are shown in Fig. 2. They were found to be between 0.01 and 0.1 mm−1. A series of nonscattering phantoms that consisted of various amounts of an absorbing stock solution (1 mg of an infrared dye, ProJet 900 NP by Zeneca Colors, Manchester, England, solved in 10 ml ethanol) in resin was manufactured. The relative absorptivity Δμa/Δf abs (i.e., the absorption coefficient per unit volume of absorber) of these phantoms was then determined with a conventional absorption spectrometer (Lambda 19, Perkin Elmer, Shelton, Connecticut). It was found that volume filling fractions of the absorber between 0.0 and 3.1 simulated best the various oxygenation states of fetal skin. According to these results, six solid scattering and absorbing phantoms (dimensions: diameter 50 mm, thickness 30 mm) with volume filling fractions of 3 scatterer and 0.0 to 3.1 absorber were manufactured and were used for further investigations.

Figure 2

Calculated absorption coefficients of fetal skin containing 5 of blood as a function of the oxygen saturation.

010304j.2.jpg

As can be seen from Eq. (4), the refractive index has to be known in order to deduce the absorption coefficient of the sample. Because more than 93 of the phantom volume is filled with resin, it was assumed that the latter determines the refractive index of the samples. To characterize the phantoms completely, we determined the refractive index of the resin by goniometric reflection measurements. Therefore, a clear resin sample was irradiated using p-polarized light in the wavelength range from 400 to 860 nm. The angle of incidence パ of the collimated beam was varied between 15 and 75 deg in steps of 2.5 deg. The refractive index n was obtained by fitting the experimental data to the Fresnel function for p-polarized light Rp(パ):

Eq. (6)

Rp(ϑ)=[(n2sin2 ϑcos ϑ)2n21]2.
Frequency-domain measurements of the phantoms were performed at source-detector separations between ρ=3 mm and ρ=9 mm using a single source fiber and a single detector fiber. Equation (4) was then used to derive the absorption coefficient from the measured DC intensity and mean time of flight.

3.3.

Interaction Volume

Prior to the in vivo testing, the interaction volume of the detected photons in the skin was determined using Monte-Carlo simulations as described previously.38 This volume is of great importance because the measured absorption coefficient represents an average value over the probed sample volume.39

Human skin consists of three layers25 40 41 with different optical properties. The uppermost layer (epidermis) is typically 60 μm thick and does not contain blood vessels. The second layer (dermis) is typically 2 mm thick and contains a fine capillary network of arteries and veins. Underneath the dermis, there is a layer of subcutaneous fat with a thickness of several millimeters, depending on the exact location at the body surface. The optical properties of the epidermis, the dermis, and the subcutaneous fat have been well characterized by several authors.24 25 26 27 28 29 30 In the epidermis, the dominant absorbing chromophore is melanin. The fraction of melanin present in the epidermis f mel depends on the skin type and is reported to vary between 1.3 to 6.3 for lightly pigmented skin and 18 to 43 for heavily pigmented skin.26 Thus, the absorption coefficient of the epidermis can be calculated from the melanin content (f mel ) and the background absorption of unpigmented skin a unpigm (λ)] 25:

Eq. (7)

μaepidermis(λ)=fmelμamel(λ)+(1fmel)μaunpigm(λ).
Here, μa mel (λ) denotes the absorption coefficient of melanin at the wavelength of interest. The absorption spectra of melanin and unpigmented skin can be obtained from the literature.25 The absorption coefficient of the dermis can be described by the absorption coefficient of unpigmented skin and the absorption coefficient of blood that depends on the concentrations of hemoglobin ([Hb]) and oxyhemoglobin ([HbO 2]):

Eq. (8)

μadermis(λ)=μaunpigm(λ)+ln 10(ϵHbO2(λ)[HbO2]+ϵHb(λ)[Hb]).
Here, ε HbO2 and ε HB denote the molar extinction coefficients of HbO 2 and Hb, respectively. The factor ln 10 accounts for the fact that the extinction coefficient is defined as the log 10 in contrast to the absorption coefficient. Thus, the various layers contribute differently to the measured absorption coefficient. The epidermal layer can be treated as a background signal, whereas the spectral information about the concentrations of Hb and HbO 2 is contained on the dermal layer.

In our simulations, we modeled the skin as a medium consisting of the three layers mentioned above. The thickness of the layers was set to 60 μm for the epidermis and to 2 mm for the dermis. A typical value for the depth of the subcutaneous fat layer is 8 mm. The influence of the underlying tissue layers can be neglected, provided that the detected photons do not penetrate more than 1 cm into the tissue for the considered source-detector separations. Thus, the thickness of the subcutaneous fat layer can be set to infinity in the Monte-Carlo model.

The absorption coefficients of the epidermis and dermis were calculated from Eq. (7) and Eq. (8). A volume filling fraction of blood of 5 according to a THC of 116 μmol/l and an oxygen saturation of 90 was assumed for the dermis. Four series of simulations were performed where the melanin content of the epidermis was varied (f mel =5, 10, 15 and 20). The reduced scattering coefficients of the dermis and epidermis were calculated as described in Ref. 25. The absorption coefficient and the reduced scattering coefficient of subcutaneous fat were obtained from Ref. 28. The scattering coefficients of the skin layers were calculated from the reduced scattering coefficients assuming the anisotropy factor of 0.9 (Ref. 30). For refractive indices of the various skin layers, a value of n=1.4 was used.42 The resulting optical properties for a wavelength of 808 nm are shown in Table 2.

Table 2

Optical properties of the epidermis (at different melanin contents), the dermis, and the subcutaneous fat for the wavelength of 808 nm. For the dermis, the S[O 2] is 90 and the THC is 116 μmol/l according to a blood volume filling fraction of 5. The anisotropy factor is assumed to be 0.9 for all layers.25262728
μa (mm −1)μs (mm −1)
Epidermis (f mel =0)0.029 13.4
Epidermis (f mel =5)0.71 13.4
Epidermis (f mel =10)1.40 13.4
Epidermis (f mel =15)2.08 13.4
Epidermis (f mel =20)2.77 13.4
Dermis (S[O 2]=90,
THC=116 μmol/l)
0.046 13.4
Subcutaneous fat 0.0084 11.3

In the calculations, photons were launched into the multi-layered semi-infinite medium. The illuminated area and the angular distribution of the launched and detected photons were chosen according to the diameter (600 μm) and numerical aperture (0.2) of the employed source and detector fiber. The propagation of the photons in the medium was calculated using a variable step size Monte-Carlo algorithm that was described in Ref. 38. When a photon crossed the boundary between two layers, the new position of the photon was calculated according to the optical properties of the new layer.39 In addition, the Fresnel reflections at the surface of the skin were taken into account.

On the surface of the medium, nine detector fibers were defined at distances between 2 and 10 mm from the source fiber in steps of 1 mm. For those photons that were diffusely reflected, the positions and the angles at which the photons left the surface were calculated. From these data the probability for launched photons to be detected by one of the detector fibers could be determined. The simulation was terminated when a total number of 1000 photons was detected at the largest distance (10 mm) from the source fiber. Consequently, much larger numbers of photons were registered for the smaller distances (>30,000 for the smallest distance of 2 mm).

For further data processing, the trajectories of those photons that reached one of the detector fibers were stored in the computer. Therefore, a Cartesian coordinate system was defined such that the surface of the medium was located in the x-y plane and the z-axis is perpendicular to the surface. The (x,y,z) coordinates of the source and detector fiber were (0,0,0) and (ρ,0,0), respectively. For those photons that entered the detector fiber located at x=ρ, a grid of cubic voxels was defined where the basic length was set to Δl ρ=ρ/100. In this discrete space, the position of a single voxel could be characterized by three integer numbers i, j and k, where the coordinates of the voxel were (xi,yj,zk)=(i*Δl ρ,j*Δl ρ,k*Δl ρ). As a measure of the interaction volume, we defined the interaction density of the detected photons Sρ(xi,yj,zk) as the number of scattering events of the detected photons in the voxel located at the position (xi,yj,zk). A two-dimensional projection Sρ(xi,zk) of the interaction volume can be obtained by adding the values of the interaction density at fixed xi and zk positions for all yj positions:

Eq. (9)

Sρ(xi,zk)=jSρ(xi,yj,zk).
In reflection geometry, this interaction volume has the shape of a banana and is therefore often referred to as the “photon-banana.” As a measure of the mean penetration depth (〈z〉) the center of mass of the interaction density at half of the distance between the source and detector fiber ρ/2 was calculated:

Eq. (10)

z=ΣkzkSρ(ρ/2,zk)ΣkSρ(ρ/2,zk).
Additionally, the mean path length of the photons in the individual layers can easily be obtained from the stored photon trajectories.

3.4.

In vivo Measurements

In contrast to the existing “large-volume” methods for the measurement of the oxygen saturation and total hemoglobin content in vivo,10 11 12 the small-volume approach measures the average absorption properties of the epidermis and dermis weighted by the interaction density of the two layers. To interpret the measured in vivo data, we consider a turbid medium that consists of two layers A and B with different scattering coefficients s A and μs B) and absorption coefficients a A and μa B) as shown in Fig. 3. The photons that are scattered into the detector fiber travel different paths in the medium. In Fig. 3, the trajectory of a single photon between the source and the detector fiber is shown. The length of the trajectory in layers A and B is referred to as dA and dB, respectively. For a large number of photons that are scattered into the detector fiber, the average pathlengths of the photons in layers A and B are denoted 〈dA and 〈dB〉. When the multi-layered medium in Fig. 3 is examined using the MBL [Eq. (4)], the average absorption coefficient μa of the two layers A and B will be obtained whereby the average is weighted with the average pathlengths of the photons in the medium:

Eq. (11)

μa=dAμaA+dBμaBdA+dB=fAμaA+(1fA)μaB.
Here, fA=〈dA〉/(〈dA〉+〈dB〉) denotes the fractional contribution of the average pathlength of the photons in the upper layer A. Regarding the measurement of the absorption coefficient μa of human skin using the modifiend MBL, Eq. (11) can be written as:

Eq. (12)

μa(λ)=fepidermisμaepidermis(λ)+(1fepidermis)μadermis(λ),
where f epidermis denotes the fractional contribution of the epidermis to the absorption coefficient. The absorption coefficient of the epidermis μa epidermis follows from Eq. (7). The absorption coefficient of the dermis μa dermis depends on the concentrations of Hb and HbO 2 as described in Eq. (8). In order to derive the hemoglobin concentration in the tissue, the absorption coefficient μa is measured at two different wavelengths. The concentrations of Hb and HbO 2 can be calculated using Eqs. (7), (8), and (12) provided that the fractional contribution of absorption and the melanin content of the epidermis are known. The oxygen saturation and the total hemoglobin content finally follow from:
S[O2]=[HbO2][Hb]+[HbO2]×100
and

Eq. (13)

THC=[Hb]+[HbO2].
In this study, in vivo measurements were performed on the forearm of a healthy Caucasian volunteer with light-colored skin. According to Ref. 26, the value of f mel =5 was used for the evaluation of the measured absorption coefficients. The fractional contribution of the epidermal layer to the overall absorption coefficient was estimated from the Monte-Carlo simulations.

Figure 3

Schematic drawing of the trajectory of a single photon between a source and a detector fiber in a turbid medium, which consists of two layers A and B with different optical properties (scattering coefficients μs A and μs B , absorption coefficients μa A and μa B ) . The pathlengths of the photon in layers A and B are d A and d B , respectively. When a large number of photons with different trajectories between source and detector fibers is considered, the mean pathlengths 〈d A and 〈d B are relevant.

010304j.3.jpg

In order to demonstrate the feasibility of the new technique to determine S[O 2] and THC in vivo, a homemade applicator consisting of two source and two detector fibers was positioned on the forearm of the volunteer at rest (blood pressure at rest was 115/80 mm Hg). The arrangement of the fibers is presented in Fig. 4. The dimensions of the applicator head are 10×8×10 mm3 (length×width×height). A homemade fiber switch consisting of a magnetic shutter and a 2-in-1 fiber coupler allowed consecutive recording of the signal obtained by the two detector fibers. For the in vivo measurements, two wavelengths 1=678 nm, λ2=808 nm) were chosen. At 678 nm, the difference of the absorption coefficients of oxy-and deoxyhemoglobin is maximal while at 808 nm there is an isosbestic point of the two absorbers (see Fig. 2).3 Thus, the sensitivity to detect small changes in S[O 2] can be expected to be largest for the available wavelengths. For both wavelengths, the refractive index of n=1.4 was assumed.42

Figure 4

In vivo experiment to determine the oxygen saturation and the total hemoglobin content at the forearm of a volunteer using a blood pressure cuff to occlude the arm vessels. The inset shows the arrangement of the source and detector fibers [wavelengths: λ1=678 nm, λ2=808 nm; source-detector separations for λ1: ρ1=5 mm, ρ2=7 mm; source-detector separations for λ2 in analogy (not depicted)].

010304j.4.jpg

At the beginning of the in vivo measurements, baseline data were acquired over 5 minutes. Thereafter, a pneumatic blood pressure cuff was inflated to a pressure of 150 to 160 mm Hg for 4.5 minutes inducing vascular occlusion. After release of the cuff, measurements of the absorption coefficients were continued for another 5 minutes. The acquisition time for a single data set was approximately 15 seconds. During the experiment, the data sets were collected in intervals of 30 seconds. The personal computer used to control the experimental setup was also employed to calculate S[O 2] and THC from the measured quantities. The sequence of the steps that were performed for the calculation of the oxygen saturation and the total hemoglobin content from the frequency-domain data is outlined in Fig. 5.

Figure 5

Sequence of the determination of the oxygen saturation S[O 2] and the total hemoglobin content THC from the frequency-domain data.

010304j.5.jpg

4.

Results

4.1.

Phantom Measurements

4.1.1.

Refractive index

The refractive index of the phantoms was determined from the goniometric reflection measurements using Eq. (6) as described above. The result of these measurements is shown in Fig. 6. From the measured values of the refractive index, the following two-parameter Sellmeier formula was obtained:

Eq. (14)

n2(λ)=1+1.3025{λ}2{λ}2(0.1375)2({λ}inμm).
The refractive index of the phantoms was calculated at the wavelengths of interest using Eq. (14).

Figure 6

Refractive index of resin: experimental values (symbols, mean and standard error) and Sellmeier fit according to Eq. (14) (solid line).

010304j.6.jpg

4.1.2.

Absorption properties

Frequency-domain measurements were then performed for the six phantoms containing different amounts of absorber to determine the time-integrated intensity I DC and the mean time of flight 〈t〉 of the detected photons. Figure 7 shows the time-integrated intensity I DC as a function of the mean time of flight 〈t〉 at various source-detector separations between 3 and 9 mm for the wavelength of λ=678 nm. The mean time of flight varied between 150 and 550 ps corresponding to a mean pathlength of the photons 〈L〉=cn〈t〉 between 29 and 107 mm. Thus, it exceeded the source-detector separation by a factor of up to 12. As predicted by the modified MBL, the logarithm of the DC intensity decreased linearly with increasing time of flight. The correlation coefficients for all wavelengths were greater than 0.98. According to Eq. (4), the absorption coefficient of the sample can be obtained from the slope of the ln{I DC } vs. 〈t〉 plots. The resulting absorption coefficients are presented in Fig. 8 for all employed wavelengths. A linear dependence of μa from the volume filling fraction of the absorbers was obtained (correlation coefficient R=0.993 for λ=678 nm, 0.992 for λ=808 nm, and 0.989 for λ=835 nm). The relative absorptivities Δμa/Δf abs obtained from the slopes of Fig. 8 were compared to the relative absorptivities of the non-scattering phantom samples determined using the conventional absorption spectrometer. As can be seen in Fig. 9, the frequency-domain technique data agreed very well with the results obtained from the conventional spectrophotometer. The resulting optical properties of the phantoms used in this study are summarized in Table 1.

Figure 7

Logarithm of the time-integrated intensity as a function of the mean time of flight for the various phantoms at a wavelength of λ=678 nm (symbols, mean and standard error; dotted line, linear regression). All correlation coefficients are >0.98.

010304j.7.jpg

Figure 8

Absorption coefficient of the phantoms as a function of the volume filling fraction of the absorber (symbols, mean and standard error; dotted line, linear regression). The regression coefficients are R=0.9929 (λ=678 nm), R=0.9917 (λ=808 nm), and R=0.9885 (λ=835 nm).

010304j.8.jpg

Figure 9

Comparison of the relative absorptivities measured using the frequency-domain spectrometer (symbols, mean and standard error) with the mean relative absorptivity determined with a conventional absorption spectrometer for a series of non-scattering phantoms (solid line).

010304j.9.jpg

4.2.

Monte-Carlo Simulations

Figure 10 shows a typical result for the interaction density as a function of the depth in the turbid medium at a distance of ρ=5 mm from the source fiber. The optical properties correspond to the wavelength of 808 nm and the melanin content in the dermis of 5 (Table 2). The banana-like shape of the probed sample volume is clearly visible. The mean penetration depth 〈z〉 is shown in Fig. 11 as a function of ρ for the wavelength of 808 nm. As can be seen in this figure, 〈z〉 increases linearly with ρ from 1.2 mm at ρ=2 mm to approximately 5 mm at ρ=10 mm. No significant dependence of the mean penetration depth on the melanin content of the epidermis was found in the Monte-Carlo simulations between ρ=2 and 9 mm.

Figure 10

Interaction density Sρ(xi,zk) of the detected photons for a three-layer semi-infinite model of human skin (epidermis, dermis, and subcutis) determined with a Monte-Carlo simulation for a source-detector separation of ρ=5 mm (logarithmic grayscale, arbitrary units). The layer boundaries are at z=0.06 mm and z=2.06 mm. The optical properties of the layers correspond to the epidermis, dermis, and subcutaneous fat at the wavelength of 808 nm and the melanin content of 5 in the epidermis. Source and detector fiber are located at x=0 mm and x=5 mm, respectively.

010304j.10.jpg

Figure 11

Penetration depths of the detected photons as a function of the source-detector separation determined with a Monte-Carlo simulation in a three-layer semi-infinite medium for different melanin contents f mel in the epidermis (mean±standard error). The optical properties correspond to the wavelength of 808 nm. For the small source-detector separations, a larger number of photons was detected. Thus, a better statistical accuracy was achieved.

010304j.11.jpg

Furthermore, the ratio of the pathlength of the photons in the epidermis to the total pathlength f epidermis was calculated for the different values of f mel . The dependence of f epidermis on the source-detector separation is shown in Fig. 12 for the wavelength of 808 nm. For the source-detector separation of 2 mm and the melanin content of f mel =5, about 2.7 of the interaction events occurred within the first layer of the medium. The fraction decreases to approximately 1.1 at ρ=5 mm and 0.8 at ρ=7 mm. At the wavelength of 678 nm and the melanin content of 5, the value of 0.9 at ρ=5 and 0.7 at ρ=7 mm was obtained for f epidermis . With regard to these findings, a mean value of f epidermis =0.9 was used for the processing of the in vivo data.

Figure 12

Fractional contribution f epidermis of the epidermal layer (thickness 60 μm26) to the photon pathlength in human skin determined from Monte-Carlo simulations at the wavelength of 808 nm for different source-detector separations and different melanin contents f mel (mean±standard error).

010304j.12.jpg

4.3.

In vivo Measurements

Figure 13 shows the absorption coefficients at 678 and 808 nm and the calculated concentrations of Hb and HbO 2 in the probed region before, during, and after occlusion of the blood vessels. Using Eqs. (12) and (13), the total hemoglobin content and the oxygen saturation have been calculated from the measured data assuming a fractional melanin content of f mel =5 and an average fractional pathlength in the epidermis of f epidermis =0.9. The result of these calculations is shown in Fig. 14. During occlusion, the calculated THC rapidly decreased from approximately 220 to 250 μmol/l to values between 150 and 190 μmol/l and the calculated S[O 2] dropped from approximately 94 to 95 to 82 to 86. After release of the blood pressure cuff, THC and S[O 2] increased rapidly and returned to the values measured before occlusion of the blood vessels.

Figure 13

Absorption coefficient and concentration of hemoglobin and oxyhemoglobin determined in the in vivo experiment. The error bars represent the uncertainties due to experimental errors. The shaded area indicates the period of cuff occlusion.

010304j.13.jpg

Figure 14

Result of the in vivo determination of the oxygen saturation and the total hemoglobin content. The error bars represent the uncertainties due to experimental errors. The shaded area indicates the period of cuff occlusion.

010304j.14.jpg

5.

Discussion

The modified time-integrated MBL has earlier been demonstrated to allow the determination of absorption coefficients in turbid media with optical properties comparable to those of biological tissues at small source-detector separations (between 3 and 10 mm).21 In this study, we evaluated its applicability towards the monitoring of the oxygen saturation and total hemoglobin content of fetal skin to provide minimally invasive oximetry sub partu.

First, a total of six scattering and absorbing phantoms with optical properties comparable to those of neonate skin in the red and near-infrared spectral range were manufactured as described in Ref. 35. These phantoms consisted of a clear transparent polyester matrix and TiO 2 particles with a volume filling fraction of 3 as scatterers. The phantoms contained various amounts of an infrared dye ranging from 0.0 to 3.1 to simulate various oxygenation states of blood in fetal skin tissue.24 30 As predicted by the modified MBL [Eq. (4)], we obtained excellent linear correlations between the logarithm of the time-integrated intensity and the mean time of flight at all investigated wavelengths (R>0.98, Fig. 7). The relative absorptivities obtained from the slopes of the absorption coefficients as a function of the volume filling fractions of absorbers (Fig. 8) were compared to the relative absorptivity spectrum obtained in a non-scattering sample using a conventional absorption spectrometer (“gold standard”). The agreement between the two methods was again excellent as can be seen in Fig. 9. This indicates that the modified MBL is well suited for the determination of the absorption coefficient of human neonate skin at the considered source-detector separations between 3 and 9 mm.

In contrast to the optically homogeneous phantoms, human skin consists of various layers with varying optical properties. In such inhomogeneous tissues, the contribution of each layer within the probed sample volume to the measured absorption coefficient has to be known in order to interpret the measured data correctly. Especially the knowledge of the background absorption coefficient (defined as all contributions to μa that are not due to hemoglobin absorption) is a prerequisite to accurately derive S[O 2] and THC from the measured quantities.12 Absorption in the uppermost epidermal layer is mainly due the chromophore melanin. Its fractional content in the epidermis depends on the skin type.26 In standard pulse oximetry, strong melanin absorption has led to misleading results. In Afro-Caribbean fetuses, for example, it contributes significantly as a background signal to the measured extinction coefficients that ultimately determine S[O 2]. 9

We investigated the influence of the layered skin structure and the contributions from absorption in the individual layers to the measured absorption coefficient using the Monte-Carlo method.38 The optical properties of the tissue layers were obtained from the literature.24 25 26 27 28 29 30 The background absorption coefficients of both layers have been calculated using published data for the absorption coefficients of melanin and unpigmented skin.25 The melanin content in the epidermal layer was varied to simulate different skin types from light to dark colored. The Monte-Carlo simulations showed that the mean penetration depth increases linearly with the separation between the source and detector fiber from approximately 1.2 mm (ρ=2 mm) to 5 mm (ρ=10 mm, Fig. 11). Thus, this technique is definitely capable to detect the oxygen saturation in the dermis at the source-detector separations used here. As can be seen in Fig. 11, no significant dependence of the mean penetration depth from the melanin content of the epidermis can be observed for the employed source-detector separations of 5 and 7 mm. For these source-detector separations, the average value of f epidermis =0.9 was found for the fractional contribution of the epidermis to the overall absorption coefficient at the considered wavelengths (Fig. 12). Thus, epidermal absorption can be neglected in Eq. (12), if μa epidermis (λ) is smaller than or comparable to μa dermis (λ), i.e., for completely unpigmented skin (f mel =0). Under practical conditions, however, the epidermal absorption at 808 nm exceeds the absorption coefficient in the dermis even for light-colored skin (f mel =5) by a factor of 18 and up to approximately 70 for dark-colored skin (f mel =20) (Table 2). In this case, a neglect of the epidermal background contribution would lead to significant deviations of the calculated values for S[O 2] and THC, because the contributions from both skin layers become comparable [i.e., f epidermis μa epidermis ≈(1−f epidermis a dermis in Eq. (12)]. It should also be mentioned that the weighting factor f epidermis depends on the thickness of the epidermis. The thickness was assumed to be 60 μm in the Monte-Carlo simulations, but it can vary in vivo. Nevertheless, by using Eq. (12) in combination with literature data for the melanin content of the epidermis,26 the new method is in principle able to account for the contribution of the epidermis to the absorption coefficient of the skin caused by melanin. Thus, this technique might in the future overcome the limitation of standard pulse oximeters, which do not allow a reliable quantification of the oxygen saturation in the skin of Afro-Carribean fetuses.9

Finally, an in vivo feasibility test was performed using the forearm of a healthy Caucasian volunteer with light-colored skin. We obtained baseline values for the tissue oxygenation of 94 to 95 using source-detector separations of 5 and 7 mm. These baseline values are slightly lower than the value for the oxygen saturation of pure arterial blood, which is commonly reported to be 97 in healthy adults.36 This finding may indicate that mainly arterial capillaries are located in the volume that is probed in this experiment. After occlusion of the upper arm with a blood pressure cuff, the measured oxygen saturation decreased to 80 to 86. These values are close to the reported values of pure venous blood.36

The baseline values of THC were between 200 and 260 μmol/l. The total hemoglobin content decreased to 150 to 180 μmol/l after occlusion of the upper arm indicating a vasocontraction of the dermal blood vessels. After release of the blood pressure cuff, S[O 2] and THC returned to their initial baseline values. Thus, these results show that the new technique is applicable in patient. The calculated data were close to the values to be expected for healthy human subjects.

Another important aspect for the practical application of the proposed method is the temporal resolution. The total acquisition time for a single S[O 2] and THC data point in our setup is approximately 15 seconds. The time is limited by the consecutive readout of the two measurement channels using the magnetic fiber switch. By using an additional APD for the second detector fiber, the temporal resolution can easily be reduced to a few seconds. On the other hand, a temporal resolution of 15 seconds can be considered satisfactory compared to the time intervals required to collect fetal blood samples in clinical practice.

Further work will be directed towards a systematic clinical evaluation including the comparison to blood gas analyzers representing the golden standard of clinical medicine.

6.

Conclusions

In conclusion, we have demonstrated that the modified time-integrated microscopic Beer-Lambert law can be used to absolutely determine the absorption coefficient of tissue phantoms with optical properties similar to those of human neonate skin with varying oxygen saturations at source-detector separations smaller than 10 mm. Using the described technique, we were able to determine S[O 2] and THC in vivo with a temporal resolution of approximately 15 seconds. The proposed method is able to quantitatively account for variations in the background absorption due to different amounts of melanin present in the epidermal skin layer. The technique is well suited for minimally invasive oxygen monitoring where small applicator dimensions and short acquisition time are required (e.g., fetal oxygen monitoring sub partu). The method, however, is still subject to clinical evaluation.

Acknowledgments

This work was supported by the Ministerium fu¨r Bildung, Wissenschaft, Forschung und Technologie (BMBF, Germany) grant No. 13N7067/2.

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©(2003) Society of Photo-Optical Instrumentation Engineers (SPIE)
Stefan Willmann, Albert Terenji, Jens Osterholtz, Joerg Meister, Peter Hering, and Hans-Joachim Schwarzmaier M.D. "Small-volume frequency-domain oximetry: phantom experiments and first in vivo results," Journal of Biomedical Optics 8(4), (1 October 2003). https://doi.org/10.1117/1.1608892
Published: 1 October 2003
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Cited by 6 scholarly publications and 6 patents.
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KEYWORDS
Absorption

Skin

Photons

Oxygen

In vivo imaging

Sensors

Scattering

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