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Enhanced imaging of choroidal vasculature by high-penetration and dual-velocity optical coherence angiography

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Abstract

Dual-beam-scan Doppler optical coherence angiography (DB-OCA) with a 1-μm-wavelength probe is demonstrated for improved in vivo choroidal angiograms of the human eye. This method utilizes two scanning beams with spatial and temporal separation on the retina, and provides two measurable velocity ranges. The method achieves higher sensitivity to very low velocity flows than conventional Doppler optical coherence tomography. Moreover, longer wavelengths allowing greater penetration, enhanced visualization of choroidal vessels is verified with en-face projection images of the Doppler shift squared. Specifically, better choroidal vasculature visibility is achieved at a wavelength of 1 μm than at 840 nm.

©2011 Optical Society of America

1. Introduction

Imaging choroidal vasculature is essential to understanding choroidal vascularization abnormalities of eye pathologies. For example, it has been shown that the severity of age-related macular degeneration (AMD) is characterized by a systematic decrease in foveolar choroidal blood flow [1]. Current standard technique to image choroidal vasculature is indocyanine green angiography (ICGA). ICGA gives qualitative and functional information and may involve patient discomfort since it requires dye injection, which has the potential to induce adverse reactions [2,3]. Laser Doppler flowmetry (LDF) is another method to obtain blood flow in absolute units [4,5]. LDF produces vasculature images but it does not give depth information, that is, it cannot be known whether vessels belong to retina or choroid.

Optical coherence tomography (OCT) [6] is a noninvasive, noncontact imaging technique for micrometer-scale, three-dimensional (3D) retinal tomography. Spectral-domain OCT (SD-OCT) [7] has a better acquisition rate than time-domain OCT. In addition, similar to time-domain OCT [810], in SD-OCT, flow information can be acquired via the Doppler OCT method [1114].

Since the first demonstration of Doppler OCT, various improved versions have been reported. Optical coherence angiography (OCA) [15] is a set of hardware and software methods for enhanced visualization of retinal and choroidal vasculature; OCA includes motion compensation and segmentation algorithms and is based on Doppler OCT [15] and intensity-based segmentation [16,17]. Another method for enhanced visualization of ocular vasculature based on OCT is resonant Doppler Fourier-domain OCT [18], which uses an electro-optical phase modulator to enhance the blood flow contrast with respect to static structures. It has also been proposed a motion contrast technique to image a larger range of velocities [19]. Optical micro-angiography (OMAG) is another angiography method based on OCT that has demonstrated enhanced contrast for retinal perfusion [20]. Ultra-high-speed Doppler SD-OCT was demonstrated using CMOS technology [21]. Single-pass flow imaging spectral-domain OCT [22] and joint spectral- and time-domain OCT [23,24] are other techniques that improve vasculature imaging of the human eye. Lately, it has been reported that a system based on swept-source OCT with multiple detectable velocity ranges can achieve enhanced slow-flow sensitivity [25].

We previously proposed dual-beam-scan Doppler optical coherence angiography (DB-OCA) [26,27] as a method for enhanced vasculature imaging. Note that another group has recently used dual-beam method to obtain vasculature imaging [28]. In general, the ability of Doppler OCT to detect low-velocity vessels diminishes as the acquisition rate increases. DB-OCA avoids this tradeoff by employing two spatially separated probing beams. And it gives access to both high and low velocities without sacrificing the acquisition rate. This makes it possible to detect slow-flow structures with a high-speed acquisition system.

In this paper, we demonstrate highly sensitive and penetrating imaging of choroidal vasculature employing DB-OCA and a 1-μm probe beam, which has recently attracted interest owing to its high penetration into the deep choroid [29,30]. We first discuss the limitations of conventional Doppler SD-OCT, and then briefly present the principle of DB-OCA. A newly developed dual-beam-scan Doppler OCA system employing a 1-μm probe beam is then described. Enhanced contrast imaging of in vivo human choroidal vasculature is demonstrated. Finally, DB-OCA results obtained with an 840-nm probe and 1-μm probe are compared.

2. Principle

2.1. Conventional Doppler OCT and its limitations

In conventional phase-resolved Doppler OCT [11], velocity information for regions within the sample is retrieved by introducing a phase difference between adjacent A-lines. This phase difference Δϕ is related to the axial velocity vz via

vz=λ0Δϕ​​4π ntA,

where λ0 is the source center wavelength, n is the refractive index of the tissue, and tA is the time separation between adjacent A-lines, which is inversely proportional to the charge-coupled device (CCD) acquisition rate. According to the phase sensitivity of OCT and the 2π ambiguity of phase (i.e., π<Δϕπ), the range of detectable velocities is given by [31]

λ0​​4πntA1SNR+σΔx|vz|λ0​​4ntA,

where SNR is the signal-to-noise ratio (SNR), and σΔx is the phase noise arising from decorrelation between adjacent A-lines and is defined as

σΔx=4π3(1exp(12(Δxr)2)),

where r is the beam radius on the sample and Δx is the distance between adjacent A-lines. In general, a high acquisition rate, equivalent to small tA, is required for less sensitivity to motion artifacts. However, according to Eq. (2) with given SNR andσΔx, small tA implies that the velocity range shifts to high velocities. Consequently, slow-flow structures will not be detected. To resolve this issue, we propose DB-OCA [26], whose principle is described in the next section.

2.2. Dual-beam-scan Doppler OCA

Figure 1 illustrates the principle of DB-OCA, where the sample is scanned by two beams, beam-1 and beam-2, having the same scanning speed. Their spatial separation d is thus a constant. This separation d is the product of the scanning step size and an integer p. The time separation is thus T = p.tA, with tA being the acquisition time of a single A-line. Beam-2 is at the same lateral position as beam-1 after the delay T. Therefore, the B-scan obtained with beam-2 is laterally shifted with respect to that obtained with beam-1. Consequently, at a given depth z, the phase of beam-2, φ2(z, t + T), acquired at time t + T is subtracted from the phase φ1(z, t) of beam-1 acquired at time t. Indeed, it corresponds to the phase difference obtained at the same lateral position but acquired at a different moment. The axial velocity of the conventional Doppler equation (Eq. (1)) is therefore rewritten as

 figure: Fig. 1

Fig. 1 Dual-beam-scan Doppler OCA: two beams scan the sample with a constant spatial separation d.

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vz=λ0[ϕ1(z,t)ϕ2(z,t+T)]​​4π nT.

From Eq. (4) and Ref. 31, the velocity range of DB-OCA is then given by

λ0​​4πnT1SNR|vz|λ0​​4nT.

From Eq. (5), we see that this technique using two beams allows the measurement of vessels with low-velocity flow since tA < T. It is noteworthy that this low-velocity sensitivity is achieved without decreasing the acquisition rate. The minimum detectable velocity depends on SNR but not on the spatial separation between adjacent A-lines. Indeed, in DB-OCA, phases that are compared are measured at the same lateral position. Therefore, the flow sensitivity is improved.

In addition, the data processing method of conventional Doppler OCT described in section 2.1 can be applied to the OCT data set obtained for DB-OCA. This additional signal processing gives access to high-velocity flow. Consequently, the combination of DB-OCA and conventional Doppler OCT processing enables simultaneous visualization of low- and high-velocity vessels.

3. Method

In this section, we present the experimental setup of DB-OCA employing a 1-μm probe beam.

3.1. System hardware

The hardware scheme of DB-OCA is shown in Fig. 2 . A broadband superluminescent diode (SLD) light source (Superlum, Ireland) with a center wavelength of 1020 nm and a spectral width (FWHM) of 100 nm was employed. This spectral width results in a measured axial resolution of 6 μm in air. Considering the refractive index of tissue (n = 1.38), the axial resolution in tissue is estimated to be 4.4 μm. The light is transmitted through a single-mode fiber to an isolator. After the isolator, a single-mode fiber delivers the light to a polarization-maintaining (PM) fiber-based coupler (50/50) (General Photonics, CA). A polarization controller is positioned before the PM fiber coupler so that the two polarization channels of the PM fiber have identical power. A variable neutral density filter (VNF) is placed at the reference arm to optimize the sensitivity as close as possible to the shot-noise limit.

 figure: Fig. 2

Fig. 2 Schematic diagram of the dual-beam-scan Doppler OCA setup. VNF: variable neutral density filter. Red lines are polarization-maintaining (PM) fibers. CCD: coupled charge device, PBS: polarization beam splitter.

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The sample arm consists of a specially designed scanning head described in Fig. 3 . In the scanning head, the two orthogonal states of polarization (SOPs) of the PM fiber are separated by a Wollaston prism (Halbo Optics, UK). The two beams with different SOPs are relayed by two achromatic lenses (f = 60 and 75 mm) and deflected by X–Y galvanometers. By means of an achromatic lens (f = 60 mm) and an ophthalmic lens (40D, Volk, Mentor, OH), the beams reach the cornea with different incident angles. The incident power on the cornea is 1.6 mW. The two beams have a spatial separation d on the retina of 162 μm. They are then backscattered by the retina and recombined by the Wollaston prism.

 figure: Fig. 3

Fig. 3 , Scanning head: Two polarization states (red and blue) are separated by a Wollaston prism. After passing through relay lenses and galvanometers, the two polarization states reach the retina with a spatial separation d.

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The probe beams interfere with the reference beam in the fiber coupler. A fiber-based polarizing beam splitter (PBS) (General Photonics, Chino, CA) then separates the two SOPs into two beams and the two beams are directed to different spectrometers, which share an identical design. Each spectrometer consists of a fiber tip collimator, a blazed grating (1200 lp/mm, Thorlabs, NJ), an achromatic lens pair (f = 200 and 150 mm, assembled into a composite lens with f = 88 mm), and a high-speed InGaAs scan camera (1024 pixels, 46.9 kHz line rate, SU1024LDH-1.7RT-0500LC, Sensors Unlimited Inc., Goodrich, NJ). The OCT sensitivities measured with the spectrometers were 96.0 and 95.6 dB. The spectral interference signal is acquired through a Camera Link frame grabber board (PCIe-1430, National Instruments, TX). The data acquisition of both CCD cameras and the scanning of the galvanometers were synchronized via control signals generated by a function generator board (PCI-6713, National Instruments, TX) built into a standard personal computer (PC).

Owing to mismatch of PM fiber lengths between sample and reference arms, there is a difference between optical pathlengths of the two SOPs. This creates an axial displacement between the two OCT signals. This axial displacement is estimated using a static phantom and by numerically shifting the two B-scans in the axial direction. The optimal shift is achieved when the variance of the phase difference between two OCT signals is minimal. Typically, the variance has been computed over a B-scan area containing 100,000 pixels. Note that the variance is the energy of the phase error, and this should take its minimum when the axial displacement is zero. Moreover, to align the two spectrometers, we blocked the sample arm and placed a glass slide in front of the mirror of the reference arm. This configuration is similar to that of a Fizeau interferometer. By doing so and then by minimizing the phase difference for all depths between the two OCT signals of the two polarization channels, we could effectively align the spectrometers.

3.2. Velocity computation

As described in the previous section, two spectra are acquired by the DB-OCA system. Standard SD-OCT processing including rescaling and Fourier transformation yields two complex OCT signals, Γ1(i,j) and Γ2(i,j), where the axial position (depth) is given by the index i and the lateral position (time) by the index j.

3.2.1. Low-velocity images

First, to image low-velocity structures, we compute the phase shift Δϕi,j between the two complex OCT signals at the position (i, j). Using Kasai autocorrelation [32,33], Δϕi,j is defined as

Δϕi,j=Arg[m=0M1n=0N1Γ1(i+m,j+n)Γ2*(i+m,j+n+p)],

where M and N are respectively the axial and lateral window sizes in units of pixels. Here M = 3 and N = 1. The integer p is the lateral shift between the two OCT signals caused by the spatial separation of the two probe beams, and defined byp=T/tA. The Doppler shift ΔfS is then obtained as

ΔfS=12πTΔϕi,j.

In the following, we use the square of the Doppler shift ΔfS2to create en-face low-velocity images.

3.2.2. High-velocity images

To obtain a high-velocity flow image, we first compute the following expression at a given location (i, j):

Γ(i,j)=Γ1(i,j)Γ1*(i,j+1)+Γ2(i,j+p)Γ2*(i,j+p+1).

The phase shift is given by

Δϕi,j=Arg[m=0M1n=0N1Γ(i+m,j+n)],

where M and N are again the axial and lateral window sizes, respectively. Here M = 1 and N = 2. The Doppler shift ΔfF for high velocity is obtained as

ΔfF=12π tAΔϕi,j.

Then, similar to low-velocity images, taking the square of the Doppler shift ΔfF2is used to produce en-face projection high-velocity images.

4. Experiment

4.1. Measurement Protocol

We imaged three 3D volumes of the healthy myopic right eye of an Asian male (25 years old). Three volumes at three locations were acquired: (1) macula, (2) between macula and optic nerve head (ONH), and (3) ONH. A fast-horizontal-scanning protocol with a scanning range of 3.07 mm (horizontal) × 3.07 mm (vertical) was employed. The scanning step size Δx between A-lines was 3.2 μm. The number of A-lines was 950, and the number of B-scans was 256. The two B-scans corresponding to the two beams have the same number of A-lines but are laterally shifted. Therefore only overlapping A-lines are conserved. Non-overlapping A-lines are located at the beginning of the B-scan generated by the following beam and at the end of that generated by the preceding beam. The beam size (1/e2) on the retina was simulated by ray-tracing (Zemax, Bellevue, WA) to be 12 μm, which gave a radius r of 6 μm.

According to the time interval between A-lines (tA) of 22 μs and a typical SNR of 15 dB, Eqs. (2) and (3) give the theoretical velocity range of a high-velocity image as 2.4 mm/s < vz < 8.4 mm/s.

The low-velocity range is calculated using Eq. (5). The separation of the two probe beams d is 162 μm, which corresponds to 50 lines. Therefore, the delay T is 50 × tA = 1.1 ms. With the assumption of a typical SNR of 15 dB, the low-velocity range is estimated to be 0.01 mm/s < vz< 0.17 mm/s.

4.2. Image presentation

The measured Doppler volume is split into retinal and choroidal volumes according to the position of the retinal pigment epithelium (RPE), where the RPE position has been identified from the corresponding OCT volume employing a segmentation algorithm described in Ref. 15. To demonstrate retinal and choroidal OCA, en-face projection (average over retina/choroid thickness) images of the Doppler shift squared (square of Eqs. (7) or (10)) are obtained. ΔfS2 and ΔfF2 are thresholded for display as described in Ref. 26.

As discussed above, DB-OCA gives two Doppler images with different velocity ranges. In the following sections, these two Doppler images are referred to as the high-velocity image (ΔfF2) and low-velocity image (ΔfS2).

4.3. Results

Figure 4 shows mosaics of high-velocity images (Fig. 4a) and low-velocity images (Fig. 4b); each mosaic consists of three patches obtained at the macula, ONH, and their center. Here strong signal (ΔfS2, ΔfF2) is indicated by white color.

 figure: Fig. 4

Fig. 4 Mosaic of high-velocity (a) and low-velocity (b) en-face images of choroidal vasculature. Location: from macula to the ONH. Inverted grayscale. The scale is the same for (a) and (b). See text for details.

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Choroidal vasculature comprises choriocapillaris, mid-sized vessels and large vessels. It can be reasonably assumed that the flow velocity differs for vessels of different sizes. The high-velocity choroidal vasculature image (Fig. 4a) predominantly shows large vessels that can be associated with high-velocity flow. Along a given vessel, ΔfF2 was not continuous (red circles). This discontinuity can be explained by an abrupt change in the axial orientation of the vessel or the existence of pulsatile flow inside the vessels. Note that, although the images presented are choroidal vessels, projections of the signals above the RPE or shadows of retinal vessels are seen (blue arrows).

Figure 4b is a low-velocity choroidal vasculature image. In comparison with the high-velocity image (Fig. 4a), smaller vessels are clearly visualized. Several small vessels are visualized with high contrast, especially around the ONH. Some vessels observed in high-velocity image (Fig. 4a) are not visible in the low-velocity image (Fig. 4b). It may be explained as follows: first, multiple phase wrapping generated by high-velocity flows will randomize Doppler signal and second, low-velocity vessels that were not visible in the high-velocity image will appear in the low-velocity image. Therefore the contrast of the high-velocity vessels is strongly reduced with respect to surrounding environment. Moreover, in order to optimize the display, the image dynamic ranges of Figs. 4(a) and (b) are not identical. Note that shadows (blue arrows) of retinal vessels appear with higher contrast than those in the high-velocity image owing to the higher flow sensitivity. Retinal vessels that are responsible for these shadows are visualized by low-velocity images of the retinal vasculature (Fig. 5 ).

 figure: Fig. 5

Fig. 5 Mosaic of low-velocity en-face images of retinal vasculature obtained fromΔfS2 volumes. Location: from macula to the ONH. Inverted grayscale.

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Strong ΔfS2 can be seen at the ONH (yellow arrows) for low-velocity mosaics (Fig. 4b). It is conjectured that this higher signal may not be due to strong blood flow but an artifact of ocular birefringence. The sclera, which is known to have strong birefringence, is closer to the retinal surface in this region. Since DB-OCA uses polarization to multiplex two probe beams, the scleral birefringence results in cross-talk between the two probe beams. This cross-talk generates the strong artifact. The artifact can be reduced if circularly polarized incident light is used instead of linearly polarized light [34] as has been demonstrated with an 840-nm probe beam [27].

In Fig. 6 , a composite mosaic is realized by choosing a color depending on velocity and depth (retina/choroid). Low-velocity retinal vasculature is represented in red color. High-velocity choroidal vasculature is indicated in green color and low-velocity choroidal vasculature corresponds to inverted grayscale. An arbitrary threshold has been applied on low-velocity retinal and high-velocity choroidal vasculatures to enhance visualization. Note that the vasculature corresponding to the conventional Doppler (high-velocity) of the retina was hardly visible and is therefore not used here. The depth information given by DB-OCA enables to establish if vessels are really connected or simply overlaid. DB-OCA can thus distinguish vessels belonging to well-separated layers such as retina and choroid. As previously observed, one limitation of the Doppler SD-OCT technique is the shadow artifact which is due to phase decorrelation below vessels. In B-scan or 3D representations, it can hinder visualization of vessels located below shallower vessels. Note also that in the case of pathological eyes, leakage cannot be directly detected by DB-OCA. Nevertheless, we have seen that 1-μm DB-OCA can provide complementary information about deep vasculature in a non-invasive and non-contact manner that is not available by conventional Doppler OCT.

 figure: Fig. 6

Fig. 6 Composite mosaic of low-velocity and high-velocity en-face images of retinal andchoroidal vasculature. Location: from macula to optic nerve head. Choroid low-velocity vasculature (inverted grayscale), choroid high-velocity vasculature (green), low-velocity retinal vasculature (red).

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5. Discussion: Comparison of 840-nm and 1-μm DB-OCA

To evaluate the advantage of 1-μm DB-OCA, the low-velocity choroidal images of 840-nm and 1-μm DB-OCA are qualitatively compared. An 840-nm DB-OCA system described in Ref. 26 was employed for this comparison. Briefly, the light source was a superluminescent diode (SLD-37-HP, Superlum Diodes Ltd., Ireland) with 840-nm central wavelength and 50-nm bandwidth (full-width at half-maximum). The scanning head was identical to that of 1-μm DB-OCT system. The power on the cornea was 750 μW.

In the 840-nm DB-OCA, the spectral interference signals were acquired by a polarization diversity spectrometer [35], with a polarization beam splitter splitting the two polarization modes after a diffraction grating. Finally, two line-scan cameras (2048 pixels, 27.8 kHz; AViiVA M2 CL 2014, e2V, Atmel, CA) detected the two polarization modes. The sensitivity was measured to be 94 dB and 93 dB for the two channels.

The 840-nm DB-OCA was configured to have the same maximum velocity as for the 1-μm DB-OCA. In this configuration, the temporal separation of the two probing beams was 0.905 ms. The reason why we selected a smaller temporal separation is to compensate for wavelength difference. From Eq. (5) and assuming similar refractive index for both wavelengths, we see that, in order to have the same velocity range and thus the same flow sensitivity, we need 840 nm/T 840 = 1020 nm/T 1020, where T 840 and T 1020 are the delay between beams for corresponding wavelengths. Since T 1020 = 1.1 ms, T 840 = 0.905 ms. The lateral spatial separation of the retina was 170 μm, and the lateral separation in the image was 24 pixels. Hence, the scanning speed of the galvanometer scanner was configured to have a scanning step size of 7.07 μm between successive A-lines. Since a B-scan is configured to have 440 A-lines, the lateral scanning range was 3.10 mm. This is nearly identical to that of 1-μm DB-OCA of 3.07 mm.

Figure 7 shows en-face projection images of ΔfS2 volumes obtained by 840-nm DB-OCA (a) and 1-μm DB-OCA (b). Here the projections were obtained by averaging ΔfS2 signals through the whole depth including retina and choroid. The contrast of choroidal vessels in the 1-μm image is significantly higher than that in the 840-nm image. Furthermore, small choroidal vessels are better distinguished in the 1-μm image than in the 840-nm image. The superior performance of 1-μm DB-OCA is particularly evident in the region indicated by the yellow boxes. Since both systems were configured to have identical velocity range, this superior contrast is mainly attributable to the superior penetration of the 1-μm probe beam.

 figure: Fig. 7

Fig. 7 En-face ΔfS2 projection image of ONH for (a) 840-nm and (b) 1020-nm light sources. Yellow boxes are zoomed areas. Inverted grayscale.

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6. Conclusion

We have demonstrated that 1-μm DB-OCA was particularly valuable for high-contrast imaging of choroidal vasculature. DB-OCA provided two angiograms that had different velocity ranges. High-velocity information was obtained with conventional phase- resolved Doppler method and low-velocity information was retrieved by using the phase difference between the two scanning beams. The low-velocity angiogram was found to have high flow sensitivity and to be undoubtedly useful for the visualization of small choroidal vessels. On the other hand, the high-velocity angiogram is important for the visualization of large choroidal vessels. The combination of the low- and high-velocity angiograms provides a more complete visualization of choroidal vasculature. An in vivo qualitative comparison of 840-nm and 1-μm DB-OCAs showed that 1-μm DB-OCA visualized the choroidal vessels with higher contrast. This non-invasive angiography may facilitate understanding and diagnosis of choroidal pathologies.

Acknowledgment

This study was partially supported by the Japan Science and Technology Agency through a contract for the Development of Systems and Technology for Advanced Measurement and Analysis.

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Figures (7)

Fig. 1
Fig. 1 Dual-beam-scan Doppler OCA: two beams scan the sample with a constant spatial separation d.
Fig. 2
Fig. 2 Schematic diagram of the dual-beam-scan Doppler OCA setup. VNF: variable neutral density filter. Red lines are polarization-maintaining (PM) fibers. CCD: coupled charge device, PBS: polarization beam splitter.
Fig. 3
Fig. 3 , Scanning head: Two polarization states (red and blue) are separated by a Wollaston prism. After passing through relay lenses and galvanometers, the two polarization states reach the retina with a spatial separation d.
Fig. 4
Fig. 4 Mosaic of high-velocity (a) and low-velocity (b) en-face images of choroidal vasculature. Location: from macula to the ONH. Inverted grayscale. The scale is the same for (a) and (b). See text for details.
Fig. 5
Fig. 5 Mosaic of low-velocity en-face images of retinal vasculature obtained from Δ f S 2 volumes. Location: from macula to the ONH. Inverted grayscale.
Fig. 6
Fig. 6 Composite mosaic of low-velocity and high-velocity en-face images of retinal andchoroidal vasculature. Location: from macula to optic nerve head. Choroid low-velocity vasculature (inverted grayscale), choroid high-velocity vasculature (green), low-velocity retinal vasculature (red).
Fig. 7
Fig. 7 En-face Δ f S 2 projection image of ONH for (a) 840-nm and (b) 1020-nm light sources. Yellow boxes are zoomed areas. Inverted grayscale.

Equations (10)

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v z = λ 0 Δ ϕ ​​ 4 π  n t A ,
λ 0 ​​ 4 π n t A 1 S N R + σ Δ x | v z | λ 0 ​​ 4 n t A ,
σ Δ x = 4 π 3 ( 1 exp ( 1 2 ( Δ x r ) 2 ) ) ,
v z = λ 0 [ ϕ 1 ( z , t ) ϕ 2 ( z , t + T ) ] ​​ 4 π  n T .
λ 0 ​​ 4 π n T 1 S N R | v z | λ 0 ​​ 4 n T .
Δ ϕ i , j = A r g [ m = 0 M 1 n = 0 N 1 Γ 1 ( i + m , j + n ) Γ 2 * ( i + m , j + n + p ) ] ,
Δ f S = 1 2 π T Δ ϕ i , j .
Γ ( i , j ) = Γ 1 ( i , j ) Γ 1 * ( i , j + 1 ) + Γ 2 ( i , j + p ) Γ 2 * ( i , j + p + 1 ) .
Δ ϕ i , j = A r g [ m = 0 M 1 n = 0 N 1 Γ ( i + m , j + n ) ] ,
Δ f F = 1 2 π  t A Δ ϕ i , j .
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