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Study of Fiber Coupling Efficiency and Adaptive Optics Correction Technique in Atmospheric Slant-Range Channels

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25 September 2023

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27 September 2023

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Abstract
Fiber coupling efficiency is one of the key technical indicators of atmospheric laser communication, which directly affects the communication system BER. According to the optical fiber coupling efficiency model, the optical fiber coupling model under atmospheric slant link is established, and the relationship between wavelength, zenith angle, receiving aperture, altitude and coupling efficiency is studied through numerical simulation. Based on the principle of adaptive optics turbulence correction, the relationship between fiber coupling efficiency and adaptive optics order is established. A fast method for estimating the coupling efficiency based on Strehl ratio is proposed. According to the principle of laser communication system, the semi-physical simulation experimental system of atmospheric slant-range channel coupling efficiency is constructed, and the coupling efficiency test and analysis are completed.
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Subject: Engineering  -   Other

1. Introduction

Laser communication technology has the advantages of wide bandwidth, large capacity, compact terminal structure, low power consumption, anti-eavesdropping, and anti-jamming [1], and has been gradually applied to military defense [2,3] civilian emergency communication [4] satellite communication [5,6,7] and deep space exploration [8,9,10] and many other fields have become new research hotspots in the field of communication . However, when the laser communication link is transmitted through the atmosphere, due to the presence of atmospheric turbulence effect leads to serious interference with the communication performance and stability of laser communication [11,12]. The coupling efficiency problem under atmospheric turbulence interference constrains the application of laser communication in the atmosphere. Coupling efficiency is a key factor in determining the final communication quality of atmospheric laser links. The laser beam must therefore be coupled into a single-mode fiber in order to use single-mode fiber-based fiber amplifiers under atmospheric turbulence and also to be connected to ground fiber optic networks [13]. In coherent optical systems, single-mode fiber coupling is also required. For free-space optical communications through atmospheric turbulence in the horizontal case, a theoretical description of the fiber coupling efficiency has been developed. Several techniques have been proposed to improve the coupling efficiency, such as coherent fiber array reception, adjusting the focus of the coupling system, adaptive optics (AO), and so on. The most common of these is the AO, which measures wavefront aberrations caused by turbulence.
In this paper, the fiber coupling efficiency model under horizontal transmission path is extended to the coupling efficiency model under inclined transmission path. Simulations are performed to analyze the coupling efficiency with respect to wavelength, zenith angle, receiving aperture and height above ground. In order to solve the problem of fiber coupling efficiency in the atmospheric slant-range channel, an adaptive optical system and a precision tracking system are used to improve the coupling efficiency, and the relationship between the coupling efficiency and the Strehl ratio (SR) is studied. A semi-physical simulation experiment system of atmospheric slant-range channel coupling efficiency was built to complete the coupling efficiency test and analysis.

2. Fiber coupling efficiency in slant atmospheric transmission path

In the star-ground link, the path of space optical coupling to SFM is shown in Figure 1. Under the influence of atmospheric turbulence, spatial light passes through the ideal receiving antenna without aberration and converges to the back focus surface to form an Airy spot. Optical energy is coupled into a single-mode fiber core placed in the focal plane position.
The theory of the fiber coupling efficiency for horizontal laser communications is defined as the ratio of the average power coupling into the fiber P c to the average power in the receiver aperture plane P a and is given by[14]
η = P c P c = A U i r U m * r d r 2 A U i r d r 2
Where U i r is the incident optical field at the receiver aperture plane and U m r the mode field distribution of the normalized single-mode fiber. For plane waves and Kolmogorov power law spectra, the coupling efficiency of a single-mode fiber after atmospheric turbulence is generally expressed by the following equation [15]
η = 8 a 2 0 1 0 1 exp a 2 + A R A C x 1 2 + x 2 2 × B 0 2 A R A C x 1 x 2 x 1 x 2 d x 1 d x 2
Where   A R = π D 2 / 4 is the area of the receiver aperture, D the receiver lens diameter. A C = π ρ c 2 is the spatial coherence area of the incident plane wave, ρ c = 1.46 C n 2 k 2 L 3 / 5 is the spatial coherence radius of horizontal path, C n 2 the atmospheric refractive index structure, k = 2 π / λ is the number of light waves, the unit is rad /m, λ is the wavelength. The ratio A R / A C enotes the number of speckles over the receiver aperture area. a = D / 2 π ω 0 / λ f is the ratio of the receiver lens radius to the radius of the backpropagated fiber mode. B 0 is zero order Bessel function.
The optimum value of the coupling-geometry parameter a that maximizes the coupling efficiency depends on the value of the number of speckles A R / A C . In the absence of turbulence, the incident plane wave is fully coherent and the optimum value of a is 1.12. It has been shown that if the lens focal length is chosen to satisfy a =1.12, corresponding to the optimum a value for a fully coherent incident plane wave, the coupling efficiency obtained for other values of A R / A C is not appreciably less than the maximum coupling efficiency that can be obtained by optimizing a [15]. Therefore we use a =1.12 in the rest of the calculation. So coupling efficiency depends only on the spatial coherence radius. Developed and expanded to slant atmospheric transmission path on spatial coherence radius by using Eq.(3),(4) and (5). Equation (3) represents the Hufnagel-Vally (H-V) model of the refractive index structure constant of the atmosphere under slope link.
C n 2 h = 0.00594 V R M S 27 2 h 10 5 2 × exp h 1000 + 2.7 × 10 16 exp h 1500 C n 2 0 exp h 100
C n 2 0 = 1.7 × 10 14 m 2 / 3 is the structure constant on ground, which are typical values for clear sky and weak turbulence conditions. v R M S is the wind velocity, which can be calculated using the Bufton wind model[16]:
V R M S = 1 15000 5000 20000 3 + 30 × e x p h 9400 4800 2 2 d h 1 / 2
The spatial coherence radius for slant atmospheric transmission path is calculated by(5)
V R M S = 1.46 k 2 sec ξ h 0 h C n 2 h d h 3 / 5
Where, h 0 is the height above the ground, ξ is the zenith angle. In addition, the relation between spatial coherence and Fried parameter   r 0 will be used in the subsequent sections and it is expressed by ρ c = r 0 / 2.1 .
It can be obtained from the above analysis coupling efficiency is the function of wavelength,receiver aperture ,height above the ground, and zenith angle. According to the parameters in Table 1 the coupling efficiency in slant atmospheric transmission path was studied.
Figure 2 shows coupling efficiency as a function of the height above ground for D=10cm to 30cm. As can be seen from the result, the larger aperture than speckle patterns degrades the fiber coupling efficiency drastically; Therefore, to obtain higher fiber coupling efficiency, the aperture size corresponding to the atmospheric coherence size must be checked and correctly selected. On the other hand, the received power will be decreased when the mirror size is small. At the aperture greater than 30mm the coupling efficiency decreases quickly, and the height above the ground greater than 500m it grows slowly.
Figure 3 shows the coupling efficiency as a function of the height above ground for ξ =0°,18°,30°,60°. The efficiency is degraded to less than 22% when ξ change from 0°to 60°at h0=500m.
Figure 4 shows the coupling efficiency as a function of the height above ground for λ =850nm, 1064nm, 1330nm, 1550nm. Long wavelengths are beneficial for improving coupling efficiency. At the height above the ground greater than 500m the coupling efficiency grows slowly.

3. AO correction for coupling efficiency

According to AO correction the coupling efficiency is improved by increasing the spatial coherence radius. For simplicity, here we restrict the attention to the case of modal AO correction by totally removing some Zernike aberration modes, the temporal response of AO system is not investigated, and it is assumed that the control bandwidth is unlimited.

3.1. Relationship between coupling efficiency and AO correction

In order to characterize the spatial variation of a wavefront in turbulence in a given time, zernike polynomials are used with a set of basis functions. According to Noll definition, a wavefront aberrations can be written as [17]
φ r , θ = i = 1 a i Z i r , θ
Where a i are coefficients of corresponding Zernike polynomials Z i . The effect of modal correction is that some of the decomposition coefficients vanish. When the first j Zernike terms have been corrected, the residual distortion in wavefront may be estimated with Noll expression for the average variance [17]
Δ j = i = j + 1 a i 2 = c o e f ( j ) ( D r 0 ) 5 / 3
Where 〈 〉 denotes an ensemble average, c o e f j is the corresponding coefficient given by Noll for the correction degree j , and c o e f ( j ) 0.2944 j 3 / 2 .
Similarly, a generalized Fired parameter ρ 0 is defined after a modal AO correction, which is the function of r 0 and j , given by[18]
ρ 0 = 0.286 ( 3.44 c o e f ( j ) ) 3 / 5 j 0.362 r 0
It is obvious from Equation(8)when spatial coherence length and spatial coherence area are increased the coupling efficiency will be increased. The simulation with different correction degree is shown in Figure 5.
Figure 5 shows the coupling efficiency as a function of the height above ground for j=3, 10, 20, 40, 80. Compared with Figure 1 the coupling efficiency is improved with AO system. When the correction degree is doubled the coupling efficiency is increased by approximately 5% at the height above ground greater than 500m.
For typical laser communication system the fine tracking system is necessary to keep in alignment between signal and detector. At the same time,when working in the atmosphere, the use of a fine tracking system eliminates the lower order terms of turbulent disturbances (j=3).

3.2. Relationship between coupling efficiency and SR

The SR is typical evaluation index to AO system, which is defined as the ratio of peak power in the center of the image plane compared to that of an equivalent unaberrated system.
S R = I I 0
where I is the imaging intensity of the focal spot on the optical axis, I 0 is the light intensity at diffraction limit. Under general conditions, not limited to weak fluctuations, the SR can be approximated by the expression [19,20]
S R = 1 + ( D / r 0 ) 5 / 3 6 / 5
Using the relation D / r 0 and A R / A C the Equation 11 can be rewritten as
A R A C = 1.1025 S R 5 / 6 1 6 / 5
Substituting Equation 12 into Equation 2 the relationship between coupling efficiency and SR can be derived, and the simulation is shown in Figure 6. The coupling efficiency can be estimated by SR. Particularly when the SR is between 0.1 and 0.9 the coupling efficiency is approximately η S R 0.1 .

4. Semi-physical simulation experiment system.

4.1. Principle of system composition

The semi-physical simulation experimental system of slant-range channel coupling efficiency consists of three parts: the transmitter side, the receiver side, and the slant-range link simulation. The slant link simulation is realized through a liquid crystal phase screen, which can simulate the intensity of turbulence, spatiotemporal distribution, etc. The receiving end is composed of a laser communication receiving optical system, a precision tracking system, an adaptive optical system, etc. The FSM, CCD is controlled as a closed loop, constituting a fine tracking system to eliminate the lower order terms of turbulence and adjust the laser beam so that it is controlled at the center of the CCD. DM, Hartmann sensor to form a closed-loop control, correct the wavefront aberration, suppress turbulence, the corrected beam coupled to a single-mode fiber and measured the received optical power. According to different parameter settings can be completed with different slant range, star-ground and other link coupling efficiency experimental testing. The basic principle is shown in Figure 7.
Among them, turbulence simulation is implemented in the following ways
Figure 8. slant path phase screen.
Figure 8. slant path phase screen.
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4.2. Simulation experiment results

The parameters of the simulation system were set as follows: receiving optical aperture of 30 cm, conditions for the setup of the slant link (height above ground of 100 m, zenith angle of 30°, wavelength of 1550 nm, and turbulence intensity in the range of 1.2 × 10 16 ~ 1.2 × 10 13 ). The number of fine tracking and adaptive optics correction higher order terms is j=40 and the test results are as follows. The coupling efficiency after fine tracking optical system is given in Figure 9a and after adaptive optics in (b)
From Figure 9a,b, it can be seen that
In the semi-physical simulation experimental system of the coupling efficiency of the slant-range channel, the mean value of the coupling efficiency is only about 2% when only the fine tracking system is available, and the mean value of the coupling efficiency is improved to about 7% when adaptive optics is added, which is basically in line with the results of the numerical simulation as mentioned before. At the same time, the Strel ratio of the receiving spot was tested, and the sr was 0.12 without adaptive optics system and 0.19 with adaptive optics. A preliminary fast analysis of the system coupling efficiency can be realized with SR. It can be seen that AO can improve the coupling efficiency in the turbulent environment to a certain extent, but due to the influence of altitude, the coupling efficiency improvement is limited, and it needs to cooperate with the appropriate altitude to achieve higher coupling efficiency.

5. Conclusion

In this study, the fiber coupling efficiency model for horizontal transmission paths is extended to inclined star-ground laser links. The function between coupling efficiency and wavelength, zenith angle, receiving aperture and altitude is established, and the coupling efficiency is quickly estimated by SR.
Build a coupling efficiency semi-physical simulation experimental system to complete the coupling efficiency test under different parameters in different environments.
Simulation and experimental results show that the fiber coupling efficiency in the star-ground laser links link is affected by atmospheric turbulence, test environment, test location, test conditions and other factors. At low altitudes, adaptive optics alone has limited coupling efficiency improvement, and it needs to be coordinated with ground station selection to achieve the best results

Author Contributions

xiaoying.Ding.; writing-original draft, xin.Zhao.; funding acquisition, tong.Wang.; data curation, xiaoyun.Wu., shu.Chen. and dewang.Liu.; investigation,

Funding

This study was being funded by the key technology and development projects of Jilin Science and Technology Department of China (NO.20180201002SF).

Institutional Review Board Statement

Not applicable.

Informed Consent Statement

Not applicable.

Data Availability Statements

Data cannot be provided, owing to data security reasons.

Conflicts of Interest

The authors no conflict of interest.

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Figure 1. Schematic diagram of spatial optical to single-mode fiber coupling under atmospheric turbulence.
Figure 1. Schematic diagram of spatial optical to single-mode fiber coupling under atmospheric turbulence.
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Figure 2. Coupling efficiency as a function of the height above ground for D=10cm to 30cm. where ξ =30°, λ   λ =1550nm.
Figure 2. Coupling efficiency as a function of the height above ground for D=10cm to 30cm. where ξ =30°, λ   λ =1550nm.
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Figure 3. Coupling efficiency as a function of the height above ground for ξ =0°,18°,30°,60°. where D=30cm, λ =1550nm
Figure 3. Coupling efficiency as a function of the height above ground for ξ =0°,18°,30°,60°. where D=30cm, λ =1550nm
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Figure 4. Coupling efficiency as a function of the height above ground for λ =850nm, 1064nm, 1330nm, 1550nm. where D=30mm, ξ =30°.
Figure 4. Coupling efficiency as a function of the height above ground for λ =850nm, 1064nm, 1330nm, 1550nm. where D=30mm, ξ =30°.
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Figure 5. Coupling efficiency as a function of the height above ground for j=3,10,20,40,80. where D=30cm, ξ =30°, λ =1550nm
Figure 5. Coupling efficiency as a function of the height above ground for j=3,10,20,40,80. where D=30cm, ξ =30°, λ =1550nm
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Figure 6. Relationship between coupling efficiency and SR.
Figure 6. Relationship between coupling efficiency and SR.
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Figure 7. Simulation experiment system .
Figure 7. Simulation experiment system .
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Figure 9. a) Coupling efficiency results after fine-tracking the optical system (b) Coupling efficiency results after adaptive optics system.
Figure 9. a) Coupling efficiency results after fine-tracking the optical system (b) Coupling efficiency results after adaptive optics system.
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Table 1. Parameter used in coupling efficiency analysis.
Table 1. Parameter used in coupling efficiency analysis.
parameter value unit
1 λ 850,1064,1330,1550 nm
2 D 10-30 cm
3 h 20000 m
4 h 0 0-3000 m
5 ξ 0,18,30,60 °
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