Polarization Properties of Quasi-Homogeneous Beams Propagating in Oceanic Turbulence
Polarization Properties of Quasi-Homogeneous Beams Propagating in Oceanic Turbulence
Journal of the Optical Society of Korea. 2013. Apr, 17(2): 130-135
Copyright ©2013, Optical Society of Korea
  • Received : February 02, 2013
  • Accepted : April 04, 2013
  • Published : April 25, 2013
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Feinan Chen
Qi Zhao
Yanru Chen
Jingjing Chen
Based on the extended Huygens-Fresnel principle and generalized Stokes theory, the evolution of polarization properties of beams generated by quasi-homogenous (QH) sources propagating in clear oceanic water was studied by the use of the oceanic turbulence spatial spectrum function. The results show that the beams have similar polarization self-reconstructed behavior under different turbulence conditions in the far field, but if the propagation distance is not long enough, the degree of polarization (DOP) fluctuates with much more complexity than state of polarization (SOP) of QH beams. The self-reconstructed ability of DOP at the special distance in turbulence would get to the best value if the values of coherence of width were chosen suitably, but for SOP, it has no best value.
The QH beams which can be generated by SLMs have been studied and used widely in recent years [1] . The coherence and polarization properties of quasi-homogenous sources in the far field has been studied by Korotokva [2] . The coherence of properties of the field generated by a beam radiated from a quasi-homogenous electromagnetic source scattering on QH media has been studied by Xin [3] . Chen and Li have been researched the coherence properties and polarization modulation of QH beams scattered from anisotropic media [4 - 5] . The propagation properties of laser beams in random media like turbulence or human tissue are important for applications such as optical imaging, remote sensing and communication systems so more and more researchers are attracted [6 - 11] . The polarization “self-reconstructed” phenomenon in atmosphere turbulence has been known for a long time. The normalized spectrum of the beam generated by QH source after propagating through turbulent media has been proved to be equal to the normalized spectrum of the source [12] . The degree of polarization of electromagnetic Gaussian-Schell beams and partially coherent electromagnetic flat-topped beams also have self-reconstructed properties in atmospheric turbulence [13 - 14] . However, recent reports have shown that beams generated from anisotropic sources don’t have polarization self-reconstructed properties in turbulent media [15 - 16] . On the other hand, oceanic turbulence is an important natural random medium but the light propagation though oceanic turbulence is a relatively unexplored topic compared to that in other media. The spatial spectrum model of oceanic turbulence combining temperature and salinity fluctuations is only used by a few articles to study the light propagation in the oceanic waters [16 - 18] .
In this paper, we focused on the polarization features of QH beams propagating through oceanic turbulence. The analytical expressions of on-axis generalized Stokes parameters of QH beams were calculated,then the variations of DOP and SOP of QH beams traveling through oceanic turbulence have been simulated. The self-reconstructed properties of such beams in the far field in turbulent media have been analyzed under different source parameters and turbulence conditions.
For beams generated by quasi-homogenous (QH) sources the spectral density S (0) ( r ) varies much more slowly with position vector than the correlation coefficients μij (0) ( r , ω ) change with difference of position vector r1 - r2 . The cross spectral density matrix of QH sources can be expressed as:
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The superscript (0) denotes quantity pertaining to the incident field. The spectral density can be expressed as the trace of cross spectral density matrix:
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( r1 , r2 , ω ), aij ( ω ) is the frequency dependent factor which connects the spectral components: Sy (0) ( ω )= α ( ω ) Sχ (0) ( ω ).
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For α =0, the source generated linearly polarized light in the x direction, for α →∞, the light is linearly polarized in the y direction. Without loss of generality, the spectral density and correlation coefficients can be described by the Gaussian-Schell model:
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A is spectral amplitude which we set A =1 in this article, and Bij is called the coefficient of correlation between the incident field components, for quasi-homogenous beams, it can be set as: Bxx = Byy =1, Bxy = B*yx , where the asterisk means complex conjugate. σ represents the width of the source, δij represents the coherent width of the source. Several conditions of the source must be satisfied in order to produce a physically reliable QH beam [19] .
The cross spectral density matrix of the beam at the receiving plane can be derived by the extended Huygens- Fresnel principle:
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Where r1 , r2 are two arbitrary position vectors of points on the source plane while ρ1 , ρ2 are two position vectors of observation points on the receiving plane. z is propagation distance and
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is the wave number of the beam. The last term in Eq. (5) represents the correlation function of the complex phase perturbed by random media:
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describes the strength of turbulence perturbation.
The model of the spatial power spectrum of refractive index fluctuations of homogenous and isotropic oceanic turbulence can be described as a linearly polynomial of temperature fluctuations and salinity fluctuations:
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In Eq. (7), ξ is the rate of dissipation of kinetic energy per unit mass of fluid, ranging from 10 -4 m 2 s -3 in turbulence surface layer to 10 -10 m 2 s -3 in the mid-water column. χT is the rate of dissipation of mean squared temperature ranges from 10 -2 K 2 s -1 below the oceanic turbulence to 10 -10 K 2 s -1 at the mid-water column. η is the Kolmogorov micro scale. Other parameters in Eq. (7) are:
AT = 1.863×10 -2 , AS = 1.9×10 -4 , ATS =9.41×10 -3 , δ = 8.284( κη ) 4/3 + 12.978( κη ) 2 ; w defines the ratio of temperature to salinity contributions to refractive index spectrum which in oceanic waters varies in the interval [-5;0], with -5 and 0 corresponding to dominating temperature-induced and salinityinduced optical turbulence, respectively.
From Eq. (3)-Eq. (6), the cross spectral density matrix of the electromagnetic field on the receiving plane can be expressed as:
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As a matter of convenience, we make changes of the spatial arguments:
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With the help of Eq. (9), the cross spectral density matrix on the receiving plane is derived:
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The polarization properties of an electromagnetic beam at a point in space can be determined by use of Stokes parameters which have recently been generalized from one-point quantities to two-point counterparts [20] . They contain not only polarization properties but also coherence properties of beams [21] and can be measured by Young’s interference experiment [22 - 23] . The changes of generalized Stokes parameters in optical system or random media are also interesting problems and have received a lot of attention [24 - 25] . The four parameters can be expressed as follows:
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are Pauli spin matrices:
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represents the cross-spectral density matrix (CSDM) of the beam:
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If we only considered polarization properties of one point, i.e., ρ 1 = ρ 2 = ρ , From Eq. (10), each element of the CSDM can be derived as the expression of:
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Inserting Eq. (11) into Eq. (12), and using the conditions of Mxy = Myx , αxy = αyx the analytical expressions of four Stokes parameters can be obtained:
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The polarization properties can be expressed as the functions of these four parameters.
We considered the degree of polarization and the state of polarization of QH beams in this paper. DOP is used to describe the polarized portion of a beam. DOP=1 means perfectly polarized beam while DOP=0 means unpolarized beam. The state of polarization (SOP) includes the azimuth angle and ellipticity. The azimuth angle θ is defined by the smallest angle formed by the positive x-direction and the direction of major semi-axis of the ellipse. ε , which determines the shape of the ellipse, is the ratio of the major semi-axis and the minor semi-axis.
For convenient, we normalized three Stokes parameters by S 0 as:
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The DOP and SOP can be expressed as the function of normalized Stokes parameters:
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Because of the uniform polarization properties of quasihomogenous beams, we only need to consider the on-axis point of the beam. And in order to prove the polarization self-reconstructed properties of QH beam, we should study far-field polarization properties of normalized Stokes parameters. First, let’s consider the limit as follow:
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Where si (0, z , ω ) are normalized Stokes parameters on the receiving plane while si (0, 0, ω ) are such parameters on the source plane. From Eq. (13),
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can be obtained from Eq. (1) - Eq. (4). Then substituting into the limit of the ratio of two parameters, we get:
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In turbulent medium,
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so F =1, then we proved the self-reconstructed property of s 1 . Other parameters in Eq. (14) can also be proved similarly, then DOP and SOP self-reconstructed properties can be derived directly. We set follow parameters to judge the ability of the self -reconstructed property of QH beams:
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Variations of turbulence strength due to temperature and salinity fluctuations. (The parameters in Fig. 1 are : (a) χT=10-9 K2(1/s)~10-10K2(1/s), ξ =10-4m2(1/s)3~,10-5m2(1/s)3, w=1.5, -2.5, -3.5, (b) χT=10-2K2(1/s)~10-10K2(1/s), ξ =10-4m2(1/s)3~,10-10m2(1/s)3, w=1.5.)
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Variations of on-axis generalized normalized Stokes parameters versus propagation distance z at different α : (a) α =0.5, (b) α =1, (c) α =1.5. Other parameters are λ =0.6328 μm, σ =1 cm, Bxy=0.25exp(-iπ/6), Byx=0.25exp(-iπ/6), δyy=2δxyδxx=1.5δxy, δxy=0.2 mm.
These parameters are modulus values of relative difference of the on-axis DOP and SOP between the source plane and the receiving plane at a special distance z in turbulences, the self-reconstructed ability will be better when these values get closer to 0.
Figure 1 shows the strength of oceanic turbulence changes with turbulence parameters: w, χT and ξ . It can be easily found out that the strength of turbulence T increases with the increase of χT and w, but reduces with the increases of ξ .
Figure 2 shows the changes of normalized Stokes parameters with distance at different a. The DOP and SOP we calculated in Eq. (17) and Eq. (19) could be expressed as the function of these parameters, so the behavior of generalized Stokes parameters decides the evolution of DOP and SOP of the beam through propagation.
In Fig. 3 , we illustrated how the DOP and SOP of the QH beams depend on the parameters of oceanic turbulence. The effect of w on the changes of DOP and SOP has been shown in Fig. 3 (a1)-(a3) and the effect of χT and ξ has been shown in Fig. 3 (b1)-(b3).
In Fig. 4 , the influence of coherent width and the coefficients αij ( ω ) on the changes of self-reconstructed properties of DOP of QH beams were revealed. While δyy and δxx are kept fixed, c 0 is the coefficient to decide the value of δxx as the form δxx = c 0 δxy .
In Fig. 5 , the self-reconstructed behavior of azimuth angle θ and the degree of ellipticity ε were judged as the same method of DOP we plotted their variation versus c 0 .
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Variations of the on-axis DOP and SOP versus propagation distance z under different turbulence conditions. a1, b1 are the changes of DOP, b1, b2 are the changes of θ, c1,c2 are the changes of ε. We set α =1, and other parameters are same with Fig. 2. The parameters of oceanic turbulence are set as (a1, b1, c1) χt =10-6K2(1/s), ξ =10-8 m2(1/s)3. solid curve: w=-1.5, dashed curve: w=-2.5, dot-dashed curve: w=-3.5. (a2, b2, c2) w=-1.5. solid curve: χt =10-6K2(1/s), ξ =10-8 m2(1/s)3, dashed curve: χt =10-7K2(1/s), ξ =10-8 m2(1/s)3, dot-dashed curve: χt =10-7K2(1/s), ξ =10-9 m2(1/s)3.
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Variations of Pd with c0 on the receiving plane at the propagation distance z=10 km under different α. c0 is the ratio of δxx to δxy. Other parameters are same with Fig. 2. δxy=0.2 mm, δxx=c0δxy, (a) σ =1 cm, δyy=0.5δxy, (b) σ =1 cm, δyyxy.
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Variations of εd and θd with c0 on the receiving plane at the propagation distance z=10 km under different α (a) σ =1 cm, δyy=0.5δxy, (b) σ =1 cm, δyy=0.5δxy. Other parameters are same with Fig. 2.
(1) Both DOP and SOP fluctuate at the range of 0.01 km1 km. DOP and SOP get more fluctuations in weak turbulence and get larger self-reconstructed distance than that in strong turbulence.
(2) S 2 and S 3 in ocean waters fluctuate less than S 1 during the propagation but they will all reach the initial value if the propagation distance is long enough.
(3) DOP varies with more complexity with distance in ocean waters than SOP. The self-reconstructed distance of both decreases with the increase of χt and w, but increases with the increases of ξ .
(4) When δyy = δxy , Pd reaches the minimum value, and it’s almost equivalent for different α ,but if δxx δxy , as what have shown in Fig. 4 (b), Pd will get to minimum value at different c 0 for different α .
(5) ε d and θ d increase as increases but will change slowly when c 0 >1. It means when other parameters are kept fixed, the coherence width δxx should be controlled to be smaller than δxy in order to obtain better SOP self-reconstructed properties, but these two variables of SOP have no minimum values with the variation of c 0 .
According to our analysis, the normalized Stokes parameters will be affected by temperature and salinity fluctuations so the DOP and SOP will also be affected. And s 1 fluctuates much more than s 3 and s 3 , DOP varies with more complexity than SOP. Furthermore, both of normalized generalized Stokes parameters of QH beams have proved to be equal to the initial value if the propagation distance is long enough, so the self-reconstructed properties of DOP and SOP of such beams can also be proved. The choice of coherence width of the QH beams can help us to get the best self-reconstructed ability of DOP, but for two parameters of SOP, there are no best choices of these parameters. Our work may be helpful to develop underwater optical imaging or communication system.
The work is supported by National Natural Science Foundations of China (Grant No.61077012, 61107011).
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