Effect of the structure of polarimeter characteristic matrix on light polarization measurements

In the paper, we carried out the comparative analysis of three polarimeters among the most usable their variants: (i) Stokes polarimeter based on phenomenological definition of Stokes parameters; (ii) Stokes polarimeter based on the method of four intensities; (iii) Stokes dynamic polarimeter. We...

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Дата:2009
Автори: Savenkov, S.N., Oberemok, Ye.A., Klimov, O.S., Barchuk, О.I.
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Мова:English
Опубліковано: Інститут фізики напівпровідників імені В.Є. Лашкарьова НАН України 2009
Назва видання:Semiconductor Physics Quantum Electronics & Optoelectronics
Онлайн доступ:http://dspace.nbuv.gov.ua/handle/123456789/118872
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Цитувати:Effect of the structure of polarimeter characteristic matrix on light polarization measurements / S.N. Savenkov, Ye.A. Oberemok, O.S. Klimov, О.I. Barchuk // Semiconductor Physics Quantum Electronics & Optoelectronics. — 2009. — Т. 12, № 3. — С.264-271. — Бібліогр.: 26 назв. — англ.

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spelling irk-123456789-1188722017-06-01T03:05:14Z Effect of the structure of polarimeter characteristic matrix on light polarization measurements Savenkov, S.N. Oberemok, Ye.A. Klimov, O.S. Barchuk, О.I. In the paper, we carried out the comparative analysis of three polarimeters among the most usable their variants: (i) Stokes polarimeter based on phenomenological definition of Stokes parameters; (ii) Stokes polarimeter based on the method of four intensities; (iii) Stokes dynamic polarimeter. We show that, since the accuracy in determination of individual Stokes parameter is different for different types of polarimeters, and, therewith, it depends on polarization of input light. All that strongly motivates the choice of type of polarimeter to provide minimum errors in determination of polarization parameters (ellipticity angle ε, azimuth β, and degree of polarization P). 2009 Article Effect of the structure of polarimeter characteristic matrix on light polarization measurements / S.N. Savenkov, Ye.A. Oberemok, O.S. Klimov, О.I. Barchuk // Semiconductor Physics Quantum Electronics & Optoelectronics. — 2009. — Т. 12, № 3. — С.264-271. — Бібліогр.: 26 назв. — англ. 1560-8034 PACS 07.60.Fs http://dspace.nbuv.gov.ua/handle/123456789/118872 en Semiconductor Physics Quantum Electronics & Optoelectronics Інститут фізики напівпровідників імені В.Є. Лашкарьова НАН України
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
description In the paper, we carried out the comparative analysis of three polarimeters among the most usable their variants: (i) Stokes polarimeter based on phenomenological definition of Stokes parameters; (ii) Stokes polarimeter based on the method of four intensities; (iii) Stokes dynamic polarimeter. We show that, since the accuracy in determination of individual Stokes parameter is different for different types of polarimeters, and, therewith, it depends on polarization of input light. All that strongly motivates the choice of type of polarimeter to provide minimum errors in determination of polarization parameters (ellipticity angle ε, azimuth β, and degree of polarization P).
format Article
author Savenkov, S.N.
Oberemok, Ye.A.
Klimov, O.S.
Barchuk, О.I.
spellingShingle Savenkov, S.N.
Oberemok, Ye.A.
Klimov, O.S.
Barchuk, О.I.
Effect of the structure of polarimeter characteristic matrix on light polarization measurements
Semiconductor Physics Quantum Electronics & Optoelectronics
author_facet Savenkov, S.N.
Oberemok, Ye.A.
Klimov, O.S.
Barchuk, О.I.
author_sort Savenkov, S.N.
title Effect of the structure of polarimeter characteristic matrix on light polarization measurements
title_short Effect of the structure of polarimeter characteristic matrix on light polarization measurements
title_full Effect of the structure of polarimeter characteristic matrix on light polarization measurements
title_fullStr Effect of the structure of polarimeter characteristic matrix on light polarization measurements
title_full_unstemmed Effect of the structure of polarimeter characteristic matrix on light polarization measurements
title_sort effect of the structure of polarimeter characteristic matrix on light polarization measurements
publisher Інститут фізики напівпровідників імені В.Є. Лашкарьова НАН України
publishDate 2009
url http://dspace.nbuv.gov.ua/handle/123456789/118872
citation_txt Effect of the structure of polarimeter characteristic matrix on light polarization measurements / S.N. Savenkov, Ye.A. Oberemok, O.S. Klimov, О.I. Barchuk // Semiconductor Physics Quantum Electronics & Optoelectronics. — 2009. — Т. 12, № 3. — С.264-271. — Бібліогр.: 26 назв. — англ.
series Semiconductor Physics Quantum Electronics & Optoelectronics
work_keys_str_mv AT savenkovsn effectofthestructureofpolarimetercharacteristicmatrixonlightpolarizationmeasurements
AT oberemokyea effectofthestructureofpolarimetercharacteristicmatrixonlightpolarizationmeasurements
AT klimovos effectofthestructureofpolarimetercharacteristicmatrixonlightpolarizationmeasurements
AT barchukoi effectofthestructureofpolarimetercharacteristicmatrixonlightpolarizationmeasurements
first_indexed 2025-07-08T14:49:00Z
last_indexed 2025-07-08T14:49:00Z
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fulltext Semiconductor Physics, Quantum Electronics & Optoelectronics, 2009. V. 12, N 3. P. 264-271. © 2009, V. Lashkaryov Institute of Semiconductor Physics, National Academy of Sciences of Ukraine 264 PACS 07.60.Fs Effect of the structure of polarimeter characteristic matrix on light polarization measurements S.N. Savenkov1, Ye.A. Oberemok, O.S. Klimov, О.I. Barchuk Taras Shevchenko Kyiv National University, Radiophysics Department, 64, Volodymyrska str., 01601 Kyiv, Ukraine, Phone: (380-44)526-05-80; e-mail: sns@univ.kiev.ua1 Abstract. In the paper, we carried out the comparative analysis of three polarimeters among the most usable their variants: (i) Stokes polarimeter based on phenomenological definition of Stokes parameters; (ii) Stokes polarimeter based on the method of four intensities; (iii) Stokes dynamic polarimeter. We show that, since the accuracy in determination of individual Stokes parameter is different for different types of polarimeters, and, therewith, it depends on polarization of input light. All that strongly motivates the choice of type of polarimeter to provide minimum errors in determination of polarization parameters (ellipticity angle ε, azimuth β, and degree of polarization P). Keywords: Stokes vector, Stokes polarimeter, Stokes parameter. Manuscript received 27.03.09; accepted for publication 14.05.09; published online 15.05.09. 1. Introduction Polarization state of electromagnetic radiation changes when interacting with various media and is an additional source of information about their properties. Polarimetric methods through their high sensitivity (in particular to object anisotropy) could be used even at a negligible level of input light intensities. The time of measurement and errors are key factors in experimental investigation of different types of media by polarimetric methods [1-6]. The state of light polarization can be completely characterized by Stokes parameters, which allow describing both completely and partially polarized light. This makes the development of the systems measuring Stokes parameters (Stokes polarimeters) to be highly important for further improvement of polarimetric methods in medium investigations. Up to date, it has been proposed a lot of schemes for Stokes polarimeter [7-10]. In all of them, to transform light polarization, used are polarization transformers with computer controlled parameters. The only polarimeter with division of intensities is exception [11], in which polarization transformers remain invariable. However, this results in considerable complication of the polarimeter calibration. Stokes polarimeters with a mechanically controlled polarization transformer (e.g. with rotating optical elements) are useful in the view of realization simplicity, adjustment and exploitation. Now, the most usable variants of polarimeters are as follows: (i) Stokes polarimeter based on phenomenological definition of Stokes parameters [12]; (ii) Stokes polarimeter based on the method of four intensities [13]; (iii) dynamic Stokes polarimeter [14, 15]. A plethora of papers [10, 13, 16- 25] is devoted to polarimeter optimization in respect of gaining the minimal errors in measurements of Stokes parameters. In particular, derived were the optimal values of phase shifts and angular positions of phase plates. Also, it has been studied the question concerning the systematic error resulted from imperfectness of polarization elements used [22-24]. However, systematic analysis of random errors was not carried out for optimal regimes of the above types of Stokes-polarimeters. Besides, the most of papers, in which errors of polarimetric measurements are considered, supposes that the Stokes parameters are measured with an equal accuracy – but this is not the case in practice. In what follows, we show that individual errors in measurements of Stokes parameters depend on exact strategy of polarimetric measurements. The aim of this paper is to estimate individual errors in measurements of Stokes parameters and effect of these errors on determination of light polarization parameters: ellipticity, azimuth and degree of polarization for the above mentioned strategies of polarimetric measurements. Semiconductor Physics, Quantum Electronics & Optoelectronics, 2009. V. 12, N 3. P. 264-271. © 2009, V. Lashkaryov Institute of Semiconductor Physics, National Academy of Sciences of Ukraine 265 2. Stokes polarimeter based on phenomenological definition of Stokes parameters According to phenomenological definition, four Stokes parameters 41S have the following physical meaning: 1S is a sum of light intensities that pass through polarizers with the orientation 0 and 90 (i.e. the total light intensity); 2S – difference between the same intensities; 3S – difference between intensities for light that pass through polarizers with the orientation 45 and 135; 4S – difference between intensities for light that pass through polarization elements transmitting light with either left or right circular polarization (for example, the quarter-wave plate and linear polarizer with the orientation 45 or 135 relative to fast axis of the plate). These definitions can be expressed in the form: ,; ;; 4135453 90029001 RL IISIIS IISIIS     (1) where xI is the light intensity that pass through corresponding polarization elements. The polarimeter operating accordingly to the definition Eq. (1) is presented in Fig. 1. Here P is the polarizer with the azimuth θ and PhPl is the phase plate with the shift  904/ and azimuth  0 , which can be introduced before the polarizer in the necessary steps of measurements. The signal of photodetector (Fig. 1) depends on the position of polarization elements and the state of input polarization as follows:                                                                 1 1 1 1 1 1 135 45 90 0 )0,90()135( )0,90()45( )135( )45( )90( )0( SMM SMM SM SM SM SM I PhPlP PhPlP P P P P R L I I I I I I , (2) where MP(θ), MPhPl(δ, ), S = [S1 S2 S3 S4] T denote the Mueller matrices of the polarizer as well as phase plate and Stokes vector for input light and have the form, correspondingly:                 1000 0)2(sin)2sin()2cos()2sin( 0)2sin()2cos()2(cos)2cos( 0)2sin()2cos(1 2 1 )( 2 2 PM , (3) From Eq. (2), we can get the equation for determination of required Stokes parameters in the matrix form: IAS  1 , (5) where 1A is the inverse matrix to the characteristic matrix of polarimeter A , which in this case, substituting Eqs. (3) and (4) in Eq. (2), will have the following form:                         5.0005.0 5.0005.0 05.005.0 05.005.0 005.05.0 005.05.0 A . (6) We assume that positioning of polarizer and phase plate occur with errors θ and , correspondingly. Besides, we assume also the deviations of phase shift from δ = /4 with value δ, and errors of intensity measurement I (additive noise) take place. Taking into account these values of errors θ, , δ and I to estimate the individual measurement errors of each of four Stokes parameters, we use the following relation [25]:               N n n n ni Ni y y yF yyyF 1 20 21 )( ),...,,( , (7) where ),...,,( 21 Ni yyyF denote the parameters calculated basing on the measured parameters ny . 0 ny is an exact value of measured parameter ny . Accordingly to Eqs. (5) and (7), the values of errors for Stokes parameters can be written in the following form: 2226 1 2                                        I I SSSS S iii k k i i . (8) Using Eq. (8) and setting the values of errors as δ = 0.5º,  = 0.2º, θ = 0.2º, and I = I0.001 (here S1 = I = 1 is the light intensity of the beam incident on the phase plate (see Fig. 1)), we derive the dependences of the measurement errors for Stokes parameters on the incident light polarization state (β is an azimuth and ε is an ellipticity angle for polarization ellipse of input light) (see Fig. 2).                 0)sin()2cos()sin()2sin(0 )sin()2cos()cos()2(cos)2(sin))cos(1)(2sin()2cos(0 )sin()2sin()))cos(1)((2sin()2cos()cos()2(sin)2(cos0 0001 ),( 22 22 PhPlM . (4) Semiconductor Physics, Quantum Electronics & Optoelectronics, 2009. V. 12, N 3. P. 264-271. © 2009, V. Lashkaryov Institute of Semiconductor Physics, National Academy of Sciences of Ukraine 266  0.000560.00210.00210.0020S  0.00770.00490.00490.0024 ppS Fig. 2. Dependences of the values of Si on polarization of input light for the Stokes polarimeter based on phenomenological definition of Stokes parameters. S(,) MP() MPhPl(δ,) Photo- detector  a y x b  = arctg(b/a); I = a2+b2; Fig. 1. Stokes-polarimeter setup. It can be seen that errors in parameters strongly depend on the polarization state of incident light. Mean errors (shown at the bottom of Fig. 2 as the vector S ) are equal for parameters S1, S2 and S3, and grow for parameters S4 by 2.6 times. The range of error changes (shown as the vector ppS at the bottom of Fig. 2) is equal for parameters S2 and S3. For S1 range of error changes is two times less than that for the parameters S2 and S3, but for S4 is approximately 1.6 times larger. The value of the measurement error for Stokes parameters increases upon the average with decrease of the ellipticity angle ε of incident light. The Stokes parameters are determined with minimum errors for light with polarization closing to the circular polarization (ε = ±π/4). Also it can be seen that the errors for S1 and S3 for input polarization with the azimuth β =±45º relatively to analyzer (θ = 0º) become minimum, and it is practically irrespective to the ellipticity angle. A similar situation with the parameter S2 is observed for polarization of input light with the azimuth β = 0±90º. 3. Stokes polarimeter based on the method of four intensities On the assumption of dimension of the Stokes vector, the set of equations for determining the vector parameters should contain four equations. This set of equations can be obtained by measuring the light intensity Ii after the polarizer MP(0º) (Fig. 1) with the fixed orientation θ = 0º and phase plate MPhPl(δ, i) with the fixed phase shift δ and four angular positions i. The expression for a light intensity Ii incident on the detector can be written in the form:     .)sin()2sin())cos(1)(2sin()2cos( )cos()2sin()2cos( ),()0(),,( 43 2 22 1 0 SS SS I iii ii iPhPlPii    SMMS (9) Thus, from Eq. (9) for Stokes parameters Si we get the following matrix equation: Semiconductor Physics, Quantum Electronics & Optoelectronics, 2009. V. 12, N 3. P. 264-271. © 2009, V. Lashkaryov Institute of Semiconductor Physics, National Academy of Sciences of Ukraine 267 It follows from Eq.(10) that the measurement errors Si are determined by errors Ii , δ and i. Values of the Stokes parameters can be derived as functions of Ii , δ, i from Eq. (10) making use of Eq. (5). Then, in conformity with Eq. (7), Si are:                                       4 1 222 k k i k ii i I I SSS S . (11) As it was in the previous case, Si depend on the polarization state (β, ε) of input light. Fig. 3 presents the dependences of Si as functions of (β, ε), which gives the following values for the parameters of the phase plate: δ = 132º, i = (–51.7º, –15º, 15º, 51.7º) that were defined in [16], and imperfections of polarimeter parameters: δ = 0.5º,  = 0.2º, I = I00.001. It can be seen that locations of maximum and minimum for errors of Stokes parameters Si are antisymmetric with respect to β = 0º. As it follows from values for the vector S (see Fig. 3), the Stokes parameter S4 was measured in this case with the largest errors. The parameter S2 is characterized by the greatest range ppS depending on the polarization state of input light. We show that a uniform distribution of angular orientations of phase plate i (say, for example, i = (–60º, –30º, 30º, 60º)) removes the asymmetric locations of maximum and minimum values of Si, but the mean error S is increased essentially. 4. Dynamic Stokes polarimeter Dynamic Stokes-polarimeter contains a retarder MPhPl(δ, ωt) before the polarizer P (see Fig. 1) rotating with a fixed frequency ω. Thus, in this case the detector signal has the form:   ).2(sin)(sin)4(sin))(cos1(5.0 ))2(sin)(cos)2((cos ),()0(),,( 43 22 21 1 tStS ttSS ttI PhPlP    SMMS (12) Eq. (12) reduces to the following set of equations for Stokes parameters Si: Here, φ0 is the initial position of the phase plate; ak, bk are the amplitudes of harmonics sin(kωt) and cos(kωt), respectively:    N i iI N a 1 0 ),,( 1 S ,            )1( 2 cos),,( 2 1 i N k I N a N i ik S ,            )1( 2 sin),,( 2 1 i N k I N b N i ik S , (14) where N is a number of samplings within the period T = 2π/ω; i – position of the phase plate at i-th sampling. The analysis shows that minimum values of errors δ and φ0 are achieved for δ = 129.6º and φ0 = 0º. It follows from Eqs. (13) and (14) that errors Si in dynamic Stokes-polarimeter depend on values δ, i and φ0. Thus, in according with Eqs. (13), (14) and (7) the expression for Si takes the form:                                                N k k i k iii i I I SSSS S 1 222 0 0 2 . (15) Fig. 4 shows the dependences Si on polarizations (β and ε) of input light, which gives the optimal set of parameters for the phase plate MPhPl (Fig. 1): δ = 129.6º and φ0 = 0º. The number of samplings was chosen as N = 360. The error in initial orientation of the phase plate is φ0 = 0.2º. Other three values Ii, δ, i are the same as in previous cases. As it can be seen from Fig. 4 the parameters S2 and S3 have been determined upon the average with equal errors and are only different in locations of maxima. The mean value of 4S is 1.3 times less than that of 2S and 3S . The value of the parameter S1 has been determined more precisely as compared with S2 and S3 (approximately by 2.6 times) and S4 (approximately by 1.9 times). The value of errors ppS for parameters S2 and S3 are equal and less than that of the parameter S1 by 2.3 times and that of S4 by 5.2 times.   ISA                                            4 3 2 1 4 3 2 1 444 2 4 2 4 333 2 3 2 3 222 2 2 2 2 111 2 1 2 1 )sin()2sin())cos(1)(2sin()2cos()cos()2sin()2cos(1 )sin()2sin())cos(1)(2sin()2cos()cos()2sin()2cos(1 )sin()2sin())cos(1)(2sin()2cos()cos()2sin()2cos(1 )sin()2sin())cos(1)(2sin()2cos()cos()2sin()2cos(1 I I I I S S S S    . (10)   ISA                                          4 4 2 0 4 3 2 1 00 00 0 0)4cos())cos(1(5.0)4sin())cos(1(5.00 0)4sin())cos(1(5.0)4cos())cos(1(5.00 )sin()2cos(000 00))cos(1(5.01 b a b a S S S S    . (13) Semiconductor Physics, Quantum Electronics & Optoelectronics, 2009. V. 12, N 3. P. 264-271. © 2009, V. Lashkaryov Institute of Semiconductor Physics, National Academy of Sciences of Ukraine 268  0.00760.00570.00550.0036S  0.00320.0560.00610.0042 ppS Fig. 3. Dependences of the Si values on polarization of input light for the Stokes polarimeter based on the method of four intensities.  0.00460.00620.00620.0024S  0.00730.00140.00140.0032 ppS Fig. 4. Dependences of the Si values on polarization of input light for the dynamic Stokes polarimeter. Semiconductor Physics, Quantum Electronics & Optoelectronics, 2009. V. 12, N 3. P. 264-271. © 2009, V. Lashkaryov Institute of Semiconductor Physics, National Academy of Sciences of Ukraine 269 .10.0,13.0,25.0,13.0;0039.0,0040.0  ppppppPP a)  15.0,26.0,16.0,17.0,0034.0,0083.0 ppppppPP b)  31.0,37.0,18.0,11.0,0058.0,0076.0 ppppppPP c) Fig. 5. Dependences of the P, ε, β values for different polarizations of input light: (a) Stokes polarimeter based on phenomenological definition of Stokes parameters; (b) dynamic Stokes polarimeter; (c) Stokes polarimeter based on the method of four intensities. 5. The effect of measurement errors Si on determination of polarization parameters of input light The given Stokes parameters, Si, polarization parameters, intensity I, degree of polarization P, ellipticity angle ε and azimuth of polarization ellipse β can be determined in the following manner: .arctg 2 1 ,arcsin 2 1 ,, 2 3 2 4 2 3 2 2 4 2 1 2 4 2 3 2 2 1                    S S SSS S S SSS PSI (16) Errors in values of Stokes parameters will be transferred into errors of polarization parameters Eq. (16). To estimate this effect, we use Eq. (7): . ,, 4 1 2 4 1 24 1 2                                  i i i i i ii i i S S S S S S P P (17) Since the values Si (β, ε) are different for different Stokes-polarimeters discussed above, thus, the errors of polarization parameters Eq. (17) are different for different Stokes-polarimeters as well. Fig. 5 exemplifies Semiconductor Physics, Quantum Electronics & Optoelectronics, 2009. V. 12, N 3. P. 264-271. © 2009, V. Lashkaryov Institute of Semiconductor Physics, National Academy of Sciences of Ukraine 270 the dependences P(β, ε), ε(β, ε) and β(β, ε) for three types of polarimeters discussed above. It follows from Fig. 5 that the ellipticity of polarization ellipse has been determined with the minimum errors by dynamic Stokes-polarimeter. Whereas, the polarization degree P and azimuth of polarization ellipse β are determined with minimum errors by Stokes polarimeter based on phenomenological definition of Stokes parameters. For Stokes polarimeter based on the method of four intensities, the effect of polarization of input light on the errors P, ε and β is minor. More sensitive to the polarization state of input light is the dynamic Stokes-polarimeter. 6. Conclusion In summary, we have analyzed the errors in determination of the Stokes parameters for three types of Stokes polarimeters: (i) Stokes polarimeter based on phenomenological definition of Stokes parameters; (ii) Stokes polarimeter based on the method of four intensities; (iii) dynamic Stokes polarimeter. Also, we have analyzed the transfer of the errors for Stokes parameters Si into the errors in determination of polarization parameters (degree of polarization P, ellipticity angle ε and azimuth of polarization ellipse β) of input light. We have shown that in general case the Stokes parameters are determined with a different accuracy both in scope of one measurement strategy and by different measurement strategies. The Stokes vector is measured as a whole with minimum errors by Stokes polarimeter based on phenomenological definition of Stokes parameters: 0017.04/ 4 1  i iS . The dynamic Stokes polarimeter and Stokes polarimeter based on the method of four intensities measure the Stokes vector with a somewhat higher value of errors: 0049.04/ 4 1  i iS and 0056.04/ 4 1  i iS , respectively. This is quite important fact because it means that, under rest equal circumstances, the parameters of polarization of input light are measured with different errors by different polarimeters. Moreover, the errors depend on the polarization state of input light as well. The results obtained for errors of the Stokes parameters allowed to determine that the ellipticity angle ε is measured more precisely by dynamic Stokes- polarimeter, whereas, the azimuth β and degree of polarization P are measured more precisely by Stokes polarimeter based on phenomenological definition of Stokes parameters. The results derived in this paper can be useful for choosing the measurement strategy for given polarization of input light. Indeed, the Stokes polarimeter based on phenomenological definition of Stokes parameters is complicated for automatization. The dynamic Stokes polarimeter is evidently unacceptable for imaging Stokes vector measurements [10]. At the same time, the Stokes polarimeter based on the method of four intensities, although characterized by a relatively higher value of errors when determining Stokes parameters, is simple for automatization and promising for imaging Stokes polarimetry. It is noteworthy that on the assumption of equality of Si there exist no reasons to prefer one Stokes polarimeter to another. An exception can be very likely made only when concerning to assembling and operating conveniences. 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