The present description generally relates to polarization dependent loss (PDL) measurement, and more particularly to measuring polarization dependent loss of a device under test using a single spectral scan.
Conventional methods for Polarization Dependent Loss (PDL) measurement include the Polarization Scanning technique and the Mueller Matrix Method.
In the Polarization Scanning technique, the Device Under Test (DUT) is exposed to virtually all States Of Polarization (SOP) and the PDL is determined from the maximum and minimum power transmission through the DUT. Because the Polarization Scanning technique needs to expose the DUT to many states of polarization, the PDL is measured at a single wavelength at a time. Measuring the PDL over a broad wavelength range can quickly become impractical.
The classic Mueller Matrix Method (see U.S. Pat. No. 5,371,597 to Favin et al.) aims at determining the first row of the Mueller matrix (4 elements) that characterizes the DUT, from which the PDL of the DUT is deduced. To this end, a lightwave having successively a small number (e.g. 4) of distinct, known input states of polarizations (SOP) is launched into the DUT, and the corresponding small number of power transmissions are measured (power of the lightwave at the output of the DUT divided by the power at the input of the DUT). To obtain the PDL characterization over wavelength, distinct wavelength scans need to be performed sequentially for each of said small number of distinct input-SOPs (minimum of 4), wherein the input-SOP is fixed (constant as a function of time) during each individual scan.
The classic Mueller Matrix Method is prone to substantial errors should the DUT be unstable over the interval between said sequential wavelength scans, e.g., due to moving patch-cords, in which case the PDL measurement can be utterly wrong. A single wavelength scan approach would resolve this problem by making the SOP of the input test lightwave vary rapidly during the wavelength scan, so the DUT response to a plurality of input-SOPs would be measured at each wavelength within a much shorter time.
A method was proposed in the art (see U.S. Pat. No. 6,856,386 to Anderson) to measure the PDL based on the Mueller Matrix Method but using a single wavelength scan, by changing the input-SOP during the wavelength scan in a cyclic manner. In this method, the input-SOP can be changed using either an active or a passive device. However, one drawback of this method is that it requires that the SOP of the input test lightwave be either carefully controlled or monitored using a polarimeter and, in the case of a passive SOP generator, the combination of a polarimeter and additional polarization controller in an feedback loop, which significantly increases the difficulty of implementation, complexity and cost of the test hardware.
There therefore remains a need for an improved single wavelength scan PDL measurement method.
There is herein provided a PDL measurement method which uses a new set of equations, i.e. different from that of the classic Mueller Matrix Method, as well as new data acquisition scheme and data processing to derive the PDL from a single wavelength scan (or spectral scan) over which the input-SOP varies. As explained in the detailed description, the proposed new set of equations can be viewed as a generalization of the mathematics of the Mueller Matrix Method. When compared to the classic Mueller Matrix Method, the new set of equations is applied to derive the same result, i.e., the 4-element response vector of the DUT (elsewhere referred to as the first row of the Mueller matrix) as a function of optical frequency (or wavelength), from a different data set obtained by a different data acquisition procedure, i.e., a single wavelength scan over which the input-SOP varies continuously over the scan instead of a few sequential scans with fixed SOPs.
Therefore, in accordance with one aspect, there is provided a method for measuring the PDL of a DUT as a function of optical frequency ν within a spectral range, which uses a single wavelength scan over which the input-SOP varies in a continuous manner, i.e. not a finite number of discrete points, but a continuous trajectory on the surface of the Poincaré sphere as a function of ν. The power transmission through the DUT, curve T(ν)=Pout(ν)/Pin(ν) is measured during the scan, where Pin(ν) and Pout(ν) represent the power of the ligthwave at the input and output of the DUT respectively. The PDL is derived from the resolved sideband components of the power transmission curve T(ν) that result from the continuously varying input-SOP. More specifically, the Discrete Fourier Transform (DFT) of the power transmission curve T(ν) is calculated, wherein the DFT shows at least two resolved sidebands in the delay (τ) domain (four in the hereindescribed embodiment), where delay τ is the conjugate variable of ν in the Fourier transform (the same way as signal-frequency f is the conjugate variable of time t). At least two sidebands are extracted individually, i.e. selected by applying a bandpass filter in the delay domain, and their inverse DFT calculated to obtain individual complex transmissions (ν), =−J . . . J, where J is the number of sidebands defined as the number of resolved peaks on a single side of the DFT, e.g. side τ>0. The transmissions (ν) are complex in the sense that they are complex numbers (real and imaginary parts, or equivalently, amplitude and phase). The 4-element response vector |m(ν) of the DUT, elsewhere referred to as the first line of the Mueller matrix, is derived from the complex transmissions (ν) and a matrix that represents a system of equations to be solved. As well known, a system of equations can be advantageously solved by arranging the known coefficients into a matrix, and inverting said matrix. In the context of RSB, said matrix only depends on the continuous trajectory of the input-SOP (continuous curve on the surface of the Poincaré sphere). Matrix thus constitutes a generalization of the corresponding matrix A of the classic Mueller Matrix Method which similarly represents a system of equations and only depends on the finite number of known discrete input-SOPs. Of note is that neither matrix A nor is the Mueller matrix; the Mueller matrix characterizes a DUT, thus is independent of any particular set of input-SOPs. Finally, the PDL of the DUT as a function of ν (PDL curve) is derived from said response vector in the same way as in the classic Mueller Matrix Method.
The provided method allows for asynchronous sampling of the power transmission curve T(ν) with respect to the variation of the input-SOP, i.e. the sampled points do not need to fall on specific input-SOPs. This property allows to circumvent the need for monitoring the input-SOP with a polarimeter in the case of an active SOP generator (see active SOP generator approach of U.S. Pat. No. 6,856,386), or to additionally control the SOP through a feedback loop in the case of a passive SOP generator (see passive SOP generator approach of U.S. Pat. No. 6,856,386).
Accordingly, measuring the power transmission curve T(ν) comprises data sampling that is allowed to be asynchronous with respect to the SOP variation of the input test lightwave, i.e. the sampled points do not need to fall on a pre-determined set of input-SOPs, and consequently, the most usual and simple kind of sampling can be performed, i.e. sampling at equal intervals dν between successive samples, regardless of the input-SOP at the values of ν corresponding to the samples.
The phase of the SOP of the input lightwave along the continuous trajectory, i.e. where exactly along the trajectory is the point that represents the SOP at a given value of ν, may be either known or measured at each sampled point.
In the provided method, said phase can be measured live through appropriate data processing of the output of a single polarizer (referred to as the phase reference signal Pφ in the detailed description), no need for a full polarimeter nor additional polarization controller and feedback loop.
In accordance with another aspect, there is provided a method for measuring the PDL of a DUT within a spectral range. The method comprises:
In accordance with another aspect, there is provided a system for implementing the provided PDL measurement method. The apparatus comprises:
Throughout this specification, spectrally-varying values, functions and equations are expressed as a function of the optical frequency ν. It is however noted that such variation could equivalently be termed as a variation as a function of wavelength λ, where λ=c/ν or the wave number σ=ν/c. Similarly, the expressions “wavelength scan” and “spectral scan” are used interchangeably herein to denote a scan that varies the optical frequency ν and the wavelength λ of a lightwave over a spectral range.
In this specification, unless otherwise mentioned, word modifiers such as “substantially” and “about” which modify a value, condition, relationship or characteristic of a feature or features of an embodiment, should be understood to mean that the value, condition, relationship or characteristic is defined to within tolerances that are acceptable for proper operation of this embodiment in the context of its intended application.
In the present description, and unless stated otherwise, the terms “connected”, “coupled” and variants and derivatives thereof refer to any connection or coupling, either direct or indirect, between two or more elements. The connection or coupling between the elements may be mechanical, physical, operational, electrical or a combination thereof.
Further features and advantages of the present invention will become apparent to those of ordinary skill in the art upon reading of the following description, taken in conjunction with the appended drawings.
It will be noted that throughout the drawings, like features are identified by like reference numerals.
It should also be understood that when the appended drawings are denoted as schematics, elements of the drawings are not necessarily drawn to scale. Some mechanical or other physical components may also be omitted in order to not encumber the figures.
The following description is provided to gain a comprehensive understanding of the methods, apparatus and/or systems described herein. Various changes, modifications, and equivalents of the methods, apparatuses and/or systems described herein will suggest themselves to those of ordinary skill in the art. Description of well-known functions and structures may be omitted to enhance clarity and conciseness.
Although some features may be described with respect to individual exemplary embodiments, aspects need not be limited thereto such that features from one or more exemplary embodiments may be combinable with other features from one or more exemplary embodiments.
The present paragraph exposes a case only as an explanatory step intended to help the reader to understand the proposed method, but there is no foreseeable advantage in doing this step as such. In the classic Mueller Matrix Method, a number J of wavelength scans are performed sequentially with fixed input-SOPs, meaning that the input-SOP does not change during the scan. Now, imagine that a number J of wavelength scans are similarly performed sequentially but with input-SOPs (i.e., SOPs of the test lightwave) that, instead of being fixed SOPs, oscillate sinusoidally as a function of the optical frequency ν, e.g., describing distinct circles on the surface of the Poincaré sphere as a function of ν. Then for each scan j, j=0 . . . (J−1), we obtain a transmission curve Tj(ν) representing the response of the DUT to said oscillating SOP (instead of the response to a fixed one). Since, in the classic Mueller Matrix Method, the set of J transmission curves obtained with J fixed SOPs is enough information to deduce the desired result, it follows that the set obtained with J oscillating SOPs, thus more individual values of SOPs in a way, is also enough. Of course, deducing the result in the case of oscillating SOPs requires a new set of equations, different from the one of the classic Mueller Matrix Method.
Part of the PDL measurement method described herein can be seen as a generalization of the mathematics of the classic Mueller Matrix Method in the context of J responses to J oscillating input-SOPs instead of fixed, constant input-SOPs. In the classic Mueller Matrix Method, the 4-element response vector of the DUT, |m(ν), is obtained by solving a linear system of equations, where the four unknowns to be determined are the four elements of the response vector. As for any linear system of equations, the coefficients that multiply the unknowns in the different equations can be grouped to form a single matrix, say matrix A (not to be confused with the Mueller matrix), and the solution of the system of equations is obtained by first computing the inverse of A. In the classic Mueller Matrix Method, said matrix A only depends on, and is deduced from the known set of J fixed SOPs. In the case of oscillating SOPs as described above, it can be shown that there still exists such a matrix representing the system of equations to be solved, which is the matrix . Notably, it has a different number of rows, and its elements are complex numbers instead of real numbers. But the important point to note is that this equivalent matrix indeed exists and only depends on, and is deduced from the known set of, in this case, oscillating SOPs. This constitutes the main aspect of said generalization of the mathematics of the classic Mueller Matrix Method.
However, as mentioned hereinabove, there is no advantage in making J sequential scans with oscillating SOPs instead of fixed one. Indeed, the goal is to get the result using a single scan. Therefore, there is herein proposed to step up from the above explanatory case to one where the responses Tj(ν) to J oscillating input-SOPs are obtained both simultaneously and separately from a single scan. For this to be, the responses Tj(ν) should be separated as, by analogy, multiple communication channels are separated in the frequency domain. Using an input-SOP that follows a suitable continuous trajectory on the surface of the Poincaré sphere as a function of ν allows to generate responses Tj(ν) that each occupies its own band in the delay domain r around a given carrier-delay ±τ1, ±τ2, etc. How to generate such trajectory will become clear in the following description of embodiments. It is noted that since the power transmission curve T(ν) is a function of optical frequency ν, the abscissa of the Fourier transform of T(ν) is delay τ (not signal-frequency f) and the oscillating components of T(ν) appear as resolved sidebands in the delay domain (τ) (not the signal-frequency domain (f)).
The above explains the name given to the method, i.e. the Resolved-SideBands (RSB) method. Resolved because said sidebands are separated enough in the delay domain (τ) for the different corresponding signals, the responses Tj(ν), not to overlap. Yet more clearly, the Fourier transforms of the responses Tj(ν), which are functions of delay τ, do not overlap in the delay domain. An enlightening analogy can be made with a much more familiar case; the carriers of TV channels which should be separated enough in the frequency domain for adjacent signals spectra (in the Fourier transform of the transmitted/received electromagnetic waves) not to overlap, enough to avoid significant “crosstalk”, this being determined by the required bandwidth of the signals that modulate the sinusoidal carriers. Similarly, in the RSB method, the equivalent of the time-varying signal bandwidth is the “DUT extent” in the delay domain (τ), i.e. how large is the Fourier transform of the DUT transmission curve TDUT(ν). For example, if the DUT is a narrow optical filter such as a WDM filter, the narrower TDUT(ν), the larger its extent in the delay domain. Of course, in order to avoid “crosstalk” the spacing between the sideband-carriers are set larger than the maximum extent of the DUT that is expected to be encountered. This spacing is a characteristic of the SOP generator that one can set in accordance with the expected application of the instrument, i.e. large enough for the sidebands not to overlap for DUTs having the largest expected extent (typically DUTs that have the narrowest and/or sharpest transmission TDUT(ν)).
As in the classic Mueller Matrix Method, the result of the measurement of the RSB method is the 4-element response vector |m(ν) (elsewhere named first line of the Mueller matrix) as a function of optical frequency ν. From the response vector |m(ν), the PDL can be derived as known in the art, in the same way as in the classic Mueller Matrix Method. The polarization-dependent center wavelength (PDCW) and the polarization-dependent bandwidth (PDBW) of the DUT can also be derived as known in the art from |m(ν) in cases where the DUT is such that these parameters have a defined meaning, e.g., optical bandpass filters.
It is worth mentioning that there is a formal equivalence between the mathematics of the classic Mueller Matrix Method and the mathematics of the RSB method, mainly through the existence of said equivalent matrix (the matrix that represents the system of equations to be solved): the most notable difference is that, contrary to the corresponding matrix (again, not the Mueller matrix) of the classic Mueller Matrix Method, matrix of RSB has complex elements (real and imaginary parts), and the measured transmission terms (ν), =−J . . . J, where J is the number of sidebands, are also complex-valued (amplitude/phase of the oscillating responses) instead of real-valued. The notation is used to clearly distinguish the complex phasor (ν) from the real response Tj(ν) (real part of (ν)). Representing such oscillating signals by complex phasors makes the mathematics of RSB much simpler and concise than would otherwise be.
The proposed PDL measurement method is now further described with reference to
Because the example trajectory of
The mathematics of RSB is now described in detail, with reference to
bra: v|=(v*0 v*1 v*2 . . . v*n−1), where * means complex-conjuguate.
ket: |v=(v0 v1 v2 . . . vn−1)τ, where τ means transposed.
scalar product: v|v′=v*0v′0+v*1v′1+v*2v′2+ . . . +v*n−1v′n−1
Although seldom mentioned explicitly, all PDL measurement methods, including the classic Mueller Matrix Method, assume that the DUT response to an input lightwave is linear. Indeed, the Mueller matrix of the DUT is by definition a linear transformation of the input Stokes vector into the output Stokes vector. Otherwise, i.e. a non-linear DUT, the very parameter to be measured, PDL, does not even exist as commonly defined. For instance, PDL at a given value of ν would be multi-valued, notably depending on the power of the input lightwave. The RSB method makes this same basic assumption as a matter of course.
The general form of such linear response is, as far as only the transmitted power is concerned,
T(ν)=s(ν)|m(ν) (1)
with T(ν)=Pout(ν)/Pin(ν), where Pin(ν) and Pout(ν) are the power of the lightwave at input and output of the DUT, |m(ν)=(m0(ν) m1(ν) m2(ν) m3(ν))τ is said response vector of the DUT measured by the method, and (s(ν)|=(1 s1(ν) s2(ν) s3(ν))τ is the 4-element bra representing the 100% polarized input-SOP, where the last three elements of s(ν)| are those of the 3-element unit Stokes vector ŝ(ν)=(s1(ν) s2(ν) s3(ν))τ, |ŝ(ν)|=1.
Mathematical note: The most general linear transformation mapping a vector (input-SOP) to a scalar (transmission T) is by definition a scalar product, as (1) is. The response vector embodies this mapping even if Mueller-matrix calculus would not exist; this is to say that reference to the Mueller matrix is incidental, including in the classic method said of the Mueller matrix; it happens that the response vector is indeed identical to the first line of the 4×4 Mueller matrix, but this matrix is nowhere used in the calculations.
As exposed hereinabove with reference to
ŝ=(=−J . . . J), =()τ (2)
where ω=2πν, and is the complex vectorial amplitude of component in the DFT of the known trajectory ŝ(ν) of the input-SOP. Observe that is a 3-element complex-valued vector; in (2), the three complex amplitudes corresponding to the three individual Stokes parameters (s1, s2, s3) are simply wrapped up in this single, complex-valued vector. It allows to write it all in a single equation instead of three, as in (2), but also everywhere else below. Analytical expressions of the for specific trajectories will be given in the description of the preferred embodiment. Of note is that the can of course be measured; having analytical expressions for the preferred embodiment is convenient, but not required. Now, since response (1) is linear, one component of ŝ(ν) in (2) generates one component of T(ν) by mere definition of linearity, i.e.,
T(ν)=(=−J . . . J) (3)
Therefore, each component of ŝ(ν) generates one and only one term in sum (3), which translates as sideband around carrier-delay in the DFT of T(ν) as shown in
(ν)=|m(ν) (4)
where | is the 4-element bra corresponding to , i.e.,
|=() where =1 if =0, 0 otherwise. (5)
Observe the presence of Kronecker symbol in (5). This reflects that the average over ω of an oscillating SOP component with ≠0 is null.
Equation (4) is a compact expression of a system of (2J+1) equations (=−J . . . 1), one equation for each value of , in which the 4 unknowns are the 4 elements of the response vector |m(ν). Also, equation (4) shows that there is one such system of equations for each value of ν. This is made more apparent by writing the scalar product (4) at length in terms of the four elements of both | and |m(ν); one equation, i.e. for one value of at one value of ν, then reads as,
·m0(ν)+·m1(ν)+·m2(ν)+·m3(ν)=(ν) (6)
which is one among a system of (2J+1) equations (=−J . . . J) where (m0(ν) m1(ν) m2(ν) m3(ν)) are the 4 unknowns to be determined, () are the known coefficients depending only on the known continuous trajectory ŝ(ν) of the input-SOP, and (ν) is the measured complex transmission curve extracted from sideband in the DFT of T(ν) as exposed previously. As well known, a system of equations can be solved by arranging the known coefficients into a matrix, and inverting this matrix. In RSB, said matrix is noted , and following from equations (4) and (5) the system of equations at a given ν is wrapped up as,
|(ν)=|m(ν) (7)
the solution of which is the measured response vector at optical frequency ν, given by,
|m(ν)=−1|(ν) (8)
where −1 is the generalized inverse of . For the sake of illustration, we show below the explicit expressions of and |(ν) in our preferred case with J=4, and then list their relevant general characteristics:
The general characteristics of ket |(ν) are:
But then is not a square matrix and thus has no inverse in a strict sense, reflecting the fact that there are more equations than unknowns (more rows than columns). It is to be understood that having more equations than minimally required is by no way a drawback of any sort. Only that mathematically speaking we have to use a generalized inverse of , here defined as follows,
−1=B−1† with B=† († means transposed complex-conjugate) (10)
The response vector |m(ν) that RSB seeks to measure is given by equations (8) and (10).
This completes the description of the part of RSB that can be said to generalize the mathematics of the classic Mueller Matrix Method. Indeed, although the compact form of equation (11) below is seldom seen in the literature, in the normed classic Mueller Matrix Method the solution can be similarly written as,
|m(ν)=A−1|T(ν) (11)
where A is a real (no imaginary part) 4×4 matrix which rows are the 4 real bras representing the 4 fixed input-SOPs, and |T(ν) is a 4-element vector consisting of the 4 real transmissions, measured at the sameν but obtained sequentially in time (i.e. one distinct scan for each fixed input-SOP, one after the other). So written, equations (8) and (11) are found to be formal mathematical equivalents.
Finally, to make sure that a possible misunderstanding is avoided: A and are indeed matrices, involved in the calculations of their respective methods, but neither of them is the Mueller matrix. The name Mueller Matrix Method may be misleading for that matter, since the full Mueller matrix is nowhere used in the calculations, only its “first line”, thus a much simpler vector which we name response vector, whereas indeed a matrix is involved, matrix A, be it explicitly or implicitly (solving a system of equations).
In some embodiments, a suitable trajectory of the input-SOP as a function of ν as described hereinabove is generated using a passive SOP generator. Such a passive SOP generator advantageously generates by laws of Physics a trajectory showing the desired small number of sidebands (J=2, 3 or 4). However, in other embodiments, suitable trajectories of the input-SOP may be generated by using an actively controlled SOP generator. Such actively controlled SOP generators are generally known in the art and commercially available and will therefore not be herein described in detail. Actively controlled SOP generators are also much more complex, bulky and costly.
A 2-segs always generate 4 sidebands, located at delay values δτ0, δτ1, (δτ0+δτ1) and (δτ0−δτ1) in the delay domain. This implies that for ratios like r=1 and 2 some of the four are superimposed (located at the same delay value). Thus, the number of distinct (not superimposed) sidebands in the Fourier transform of the transmission T(ν) depends on the ratio r. For example, an integer ratio r≥3 will generate J=4 distinct sidebands, a ratio r=2 will generate J=3 distinct sidebands and a ratio r=1 will generate J=2 distinct sidebands only. In other words, both the number J and relative locations of the distinct sidebands, at delay values referred to as (=−J . . . J, ≠0) in this specification, depend on the ratio r of the 2-segs.
In one embodiment, the passive SOP generator is designed with a ratio r˜3, which advantageously generates J=4 substantially equally spaced sidebands, and the targeted coupling angles are φŝo90° and φp=90°. Almost any other coupling angles may be used, except 0° or 180°, but the above-mentioned choice minimizes the sensitivity of the measurement to both additive noise and uncertainty on the knowledge of the actual coupling angles.
The input polarizer 306 sets the SOP at the input of the first piece of PMF 302, and thus the coupling angle φŝo. The two pieces of PMF 302, 304 are fused at an angle φp between their respective PSPs (p0 and p1). Of note is that the specific values of the coupling angles φŝo and φp are not critical in the sense that no high precision alignment is required, as long as the actual angles are known or determined afterwards. The actual coupling angles φŝo and φp can be determined afterwards through a calibration process, e.g. using a polarimeter.
Respective lengths of PMF pieces 302, 304 determine the value of their DGDs δτ0, δτ1, thus also the ratio r. Here again, there is no high precision requirement in cutting the PMF pieces to a given length. The two DGDs may be effectively measured live through appropriate data processing of the phase reference signal Pφ(ν). More to the point, the two effective DGDs determine the phase of the SOP of the input lightwave along the trajectory, i.e. where exactly along the trajectory is the point that represents the SOP located at a given value of ν. This phase may be either known or measured at each sampled point. One may target design values of angles φŝo and φp, DGD δτ0 and DGD δτ1 with reasonable care, but the true angles and DGDs after assembly do not need to be precisely equal to the design values.
The phase reference arm 310 comprises a coupler 308 used to extract a small portion of the light at the output of the second PMF piece 304 toward a polarizer 312 (analyzer â) followed by a photodetector 314, which output constitutes a phase reference signal Pφ(ν). This phase reference signal would not be needed in a perfect world where the DGDs and corresponding phases φ0(ν), φ1(ν) (see
The angle φâ between â and p1, or in words between the analyzer axis and the PSP of the second PMF piece 304, is set by rotating polarizer 312 (or by an angular fusion splice between the second PMF piece 304 and the PMF-fiber pigtail of the polarizer 312). In practical embodiments φâ is set to roughly 45° (not critical, but it should not be 0°, 90° or 180°, because then either one of the oscillating components of the signal Pφ(ν) that are analyzed in the data processing to measure said phases live would have zero amplitude).
It is noted that, although simple, the embodiment of
But larger DGD values, e.g. in the nanoseconds order of magnitude or even greater if needed, may be obtained by replacing the PMF pieces 302, 304 by devices 402, 404 which may be named Polarization-Splitting Mach-Zehnder interferometers PS_MZ.
The passive SOP generator 400 also comprises an optional phase reference arm 410. As in the embodiment of
The coupling angle φŝo is set by rotating the assembly comprising the input polarizer 406 and collimator c0. The coupling angle φp is set by the angled fusion between the two pieces of PMF 420, 422 attached respectively to collimators c3 and c4. The PSP of each of these two pieces of PMF 420, 422 is aligned with the polarization axis of the PBS that faces the collimator to which they are attached.
The angle φâ between â and p1, or in words between the analyzer axis and the PSP of the second PS-MZ, is set by rotating polarizer 412.
The lengths of the PMF pieces 418 (denoted PMF0 and PMF1) mainly determine the DGDs of the two PS_MZs 402, 404: δτq˜nLq/c, wherein Lq is the PMF length and n is the mean group index of the fiber (˜1.5). For an accurate pre-calculation of the lengths before cutting the fibers, the small light path lengths in air, into the PBSs and into the collimator lenses should be taken into account. It is noted that the use of PMFs in the PS_MZ 402, 404 is optional although advantageous to properly align the polarization that comes out of the first PBS with the polarization axis of the second PBS, in order to minimize and stabilize the loss of this path (a misalignment has no other adverse effect).
Collimators c3 and c4 and their attached pieces of PMF are inserted for the purpose of simplifying the assembly. The two assemblies constituting the two PS_MZ 402, 404 may then be mounted on a single plane. Otherwise there should be two planes making an angle θ=φp/2 (see
The passive SOP generator 500 comprises two all-bulk PS_MZs 502, 504. The optical path is split in two arms and then recombined using two Polarization Beam Splitters (PBS) 516. For each PS_MZ 502, 504, a path length difference (delay) between the two arms is set by a free-space optical path that is made longer in one of the arms 518, using a mirror arrangement. The DGD of each PS_MZ 502, 504 is equal to the delay between the two arms. The passive SOP generator 500 also comprises an input polarizer 506, and again, as in the embodiment of
The coupling angle φŝo is set by rotating the input polarizer 506. The coupling angle φp is set by rotating the mounting plane of the second PS_MZ 504 (normal û1) with respect to the mounting plane of the first PS_MZ 502 (normal û0). The angle θ between normal û1 and normal û0 is θ=½φp (θ represents the physical angle between the normal vectors of two planes, whereas the coupling angles φ refer to angles between Stokes vectors such as ŝo, p0, p1, â; Stokes vectors are not limited to representing linear polarizations; when linear SOPs are involved, a corresponding physical angle do exists, but equal to half the angle between the Stokes vector).
It is noted that the two PS_MZs 502, 504 may alternatively be mounted on the same plane by inserting a retardation waveplate (λ/2) in-between. The coupling angle φp is then set by rotating the waveplate. Although apparently convenient, there is a drawback; waveplates that would be substantially achromatic (constant retardation as a function of ν) over a very large scanning range (e.g. from 1250 to 1650 nm) are rare and exceedingly expensive.
It will be understood that the above-described implementations of the passive SOP generator may be varied by mixing portions thereof. For example, the phase reference arm 310 or 410 may be replaced by the bulk phase reference arm 510 and vice versa. The bulk delay lines 518 of the all-bulk embodiment 500 may also be replaced by segments of PMF and associated collimator lenses c1-c2, c5-c6 as in the bulk and fiber embodiment 400.
It should be noted that the RBS method, notably its new mathematics (see equations (1) to (10)) constituting a generalization of the mathematics of the classic Mueller Matrix Method, is more general than this embodiment, is not limited to this embodiment and does not require data to be acquired using a single wavelength scan. It rather allows dealing optimally with this much more challenging case. Data may as well be acquired using multiple scans sequentially in time with different oscillating SOPs, and whether the SOP generator is active or passive. The PDL measurement system 600 is still mostly advantageous compared to the classic Mueller Matrix Method in that the PDL can be derived from a single wavelength scan over which the input-SOP continuously varies instead of a few sequential scans with fixed SOPs.
The PDL measurement system 600 comprises a tunable light source 602, an SOP generator 604, a power transmission measurement apparatus 606, an acquisition device 608 (also referred to as data sampling), a processing unit 610 implementing the RSB data processing, a data output 612 for displaying, saving in memory or otherwise outputting the measurement results.
The tunable light source 602 generates a test lightwave and spectrally scans the test lightwave over the spectral range over which the PDL is to be measured.
The SOP generator 604 is used to vary the SOP of the test lightwave according to a continuous trajectory on the surface of the Poincaré sphere while the test lightwave is spectrally scanned, before the test lightwave is launched into the DUT. Although, as explained hereinabove, passive SOP generators offer many advantages, in some implementations it may still be chosen to use an active SOP generator.
The power transmission measurement apparatus 606 measures the power of the ligthwave at both the input and output of the DUT, i.e. Pin(ν) and Pout(ν) respectively, so that the transmission through the DUT, T(ν)=Pout(ν)/Pin(ν), can be computed.
The acquisition device 608 simultaneously samples values of Pin(ν), Pout(ν) and optionally Pφ(ν) during a spectral scan of the test lightwave.
The processing unit 610 computes the power transmission curve T(ν) from the sampled power Pin(ν) and Pout(ν) as T(ν)=Pout(ν)/Pin(ν), and processes said computed curve T(ν) and optional phase reference output Pφ(ν) in accordance with the RSB method to derive therefrom the spectrally-varying PDL of the DUT.
The data output 612 outputs the measured characteristics which, in addition to the spectrally-varying PDL may include the polarization-dependent center wavelength (PDCW) and the polarization-dependent bandwidth (PDBW) of the DUT.
The tunable light source 602 generates a test lightwave and spectrally scans the test lightwave over the spectral range over which the PDL is measured. The tunable light source 602 may be based on a tunable narrowband single-mode laser or, alternatively, a broadband light source (e.g. a super-LED) followed by a tunable optical filter (also named “monochromator”).
It will be understood that the term “single-mode” intends to comprise a laser source which output spectrum substantially consists of a single peak, which peak always has some finite width in practice, the laser linewidth.
The term “narrowband” refers to said laser linewidth. In the case of the broadband source and optical filter embodiment, in refers to the width of the passband of the optical filter. The maximum acceptable linewidth depends on the intended application as it determines the minimal spectral resolution of the measurement. For example, the characterization of a broadband DUT, having a constant SOP-averaged transmission and constant PDL over a large range of ν, is less stringent on the linewidth than other DUTs including WDM optical filters having a 3-dB bandwidth as small as 25 to 30 GHz. To give some figures: for example, in the case of the passive SOP generator described hereinabove for which the DGDs of the 2 segments are δτ0˜3 ns and δτ1˜1 ns (case r=3), which are large enough for said DUTs to be measured with negligible crosstalk between the sidebands, the resulting extent of T(ν) in the delay domain requires that the laser linewidth be smaller than about 10 MHz (but up to 5 times this value may be acceptable if a compensation of the lowpass filtering effect of the finite laser linewidth is applied by the data processing based on the knowledge of the laser lineshape).
The term “tunable” intends to mean that the optical frequency ν of the laser or the center optical frequency ν of the tunable filter passband in the broadband source alternative, can be set to a plurality of values over the spectral range of the measurement. The spectral range may be determined by the application or be selected by the user depending on the spectral range over which the PDL of the DUT is to be characterized. In any case, the RSB method requires (to obtain a single point of PDL(ν)) that the spectral range at least covers about one cycle of the SOP trajectory (e.g. ˜1 GHz for δτ1=1 ns).
The spectral scan typically involves that, starting from a given initial optical frequency νo at t=0, the optical frequency ν is tuned to increase or decrease in a substantially continuous manner as a function of time t and with a substantially linear variation as a function oft, i.e. ν(t)=νo+vs t, where vs is the scanning speed. Such spectral scan may be obtained using what is widely referred to as a “swept-wavelength system”, which allows to sample data over a very large number of values of ν in a very swift way. It is however noted that such continuous scan is not necessarily required by RSB. Indeed, data could as well be acquired by varying the optical frequency ν in a random order, then re-ordered in ascending order afterward, as long as the power transmission T(ν) of the DUT is obtained as a function of ν. But in practice, it is obviously more convenient to proceed with a continuous scan.
That being said, in practice, sampling data (Pin(ν), Pout(ν), Pφ(ν)) with a constant step dν in optical frequency or re-sampling in the data processing (using interpolation) to obtain such constant step dν, allows computing the Discrete Fourier Transforms (DFT) using the Fast Fourier Transform algorithm (FFT), although a very much slower general DFT computation does not require the samples to be equally spaced.
The power transmission measurement apparatus 606 splits the incoming ligthwave in two paths for the purpose of measuring the power of the ligthwave at both the input and output of the DUT, i.e. Pin(ν) and Pin(ν) respectively, so that the transmission through the DUT, T(ν)=Pout(ν)/Pin(ν), can be computed afterward. Power transmission measurement apparatuses commonly used in the classic Mueller Method, or in simpler insertion loss measurements, may be used for this purpose.
The power transmission measurement apparatus 700A comprises an optical fiber power coupler 702, which may consist of a singlemode fiber coupler, to extract a portion of the input test lightwave toward a first photodetector 704 in order to measure values of input optical power Pin. A second photodetector 706 received the test signal lightwave at the output of the DUT to measure values of output optical power Pout.
The power transmission meaurement apparatus 700B is similar to apparatus 700A but for the optical fiber coupler 702 that is replaced by a bulk beam splitter 712 and a pair of collimating lenses 708, 710.
The power transmission curve T(ν) is obtained by sampling both Pout and Pin while scanning the optical frequency ν. Data Sampling can be applied using conventional data sampling.
Referring to the
Assuming for example δτ0=3 ns and δτ1=1 ns, then with r=3, the total extent in the delay domain, τ+, is about 5 times the spacing τg between sidebands (τ+˜5 τg). Since f+=vsτ+, then f+˜5 vsτg. To avoid aliasing artefacts, the sampling frequency should be fe≥2 f+. Therefore, if vs=10 THz/s for example, i.e. vs.λ˜80 nm/s@λ=1550 nm, then f+=50 kHz and fe should be greater than 100 kHz.
The following care should be taken regarding the anti-aliasing filter 802. It is a well-known and good practice to limit the bandwidth of the signal (including wideband noise and/or high-frequency spurious) before sampling. But here, care should be taken to make the filter response substantially flat over the range −f+ to f+ because any attenuation of the sidebands by the anti-aliasing filter 802 will result in a bias on the measured PDL. Indeed, the PDL is directly represented by the amplitude of the sidebands (relative to the mean DC part). So only 1% attenuation translates directly to roughly −1% bias. A good choice in that case may be a second-order filter which gives a flat response over a large range relative to its 3-dB cut frequency.
Care should also be taken to sample all signals (Pφ, Pin, Pout) synchronously (negligible delay between them). Of course, the requirement becomes more stringent as the scan speed increases.
Before describing the RBS processing in detailed steps, it is worth exposing an analytical expression of matrix that may be implemented in the algorithm in the case of embodiments using the passive SOP generator. Remind that matrix represents the system of equations to be solved by the RSB processing in accordance with equation (8), and only depends on the known trajectory of the input-SOP as stipulated by (9). Yet more precisely, what is given below in equations (13) are analytical expressions of the complex vectorial amplitudes that appear in the general expression (9) of matrix .
The trajectory ŝ(ν) of the SOP at the output of the 2-segs of the passive SOP generator, which is characterized by said complex vectorial amplitudes as specified in (2), only depends on two parameters, the two coupling angles φŝo and φp, or equivalently the three governing Stokes vectors ŝo, p0 and p1. Remind that ŝo is the SOP at the input of the 2-segs, whereas p0 and p1 are the PSPs of first and second segment respectively. Said analytical expressions of the given below derive from the laws of Physics. The specific set of equations (13) assumes that the following conditions are met:
Setting p1=û1 as mentioned above, ŝo, po and p1, are computed as,
p1=Stokes(0,0)
p0=Stokes(−φp,0)
ŝo=Stokes[(φšo−φp),0] (12)
where Stokes(φ, ψ) represents the specification of a 3-element unit Stokes vector in terms of spherical coordinates. Of note is that ψ=0 (“equator” of the Poincaré sphere) is the circle encompassing all possible linear SOPs.
Then the announced analytical expressions of the complex vectorial amplitudes , with =−4.4 since here J=4 for the specified r≥2.5, reads as,
z0=(cos φšo cos φp)p1
z1=½[cos φšo(p0−cos φpp1)]+i½[cos φšo(p1×p0)]
z2=¼[ŝo−cos φ′šp1+cos φšo(cos φpp1−p0+vxx]+i¼[(p0−p1)×ŝo+cos φšo(p1×p0)]
z3=½(cos φ′š−cos φp)p1
z2=¼[ŝo−cos φ′šp1+cos φšo(cos φpp1−p0+vxx]+i¼[(p0−p1)×ŝo+cos φšo(p1×p0)]
= (13)
where we defined cos φ′š=(p1·ŝo) and vxx=p1×(p0×ŝo). Whenever the above specified conditions 1) and 2) are met, the values (13) of the can be put in (9) to construct matrix and then compute the response vector of the DUT according to (8) and (10).
After some usual data conditioning of the sampled data, e.g. cropping ends having transients, resampling and/or decimation if necessary or useful, etc., the inputs to the processing of RSB are:
(1) a vector T of N values Tn=T(νn) of the power transmission curve, n=0 . . . (N−1), at optical frequencies νn with a substantially constant step dν between successive samples. T is computed beforehand from the sampled outputs Pin(νn) and Pout(νn) as Tn=Pout.n/Pin.n.
(2) a vector Pφ of N values Pφ.n=Pφ(νn) of the phase reference output Pφ(ν) at the same optical frequencies vνn as for T.
The processing of these inputs by RSB is described in detail below in the form of comments, definitions and other pertinent information put around the actual procedures applied to real data.
In step 1002, a processing unit receives the sampled phase reference output Pφ(νn) or, more specifically, a vector Pφ of N values Pφ.n=Pφ)(νn) of the phase reference output at optical frequencies νn, n=0 . . . (N−1). From these values, the procedure of step 1002 derives the phases (νn) of the sideband-carriers with =1 to J, n=0 . . . (N−1), which are used in step 1004 (Procedure_2).
In step 1004, the processing unit receives the sampled power transmission curve T(νn) or, more specifically, vector T of N values Tn=T(νn) of the power transmission curve at optical frequencies νn, n=0 . . . (N−1). From these values, the procedure of step 1004 extracts individually each sideband from the DFT of said vector T to compute complex transmissions (νn) with =−J . . . J, n=0 . . . (N−1).
The procedure involves:
More specifically, at the end of Procedure_2 the processing unit reshuffles the resulting (νn) data into a single vector | of N values |n at sampled points n, wherein each |n is itself a vector whose elements are the 9 values (νn) where −4≤≤4. This reshuffling is not fundamentaly required, but it eases the next calculations in Procedure_1 by making them faster than otherwise, as well as making this procedure very compact from a programmatic point of view.
In step 1006, the processing unit receives the complex transmissions (ν) derived in step 1004, or more specifically vector |, and computes the response vector |m(ν) of the DUT.
More specifically, the processing unit computes |m(νn)) from vector |n obtained in step 1004 and known matrix defined hereinabove, for each sampled point n=0 . . . (N−1)).
In step 1008, the processing unit computes the spectrally-varying PDL of the DUT from the response vector |m(ν).
The input to the procedure is a vector |m of N values |mn=|m(νn) of the response vector, n=0 . . . (N−1), wherein each |mn is itself a 4-component vector. The output may comprise a vector PDL or PDLdB of N values PDLn or PDLdB.n of the PDL of the DUT at optical frequencies νn, where n=0 . . . (N−1). Of note is that, in accordance with the most widespread definition and tradition, the PDL value returned by Procedure_0 is expressed in dB.
The embodiments described above are intended to be exemplary only. The scope of the invention is therefore intended to be limited solely by the appended claims.
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Number | Date | Country | |
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Number | Date | Country | |
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