A polarimeter is an instrument that measures the polarization state (or state of polarization (SOP)) of an optical signal, thereby enabling its user to 1) determine an unknown polarization state of the optical signal, or 2) determine whether the polarization state of the optical signal changes. Also, and by measuring the polarization state of an optical signal that is transmitted through a material, a polarimeter can be used to ascertain various optical properties of the material, such as linear birefringence, circular birefringence, linear dichroism, circular dichroism and scattering.
Most frequently, polarimeters determine a polarization state by estimating the power transmitted through polarizers of different types. See, for example, D. Derickson, Ed., Fiber Optic Test and Measurement, Prentice-Hall (1997). In some cases, measurements from the different types of polarizers are taken sequentially, i.e., after a power measurement is taken for one type of polarizer, the polarizer is reconfigured to another type of polarizer, and another power measurement is taken. Depending on the polarizer, reconfiguration can be accomplished via rotation of an element, or via insertion/removal of one or more optical elements (e.g., waveplates).
Sequential mechanical reconfiguration of a polarizer is inherently slow. As a result, an optical signal is often split into multiple signals, with each of the signals being simultaneously transmitted through a polarizer of a different type. However, while increasing measurement speed, the use of multiple polarizers is more complex and more expensive. Furthermore, the multiple optical channels of a parallel implementation need to be properly calibrated to provide accurate measurements.
Illustrative embodiments of the invention are illustrated in the drawings, in which:
Having provided a brief overview of the components and operation of the polarimeter 100, each of its components will now be described in detail, beginning with the modulated polarizer 102.
As mentioned above, a modulated polarizer 102 is modulated at a modulation frequency and is configured to transmit a portion 110 of an optical signal 108 based on its (i.e., the modulated polarizer's) modulation. From one perspective, the modulated polarizer 102 can be thought of as a polarizer whose type is modulated. From another perspective, the modulated polarizer 102 can be thought of as a polarizer that alters, at one or more modulation frequencies, an alignment between 1) a vector that represents the input polarization state of an optical signal 108, and 2) a vector that represents the modulated polarizer 102. The alignment of the vectors is altered by modulating the orientation of the vector that represents the modulated polarizer 102. As the alignment of the vectors is altered, the modulated polarizer 102 transmits a portion 110 of the optical signal 108 based on the altered alignment.
As described in the preceding paragraph, the modulated polarizer 102 and the input polarization state of the optical signal 108 can both be represented by vectors, however, for simplicity the term “vector” will often be omitted in this description.
In one embodiment, and as shown in
As the alignment between the modulated polarizer 102 and the input polarization state of the optical signal 108 is altered, the portion 110 of the optical signal 108 that is transmitted by the polarizer 202 is altered as well. That is, when the polarization controller 200 alters the modulated polarizer 102 such that its type is aligned with the input polarization state of the optical signal 108, all of the optical signal 108 (ideally) is transmitted by the polarizer 202. However, when the polarization controller 200 alters the modulated polarizer 102 such that its type is orthogonal to the input polarization state of the optical signal 108, none of the optical signal 108 (ideally) is transmitted by the polarizer 202. The orthogonality of the polarizer and the input polarization state corresponds, in the vector space of
Preferably, the polarization controller 200 alters the optical signal 108 in a continuous manner, and without substantially altering the power (or intensity) of the optical signal 108. Specifically, and considering for a moment an optical signal that propagates through the modulated polarizer 102 in the reversed direction, the modulation of the polarizer 102 is uniquely described by a transformation of the polarization state of an optical signal that passes through the polarizer 202 and into the polarization controller 200 in the reversed direction. The new polarization state is defined by the polarization controller 200. By reciprocity only that new polarization state is fully transmitted through the polarizer 202 when an optical signal propagates through the modulated polarizer 102 in the forward direction. Thus, by examining that transformation, we can precisely determine the polarizer modulation.
The polarization state of an optical signal, as well as a polarizer type, can be described in terms of Stokes vectors. The Stokes vector has four components, S0-S3. The first component, S0, is the intensity of the optical signal, and the remaining three components describe the polarization state of the optical signal. The polarization state of the optical signal is represented as a vector in a three dimensional space, in which the three axes can be viewed as representing the content of different types of polarized light found in the optical signal.
Refer now to
In the context of the polarization space shown in
Refer now to
For the purposes of this discussion, it will be assumed that q(t), u(t), and v(t) are periodic functions that define the movement of a time-varying (i.e., modulated) polarizer, P(t), along a particular trajectory. This will be the case if a desired trajectory on the Poincare sphere is a closed loop, and if each modulation cycle of the polarization controller 200 results in the polarizer 102 moving once around the loop. As will be discussed in more detail below, the movement of a time-varying polarizer can also be defined by periodic functions that trace an open path (i.e., not a closed loop) on the Poincare sphere. It should be noted, however, that while q(t), u(t), and v(t) are periodic, q(t), u(t), and v(t) cannot each be pure tones simultaneously. For the components to be pure tones, there must be three modulation frequencies, ωq, ωu, and ωv, for which
q(t)=cos(ωqt)
u(t)=cos(ωut+Du)
v(t)=cos(ωvt+Dv)
q(t)2+u(t)2+v(t)2=1 (1)
where Du and Dv are fixed phase shifts. It can be shown that this system of equations has no solutions.
While a solution in which each of the components is a single tone cannot be found, a solution that only depends on three tones is possible. For example,
q(t)=cos(2ωt)
u(t)=(sin(ωt)+sin(3ωt))/2
v(t)=(−cos(ωt)+cos(3ωt))/2 (2)
The above equations satisfy the constraint q(t)2+u(t)2+v(t)2=1 and describe a trajectory that produces only three tones.
A more detailed discussion of the considerations that go into choosing a particular trajectory on the Poincare sphere is provided below. However, for the purposes of the present discussion, it will simply be assumed that the polarizer 102 has a predetermined trajectory on the Poincare sphere.
Now consider a polarizer 102 described by the normalized Stokes vector, P, where
and where the first component of the Stokes vector (i.e., intensity) is omitted for simplicity. In this description, a polarizer 102 fully transmits the optical signal having a polarization state that is described by the same Stokes vector P (aligned vectors) and fully rejects an optical signal whose polarization state is described by the vector −P that points in an opposite direction.
If the Stokes vector that describes a polarizer modulation executes a closed loop on the Poincare sphere, at an angular frequency, ω, then each polarization dependent component can be expanded in a Fourier series with ω as the fundamental frequency. The number of significant harmonics in the series depends on the details of the trajectory on the Poincare sphere. For example, the trajectory described by Eq. (2) has only three significant harmonics. In the more general case, the components of the Stokes vector can be written in the following form:
q(t)=q0+A1,1 sin(ωt+φ1,1)+A1,2 sin(2ωt+φ1,2)+A1,3 sin(3ωt+φ1,3)
u(t)=u0+A2,1 sin(ωt+φ2,1)+A2,2 sin(2ωt+φ2,2)+A2,3 sin(3ωt+φ2,3)
v(t)=v0+A3,1 sin(ωt+φ3,1)+A3,2 sin(2ωt+φ3,2)+A3,3 sin(3ωt+φ3,3) (4)
The constants Aijj and φi,j, where i=1 to 3 and j=1 to N, represent amplitudes and phases of individual harmonics. The constants q0, u0, and v0 represent the unmodulated part of each Stokes component (the 0th harmonic). As will become clear from the following discussion, the number of harmonics that are significant, N, must be at least 3. This excludes some solutions like solutions when a polarization controller behaves like a rotating waveplate generating only two harmonics.
Alternatively, using a complex notation, Eq. (4) can be rewritten in the following form:
q(t)=q0+q1 exp(jωt)+q2 exp(j2ωt)+q3 exp(j3ωt)+
u(t)=u0+u1 exp(jωt)+u2 exp(j2ωt)+u3 exp(j3ωt)+
v(t)=v0+v1 exp(jωt)+v2 exp(j2ωt)+v3 exp(j3ωt)+ (5)
where qm=A1,m exp(jφ1,m), um=A2,m exp(jφ2,m), and vm=A3,m exp(jφ3,m), and where j=√{square root over (−1)} is an imaginary number.
The above equation simply implies that periodic functions can be expressed as sums of harmonics. Conceptually, this property is captured by the following symbolic equation:
where the subscripts denote the number of the harmonic. The exponential terms that represent the frequencies have been omitted for simplicity of notation. It is important to note that the harmonics qi, ui and vi are complex numbers.
The above-described modulations all involve expanding the polarization dependent components of the normalized Stokes vector, P, that describes the modulated polarizer 102 in a harmonic series. That is, each component is expanded in terms of a number of component frequencies, in which the component frequencies are integer multiples of some fundamental frequency. However, as will be discussed in detail below, there are cases in which the polarization dependent components of the modulated polarizer 102 can be expanded in a series in which the frequencies are not integer multiples of a predetermined frequency. Hence, in the general case, it will be assumed that:
q(t)=C1+A1,1 sin(ω1t+φ1,1)+A1,2 sin(ω2t+φ1,2)+A1,3 sin(ω3t+φ1,3)
u(t)=C1+A2,1 sin(ω1t+φ2,1)+A2,2 sin(ω2t+φ2,2)+A2,3 sin(ω3t+φ2,3)
v(t)=C1+A3,1 sin(ω1t+φ3,1)+A3,2 sin(ω2t+φ3,2)+A3,3 sin(ω3t+φ3,3) (7)
As will become clear from the following discussion, there must be at least three frequencies ωj. In the case of a harmonic expansion, ωj=j*ω, where ω is the fundamental frequency.
Refer now to
The manner in which the potentials applied to the crystal 502 are chosen will be explained in more detail below. However, for the present discussion, it is sufficient to note that a first periodic waveform is applied between electrodes 512 and 510, and a second periodic waveform is applied between electrodes 512 and 508. Electrode 512 is a reference (ground) electrode. In general, the waveforms have the same period. By correctly choosing the potentials that are applied to the crystal 502, the effective polarizer 102 can be altered to produce a polarizer described by a time-varying Stokes vector, which time-varying Stokes vector traces a predetermined trajectory on the Poincare sphere, as previously discussed. The potentials applied to the crystal 502 may be chosen such that the trajectory will have its center of gravity at the center of the Poincare sphere.
Now consider the propagation of an optical signal through the modulated polarizer 102 (
Having described an exemplary embodiment and operation of the modulated polarizer 102, reference is again made to the polarimeter 100 (
where the first component of the Stokes vector (i.e., intensity) is omitted for simplicity.
The modulated polarizer 102 transmits a time-varying portion 110 of the optical signal 108 based on an alignment between the modulated polarizer 102 and the optical signal's polarization state. For an instantaneous state of the modulated polarizer 102, the angle between the Stokes vector of the optical signal 108 and the instantaneous state of the modulated polarizer 102, as viewed on the Poincare sphere, is equal to σ. By way of example,
Given the angle σ, the fractional power, f, of the transmitted portion 110 of the optical signal 108, as seen by the detector 104, is:
Alternately, the power, p(t), seen by the detector 104 can be described by the equation:
where the fraction ½ is further multiplied by the intensity of the optical signal 108 (
The detector 104 (e.g., a photodetector) generates a time-varying output signal 112 that is related to the power, p(t). The processing system 106 detects frequency components of the time-varying output signal 112. The detected frequency components correspond to frequency components of the signals that define (or control) the modulated polarizer 102. Thus, the harmonics of p(t) correspond to the harmonics of q(t), u(t), and v(t) that define the modulated polarizer. In particular, the first three harmonics (p1, p2, p3) detected by the processing system 106 can be described by the equation:
where qm, um and vm are the m-th harmonics of q(t), u(t) and v(t) (see Eq. (6)). Eq. (11) shows that the polarization state (x, y, z) of the optical signal 108 can be found by detecting the harmonics p1, p2, and p3 in the time-varying signal 112 generated by the detector 104. Harmonics p1, p2, and p3 may be detected in a synchronous demodulation process utilizing a vector spectrum analyzer or a lock-in amplifier implemented in software or hardware. It is assumed here that the trajectory of the modulated polarizer is known an described by the modulation matrix containing harmonics qi, ui and vi. In order for the solution to exist the determinant of the modulation matrix must be non-zero. It is important to note that the reference phase of the phase sensitive detection process has to be properly chosen in order to provide a real solution for the polarization state (x, y, z). This can be accomplished by testing various reference phases and selecting the one that provides real solutions.
The above-described embodiment of the processing system 106 only detects three harmonics in the signal 112 generated by the detector 104, even in those cases in which the harmonic expansion of the modulated polarizer Stokes vector P (see Eq.(6)) includes additional harmonics or other frequencies. However, embodiments in which more of the components are utilized to provide an over-determined system in which noise is further reduced could be constructed.
The final Stokes vector component that needs to be determined is the intensity, i, of the optical signal 108. Based on Eq. (10), the intensity, i, can be found as the DC component of the time-varying signal 112 generated by the detector 104, under the assumption that q0=u0=v0=0. This assumes that, on average, the modulated polarizer 102 does not favor any polarization component, and that the trajectory of the modulated polarizer 102 is balanced, having a center of gravity in the center of the Poincare sphere. From Eq. (10), and for q0=u0=v0=0,
2p0=i, (12)
where p0 is the DC component of the signal 112 generated by the detector 104. Thus, the DC component of the detector's signal 112 is proportional to the intensity of the optical signal 108, and in some embodiments of the polarimeter 100, the processing system 106 can be configured to determine the intensity i based on Eq. (12).
In some cases, the processing system 106 may be configured to determine a degree of polarization (DOP) of the optical signal 108. The DOP of the optical signal 108 may be determined from the Stokes vector of the optical signal 108 as follows:
Of note, Eq. (11) illustrates how to calibrate the polarimeter 100 (
where (xn, yn, zn) denotes the n-th polarization state of the optical signal 108, pnm denotes the m-th harmonic of the signal 112 detected for the n-th input polarization state, and qm, um, and vm denote the sought harmonics that describe the modulation of the modulated polarizer 102. The above applies to all harmonics m, thus, it determines the trajectory of the modulated polarizer 102.
The optical signal 108 used to calibrate the polarimeter 100 may, in some cases, be provided by a polarized laser light source. However, other light sources, such as light emitting diode (LED) light sources, can also be used. If the light source does not provide light with a constant fixed polarization, a polarization filter can be introduced between the light source and the modulated polarizer 102.
Referring again to the processing system 106 (
One exemplary addition to the polarimeter 700 is an optical coupler 710. The optical coupler 710 may include a fiber pigtail 712 for transmitting the optical signal 108 to the modulated polarizer 702. In the same or different embodiments, the optical coupler 710 may be a single mode (SM) optical coupler having an optical input and first and second optical outputs, wherein the optical input is configured to receive the optical signal 108, wherein the first optical output is configured to transmit a portion of the optical signal to the modulated polarizer 102, and wherein the second optical output is configured to transmit a portion of the optical signal to a second detector 714. If a known fraction of the optical signal is transmitted to the second detector 714, the second detector 714 may generate a signal on line 716 that is related to the intensity of the optical signal 108, thereby eliminating the need for the processing system 706 to determine the intensity of the optical signal 108 from the DC component of the signal it receives from the detector 704. The fraction of optical power diverted to the second detector 714 may be factored into the calculations of the processing system 706.
As also shown in
In the above-described polarimeter embodiments 100, 700 (
Refer now to
The choice of modulated polarizer trajectory, from among those trajectories that generate modulation matrices having non-zero determinants (see Eq. (11)), can be guided by some general principles that are listed below. Trajectories that generate fewer frequencies for all polarization components q(t), u(t) and v(t) of the modulated polarizer 102 are preferred; however, at least three harmonics are required. Only three harmonics are needed to solve for the polarization state (x, y, z). The additional harmonics divert energy that would have gone into the harmonics that are being used; hence, trajectories that generate a significant number of additional harmonics are likely to lead to lower signal-to-noise ratios.
The number of harmonics that are generated by any given trajectory may depend on the number of harmonics in the corresponding voltages that are applied to the electrodes of the modulated polarizer 102. Also, complicated voltage waveforms are more difficult to synthesize, and hence, can lead to more complex driving circuitry for the modulated polarizer 102.
There is also a limit on the voltages that can be generated by the control system 114 and applied to the modulated polarizer 102. Hence, a trajectory on the Poincare sphere must be traversable using voltages that are within some predetermined range of voltages.
Refer now to
The modulation of the components q(t), u(t) and v(t) of the modulated polarizer 102 (
Refer now to
The above-described trajectories on the Poincare sphere are closed loops, and hence, the modulation frequencies are harmonics of the frequency with which the closed loop is traversed. For the purposes of the present discussion, a path will be defined as being closed if it begins and ends at the same point on the Poincare sphere. This will always be the case when polarizer modulation is performed in accord with a periodic function. In some cases, it may be advantageous to use modulation frequencies that are unrelated frequencies instead of harmonics. For example, such unrelated frequencies could reduce some errors caused by harmonics produced by non-linearities of the detector 104 (
q(t)=cos(2ω1t)
u(t)=(sin(2ω1t−ω2t)+sin(2ω1t+ω2t))/2
v(t)=(cos(2ω1t−ω2t)+cos(2ω1t+ω2t))/2 (15)
where ω1=eω/2 and ω2=ω. Here e is the irrational number, 2.71828 . . . . The processing system 106 (