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Nov 10, 2006 - Frequency-domain intermodal interferometer for the bandwidth measurement of a multimode fiber. Tae-Jung Ahn, Sucbei Moon, Soan Kim, ...
Frequency-domain intermodal interferometer for the bandwidth measurement of a multimode fiber Tae-Jung Ahn, Sucbei Moon, Soan Kim, Kyunghwan Oh, Dug Young Kim, Jens Kobelke, Kay Schuster, and Johnnes Kirchhof

A new bandwidth measurement technique for a multimode optical fiber (MMF) using a frequency-domain intermodal interferometer is proposed. We have demonstrated that the relative modal delay (RMD) of a MMF can be obtained easily and accurately based on an optical frequency-domain reflectometry (OFDR) technique by using an intermodal interference signal among the excited modes of a MMF. As an example, a photonic crystal fiber with a few modes is prepared and its RMD is measured by using our proposed measurement technique. Measurement results are compared with those from a previously reported frequency-domain method. We have also measured the RMD of a commercial MMF as a practical application and compared our result with the one obtained from a well-known time-domain differential mode delay measurement technique. © 2006 Optical Society of America OCIS codes: 060.2300, 120.3180.

1. Introduction

Recently, multimode optical fibers (MMFs) have been employed to increase data capacity of local area networks. In particular, the development of a new type of MMF has been focused on decreasing its modal dispersion or differential mode delay (DMD), which limits the bandwidth of Ethernet communications. As examples, a plastic optical fiber with a W-shaped refractive index profile has been demonstrated to enhance the modal bandwidth in optical fiber links,1 and a multimode dispersion compensation fiber based on silica glass has been demonstrated to overcome the modal dispersion at the wavelength of 850 nm in gigabit Ethernet.2 The dispersion characteristics of specialty optical waveguides, such as a hollow optical fiber,3 a photonic crystal fiber (PCF),4 and a planar light-wave circuit,5 with several modes have been studied for the applications of dispersion management and compensation. Thus, a reliable measurement tool for modal disperT.-J. Ahn ([email protected]), S. Moon, S. Kim, K. Oh, and D. Y. Kim are with the Department of Information and Communications, Gwangju Institute of Science and Technology, 1 Oryongdong, Buk-gu, Gwangju 500-712, South Korea. J. Kobelke, K. Schuster, and J. Kirchhof are with the Institut für Physikalische Hochtechnologie Jena, e. V. Albert Einstein-Strasse 9, 07745 Jena, Germany. Received 20 December 2005; revised 31 March 2006; accepted 14 April 2006; posted 13 July 2006 (Doc. ID 66792). 0003-6935/06/328238-06$15.00/0 © 2006 Optical Society of America 8238

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sion of a MMF is required to exploit optimized MMFs. The time-domain measurement method utilizing pulse broadening in a MMF has been traditionally used to analyze its modal dispersion.6 The time-domain measurement system consists of a pulsed laser with a temporal width of a few tens of picoseconds, a single-mode optical fiber as a probe, an offset launching positioner or mode scrambler to excite all modes, and a streak camera5 or an optical sampling oscilloscope with a high-speed photodetector (PD).1,2,6 Recently, the Telecommunication Industry Association standardized the DMD as an important specific value for a MMF and its measurement method in the time domain with a micrometer-order axial offset launching scanning system.7 However, this time-domain DMD measurement method based on pulse broadening has several disadvantages, such as its long measurement time, complex structure, and expensive cost. Using this method, it is also difficult to obtain the dispersion under a wide range of optical wavelengths since pulse lasers are available only at particular optical wavelengths. Furthermore, the measurement resolution limitation of the time-domain measurement method that depends on the optical pulse width of the laser used in the measurement setup makes it difficult to measure the bandwidth of a short-length MMF. Commercially available bandwidth measurement systems can generally measure a MMF that is over 500 m in length at a 850 nm wavelength. Because adequate gigabit Ethernet links are usually built using shorter (a few hundred meters) fiber, a reliable bandwidth

measurement method with an enhanced high resolution for shorter fiber lengths is needed. In addition, the commercial method mentioned above cannot measure the value of a long MMF due to high chromatic dispersion and optical loss at short optical wavelengths such as 850 or 650 nm. To overcome these problems, we have recently proposed a new very-high-resolution modal delay measurement method for a MMF by using a modified optical frequency-domain reflectometer (OFDR) with a frequency-swept laser and a Mach–Zehnder interferometer instead of a Michelson interferometer.8 –10 DMD resolution with our proposed OFDR technique is more than an order of magnitude better than a result obtainable with a conventional time-domain method. In this paper we propose a much more simplified optical frequency-domain bandwidth measurement technique by using the intermodal interference among the excited modes of a MMF used as the fiber under test (FUT) instead of a Mach–Zehnder interferometer. With this new measurement scheme, we do not have to form a Michelson or Mach–Zehnder interferometer, where a proper length of a single-mode fiber (SMF) that is compatible with the length of a FUT needs to be installed in the reference arm of an interferometer to compensate chromatic dispersion effects in measurement. This proposed method also removes the radial offset launching position stage in a typical OFDR setup for modal delay measurement. We have measured the bandwidth of a MMF that supports a few modes and compared this with another frequency-domain measurement result at a 1550 nm wavelength. We have also compared the bandwidth of a commercial MMF measured with our proposed method using a frequency-domain intermodal interferometer (FDI-I) with the result obtained by a traditional time-domain DMD measurement method. 2. Experiments and Results

Figure 1 is a schematic diagram of our previously reported experimental setup with a Mach–Zehnder interferometer to measure the DMD of a MMF using an OFDR technique. A tunable light source (TLS) (Agilent Inc., 81640A) was operated within its tuning range of 1522–1524 nm to generate a linearly timevarying optical frequency (like a sawtooth waveform) as shown in the dotted box above the TLS in Fig. 1. The frequency tuning rate, which is defined as the slope of the swept instantaneous frequency as a function of time, was set to 647 GHz兾s. The output optical power of the TLS was kept constant at 2 mW during the frequency tuning process. The beating signals, whose frequencies carry the information about time delays of the excited modes in a MMF, were acquired using a data acquisition (DAQ) board with a triggering signal generated by the TLS at the sweep starting time. The first 3 dB optical fiber coupler just after the TLS divides the optical power of frequency-swept light from the TLS by two. Fifty percent of the output optical power is directed into an auxiliary interferom-

Fig. 1. Frequency-domain interferometric setup for DMD measurement of a MMF. BS, beam splitter; PC, polarization controller.

eter, as shown in the dashed box in Fig. 1, while the other 50% of the laser output is used in the main interferometer to measure a sample fiber. The auxiliary interferometer is used to measure the nonlinearity of the frequency sweep of the TLS by obtaining the phase information of a beating signal through Hilbert transformation and thus to reduce the effect of a nonlinear frequency sweep from the TLS in our experiments.11–13 A detailed operational principle of the auxiliary interferometer for obtaining the nonlinear frequency-swept information of a TLS can be found in Ref. 13. Optical power in the main interferometer is split into a reference arm and a test arm, which are made of a SMF and a FUT, respectively, by using a 3 dB fiber coupler. In this case, a proper length of an SMF that is compatible with the length of a FUT needs to be installed in the reference arm of an interferometer. A wave propagated through the FUT is combined with another wave from the reference arm of the interferometer by using a bulk beam splitter and two objective lenses, as shown in Fig. 1. These two waves interfere at a PD that has a detector area of 1 mm2 and a bandwidth of 125 kHz. A beating signal in the PD was acquired by using a DAQ board with a bandwidth of 1.2 MHz, and the beating spectrum was obtained by Fourier transformation of the signal. A homemade PCF that supports a few modes at a 1550 nm wavelength was used as a FUT. As illustrated in the dashed box at the bottom of Fig. 1, an offset launching method with a radial offset of ⬃10 ␮m between a launching SMF and the PCF was adapted to excite all the possible modes in the fiber.14 A polarization controller in the reference arm is to ensure high visibility of the interference signal. Figure 2(a) shows an interference signal obtained with our conventional OFDR system with a MMF. There are two different frequency components in this interference data; a fast oscillating component around 1 kHz frequency is embedded in a slowly oscillating signal of 100 Hz frequency. The high-frequency component oscillates too fast to be seen in the figure, and it makes the data look like a thick line; the dark region in the graph is due to fast oscillation. The high-frequency component is due to interference between lights from the two different arms of the 10 November 2006 兾 Vol. 45, No. 32 兾 APPLIED OPTICS

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Fig. 2. (a) Beating signal from both EMI and IMI in a conventional OFDR setup and (b) interfered signal by IMI after blocking the reference light using a shutter in front of a cubic beam splitter in the OFDR system.

Mach–Zehnder interferometer, that is, a SMF as a reference arm and a PCF as a FUT. We call this external mode interference (EMI). The low-frequency component originates from the intermodal interference (IMI) among the excited modes of a MMF. This slowly oscillating IMI signal is used in many optical fiber sensors.15–17 Low-frequency beating components in an IMI correspond to the temporal delays associated with propagation time differences among modes, whereas high-frequency components in an EMI are linearly proportional to the differences in temporal delay between the fundamental mode of the reference SMF and the excited modes in a MMF. We have observed that the fast-oscillating EMI signal disappeared when the reference light from the SMF was blocked with a shutter placed in front of a cubic beam splitter in Fig. 1. Figure 2(b) shows only the slowly varying IMI signal without the reference light. The slow oscillation in Fig. 2(a) is outwardly consistent with that in Fig. 2(b). To analyze the beating signal in Fig. 2(a), the spectrum of the beating signal was obtained by Fourier transformation. The frequency axis in the spectrum is converted to a time scale with a conventional technique used in an OFDR by dividing the frequency domain on the abscissa by the settable optical frequency sweep rate.9 Here, the frequency-swept rate was set to ⬃645 GHz兾s at the lasing wavelength of 1522 nm. Figure 3 shows the analyzed relative group delays of both EMI and IMI signals in Fig. 2(a) after the time domain was divided once again by a sample fiber length of ⬃20 m. The intensity was also normalized by the peak value in this graph. There are two groups of peaks in this relative group-delay plot; the first group that shows small relative group delays around 10 ps兾m results from the IMI in the PCF near 100 Hz frequency in Fig. 2(a), whereas the second group with large relative group delays around 70 ps兾m is due to the EMI between the reference 8240

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Fig. 3. Analyzed relative group delays for IMI and EMI signals of Fig. 2(a).

light from the SMF and the excited modes in the PCF near 1 kHz frequency. From the peaks of the large group delay, we have verified that the offset launching method between a probe SMF and the PCF was good enough to excite all three linearly polarized modes (M1, M2, and M3) at a 1522 nm wavelength. The inset in Fig. 3 shows the magnification of the three peaks in relative group delay in the IMI signal. There are also three peaks (P1, P2, and P3) corresponding to the interferences among the three excited modes in the PCF. To verify the accuracy of the modal delay measurement method with an IMI signal, we have compared the relative group delays measured with an IMI signal with those measured with an EMI signal. Relative group delays among three excited modes in our PCF sample were measured by using both EMI and IMI signals and compared at three different operating wavelengths of 1522, 1538, and 1572 nm in Table 1 instead of three different MMF samples. P1, P2, and P3 are three peaks of relative group delays among the three guiding modes of the sample PCF while M1, M2, and M3 are relative group delays between the fundamental modes of the reference SMF and the three excited modes of the PCF. From M1, M2, and M3 we have calculated three relative group delays among excited modes in the PCF sample corresponding to P1, P2, and P3. ⌬M1 in Table 1 is group-delay difference between the M1 and M2 peaks in Fig. 3. Similarly ⌬M2 and ⌬M3 are defined as group-delay differences between M3 and M2 peaks and M3 and M1 peaks, respectively. The errors shown in the last column of Table 1 give the difference between P3 and ⌬M3 for a given wavelength. At the wavelength of 1522 nm, the error between P3 and ⌬M3 is ⬃4.6%. At the different operating wavelengths of 1538 and 1572 nm, the group delay of each mode is changed due to the chromatic dispersion of the sample PCF, which causes ⌬M1 to become larger than ⌬M2 at the longer wavelength. The errors between P3 and ⌬M3 at the wavelengths of 1538 and 1572 nm are ⬃4.4% and 2.2%, respectively. This shows that the relative group de-

Table 1. Time-Delay Components by IMI (P1, P2, and P3) and Time-Delay Differences (⌬M1, ⌬M2, and ⌬M3) among Three Excited Modes (M1, M2, and M3) by EMI at the Three Different Operating Wavelengths of 1522, 1538, and 1572 nma

␭ (nm)

P1

P2

P3

⌬M1 (⫽ M2 ⫺ M1)

⌬M2 (⫽ M3 ⫺ M2)

⌬M3 (⫽ M3 ⫺ M1)

Error (%)

1522 1538 1572

5.19 4.56 5.16

6.02 5.66 5.92

10.38 11.21 11.46

5.31 5.54 6.04

5.67 5.18 5.67

10.86 10.72 11.71

4.6 4.4 2.2

a

Columns 2– 6 are in units of picoseconds per meter.

lays among excited modes of a multimode sample fiber calculated from a measured IMI signal are consistent with the relative group delays calculated from an EMI signal. Here, P3 as the largest value in calculated relative group delays from the IMI signal is the relative modal delay (RMD) of the sample fiber, which is defined as the maximum group-velocity difference between the fastest and slowest modes in a MMF.6,7 Our measurement results show that the modal dispersions of the PCF at 1522, 1538, and 1572 nm wavelengths are ⬃10.38, 11.21, and 11.46 ps兾m, respectively. Therefore, we can conclude that the RMD of a MMF can be easily determined by measuring the largest relative group delay in an IMI signal with a simple OFDR measurement setup. We have measured the bandwidth of a commercially available MMF by using an IMI signal without a reference fiber and compared our result with the one obtained from a conventional time-domain method. Figure 4 shows a schematic diagram of our experimental setup for bandwidth measurement of a MMF using a FDI-I with an optical frequency-swept laser. We used an external-cavity tunable laser source that was operated over a tuning range of 1545–1550 nm with a tuning rate of 625 GHz兾s. An auxiliary interferometer shown inside the dashed box in Fig. 4 was also used to compensate the nonlinear swept frequency of the laser source. Optical power was kept constant at 2 mW during the frequency tuning process. In our new setup shown in Fig. 4, we have removed the reference arm of the Mach– Zehnder interferometer containing a polarization controller, bulk optical components, and a radial offset launching position stage used in Fig. 1. A mode scrambler (MS-1, Newport Inc.) was used at the be-

Fig. 4. Our simple DMD measurement setup for a MMF using an intermodal interferometer and an optical frequency-domain interferometric technique with an optical frequency-swept laser. PC, polarization controller.

ginning of a sample MMF to excite all the possible modes in the fiber. The corrugation pitch of this scrambler is ⬃87.5 ␮m to obtain an optimum excitation of modes. The sample MMF was a 48 m long InfiniCor SX⫹ 50兾125 from Corning Inc., which is optimized for an 850 nm wavelength. Unlike in the previous experiment, the light from a launching SMF was put into the center of the MMF without any radial offset to obtain optimum power coupling. Output optical power from the other end of the MMF was directly butt coupled into a PD whose area is ⬃1 mm2, which is much larger than the effective area of the MMF. A frequency-domain intermodal interference signal was measured with a DAQ board and its spectrum was obtained by fast Fourier transformation. The calculated frequency spectrum is once again converted into a graph that shows relative group delays between the excited modes of the MMF by using the same OFDR technique introduced in Fig. 3. The dashed and solid curves in Fig. 5 show relative group delays between excited modes without and with a mode scrambler, respectively. There are few visible peaks in the spectrum from an IMI without mode scrambling, whereas several peaks are generated with proper mode scrambling. The temporal position of the last peak in Fig. 5 represents the relative group delay between the fastest and the slowest modes and is the RMD of the sample MMF. It shows that the RMD of this fiber is ⬃1.36 ps兾m.

Fig. 5. Relative group delays between excited modes in a sample MMF measured with our FDI-I without (dashed curve) and with (solid curve) mode scrambling. 10 November 2006 兾 Vol. 45, No. 32 兾 APPLIED OPTICS

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Fig. 6. Split modes in the MMF as a function of axial offset position in the time domain obtained from directly measured pulse separation.

The DMD of the commercially available Corning MMF was also measured by using a conventional time-domain measurement method7 with a shortpulse laser and a radial offset launching system. A gain-switched short-pulse laser (OPG-100, Optune Technologies Inc.) operating at a 1550 nm wavelength with a pulse width of 40 ps and a scanning radial offset launching system with a step size of 1 ␮m were used. We used the same MMF as in the previous experiment, but its length 共450 m兲 had to be longer than the previous one 共48 m兲 due to poor DMD resolution of the time-domain DMD measurement method. The output optical pulse through the sample MMF was measured using a fast PD with 10 GHz bandwidth and was directly monitored and analyzed by a sampling oscilloscope at each offset launching position. Output pulse forms are plotted in the time domain for various offset launching positions and are shown in Fig. 6. Forty-eight curves are separated by a constant space from the top to the bottom. The uppermost curve is when the offset is 24 ␮m and the lowermost curve is when the offset is ⫺24 ␮m. Each waveform has a 1 ␮m difference in its offset launching position compared with its upper or lower adjacent curve and was normalized with respect to its maximum value. Figure 6 shows that the sample MMF has eight supporting mode groups. The fastest mode group is excited when the input pulse is launched at the center of the MMF. Slowly propagating modes are excited when the offset is increased and the slowest mode group is excited when the input light is launched at the boundary between the core and the cladding of the MMF or when the offset is 24 ␮m. From the depiction in Fig. 6, the RMD was found to be ⬃1.38 ps兾m when we subtracted the time value 共0.72 ps兾m兲 of the fastest mode from that 共2.10 ps兾m兲 of the slowest mode. The value is very close to the RMD value obtained 共1.36 ps兾m兲 by using the FDI-I with an error of ⬃1.3%. Therefore, we have verified that the measured RMD valued of a MMF by using our suggested 8242

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measurement method is consistent with the one obtained by a conventional time-domain measurement method. Our RMD measurement method based on the IMI has several advantages compared with the conventional time-domain method or the previously reported frequency-domain interferometric method using an EMI signal.8,9 First, our proposed method with a FDI-I yields a much better RMD resolution compared with the time-domain method due to the availability of a high-speed frequency-swept laser source combined with well-established optical frequency-domain reflectometer techniques. For example, the resolution of our measurement was ⬃0.058 ps兾m by evaluating the full width at half-maximum (FWHM) of peaks in the relative group-delay graph of Fig. 5. This means that we can measure at least a 0.058 ps time difference in measured group-delay data for a MMF of 1 m in length. However, in the conventional measurement, the resolution is estimated to be ⬃6.3 ps兾m based on the average FWHM of a peak in Fig. 6. Thus the resolution of our proposed method is a hundred times better than that of the conventional RMD measurement method. Second, our method can be used to measure longlength MMF without using a reference SMF. The coherence length or the instantaneous linewidth of a frequency-swept light source limits the measurable fiber length of a MMF in a conventional frequency-domain interferometric method based on an OFDR.8 –12 When the length difference between a sample fiber and a reference fiber in a conventional interferometric method is over the coherence length (⬃1 km) of our TLS with a linewidth of ⬃300 kHz, the visibility of the interference signal is not strong enough and phase noise is increased in the interference signal with an increasing length of the sample fiber. Therefore, a reference fiber with a proper length is required to maintain the length difference between the sample fiber and the reference SMF below a coherence length of the laser.8,9 In our case, the differences in group delay after propagation along a 300 km fiber, for instance, is only 408 ns since the RMD of our MMF is 1.36 ps兾m as shown in Fig. 5. The value of 408 ns means that the optical path difference between the fastest mode and the slowest mode in a MMF is 816 m 共⫽ 3 ⫻ 108 m兾s ⫻ 408 ns兾1.5) assuming the core index of the MMF to be 1.5. As this length difference is smaller than the coherence length of our TLS, which is 1 km, we can measure the RMD of our MMF up to a 300 km sample distance by using our proposed DMD measurement method with a FDI-I when a TLS whose linewidth is ⬃300 kHz is used. Finally, the experimental setup for our FDI-I is simple and economical compared with any other methods for the RMD measurement of a MMF. The conventional time-domain measurement method requires expensive equipment such as a short-pulse laser source, a streak camera or a sampling oscilloscope to improve its measurement resolution, radial

offset launching positioners, etc. The previously reported frequency-domain interferometric method using an EMI signal8 –10 requires an extra reference fiber and other bulk optics components. With these practical advantages, our proposed RMD measurement method with a FDI-I is a powerful, convenient, and economical tool for analyzing the bandwidth of an MMF. 3. Conclusion

A new measurement method for the RMD of a MMF has been proposed using an intermodal interferometer and an OFDR system. We have measured the RMD of a few-mode PCF with our proposed method by using an IMI signal, and its measured value is compared with the one obtained by using another frequency-domain measurement method that uses an EMI signal. In addition, we have also demonstrated that the RMD of a commercial MMF can be measured with our proposed method. The measured RMD was 1.36 ps兾m and has an error of ⬃1.3% compared with that of a conventional time-domain measurement result. We believe that our new frequency-domain RMD measurement method with a FDI-I and a wellestablished conventional OFDR technique could become a powerful and practical tool for characterizing MMFs. This research was partially supported by the Korea Science and Engineering Foundation through the Ultrafast Fiber-Optic Networks, an Engineering Research Center program of the Gwangju Institute of Science and Technology; by the Korea Institute for Science and Technology 21 programs; and by the Brain Korea 21 Information Technology Project of the Ministry of Education of South Korea. References 1. T. Ishigure, H. Endo, K. Ohdoko, K. Takahashi, and Y. Koike, “Modal bandwidth enhancement in a plastic optical fiber by W-refractive index profile,” J. Lightwave Technol. 23, 1754 – 1762 (2005). 2. N. Guan, K. Takenaga, S. Matsuo, and K. Himeno, “Multimode fibers for compensating intermodal dispersion of graded-index multimode fibers,” J. Lightwave Technol. 22, 1714 –1719 (2004).

3. M. Mohebbi, “Dispersion of femtosecond laser pulses in hollow fibers,” J. Opt. Soc. Am. B 21, 893– 896 (2004). 4. C. E. Kerbage, B. J. Eggleton, P. S. Westbrook, and R. S. Windeler, “Experimental and scalar beam propagation analysis of an air-silica microstructure fiber,” Opt. Express 7, 113–122 (2000). 5. P. May, S. Basu, G. L.-T. Chiu, and G. Arjavalingam, “Modal dispersion and attenuation measurements of silicon nitride and silicon oxynitride waveguides using a streak camera,” J. Lightwave Technol. 8, 235–238 (1990). 6. R. Olshansky and D. B. Keck, “Pulse broadening in gradedindex optical fibers,” Appl. Opt. 15, 483– 491 (1976). 7. Telecommunication Industry Association, “Differential mode delay measurement of multimode fiber in the time domain,” TIA-455-220-A (2003). 8. T.-J. Ahn, S. Moon, Y. Youk, Y. Jung, K. Oh, and D. Y. Kim, “Mode analysis and modal delay measurement of a few-mode fiber by using optical frequency domain reflectometry,” J. Opt. Soc. Korea 9, 54 –58 (2005). 9. T.-J. Ahn, S. Moon, Y. Youk, Y. Jung, K. Oh, and D. Y. Kim, “New optical frequency domain differential mode delay measurement for a multimode optical fiber,” Opt. Express 13, 4005– 4011 (2005). 10. T.-J. Ahn and D. Y. Kim, “High-resolution differential mode delay measurement for a multimode optical fiber using a modified optical frequency domain reflectometer,” Opt. Express 13, 8256 – 8262 (2005). 11. R. Passy, N. Gisin, J. P. von der Weid, and H. H. Gilgen, “Experimental and theoretical investigations of coherent OFDR with semiconductor laser sources,” J. Lightwave Technol. 12, 1622–1630 (1994). 12. U. Glombitza and E. Brinkmeyer, “Coherent frequencydomain reflectometry for characterization of single-mode integrated-optical waveguides,” J. Lightwave Technol. 11, 1377–1384 (1993). 13. T.-J. Ahn, J. Y. Lee, and D. Y. Kim, “Suppression of nonlinear frequency sweep in an optical frequency domain reflectometer by using Hilbert transformation,” Appl. Opt. 44, 7630 –7634 (2005). 14. L. Jeunhomme and J. P. Pocholle, “Selective mode excitation of graded index optical fibers,” Appl. Opt. 17, 463– 468 (1978). 15. A. M. Vengsarkar, W. C. Michie, L. Jankovic, B. Culshaw, and R. O. Claus, “Fiber-optic dual technique sensor for simultaneous measurement of strain and temperature,” J. Lightwave Technol. 12, 170 –177 (1994). 16. D. Menashe, M. Tur, and Y. Danziger, “Interferometric technique for measuring dispersion of high order modes in optical fibres,” Electron. Lett. 37, 1439 –1440 (2001). 17. T. Okoshi, Optical Fibers (Academic, 1982).

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