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Optical VSB Filtering of 12.5-GHz Spaced 64 × 12.4 Gb/s WDM Channels Using a Pair of Fabry-Perot Filters
Optical VSB Filtering of 12.5-GHz Spaced 64 × 12.4 Gb/s WDM Channels Using a Pair of Fabry-Perot Filters
Journal of the Optical Society of Korea. 2013. Feb, 17(1): 63-67
Copyright ©2013, Optical Society of Korea
  • Received : October 10, 2012
  • Accepted : January 01, 2013
  • Published : February 25, 2013
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About the Authors
Budsuren Batsuren
Department of Electronic Engineering, Kwangwoon University, Kwangwoon-ro 20, Nowon-gu, Seoul 139-701, Korea
Hyung Hwan Kim
Department of Electronic Engineering, Kwangwoon University, Kwangwoon-ro 20, Nowon-gu, Seoul 139-701, Korea
Chan Yong Eom
Department of Electronic Engineering, Kwangwoon University, Kwangwoon-ro 20, Nowon-gu, Seoul 139-701, Korea
Jin Joo Choi
Department of Electronics Convergence Engineering, Kwangwoon University, Kwangwoon-ro 20, Nowon-gu, Seoul 139-701, Korea
Jae Seung Lee
Department of Electronic Engineering, Kwangwoon University, Kwangwoon-ro 20, Nowon-gu, Seoul 139-701, Korea
jslee@kw.ac.kr
Abstract
We perform an optical vestigial sideband (VSB) filtering using a pair of Fabry-Perot (FP) filters. The transmittance curve of each FP filter is made to have sharp skirts using an offset between input and output coupling fibers. Moreover, the accurate periodicity of FP filters in the optical frequency domain enables the simultaneous VSB filtering of a large number of optical channels. With this VSB filtering technique, we transmit 12.5-GHz spaced 64 × 12.4-Gb/s wavelength-division-multiplexing channels over a single-mode fiber up to 150 km without any dispersion compensations. When the channel spacing is reduced to 10 GHz, we achieve the spectral efficiency of 1 bit/s/Hz in conventional optical intensity modulation systems up to 125 km.
Keywords
I. INTRODUCTION
Optical vestigial sideband (VSB) filtering is a useful method for optical transmission systems to increase spectral efficiencies and transmission distances [1 - 9] . It carves out one of the sidebands from a modulated optical channel using narrow optical filters which will be called VSB filters here. The other sideband still retains the entire modulation information. Optical VSB filtering, henceforth VSB filtering, is simple and additional costs are low.
Recently, coherent optical communication systems have been investigated extensively and will likely be used for 100-Gb/s and higher wide-area networks [10 , 11] . In this case, the two sidebands of a single channel usually have different information. However, the coherent optical communication systems need many subsidiary devices such as lasers, radio-frequency (RF) driver amplifiers, photodiodes, and heavy digital signal processing circuits. Thus the VSB filtering will be still popular, especially in metro and access networks where many wavelength-division-multiplexing (WDM) channels would be used with relatively low bit rates.
The VSB filters should have steep skirts in transmittance curves to remove one of the sidebands efficiently. This is important especially for relatively low bit rate channels in metro and access networks. In addition, it will be advantageous to use a single VSB filter for multiple WDM channels in a parallel way. This property is important to reduce the cost when the channel number is large. Typical VSB filters reported to date are Mach-Zehnder filters [1 , 2] , fiber-Bragg gratings [3 , 4] , optical band-pass filters [5 - 7] , WDM demultiplexers [8] , and optical interleavers [9] . The bit rate of [1] is 6 Gb/s. The bit rates of [2] , [3] , [8] , and [9] are ~10 Gb/s. In other cases, channel bit rates are much higher than 10 Gb/s. Usually, a single VSB filter is needed per channel. In [8] and [9] , 8 channels are VSB filtered simultaneously using a single VSB filter.
In this paper, we suggest using a pair of Fabry-Perot (FP) filters for the VSB filtering. Each FP filter covers even
Lager Image
Experimental setup. LD: laser diode, AWG: arrayed-waveguide grating, PM-C: polarization maintaining coupler, MZM: LiNbO3 Mach-Zehnder modulator, PC: polarization controller, FP: Fabry-Perot, PBC: polarization beam combiner, EDFA: erbium-doped fiber amplifier, SMF: single-mode fiber, BPF: band-pass filter, Rx: optical receiver, BERT: bit-error-rate tester.
or odd channels separately. With an offset between input and output coupling fibers, the FP filters may have very steep skirts in transmittance curves [12] . Moreover, the FP filters naturally have a very accurate periodicity in spectral domain and are appropriate for the simultaneous VSB filtering of many WDM channels. In our experiment, we perform a VSB filtering of 12.5-GHz spaced 64 × 12.4 Gb/s WDM channels. After the VSB filtering, we transmit the WDM channels over a conventional single mode fiber (SMF) of 150 km without any dispersion compensations. To our knowledge, this is the first VSB filtering experiment using FP filters.
II. EXPERIMENT
Our experimental setup is illustrated in Fig 1 . The channel wavelengths ranged from 1554.2 nm to 1560.5 nm with the channel spacing of 12.5 GHz. Four 50-GHz arrayed waveguide gratings (AWGs) were used to multiplex these channelsnel wavelengths were monitored using a wavelength meter. The output power of each laser diode was 0 dBm. Even and odd channels were externally modulated using data and delayed data-bar signals, respectively. The data signal was a 2 31 -1 pseudorandom bit sequence. The modulation format was non-return-to-zero type and the bit rate was 12.4-Gb/s assuming a block-turbo-code (BTC) based forward-error correction (FEC) [13] . Its FEC threshold is at 1.98 × 10 -2 bit error rate (BER) corresponding to a quality factor Q = 6.26 dB.
The VSB filtering was done separately for even and odd channels using a pair of FP filters. Fig. 2 (a) shows the FP filter structure used in our experiment. The FP filter consisted of input/output coupling fibers and two parallel
Lager Image
Fabry-Perot filter with an offset. OSA: optical spectrum analyzer. (a) Schematic of the Fabry-Perot filter with an offset. (b) Photograph of the Fabry-Perot filter with an offset.
glass plate mirrors with a reflectivity of 30 %. The freespectral range (FSR) of the FP filter was 25 GHz obtained by adjusting the distance between two dielectric mirrors. The beam incidence angle to these mirrors, denoted as θ , was 0.5° for the even channel FP filter. It was 0.75° for the odd channel FP filter. We introduced an offset of 200 μm between the input and the output coupling fibers to increase the slopes of skirts in FP filters’ transmittance curves [12] . The filter insertion losses were 8.1 dB and 8.8 dB for the even and the odd channel FP filters, respectively. Also, we show a photograph of our Fabry-Perot filter in Fig. 2 (b). The position of the right coupling fiber was adjusted using a multi-axis positioning stage while the left coupling fiber was fixed. The two mirror mounts were fixed on a rotary stage.
After the VSB filtering, the even and the odd channels were polarization multiplexed using a polarization beam combiner (PBC). The PBC output was amplified using an erbium-doped fiber amplifier (EDFA) and transmitted over an SMF of 150 km. The total launched power was 15 dBm. After the transmission, the received channels were demultiplexed using a 12.5-GHz AWG.
After the 12.5-GHz AWG, we used a tunable 3-nm optical filter to obtain a single channel. The 12.5-GHz AWG had a loss of about 6.1 dB. Unfortunately, the 12.5-GHz AWG had only 24 outputs. Thus its temperature was adjusted to measure the whole 64 channels. The optical power was –12 dBm at the receiver input. A pin photodiode was used at the receiver. We also performed the same experiment changing the bit rate to 10.7 Gb/s assuming a Reed-Solomon (RS) based FEC that has the FEC threshold at BER = 1 × 10 -4 or Q = 11.4 dB [14] .
III. RESULTS AND DISCUSSION
In Fig. 3 , we show the transmittance curves of the odd channel FP filter obtained by applying the amplified spontaneous emission from an EDFA. Three offset values, 0, 100, and 200 μm, are compared. The optical resolution is 0.05 nm. The transmission peak levels are adjusted to be the same. As the offset increases, the skirts become steeper. The insertion losses are 7.5, 7.7, and 8.8 dB for the offset values 0, 100, and 200 μm, respectively. We have fixed the offset to 200 μm in our experiment throughout.
Lager Image
Transmittance curves of the FP filter used for the odd channels at θ = 0.75° with the offset of (a) 0 μm, (b) +100 μm, and (c) +200 μm.
As θ increases, the transmittance peak wavelengths of the FP filters move towards longer wavelengths where we have higher insertion losses and wider transmission bandwidths [12] . In contrast, when θ is too small, the slopes of the transmittance skirts become insensitive to the offset. We have used these properties to implement the even and the odd channel FP filters. For the even channel FP filter, the appropriate θ values for the VSB filtering are 0.5°, 1.0°, 1.5°, etc . We have chosen θ = 0.5° at which the insertion loss and the 3-dB bandwidth are 8.1 dB and 14.8 GHz, respectively. For example, at θ = 1.0°, the insertion loss and the 3-dB bandwidth are 11.9 dB and 16 GHz, respectively. Similarly, for the odd channel FP filter, we have chosen θ = 0.75° where the insertion loss and the 3-dB bandwidth are 8.8 dB and 15.1 GHz, respectively. We have not chosen θ = 0.25° since the skirts are not steep. The FP filter transmission peaks are 0.05 nm shifted to longer wavelengths from the channel centers.
Figure 4 shows the RF spectra of the 41st channel before and after the odd channel FP filter measured by a heterodyne detection with a tunable laser [15] . The tunable laser line is placed near the end of the sideband suppressed by the VSB filtering. Note that the RF spectra in Fig. 4 are for electrical fields not intensities. The suppression of the sideband intensity is twice that of the fields, around 10 dB. The heterodyne detection gives very precise shapes of fields before and after the VSB filtering. Fig. 5 spectrum of the 64 channels after the PBC.
Figure 6 shows the Q-factor values after 125 and 150 km without any dispersion compensations. All of the Q-factor values are above the FEC threshold. For the 125-km transmission, the minimum BER is 1.1 × 10 -3 . For the 150-km transmission, the minimum BER is 1.9 × 10 -2 . Thus, if we neglect the system margin, 150 km is the maximum transmission distance of our system. Without the VSB filtering, the maximum transmission distance of the same system is measured to be less than 100 km.
Lager Image
Spectra of a single channel measured by a heterodyne detection technique (a) before and (b) after the FP filter.
Lager Image
64 channel spectrum after the PBC. The optical resolution is 0.05 nm.
Lager Image
Q-factor values for the 12.4 Gb/s channels after the SMF 125 km and 150 km.
When we change the bit rate to 10.7 Gb/s with all other conditions the same, we have BER ~ 3 × 10 -3 typically after the 100 km. This is worse than the FEC threshold, BER = 1 × 10 -4 . For the 12.4-Gb/s bit rate, but with the reduced channel spacing of 10 GHz, we have BER ~ 4.8 × 10 -4 and 1.8 × 10 -2 for the back to back and the 125-km transmission, respectively. Thus, with the VSB filtering, we have achieved the spectral efficiency of 1 bit/s/Hz up to 125 km.
Note that the FP filter’s FSR is dependent only on the mirror spacing. Over the whole C-band, the dielectric mirror’s reflectivity changes within a few percent. Thus, in stable conditions, our FP filters may cover hundreds of 12.5-GHz spaced optical channels.
To demonstrate the usefulness of our Fabry-Perot filter pair, we have chosen 10 Gb/s bit rate rather than 40 Gb/s or higher bit rates. To achieve high spectral efficiencies, 12.5 and 10 GHz channel spacing values are used. In this narrow channel spacing, the FEC techniques are indispensible because of high cross talks [16] . Our transmission system, in its present form, may be used for metro networks [17] and WDM passive optical networks [18 - 20] where many low bit rate channels are preferred. The transmission distance can be increased to a long-haul scale if we use dispersion-managed transmission techniques [21] .
In our experiment, the FP filters are placed on a vibrationfree optical table. With our thermally-matched mechanical mounts in Fig. 2 (b), the FP filters operate stably during the experiment and their transmission peak wavelengths change by 4 pm/deg. However, to obtain long-term stabilities, active controlling apparatuses will be needed. The stability of FP filters can be enhanced greatly if they are integrated within a single chip using, for example, micro-electromechanical systems technologies [22 - 24] .
IV. CONCLUSION
We have proposed to use a pair of FP filters for the VSB filtering of WDM channels. The transmittance curve of each FP filter is made to have sharp skirts using an offset between input and output coupling fibers. Having an excellent periodic property, the FP filters are advantageous over conventional VSB filters covering a large number of optical channels simultaneously. We have demonstrated a simultaneous VSB filtering of 12.5-GHz spaced 64 × 12.4 Gb/s channels using a pair of FP filters achieving a record high 64 simultaneously VSB filtered channels. The VSBfiltered channels have been transmitted successfully over an SMF up to 150 km.
Acknowledgements
This research was supported partly by the Basic Science Research Program through the National Research Foundation of Korea (NRF) funded by the Ministry of Education, Science, and Technology (NRF-2010-0012979) and also partly supported by the Research Grant of Kwangwoon University in 2011.
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