Comparison of Three Dispersions Normal Anomalous.
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Transcript of Comparison of Three Dispersions Normal Anomalous.
1550nm1310nm
色散ps/nmkm
普通光纤(SMF)非色散位移光纤(NDSF,G.652)已有光纤的>95%
波长
色散位移光纤(DSF,G.653)非零色散位移光纤(NZDSF,G.655)
18
0
DWDM
波长范围
Comparison of Three DispersionsComparison of Three Dispersions
Normal
Anomalous
Calculating DispersionCalculating Dispersion• In a typical single-mode fibre using a laser with a spectral
width of 6 nm over a distance of 10 km :
Dispersion = 17ps/nm/km × 6 nm × 10 km = 1020 ps• At 1 Gbps a pulse is 1 ns long. So the system would not w
ork. (20% is a good guideline for the acceptable limit.) But it would probably work quite well at a data rate of 155 Mbps (a pulse length of 6.5 ns).
• A narrow spectral width laser might produce only one line with a linewidth of 300 MHz. Modulating it at 1 Gbps will add 2 GHz. 2,300 MHz is just less than .02 nm (at 1500 nm). So now:
Dispersion = 17ps/nm/km × .02 nm × 10 km = 3.4 ps• In this case, dispersion just ceased to be a problem.
What is an Optical AmplifierWhat is an Optical Amplifier
• An optical amplifier is a device which amplifies the optical signal directly without ever changing it to electricity. The light itself is amplified.
How to make an OAHow to make an OA
• Amplifiers can be built in semiconductor: Semiconductor Optical Amplifiers (SOAs). – Almost any semiconductor laser can be made into an a
mplifier with a few modifications - • Amplifiers can be built in fibres: Fibre Amplifiers
– EDFA: Erbium Doped Fibre Amplifiers– PDFA: Praseodymium Doped Fibre Amplifiers– NDFA: Neodymimum Doped Fibre Amplifiers– SRFA: Stimulated Raman Fibre Amplifiers– PFA: Plastic Fibre Amplifier
1550
EDFA增益窗口30nm ~ 60nm
光放大器增益
光纤衰减
Low loss window
波长
nm850 1310
PDFA
SOA
SRA
Development of OADevelopment of OA
EDFA增益窗口
30nm ~ 60nmPDFA
SOA
SRA
Technical Characteristics Technical Characteristics of EDFAsof EDFAs
• Efficient pumping• Minimal polarisation sensitivity• Low insertion loss• High output power (this is not gain but raw am
ount of possible output power)• Low noise• Very high sensitivity• Low distortion and minimal interchannel cross
talk
DefinitionsDefinitions
• Gain (amplifier) : the ratio in decibels of input power to output power. (dB)
• Gain Coefficient: the small signal gain divided by the pump power. (dB/mW)
• Bandwidth: the range of wavelengths over which the amplifier will operate.(nm)
DefinitionsDefinitions
• Gain Saturation: the point where an increase in input power ceases to result in an increase in output power. (dBm)
• Polarisation Sensitivity: the difference in gain of an input signal in one polarisation to the gain in the orthogonal polarisation. (typical .01 ~ .1 dB).
• Noise Figure: the ratio of the SNR at the input to the SNR at the output (dB).
Flattening the Gain CurveFlattening the Gain Curve
• Operating the device at 77oK. • Introducing other dopant materials (such as al
uminium or ytterbium) along with the erbium into the fibre core.
• Amplifier length is another factor influencing the flatness of the gain curve.
• Controlling the pump power (through a feedback loop) is routine to reduce ASE.
Flattening the Gain CurveFlattening the Gain Curve
• Adding an extra WDM channel locally at the amplifier. This is called “gain clamping”.
• Manipulating the shape of the fibre waveguide within the amplifier. Fibres with dual cores have recently been shown to produce much superior gain flatness characteristics.
Flattening the Gain CurveFlattening the Gain Curve
• Using “blazed” fibre Bragg gratings as filters to reduce the peaks in the response curve. In other words, reduce the response at all wavelengths to that of the worst wavelength. This approach has been reported to work well in field trials.
• Using channel preemphasis on the signals as they are transmitted. That is,transmit different WDM channels at different power levels to compensate for later amplifier gain characteristics.
Wideband EDFAsWideband EDFAs
• usual gain window (S- & C-band)– 1525 - 1565 nm
• Second gain window (L-band) – 1570 - 1610 nm– Using co-dopants, principally aluminium
and phosphorus
• Wideband EDFAs – 80 nm.
Co-DopantsCo-Dopants• Common co-dopants us
ed are aluminium (Al), ytterbium (Yb) and germanium (Ge).
• Ge co-doping produces 1536 nm and 1550 nm gain peaks.
• Al broadens and flattens the gain spectrum in the region 1540 nm to1560 nm.
Design of Amplifier LengthDesign of Amplifier Length
• Both the signal power level and the pump power level vary along the length of the amplifier: signal travels stronger; pump power level decreases.
• Single wavelength operation:
Lopt=f(Psig,Ppump,Ce,G)
• WDM operation: the flatness of the gain.• The gain spectrum at any point along the amp
lifier will be different from the spectrum at any other point along the amplifier.
Select Pump WavelengthsSelect Pump Wavelengths
• 980 nm is almost twice as efficient, as a pump wavelength, than 1480 nm.– 1480 is within the gain spectrum– 1480 is a two-level laser system– 1480 is temperature-sensitive
• disadvantage of 980 nm: quite narrow pump bandwidth
WarningWarning
• Pumps need to produce an output of up to 250 mW.
• Unless the laser is very carefully designed to protect it you can burn the end facet and erode the LD.
MultiStage EDFAsMultiStage EDFAs
1) To increase the power output whilst retaining low noise2) To flatten the total amplifier gain response3) To reduce ASE noise
Remote PumpingRemote Pumping
•Two fibres are used in the connection - one for the signal and one for the pump.•to pump at 1480 nm •In a typical undersea system to extend the distance from around 100 km to 150 or even 200 km.
EDFA System ResilienceEDFA System Resilience
• Signal passes through the failed amplifier relatively unchanged!
Using OTDRs in Amplified LinksUsing OTDRs in Amplified Links
• OTDR: optical time-domaim reflector
• To diagnose link condition right through the amplifier.
Second-Generation EDFAsSecond-Generation EDFAs
• An amplifier with any of the following characteristics is “second-generation”:– Multi-stage designs– Use of co-dopants such as ytterbium– Use of multiple pumps– Use of gain-equalisation techniques
Summary of EDFA Summary of EDFA CharacteristicsCharacteristics
• It is significantly simpler than a repeater and will have a much longer mean time to failure.
• It is significantly lower in cost than a repeater.
• It will operate at almost any speed.
• It can be made physically small enough to fit on a printed circuit card.
Summary of EDFA Summary of EDFA CharacteristicsCharacteristics
• It will produce a gain in optical signal of about 25 dB. Some amplifiers can produce a gain of 50 dB or even higher.
• It will amplify many different wavelengths simultaneously (with some small limitations).
Summary of EDFA Summary of EDFA CharacteristicsCharacteristics
• Both amplitude (pulse) modulated and coherent (frequency modulated) light as well as cable TV signal could be amplified without distortion.
• There is effectively no delay in the amplifier.• It is possible to do end-to-end diagnosis of
link faults right through an EDFA.• Amplifiers (like their electrical counterparts)
can saturate.
Summary of EDFA Summary of EDFA CharacteristicsCharacteristics
• There are of course some limitations:– The amplifier itself adds some noise.– Wavelength range limitation– The gain spectrum is not perfectly flat.– Amplifiers do not re-create pulses.– amplifiers must be placed closer together (30 kilo
metres) than repeaters (50 kilometres)
• Transmission at 2.4 Gbps over a distance of 21 000 kilometres was reported
Praseodymium (Pr) Doped FibrPraseodymium (Pr) Doped Fibre Amplifierse Amplifiers
• Operate in the 1300 nm band
• The gain available in commercial PDFAs is only around 12 dB
• Fluorozirconate (ZBLAN) glasses are used instead of silica.
• Nd:YLF at 1047 nm pumps are the ones used in commercial PDFAs.
Neodymium (Nd) Doped Neodymium (Nd) Doped Fibre AmplifiersFibre Amplifiers
• Nd will amplify over the range 1310 to 1360 nm in ZBLAN glass and between 1360 and 1400 nm in silica.
• Efficient pump wavelengths are at 795 and 810 nm.