josef vojtěch, miroslav karásek, jan radil field and lab experiences with deployment of optical...
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May 30, 2006 CEF Workshop Praha, Czech Republic 3 Utilization of dark fibres – CEF networks (the first DF line lighted by CESNET in 1999, 2.5 Gb/s PoS) National Research and Educational Networks (NRENs) rely on leased dark fibres and prefer to have no active components between the transmitter and the receiver Repeater-less or better Nothing-in-line (NIL) approach Cost effective deployment of multi-gigabit lines (N x 10 GE) Single fibre bidirectional N x 10 GE transmission Field and lab experiences with optical amplifiers and FBGs MotivationsTRANSCRIPT
Josef Vojtěch, Miroslav Karásek, Jan Radil
www.ces.net
Field and lab experiences with deployment of optical amplifiers and FBGs
May 30, 2006 CEF Workshop
Praha, Czech Republic 2
Field and lab experiences with optical amplifiers and
FBGs Outline Motivations
Laboratory experiments Field Deployment (+ planned) Conclusions
WarningPresented ideas are of authors and do not necessarily
reflect an official opinion of the CESNET or any other institution or project, and are opened to improvement.
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Utilization of dark fibres – CEF networks (the first DF line lighted by CESNET in 1999, 2.5 Gb/s PoS)National Research and Educational Networks (NRENs) rely on leased dark fibres and prefer to have no active components between the transmitter and the receiverRepeater-less or better Nothing-in-line (NIL) approachCost effective deployment of multi-gigabit lines (N x 10 GE)Single fibre bidirectional N x 10 GE transmission
Field and lab experiences with optical amplifiers and
FBGs Motivations
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1GE NIL 300 km G.652 (EDFA only) 325 km G.652 (EDFA + Raman)
10GE NIL 2x10G+2x1G WDM 202km G.652 (EDFA + DCF) 2x10G WDM 250km G.652 (EDFA + Raman + DCF)
10G DWDM 302 km G.655+652 (EDFA + Raman)
Field and lab experiences with optical amplifiers and
FBGs Laboratory Experiments I
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Field and lab experiences with optical amplifiers
and FBGs 2 x 10G + 2 x 1G NIL WDM 200km G.652
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Field and lab experiences with optical amplifiers and
FBGs 2 x 10G WDM NIL 250km G.652
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Field and lab experiences with optical amplifiers and
FBGs 10G DWDM NIL 302km G.655+G.652
EDFA 2EDFA 1
227 km G.655 + 75 km G.652
Tx
Rx
Raman pump
10GE1550,12 nm
Rx
Tx
OF1 OF2
Simulation of real lineNo CD compensation at all due to NZDSF
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10GE NIL 8x10G DWDM 250km G.652 (EDFA + FBGs)
10GE NIL bidirectional (single fibre) transmission 2x4x10G 210km G.652 (EDFA + FBGs)
Field and lab experiences with optical amplifiers and
FBGs Laboratory Experiments II
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Field and lab experiences with optical amplifiers and FBGs
8 x 10G DWDM 250km G.652Tx1
MUX
Tx8
.
.
EDFA 1 EDFA 2
FBG
Rx1
Rx8
.
.
250 km G.652
DEMUX
Optical spectrum of multiplexed channels before
amplification
Input spectrum and „eye“ diagram at Rx 7 input
1540 1545 1550 1555 1560-80
-70
-60
-50
-40
-30
-20
-10
0
Po
we
r (d
Bm
)
W ave leng th (nm )
1540 1545 1550 1555 1560-70
-60
-50
-40
-30
-20
-10P
ow
er
(dB
m)
W avelength (nm )
1551.72nm R x
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Field and lab experiences with optical amplifiers and FBGs
2 x 4 x 10G DWDM 210km G.652Tx1
MUX 1
Tx4
EDFA 1 EDFA 2Tx5
Tx8
210 km G.652
MUX 2
FBG 1 FBG 2
Rx1Rx8Rx5 Rx4
EDFA 3 EDFA 4
DEMUX 2DEMUX 1
λ1+λ2+λ3+λ4
λ5+λ6+λ7+λ8
λ5+λ6+λ7+λ8
λ5+λ6+λ7+λ8
λ1+λ2+λ3+λ4
λ1+λ2+λ3+λ4
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Field and lab experiences with optical amplifiers and FBGs
2 x 4 x 10G DWDM 210km G.652
1542 1544 1546 1548 1550 1552 1554-70
-60
-50
-40
-30
-20
-10
0
pow
er, d
Bm
wavelength, nm
1544 1546 1548 1550 1552 1554 1556-70
-60
-50
-40
-30
-20
-10
0
pow
er, d
Bm
wavelength, nm
Optical power at the output of MUX 1 Optical power at the output of MUX 2
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Field and lab experiences with optical amplifiers and FBGs
2 x 4 x 10G DWDM 210km G.652
1544 1546 1548 1550 1552 1554 1556
-40
-30
-20
-10
0
pow
er, d
Bm
wavelength, nm
Optical power at the output of EDFA 3 Optical power at the output of MUX 2
1549.0 1549.5 1550.0 1550.5 1551.0 1551.5-70
-60
-50
-40
-30
-20
pow
er, d
Bm
wavelength, nm
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Field and lab experiences with optical amplifiers and FBGs
2 x 4 x 10G DWDM 210km G.652Eye diagram of the transmitter -
DWDM XENPAKEye diagram recorded at the input of Rx1
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1GE NIL 189 km G.652 Praha – Pardubice CESNET2 since May
2002 235 km G.652 Brno – Ostrava CESNET2 since June
2003
10GE 1(8 ready) x 10G DWDM 298km G.655+652
Praha - Brno CzechLight (no CD comp.) since May 2005 1(4 ready) x 10G DWDM NIL 190 km G.652 CBF Brno-CESNET2 Bratislava-SANET (FBGs) since Feb 2006
Field and lab experiences with optical amplifiers and
FBGs Field deployment
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Field and lab experiences with optical amplifiers and
FBGs 4 x 10 GE DWDM CBF Brno - Bratislava
1550.12Tx1
DWDM Mux
190 km
43 dB
Booster-1 Preamp-2
FBG
-1700 ps/nm 1550.12
DWDMDemux
Rx1
1550.12
DWDMDemux
FBG
-1700 ps/nm190 km
43 dB
Preamp-1 Booster-21550.12
DWDM Mux
Rx1 Tx1
Brno Bratislava
Fiber 1
Fiber 2
190 km 43 dB
G.652
CLA PB01
Booster/Preamp
DCU CLA PB01
Booster/Preamp
DCU
1550.12
Xenpak-DWDM
1550.92
1552.52
DWDMMux/Demux
1550.12
Xenpak-DWDM
1550.921551.72
1552.52
DWDMMux/Demux
1551.72
Detail
FBG
-1000 ps/nm
FBG
-1000 ps/nm
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Field and lab experiences with optical amplifiers and
FBGs planned up to 8 x 10 GE DWDM Brno –
ViennaCBF between Brno-CESNET2 and Vienna-ACONET (last side of triangle)Approximate length over 220 km of G.652 fiber(attenuation about 65 dB)
Real challenge – NIL (Raman amplification necessary)
CESNETBrno
SANETBratislava
ACONETVienna
190 km
108 km
220 km
Czech Rep. Slovakia
Austria
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Field and lab experiences with optical amplifiers and
FBGs Conclusions I
Thanks to persistent technology progress - lighting of dark fibers is getting easier and easierIf static DWDM multiplex at 10 G is enough – you need only: fibres, transceivers, (amplifiers) and passives
Note: Exact setup and component needs depend on parameters as transceivers, fibre types, attenuation, etc.
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Field and lab experiences with optical amplifiers and FBGs
Conclusions I cont.
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Field and lab experiences with optical amplifiers and FBGs
Conclusions I cont.
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Field and lab experiences with optical amplifiers and
FBGs Conclusions II
Not only higher transmission speeds but reconfigurability and all-optical signal processing also becoming more importantPresent generation of systems (ROADMs, WSSs, OXCs)For next generation - deployment and development and of new components (wavelength and NRZ/RZ conversions, pure optical OOO regenerators)Especially important (in our opinion) for academic and research community
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[1] Karásek, M. - Peterka, P. - Radil, J. , „202 km repeaterless transmission of 2 x 10 GE plus 2 x 1 GE channels over standard single mode fibre. “, In: Optics Communications 235, pp. 269-274., 2004.[2] Karásek, M. - Peterka, P. - Radil, J. , „Repeaterless Transmission of 2 x 10 GE Channels over 252 km of Standard Single Mode Fibre without in-line EDFA “, In: IEEE J. on Selected Areas in Communications, sfp, 2004.[3] Radil, J. - Karásek, M., „Experiments with 10 GE long-haul transmissions in academic and research networks.“, In: I2 member meeting, Arlington, VA, 2004.[4] Altmanová L., Radil J., Šíma S., Vojtěch J., „CzechLight testbed“. In: GN2 APM meeting, Praha, Czech Republic, February 2005.
Field and lab experiences with optical amplifiers and
FBGs References
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Field and lab experiences with optical amplifiers and
FBGs Acknowledgement
Lada Altmanová, Jan Gruntorád, Martin Míchal, Václav Novák, Stanislav Šíma
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Field and lab experiences with optical amplifiers and
FBGs Thank you for your attention!
Q&A