first ever 40gigabit internet connection to the home challenge

67
1 Street, Suite 553, Los Altos, CA 94022, USA Peter Löthberg, <[email protected]> Challenge: A: There was no Internet at my parents house and the local ISP’s suck (the lack of performance is scary, and they have no IPv6 etc.). B: Explain that if your house is fiber attached by a open neutral provider, there are many possibilities C: We have hit another Bellhead bump in the road to remove unnecessary elements from the IP network. If my mother can make it work i, it must be a political/”my_job problem”. First Ever 40Gigabit Internet Connection to the Home Ripe 55, Amsterdam, October 2007

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1

Stupi LLC, 101 1St Street, Suite 553, Los Altos, CA 94022, USA

Peter Löthberg, <[email protected]>

Challenge:A: There was no Internet at my parents

house and the local ISP’s suck (the lack of performance is scary, and they have no IPv6 etc.).

B: Explain that if your house is fiber attached by a open neutral provider, there are many possibilities

C: We have hit another Bellhead bump in the road to remove unnecessary elements from the IP network. If my mother can make it work i, it must be a political/”my_job problem”.

First Ever 40Gigabit Internet Connection to the Home

Ripe 55, Amsterdam, October 2007

2

Mamma NET

Why:I’m crazy (sorry, no banana for pointing that out)The Swedish policy scene is full of FUD Fiber based optical networks are flexible and future proofVideo Conferencing with my parentsBBQ Bellheads said it can’t be doneIt has not been done, so why not give it a tryEvaluate the performance of SUnet’s new optical networkIt’s better than DSL and supports large packets..etc...

.... and to see if I can outperform “Mr Hype” in press releases

3

Mamma NET

Yes, 40G to my mom’s house isn’t what everyone can do:

The reason I’m giving this talk at Ripe is to help you break down the barriers that your transport people put up to stop you from building more efficient IP networks.

Remember X25, Frame Delay, ATM, Routers directly attached to DWDM systems without ADM’s etc

This is simple, you can do it, just look at the design criteria;If you have enough OSNRProperly manage your chromatic dispersionAre within PMD limitsProperly clean your connectors

4Ripe 55, Amsterdam, October 2007

Why IPoDWDM

40G DWDM

40G DWDM

TXRX

TXRX

TXRX

TXRX

TXRX

40GDWDMTX

RX

TXRX

TXRX

OC768-SR

40GDWDM

OC768-SR

OC768-ITU OC768-ITU

Transponder Transponder

1 2 3 5

1 2

4

IPoDWDM

Traditional Model: External Transponder

6

5

Special Thanks to:....Mom and DADHans Wallberg and Börje Josefsson SUnetThe NuNoc STAFFSanta Claus, Kelly Ahuja, Björn Ehn, Walid Wakim CiscoHafstein Johnsson, Raimo Vekhajarvi, Malin Thorsen City of KarlstadHakan Syren, ELTEL NetworksRoss Saunders, Stratalight ”Ethernet Micke” Abrahamson, LM Jogback Tele2Marko Ivanov CienaAnders Magnusson LTUThomas Svensk Imtech

Thanks to:....

”It cant be done!” BBQ divisionNiklas Montin, Håkan Karlsson, Jim Houts, Dennis Davidsson ,Dave Meyer, Samer Parikh, and many more CiscoLeon Pavlov MobinetLars Molin GeosonicChase Cotton, Wes George, Björn Carlsson, Dave Harris SprintBob Rodeo, Mike Pellegrini CienaKalix FiberFredrik Holmqvist DCS

6Ripe 55, Amsterdam, October 2007

MotherNet Don’t forget to take the cards out before attempting shiping.

Greatly improves value of the 1988 WV-bus...

7Ripe 55, Amsterdam, October 2007

Moving the broadband router in to the garage.

My dad is performing damage management.

Leon is providing muscle resources

8Ripe 55, Amsterdam, October 2007

My mother Sigbritt doing the fiber installation.

9Ripe 55, Amsterdam, October 2007

MotherNet

10Ripe 55, Amsterdam, October 2007

World’s First and Fastest Internet Connection to the home, 40Gig!

Karlstad Stockholm

412.1Km

CRS-1 w/ Integrated 40Gig DWDM Optics

412Km3.5 dBQ

Un-optimized

Karlstad

Stockholm

40Gig CircuitOver Fiber

No Repeaters

40Gig, Plug and Play Circuit Turn Up“The most difficult part of the whole project was installing

Windows on Sigbritt’s PC,”said Hafsteinn Jonsson of Karlstad Stadsnat.

11Ripe 55, Amsterdam, October 2007

Network Layout

CRS-140G

DWDM10Km

TXRX

Existing Transport

OC768-ITU(ODB)

3rd Party DWDM Provider(Ciena)

40Gig Integrated DWDMOptics on CRS-1

Connectivity at Stockholm and Karlstad

12Ripe 55, Amsterdam, October 2007

Physical Network

CRS-140G

DWDM10KM

TXRX

Existing Transport

OC768-ITU(ODB)

3rd Party DWDM Provider( Ciena )

40Gig IntegratedDWDMOptics on CRS-1

84.3Kmor

(19.6dB)

102.2Kmor

(23.3dB)

107.4Kmor

(24.5dB)

110.8Kmor

(26.6dB)

Cummulative Fiber Dispersion W2E (at 1545 nm)

-1200-1000

-800-600-400-200

0200400600

Stockholm Savja Vasteras Orebro Karlstad Cummulative Fiber Dispersion W2E(at 1545 nm)

CRS-1

40GDWDMTX

RX

Existing Transport

OC768-ITU(ODB)

3rd Party DWDM Provider (Ciena) 40Gig IntegratedOptics on CRS-1

-501psDCU

Line CD Map, Does not include DCU at CRS

RXTX

13Ripe 55, Amsterdam, October 2007

The Local Loop: 10 795m

Hafstein Johnsson

Malin Thorsen

Installation and measurements by ELTEL Networks

14Ripe 55, Amsterdam, October 2007

15Ripe 55, Amsterdam, October 2007

Broad Band to My Mother, Optics

SavjaStockholm Orebro KarlstadVasteras

60 50 11080 80

23.3dB102.2km

0.062ps/n

19.6dB84.3km

0.081ps/n

24.5dB107.4km

0.122ps/n

26.6dB110.8km

0.188ps/n

5dB10.8km

0.0193ps/n

Sunet / Opto SUnet Karlstad Stadsnat

30

Ciena Band 5, Channel 5, Frequency = 193.30 THz, Wavelength = 1550.918 nm, MSA Channel 57

40G MPR

70 120 110110

23.3dB102.2km

0.167ps/n

19.6dB84.3km

0.138ps/n

24.5dB107.4km

0.098ps/n

26.6dB110.8km

0.079ps/n

40G MPR

+10 +15dB

120EDFA amplifier

Dispersion Compensation fiber SMF28 equivalent length

RX Power = -4.41 dBmTX Power = 1.19 dBm

TX Power = -2.81 dBmRX Power = -12.91 dBm

4.8dB10.8km

0.0385ps/n

PMD=0.472 ps+1.5ps=2.472ps

PMD=0.501 ps+1.5ps=2.501ps

16Ripe 55, Amsterdam, October 2007

MotherNet

17Ripe 55, Amsterdam, October 2007

CHAN 5

LC UPC connector

18Ripe 55, Amsterdam, October 2007

Stupi Test Network

19Ripe 55, Amsterdam, October 2007

Mothers Alternate use of the broadband gateway

20Ripe 55, Amsterdam, October 2007

Power Consumption

Operated for 48 days

- Power 1.56 KW

- Cost EUR 293/month

21Ripe 55, Amsterdam, October 2007

MotherNet

D-WDM 1-GE SFP,

Same color as the 40G signal

Same setup at Stockholm side

22Ripe 55, Amsterdam, October 2007

MotherNet

23Ripe 55, Amsterdam, October 2007

Optical ImpairmentsDWDM Building Blocks

TranspondersDWDM

Multiplexer

OpticalAmplifiers

OpticalAdd/Drop

ReceiveTransponders

DWDMDemultiplexer

ITU-T Transmitters

OA OADM OA

LTE

LTE

LTE

OEO

OEO

LTE

LTE

LTE

24Ripe 55, Amsterdam, October 2007

Optical Impairments

Chromatic Dispersion (CD)The refractive index of fiber has a wavelength dependence. This causes the higher frequencies to travel faster then lower frequencies causing a pulse broadening effect. Measured in ps/nm*km, threshold / limit measured in ps/nm.

Confusion, do I want it or not? Is it good or bad?Reducing Dispersion will increase distance and performance

Reducing / Eliminating Dispersion will also increase nonlinear effects thus limiting distance / performance

Dispersion Compensating Units (DCUs) are used to compensate for CD

tt+16.7ps

1 Km of SMF28 Fiber16.7 ps/nm

25Ripe 55, Amsterdam, October 2007

Optical Impairments

Optical Signal-to-Noise RatioCompensate for Attenuation with Optical Amplifier

Compensate for Dispersion with DCU

Can we now travel an infinite distance without Regen?No! We are limited by OSNR (besides other effects)

As we start to cascade Amplifiers we introduce noise in the form of ASE

Signal degradation caused by 2 factors:

1. Noise to noise beatings

2. Noise to signal interference

#1 we can take care of using a narrowband filter

#2 is the true problem since it is beating against the actual signal hence key limiting factor

26Ripe 55, Amsterdam, October 2007

Optical Impairments

How do we calculate Signal to Noise?In its simplest form OSNR is:

OSNR = 58 + Pin - NF - 10*log(N) - 10*log(M)Where:58 = power density in 0.1nm BWPin = input to EDFANF = Noise Figure of EDFAN = # of Optical ChannelsM = # of Amps in cascade

27Ripe 55, Amsterdam, October 2007

Optical ImpairmentsG.709 and Forward Error Correction (FEC)

Ethernet is the transport of choicePerformance Monitors similar to SONET would be required to ensure proactive monitoring and health of system

SolutionWavelength monitoring via standards based G.709

Provides SONET like OAM&P

Standard specifies OTU1(2.5G), OTU2(10G) and OTU3(40G)

Ethernet cost with SONET like OAM&P

28Ripe 55, Amsterdam, October 2007

Optical ImpairmentsG.709 Wrapper

3825

4080

1 7 8 14 15 16 17 3824

1

2

3

4

OPU k PayloadO

PUk

OH

OPUkŃ Optical Channel Payload Unit

ODUk

ODUkŃ Optical Channel Data Unit

Client SignalMapped in

OPUk Payload

Client Signal

OTUkFEC

OTUk OH

OTUkŃ Optical Channel Transport Unit

Alignm

Alignment

k Indicatesthe Order:1 2.5G2 10G3 40G

29Ripe 55, Amsterdam, October 2007

Log

(BER

)

4 5 6 7 8 9 10 11 12 13 14 15–15

–14–13

–12

–11

–10–9

–8

–7

–6–5

–4

–3

–2–1

0

S/N (dB)

UncodedNo FEC

G.709RS(255,239)

Raw Channel BER=1.5e-3

EFEC=8.4 dBFEC=6.2 dB

Optical ImpairmentsFEC

FEC extends reach and design flexibility, at “silicon cost”

G.709 standard improves OSNR tolerance by 6.2 dB (at 10–15 BER)

Offers intrinsic performance monitoring (error statistics)

Higher gains (8.4dB) possible by enhanced FEC (with same G.709 overhead)

Benefit: FEC/EFEC Extends Reach and Offers 10–15 BER

30Ripe 55, Amsterdam, October 2007

Optical Impairments

Polarization Mode Dispersion (PMD)Since fiber cores are not perfectly symmetrical, the light will travel down the X and Y axis at different rates leading to a pulse broadening effect. This is a function of a coefficient multiplied by the square root of the total distance measured in ps/km1/2

Function of bit rate, greater the bit rate the greater the dependence on PMDPMD is statistical in nature, one must account for mean value rather then instantaneousPMD compensators are available

nx

nyEx

Ey

Pulse As it Enters the FiberSpreaded Pulse As it Leaves the Fiber

nx

nyEx

Ey

Pulse As it Enters the FiberSpreaded Pulse As it Leaves the Fiber

31Ripe 55, Amsterdam, October 2007

Optical Impairments

FPM or FWMBeating between two channels at their difference frequency, modulates the phase at that frequency generating new tones as side bands. These new products interfere with other channels

BER degradation

Counter MeasuresUnequal Channel Spacing

Increase Channel Spacing

Chromatic Dispersion, waves alternate in and out of phase, reducing mixing efficiency

Total Beats = N(N-1)^2

λ1 λ2 λ3

f113 f112

f123

f213

f223 f132

f312

f221 f332

f321

f231

f331

32Ripe 55, Amsterdam, October 2007

Optical Impairments

XPMThis arises due to the weak dependence of the refractive index on intensity: n=n0 + n2*I. Here the nonlinear refractive index modulates one of the carriers onto the other.

Pulse broadening gets exaggerated with Chromatic Dispersion

Counter MeasuresChromatic Dispersion, the group velocity causes the interfering pulse to walk thru the other

Larger spacing between carriers

33Ripe 55, Amsterdam, October 2007

Modulation SchemesAcronyms

(N)RZ—(Non) Return to Zero

PSBT—Phase Shaped Binary Transmission

CS-RZ—Carrier Suppressed Return to Zero

DPSK—Differential Phase Shift Keying

DQPSK—Differential Quadature Phase Shift Keying

QPSK—Quadature Phase Shift Keying

PM-’X’—Polarization Multiplexing

34Ripe 55, Amsterdam, October 2007

Modulation Schemes

Modulation Attributes

Amplitude Phase Polarization

CS/RZ

NRZ

PSBT

DPSK

QPSK

DQPSK PM-’X’

Where ‘X’ Can Be DPSK, DQPSK, QPSK, etc. …

35Ripe 55, Amsterdam, October 2007

-40

-35

-30

-25

-20

-15

-10

-5

0

5

10

-100 -50 0 50 100

Relative Frequency (GHz)

Ral

ativ

e O

ptic

al P

ower

(dB

)

40G CS-RZ

10G NRZ

40G Duobinary

50 GHz Filter

Modulation Schemes PSBT Implementation

CW Laser

NRZ Data

Photodiode NRZ Data

EDFA

Optical Out

Serial 40G

Serial 40G

Optical In

Serial 40G

1 10

+E+E

+E-E

1 -10

NRZ Sequence

Dispersed NRZ+E field add lifting 0s

+1

0

+1

0

-1

Duo Binary Sequence

E fields cancelReducing ISI

Driver/Encoder

MZM

Tx Block Diagram

Rx Block Diagram

36Ripe 55, Amsterdam, October 2007

DWDM Filter Compatibility

-40

-35

-30

-25

-20

-15

-10

-50 -40 -30 -20 -10 0 10 20 30 40 50

Frequency (GHz)

Rel

ativ

e O

ptic

al P

ower

(dB

)

43Gb/s PSBT43Gb/s CS-RZ43Gb/s DPSK50GHz Interleaver

37Ripe 55, Amsterdam, October 2007

Modulation Schemes DPSK Implementation

CW Laser

BalancedPhotodiode

NRZ Data

NRZ Data

EDFA

Encoder/Driver

0 1 1 0 1 0 0

0 1 0 1 1 1 0

MZM

0 0 1 1 0 1 0 0 1 0 1 1 1 0

0 1 0 1 1 1 0

Re(E)

Im(E)

OOK

Re(E)

Im(E)

DPSKAs You Can See, Symbol Separation Is a Factor of 2 for the Same Average

Power Hence 3 dB First Order.

Why Is DPSK Have Better OSNR Performance?

DI

R

Serial 40G

Serial 40G

Serial 40G

Optical Out

OpticalIn

Tx Block Diagram

Rx Block Diagram1 0 1 0 0 0 1

38Ripe 55, Amsterdam, October 2007

Some Modulation Schemes of todayComparison Table

High

High

+/–800ps/nm

10ps

11dB/

0.1nm

PM-(D)QPSK

HighMediumLowLowLowPhotonics Complexity

LowLowMediumMediumMediumElectronics Complexity

+/–200ps/nm

+/–200ps/nm

+/–100ps/nm

+/–150ps/nm

+/–50ps/nmCD Tolerance

5ps5ps2.51ps2.5ps1psPMD Tolerance

13dB/

0.1nm

15dB/

0.1nm

13dB/

0.1nm

16dB/

0.1nm

16dB/

0.1nmOSNR Sensitivity

QPSKDQPSKDPSKPSBTOOK

39Ripe 55, Amsterdam, October 2007

Modulation Schemes DQPSK Implementation

While maintaining full data rate we half the line rate thus improving both CD and PMD robustness

More robust to OSNR then OOK although not as robust as DPSK due to separation

CW Laser

BalancedPhotodiode

π/2

BalancedPhotodiode

23π

MZM

MZM

23π

23π

Re(E)

Im(E)

Re(E)

Im(E)

R

R

Serial 20G

Serial 20G

Four Phase Levels:Decoder:Phase Data

0 0 0π/2 1 0

−π/2 0 1 π 1 1

Encoder / Driver

Basically DPSK with π/2 Phase Shift

Tx Block Diagram

Rx Block Diagram

40Ripe 55, Amsterdam, October 2007

Modulation SchemesQPSK Implementation

Similar to DQPSK although utilizes coherent detection

More complex and costly to implement, requires a laser source at Rx

BalancedPhotodiode

BalancedPhotodiode

LocalOscillator

CW Laser

π/2

MZM

MZM

Serial 20G

Serial 20G

Encoder / Driver

R

R

Tx Block Diagram

Rx Block Diagram

41Ripe 55, Amsterdam, October 2007

Modulation SchemesPolarization Mux (PM)-(D)QPSK

Theoretically 10 Gig performance

Utilized 10Gig electronics

Must control polarization

Most complex of all schemes

Serial 10G

(D)QPSK Modulator

Serial 10G

Serial 10G

(D)QPSK Modulator

Serial 10G

CW Laser

(D)QPSK Demodulator

(D)QPSK Demodulator

Tx Block Diagram

Rx Block Diagram

42Ripe 55, Amsterdam, October 2007

Modulation Schemes Implementation Complexity

Photonic Complexity

OOKDPSK

DQPSK

PSBT

4-Poly

Elec

tron

ic C

ompl

exity

Low High

Low

Hig

hCoherentDetection

Soft

Dec

isio

nM

LD

MSK

QPSK

16 QAM

PSK

TCM

43Ripe 55, Amsterdam, October 2007

Why IPoDWDMPossible Feature

Optical impairmentsCor

rect

ed b

its FEC Limit

Tran

spon

der

Working Path

Switchover Lost Data

ProtectedPath

BER

LOF

POS

on R

oute

r

Optical impairmentsCor

rect

ed b

its FEC Limit

10G

E W

DM

+ G

.709

on

Rou

ter

ProtectionTrigger

Working Path Protected

BER

Hitless Switch

Superior Protection Compared to Transponder-Based Networks

44Ripe 55, Amsterdam, October 2007

Network ArchitectureDesign Considerations

Noise Tolerance of 40G Receiver differs from 10GNoise and Impairment Limit: OSNR

0 to –23 dBm5 to –18 dBmRx Windows

~ 15 dB~ 18.6 dBOSNR (.1nm)

0 dBm0 dBmLaunch Powers

10G Transponder40G IPoDWDM Transceiver

45Ripe 55, Amsterdam, October 2007

Network ArchitectureDesign Considerations

Impairment Tolerance of 40G Receiver differs from 10GNoise and Impairment Limits: Dispersion

10 ps2.5 psPMD

+/– 2000 ps+/– 150 psCD

10G Transponder40G IPoDWDM Transceiver

46Ripe 55, Amsterdam, October 2007

Network ArchitectureDesign Considerations

CD Map

0

100

200

300

400

500

6000

103

212

292

374

455

485

547

637

697

753

826

856

955

Distance

Res

CD

CD Map

954 km Link Across 8 ROADM Nodes and 6 Line Amplifier Nodes

Noise and Impairment Limits: Dispersion (Cont.)

47Ripe 55, Amsterdam, October 2007

Network ArchitectureDesign Considerations

Q Margin vs. Dispersion

00.20.40.60.8

11.21.41.61.8

-150 -100 -50 0 50 100 150Dispersion (ps/nm)

Q M

argi

n (d

BQ

)

Fine Tuning Dispersion for Optimal Operating Margin

Noise and Impairment Limits: Dispersion (Cont.)

48Ripe 55, Amsterdam, October 2007

Network ArchitectureDesign Considerations

Smaller Window of Tolerance for Chromatic DispersionLine Compensation was deployed throughout the network to solidify the “Open” Architecture

Dispersion Grooming is deployed at the receiver where needed

RO

ADM

DWDM Line System

DSCM

DSC

M

Dispersion Grooming

Dispersion Grooming

Routing Platform

Routing Platform

RO

ADM

Integrated 40G DWDM

Interface

Integrated 40G DWDM

InterfaceLine

Compensation

Noise and Impairment Limits: Dispersion (Cont.)

49Ripe 55, Amsterdam, October 2007

Network ArchitectureDesign Considerations

Calculating Line Dispersion:

Determining Residual Dispersion:

−= 3

400

4)(

λλλλ SCD SMF

S0 = 0.092 ps/(nm2 * km)

λ0 = 1311nm

)()()( λλλ LineSMFRES CompCDCD −=

System Engineering: Engineering for Dispersion

50Ripe 55, Amsterdam, October 2007

If the Residual Dispersion, CDRES, is outside of the Receiver’s CD Tolerance window, additional Dispersion Grooming must be performed via additional compensation.

CDRX = CDRES – [CDGrooming]

For an IPoDWDM Transceiver with a CD Receiver Tolerance of +/– 150 ps, the dispersion at the receiver, CDRX, must be:

–150 ps < CDRX < +150 ps

Network ArchitectureDesign Considerations

RO

ADM

DWDM Line System

DSCM

DSC

M

Dispersion Grooming

Dispersion Grooming

Routing Platform

Routing Platform

RO

ADM

Integrated 40G DWDM

Interface

Integrated 40G DWDM

InterfaceLine

Compensation

Engineering for Dispersion (Cont.)

51Ripe 55, Amsterdam, October 2007

Network ArchitectureDesign Considerations

Spectrum Analysis of 954 km Link6 x 10G Production Channels + 2 x 40G Production Channels

Measured (shown): 18.95dB (0.1nm RBW) PostFEC BER (bps): 0

52Ripe 55, Amsterdam, October 2007

Network ArchitectureDesign Considerations

Fiber Characterization is a mustOTDR for loss and DistanceDispersion Compensation

Electronic/Tunable Dispersion CompensationCoherent Receivers

PMD CompensationORL/ReflectanceOSNR Gains

Narrow Band FiltersRAMAN Amplifiers

53Ripe 55, Amsterdam, October 2007

90 270

450

630

810

990

1170

1350

1530

1710

1530

1532

1534

1536

1538

1540

1542

1544

1546

1548

1550

1552

1554

1556

1558

1560

Length (km)

Wavelength (nm)

SMF28 fiber

No Slope Compensation

No TDC

No PMD

54Ripe 55, Amsterdam, October 2007

90 270

450

630

810

990

1170

1350

1530

1710

1530

1532

1534

1536

1538

1540

1542

1544

1546

1548

1550

1552

1554

1556

1558

1560

Length (km)

Wavelength (nm)

SMF28 fiber

No Slope Compensation

TDC

No PMD

55Ripe 55, Amsterdam, October 2007

90 270

450

630

810

990

1170

1350

1530

1710

1530

1532

1534

1536

1538

1540

1542

1544

1546

1548

1550

1552

1554

1556

1558

1560

Length (km)

Wavelength (nm)

SMF28 fiber

Slope Compensation

TDC

No PMD

56Ripe 55, Amsterdam, October 2007

Watch out for enemy tactics:Back to Back Systems, ROADMs, ...

57Ripe 55, Amsterdam, October 2007

PSBT and DPSK Distances on NDSF

FEC Limit

Margin3

dBQ

760BL-PSBT 40/50

795DPSK-NRZ 40/50

852DPSK-NRZ 40/100

1128

BL-PSBT 40/100

Reach (km)Format

Calculated at 3 dBQ margin

58Ripe 55, Amsterdam, October 2007

Lulea

BBQ: But that’s only 400Km...

OK, let’s make it longer..

Stockholm – Lulea

SMF28 fiber lenght is 1090Positivie PMD compensation is 46kmPMD N->S is 0.905ps+1.5ps=2.4ps PMD S->N is 1.655ps+1.5ps=3.15psTotal 1090909M + 46000M = 1136909MEDFA’s in System 15COADM’s in System 4Stockholm->Lulea Extra EDFA 1

59Ripe 55, Amsterdam, October 2007

Lulea is 1000KM away... (total project 2800Km drive)

60Ripe 55, Amsterdam, October 2007

MotherNet

61Ripe 55, Amsterdam, October 2007

62Ripe 55, Amsterdam, October 2007

-1500

-1000

-500

0

500

1000

1500

2000

Sto

ckho

lmU

ppsa

laO

stha

mm

ar

Gav

leS

oder

ham

n

Hud

iksv

all

Sun

dsva

llH

arno

sand

Doc

ksta

Nor

dmal

ing

Um

ea

Ana

set

Ske

llefte

aP

itea

Lule

a

Fiber Dispersion W2E (at 1545nm)Cummulative Fiber DispersionW2E (at 1545 nm)

-1500

-1000

-500

0

500

1000

1500

2000

Stockholm

Osthammar

Soderham

nSund

svall

Docks

ta

UmeaSke

llefte

a

Lulea

Fiber Dispersion E2W (at 1545nm)

Cummulative Fiber DispersionE2W (at 1545 nm)

Stockholm – Lulea dispersion map

N->S

S->N(Need to

add SMF28)

63Ripe 55, Amsterdam, October 2007

MotherNet

64Ripe 55, Amsterdam, October 2007

CRS1 and DCMin Stockholm

(Peter Style Instrall)

65Ripe 55, Amsterdam, October 2007

66Ripe 55, Amsterdam, October 2007

67Ripe 55, Amsterdam, October 2007

MotherNet

OK, ENOUGH!

Questions?