HP AN1550 6_High Speed Lightwave Component Analysis

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    High-spe ed lightwavecomponent analysis

    Application Note 1550-6

    Characterizing

    sys tem components

    Laser and LED transmit ters

    Ph otodiode receivers

    External modulators

    Optical components

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    2

    As lightwa ve tra nsm ission systems become m ore advan ced, component designers an d

    ma nu factu rers m ust ma ximize the per form an ce of th eir devices. For example, one

    par am eter often used t o specify digita l system performan ce is bit err or rat e. However,

    it is difficult to specify individual components in such terms. Rather, fundamentalmeasu rement s such as gain, bandwidth, frequency response an d retu rn loss can be

    appr opriat e. The Lightwave Component Analyzer (LCA) is used t o measur e th e linear

    tr an smission an d r eflection char acteristics of a component as a function of modulation

    frequency. Measuremen ts ar e calibrated a nd can be performed a t modulat ion ra tes up

    to 20 GHz.

    Table of Conte nts

    Introduct ion

    Genera l measurement t echniques and considera t ions 3The Lightwave Component Analyzer (LCA) family 4

    Lightwave transmitter measu remen ts (E/O)

    Modu la tion ba ndwidth , frequ en cy r espon se, a nd con version efficien cy 5

    The effect s of bias on laser per formance 7

    Laser pulse measurements 7

    Laser reflect ion sensit ivity 8

    Modula t ion phase response 8

    Laser input impedance 9

    Electro-opt ic e xternal m odulator me asurem en ts (E/O)

    Modula tor bandwidth and responsivity 11

    Lighwave receive r measurem ents (O/E)

    Modu la tion ba ndwidt h, fr equ en cy r espon se, a nd con ver sion efficien cy 12

    Photodiode pulse measurements 13

    Photodiode modula t ion phase measurements 15

    Photodiode output impedance 15

    Optical compo nen t meas ureme nts (O/O)

    Transmiss ion measurements 17

    Fiber length and propagat ion delay 17

    Fiber modulation pha se sta bility 18

    Reflect ion me asurements 18

    Methods for measur ing lightwave reflect ions vs. distance 18

    Achieving both high resolut ion an d long ra nge 20

    Electrical compo ne nt measu remen ts (E/E) 21

    Appen dix 1: Signal relat ionships in op to-electric de vices 21

    Appen dix 2: Operat ion in the t ime dom ain

    Basic considera t ions 22

    Range and resolu t ion 23

    Improving measurement accu racy through ga t ing 23

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    Introduct ion

    General Measurem ent

    Techn i ques a ndConsiderations

    The concept of lightwa ve

    component a nalysis is str aight-

    forward. Measurements ar e made

    of th e small-signal linear tra ns-

    mission and reflection character-

    istics of a va riety of lightwa ve

    componen ts. A pr ecise electrical

    (signal genera tor) or optical (laser)

    source is used to stimulate th e

    component under test an d a very

    accurate optical or electrical

    receiver measures t he t ransmit-

    ted (or r eflected) signal. Sin ce

    characterization over a range

    of modulation frequencies is

    required, the frequency of mod-

    ulat ion is norma lly swept over

    the bandwidth of interest.

    Measurem ents a re typically

    comprised of the appr opriate ra tio

    of microwave modulat ion cur ren t

    (or power) and lightwave modu-

    lation power (see Figure 2).

    While Figure 1 demonstra tes

    th e basic concepts of lightwa ve

    component analysis, the specific

    measur ement processes are illus-

    tr ated later. An a na lysis of how

    various signa ls are used in the

    measu remen t pr ocess is found

    in Append ix 1, "Signa l Relation-

    ships in O pto-electric Devices."

    LWSource

    LWReceiver

    Display

    Amp

    O/O

    E/E

    RF Source

    E/O

    O/E

    O/O, E/O, O/E, or E/E

    Deviceunder test

    Modulated Lightwave

    modOpticalModulationPower

    modElectricalModulationCurrent

    InputDevice

    Under Test Output

    P : I :

    E/O measurement =

    O/O measurement =

    P Out

    I In

    P Out

    P In

    mod

    mod

    O/Emeasurement =

    I Out

    P In

    mod

    mod

    mod

    mod

    Laser

    Photodiode

    Fiber

    Figu re 1. LCABlock diagram

    Figure 2.Measurementsignals

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    O/ O Measurem ents

    Characteristics of purely optical

    devices can a lso be measur ed. Inthis case, both the stimulus and

    response are m odulated light. The

    rat io measur ement is simply one

    of gain or loss versu s modula -

    tion frequen cy.

    Measurement Process

    To simplify th e pr ocess of mak ing

    measur ements , LCAs ha ve a

    built in Guided setu p featu re.

    This will lead th e user th rough

    the basic measurement setup

    an d calibration featu res.

    Measurement Calibration

    The key to making accurate E/O,

    O/O, or O/E m easur ements is

    calibrated instrument ation. Th e

    instru ment lightwave source and

    receiver a re individua lly cha ra c-

    terized. The systematic responses

    of the components ma king up t heLCA can th en be rem oved, yield-

    ing the response of the device

    under test (DUT). (See Appendix

    1, Signal relationships in opto-

    electric devices for m ore det ail.)

    The LCA Family

    There are several instrum ents

    in the LCA family. Their charac-

    teristics are sum mar ized below:

    Please refer to the Hewlett-Packard

    Lightwave Test an d Measur e-

    ment Catalog for a complete

    listing of Lightwave Component

    Analyzers a s well as other light-wave test equipment.

    An LCA measu res input m odulat-

    ing curr ent and output modulation

    power a nd displays the rat io of the

    two in Wat ts/Amp, either linearly

    or in decibels.

    O/ E Measurements (Photodiodes)

    The m easur ement process for O/E

    devices is s imilar to E /O devices.

    The measu rement consists of th e

    ratio of output electrical modu-

    lation cur rent to inpu t optical

    modula tion power. Slope respon-

    sivity for O/E devices describes

    how a change in optical power

    produces a cha nge in electrical

    current . Graph ically this is

    shown in Figure 4.

    The LCA measures th e input

    optical m odulation power a nd

    output modulation current and

    displays the rat io of th e two in

    Amps/Watt.

    E/ O Measurem ents

    (Lasers, LED's)

    The measurement of an E/O

    tr an sducer is a combinat ion ofinput modulating current and

    outpu t optical modulat ion power.

    Slope r esponsivity is used to

    describe how a chan ge in input

    current produces a cha nge in

    optical power. Graph ically th is

    is shown in Figure 3.

    Responsivity Rs (W/A)= Pout/ IinRs (dB)= 20 log10 (Rs(W/A))/(1(W/A))

    PoutmW

    Iin mA

    Figure 3. E/O sloperesponsivi ty

    Responsivity Rr (A/W)= Iout/ PinRr (dB)= 20 log10 (Rr(A/W))/(1(A/W))

    IoutmA

    Pin mW

    Figu re 4. O/Eslope responsivi ty

    Modulation

    LCA (nm) Frequency Range

    HP 8702 850, 1300 or 300 KHz3/6 GHz1550

    HP 8703 1300 or 1550, 130 MHz20 GHzFP or DFB

    HP 8510/834201 1300 or 1550, 45 MHz20 GHzor FP or DFB

    HP 8720/83420

    1 See HP Product Note 8510-15.

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    Figu re 5. E/Omodulation band-width measurement

    Lightwave TransmitterMeasure me nts (E/O)

    The LCA is used t o cha ra cterizeth e tra nsmission and r eflection

    para meters of laser and LED

    sources with respect to modula-

    tion frequency. The transmission

    measu remen ts to be discussed

    include:

    modulation bandwidth and

    frequency response

    conver sion efficiency

    th e effects of bias

    pulse measurements

    reflection sensitivity modulation ph ase response

    laser input impedance

    Other laser m easurements includ-

    ing linewidth, chirp, and RIN

    ar e discussed in H P Applicat ion

    Note 1550-5 (or 371).

    Modulat ion Bandw idth,Frequency Response , andConversion Efficiency

    Modulat ion ban dwidth r efers

    to how fast a laser can be inten -

    sity modu lated, wh ile conversionefficiency (responsivity) refers

    to how efficient ly an electr ical

    signal driving a laser is converted

    to modulated light . Alth ough

    responsivity is often used to

    describe a sta tic or DC par am e-

    ter, the conversion efficiency of

    a device for modulation signals

    is a dynam ic chara cteristic and

    can be r eferred t o as slope

    responsivity.

    It is not un usu al for slope

    responsivity to vary according

    to how fast the electr ical signal

    is varied. As th e frequency of

    modulation increases, eventua lly

    th e conversion efficiency will

    degrade or roll off. The fre-

    quency wher e th e conversion

    efficiency drops to one-half of

    th e maximum is the 3 dB

    point (when dat a is displayed

    logarith mically) an d det ermines

    a laser s modulat ion ba ndwidth .

    Distortion of modulation signalswill occur if the frequency response

    is not flat an d th ere a re fre-

    quency componen ts wh ich exceed

    a laser s ban dwidth.

    The measu remen t of modulation

    bandwidth consists of stimulat-

    ing a laser with a n electr ical

    (microwave or RF) signal a nd

    measu ring its response (modu-

    lated light) with a l ightwave

    receiver. Normally th e frequency

    of an electrical signal into alaser is swept t o allow cha racter-

    ization of the laser over a wide

    range of modulation frequencies.

    Measurement Results

    and Interpretation

    Figure 5 shows the m easure-

    men t of the conver sion efficiency

    of th e laser as a function of mod-

    ulation frequency. The display

    uni ts a re Watt s per Amp (the

    vertical axis). In t his case, the

    display is in a logarithmic format

    where 0 dB represents 1 wat t

    per a mp. The h orizontal axis is

    modulation frequency, indicating

    that the measurement is being

    made over a wide range of fre-

    quencies, in th is case from

    300 kHz to 3 GHz.

    As stated, this measurement

    indicates h ow fast th e laser can

    be modulated. This part icular

    laser has a modulation ban dwidthof about 1.5 GHz. Beyond th is

    frequen cy, t he conver sion effi-

    ciency is gradually degraded.

    There are two significant compo-

    nents tha t limit t he modulation

    bandwidth. One is the actual

    const ruction of a laser including

    the physical dimensions and

    fabrication process. The other is

    how efficient ly an electr ical signa l

    is delivered to th e laser. (See

    Laser input impedance.)Measurement Procedu re

    An accura te measur ement

    requires a user calibration. A

    user calibration will allow the

    LCA to remove the response of

    the t est system, including the

    electrical cables, optical fiber,

    and the instr ument i tself. Prior

    to the a ctu al calibrat ion st ep,

    th e LCA needs to be configured.

    This in cludes:

    start and st op frequencies sweep type (linear or logarithmic)

    number of measurement points

    measurement sweep t ime

    sour ce power level

    Note: LCAs have a Guided

    Setup feature t hat leads th e user

    thr ough al l the s teps that a re

    described here. Guided setu p is

    accessed by press ing SYSTEM

    key an d th e [Guided setup] soft-

    key. The following t ext d iscusses

    th e processes that th e guidedsetup executes.

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    Figu re 7. E/Omeasurement

    To perform a simple frequency

    response calibration, th e con-

    nections sh own in F igur e 6 must

    be made. The analyzer mea suresthe a ppropriate path s so the fre-

    quency and phase response of the

    un known path (s) is/are then

    char acterized. The a nalyzer then

    uses t his inform at ion in conjunc-

    tion with t he int ernal calibrat ion

    data to generate an error matrix.

    (The lightwave source and receiver

    characteristics a re pre-determined

    dur ing a factory calibration an d

    stored in m emory. The st orage

    meth od depends on th e type of

    LCA used). The end r esult is th edisplayed response of the laser

    under test alone.

    After the calibration is complete,

    one might expect t o see a flat

    response at 0 dB indicating th e

    test system r esponse ha s been

    removed. When using an HP 8702,

    th e display seen u pon completion

    of th e response calibra tion pr o-

    cess will not n ecessarily be a flat

    line. The laser used in th e cali-

    bra tion is sti l l conn ected a ndha s become the DUT. Thus, its

    response is displayed unt il it is

    replaced with th e actual tes t

    device. When the HP 8703 cali-

    bration is completed, no response

    (other th an noise) is displayed

    until an E/O test device is con-

    nected between the electrical and

    optical measurement planes.

    In a ddition to the simple response

    calibration, there are also the

    resp onse plus isolation andthe response plus match cali-

    brat ions. Th e isolation calibra-

    tion is used for high insert ion

    loss (low conver sion efficiency)

    devices wher e an y signal leak-

    age within the instrument m ay

    be significan t r elative to the

    actual signals measured. The

    ma tch calibrat ion is used to

    remove the effects of reflections

    between the instrument electri-

    cal test port a nd th e laser undertest. If the laser being tested ha s

    a poor electr ical input ma tch, the

    response and m at ch calibration

    can pr ovide a significan t improve-

    ment in measurement accuracy.

    (The response an d ma tch cali-

    bra tion is only available with the

    HP 8703 LCA.) An exam ple of

    the r esponse plus ma tch calibra-

    tion is found in t he section on O/E

    receiver measurements.

    Once the setup a nd calibrat ionha ve been completed, th e laser

    under test is connected an d accur-

    ate measur ements can be made.

    Accuracy Considerations

    There a re several items to con-

    sider with respect to measur e-

    ment accuracy. These include:

    Keeping all electrical an doptical connectors clean and in

    good cond ition

    Operating the test device in

    l inear regions (unsat ura ted

    conditions)

    Avoid overdriving th e instr u-

    ment receiver

    Minimizing cable movement

    Allowing the instru ment t o

    warm-up

    Keeping both optical an d elec-

    tr ical reflections at a m inimum

    (for tra nsmission measur ements)

    Figu re 6. E/Ocalibrationconfiguration

    HP 8702 HP 8703

    HP 8340XSource

    HP 8341XReceiver

    HP 8702 HP 8703

    E/O DUT HP 8341XReceiverE/O DUT

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    7

    The Effects of Biason Laser Performance

    The frequency response of

    a laser is also dependent onbiasing conditions. As th e DC

    bias of th e laser is increased,

    the bandwidth will generally

    increase. This is typically due

    to th e rela xat ion oscillation

    characteristics that vary with

    bias. The relaxation oscillation

    phenomenon creates a r esonan ce

    in th e frequency response, noise,

    an d distortion of th e laser.

    Figur e 8 is a composite of a

    bandwidth measurement made

    at th ree different bias levels.

    (The horizont al a xis is log fre-

    quen cy.) As bias is increa sed,

    both responsivity and band-

    width increase. For th is laser,

    as bias rea ches a certa in point,

    the high-end r esponse begins to

    degrade.

    Note in th e two lower tr aces

    that the response tends to peakbefore rolling off. This is t he

    region of relaxat ion oscillation.

    Care must be tak en when mod-

    ulat ing a laser in th is region,

    becau se this is where n oise and

    distortion properties ar e often

    at th eir worst. (See HP Appli-

    cation N ote 1550-5 (or 371),

    Measur ing Modulated Light.)

    Laser Pulse Measurements

    Fr equency doma in informa tion

    (modulation bandwidth) is related

    to time domain perform an ceusing th e an alyzer s time domain

    featu re. An LCA uses the mea-

    sur ed frequency domain (band-

    width) data and math ematically

    man ipulates it thr ough a form of

    an inverse Fourier tra nsform to

    pred ict t he effective step an d/or

    impulse r esponse of a laser. (See

    Appendix 2, "Operat ion in t he

    time domain;" Basic considera-

    tions.)

    Measurement Resultsand Interpretation

    Figure 9 shows th e predicted

    impulse response of a high-speed

    laser. The da ta is displayed in

    a linear m agnitude format (as

    opposed t o logar ithmically in dB).

    Several items of informa tion ar e

    available from this measurement.

    One is basic impulse width, which

    is a measure of device speed. Two

    time values a re shown. The PW

    value is the time between mark-

    ers at the half-maximum points.However, part of the response is

    due to th e finite bandwidth of

    the inst ru ment itself. The Net

    PW value is impu lse response

    with th e instru ment s response

    removed.

    Figure 8. Compositeplot of bandwidth at3 bias levels

    Mark er 1, at 10.337 ns, is the

    effective delay or propa gat ion

    time through the laser device

    from t he electr ical inpu t t o theoptical outpu t. The device ha s a

    long len gth of fiber pigtail wh ich

    is the main cont ributor to the

    tota l delay.

    Note also th at t here is a

    secondary impu lse. This typi-

    cally indicates the presence of a

    reflection and re-reflection.

    Figure 10 shows the pr edicted

    step r esponse of th e sam e laser.

    From this measur ement we can

    determine r isetime, ringing, andovershoot performance. In gen-

    eral, these parameters a re directly

    related to the frequency response

    of th e device. (For a compa rison

    of time-doma in measu remen ts

    generat ed by an LCA versus a n

    oscilloscope, see Figur e 24, page

    14 under Ph otodiode Pu lse

    Measurements).

    Figu re 9. E/Oimpulse response

    Figu re 10. E/Ostep response

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    8

    Figure 11.Reflectionsensi t ivi tyse tup

    Measurement Procedu re

    Pulse measurements ar e gener-

    ated by manipulating measured

    frequency response da ta. Conse-quently, the measurement pro-

    cedure is almost identical to that

    used for th e modulation ban d-

    width. (Potent ial differences

    exist du e to requirements of th e

    math ematical t ransform. See

    Appendix 2, "Operat ion in th e

    time domain.")

    Laser Reflection Se nsit ivity

    The frequ ency response of a

    laser ma y be modified if light is

    reflected back int o th e laser scavity. The r eflection sen sitivity

    of a laser can be mea sur ed as

    shown in F igure 11.

    Measurement Procedu re

    The measurement setup is simi-

    lar to the measu remen t of mod-

    ulation bandwidth. In addition,

    a directiona l coupler is inserted

    in the optical path (prior to cali-

    brat ion) in order t o monitor th e

    tra nsmitted light and minimize

    th e instru ment s response to the

    reflected light. The controlled

    reflection is conn ected to the other

    arm of the coupler. For an accu-

    rat e measurement , it is essential

    th at all optical reflections, except-

    ing th e cont rolled reflection, be

    kept at a minimum.

    Typically, a las er s frequ ency

    response with back-reflected

    light is compared t o the response

    when n o reflections are pr esent.

    The r esponse calibration for the

    reflection sen sitivity measu re-ment (un der th e Guided setup

    menu ) norma lizes the frequency

    response to a flat line when no

    reflections a re pr esent. As the

    back-reflection is increased, and

    the polarization of the reflectedlight is adjusted for worst case

    results, th e modulation response

    will deviate from th is norma lized

    tra ce and sh ow the r eflection

    sensitivity.

    Measurement Interpretation

    In t his case, the r esponses for

    severa l levels of reflections ar e

    shown in F igure 12, a composite

    diagram (th rough offsett ing

    subsequent measu rements by

    changing th e display reference

    level). The magnitude and polar-

    ization of the reflected light are

    adjusted wh ile th e laser s outpu t

    is monitored by the LCA. Depend-

    ing on how well the las er is iso-

    lated, and its inherent sensitivity,

    the frequen cy response of the

    laser can be significan tly impacted

    by reflected light. In the worst

    case, (a reflection of approximately

    4 dB retu rn loss) the modulation

    response shows a 3 dB pea k-to-

    peak variation.

    When a laser is used in an actualsystem, th e amoun t of back-

    reflected light m ay be u nkn own.

    Thus, it is desirable to develop

    a r obust laser wh ose chara cteris-

    tics will be consist ent over a diver-

    sity of opera ting en vironm ents.

    Modulat ion Phase Response

    Idea lly, a laser s m odulat ion

    envelope will exhibit a linea r

    phase response versus modula-

    tion frequen cy. If th e relat ive

    pha se relationships of the mod-ulation frequencies do not remain

    const an t, a form of distortion will

    occur. The pha se response of the

    laser can be displayed in two

    ways. One way is to display the

    pha se r esponse directly. The

    second is to display th e pha se

    resp onse in a delay form at .

    HP 8702 (or 8703)

    E/O DUT HP 8157/8Attenuator

    v

    HP 81000BRReflector

    HP 11894Polarization

    Adjuster

    HP 11890/1Directional

    Coupler

    HP 8341XReceiver

    Figure 12. Reflectionsensi t ivi ty for severallevels of reflection

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    9

    Measurement Procedu re

    and Interpretation

    Ph ase dat a is displayed by

    simply choosing the dat a formatto be ph ase as opposed to th e

    defau lt log mag. If th e DUT

    ha s any significan t length in

    either th e optical or electrical

    pat h, some compensat ion in

    length (thr ough the electr ical

    delay function un der the Scale

    Ref key) will be r equir ed for

    viewing the ph ase r esponse of

    the laser. In th is measurement,

    10.315 ns of electr ical dela y is

    added, because t he fiber pigtail

    is about 2 m long.

    The p ha se res ponse often fol-

    lows th e frequ ency response.

    The frequency response of this

    laser rolls off at the same fre-

    quency range where the phase

    begins to deviate from a linear

    response.

    Figu re 14. E/Odelay measurement

    Figu re 13. E/Ophase response

    Sometimes the phase response

    is easier to interpret an d use

    when viewed in the delay dataform at . The plot of delay is us ed

    to indicate t he effective time it

    ta kes for a m odulat ing signal at

    the input of the E /O DUT t o exit

    the device as m odulated light.

    Ideally, th is tr an sition time will

    be th e sam e for all modulationfrequencies of interest.

    Figure 14 sh ows the delay for a

    3 GHz laser. The average pr opa-

    gation t ime over the 3 GH z band-

    width is near 6.3 ns.

    Laser Inpu t Imped ance

    The convers ion efficiency of a

    laser is dependen t n ot only on

    the inh erent pr opert ies of the

    laser, bu t a lso on h ow efficientlythe electr ical m odulation signa l

    is delivered to th e laser. High-

    speed modulation signals are

    general ly t ran smit ted to the

    laser over tr an smission lines

    with a 50 or 75 ohm char acteris-

    tic impedance. Maximum power

    tra nsfer will occur if th e input

    impedan ce of th e laser is th e

    same as the t ran smission line.

    Unfortun at ely, the input imped-

    an ce of an active laser is much

    lower tha n th e tran smission sys-

    tem used to drive it. Two problemsoccur when such an impedan ce

    misma tch exists. First, a signifi-

    cant amoun t of energy will be

    reflected at the transmission

    line/laser inter face. This r eflected

    energy may eventu ally be re-

    reflected a nd distort the desired

    data signal. The second problem

    is tha t t he reflected ener gy is

    wast ed since it is never effec-

    tively used t o modulat e the las er.

    Thu s, th e overall conversion

    efficiency of the laser is degra ded.

    Measurement Procedu re

    Figure 15 shows th e retur n loss

    of a laser with a simple resistive

    matching circuit as measured

    on the component an alyzer. The

    measurement is made by send-

    ing a swept RF signa l to the laser

    under test and measuring the

    energy tha t r eflects back. The

    setup a nd calibrat ion pr ocedur e

    will depend on the model of LCA

    used. In all cases, a calibrat ionkit containing k nown electr ical

    reflection stan dar ds is required

    to improve the accuracy of the

    reflection measur ement s.

    Figure 15. E/O returnloss measurement

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    10

    Measurement In terpretation

    The retu rn loss over a 6 GHz

    ra nge varies from a best case of

    near ly 34 dB to a worst case of17 dB. It is not unu sua l for th e

    reflection level to get worse as

    th e modulation frequency is

    increased.

    Retur n loss is th e rat io of

    reflected to incident energy

    (10 Log (P refl/ P inc)). The larger

    the retu rn loss magnitude, the

    smaller th e reflected signal an d

    the better t he impedance match.

    Figure 16 uses the same mea-

    sured dat a as th e return loss plot,except in th is case th e data is

    displayed in a Sm ith Cha rt for-

    ma t. A Smith Ch art is a form of

    an impeda nce map. The display

    shows the laser input impedan ce

    as a fun ction of frequen cy. For

    th is laser, the impedan ce is close

    to 50 ohms over th e 6 GHz ran ge,

    as t he response does not deviate

    much from t he center of the char t.

    The Smith Char t data presenta-

    tion is selected under the Format key menu.

    Figure 16. Retu rnloss in Smith chartformat

    The impedance data from the

    Smith Cha rt can be used to model

    the inpu t str uctur e of th e laser.

    The laser s effective inpu t imped-

    an ce can be improved with a

    mat ching network. Simple meth -

    ods ar e usua lly resistive, while

    more efficient bu t complex meth-

    ods use reactive elements.

    Im plications of

    Impedance Mism atch

    on Measurement Accuracy

    When th e inpu t impedan ce ofth e E/O device under t est is far

    from 50 ohms, a significant por-

    tion of the electrical energy sent

    to th e device will be reflected.

    This r eflected energy can degrade

    measu remen t a ccur acy. This is

    typically seen a s r ipple in fre-

    quency r esponse measurements.

    Two techn iques ar e available to

    overcome t his pr oblem including

    th e response/match calibra tion

    (discussed in O/E measurements)

    an d gating (discussed in Appen-dix 2, "Operat ion in th e time

    domain").

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    11

    Electro-opticExternal ModulatorMeasurements

    External intensity modulators

    can be cha ra cterized in mu ch

    th e same way as laser sources.

    This is an other class of E/O

    measurements where the stimu-

    lus is a swept frequency electri-

    cal signal an d th e response out

    of th e modulator is inten sity

    modulated light . In par ticular,

    modulation bandwidth, phase,

    an d electrical impedance mea-

    surements are made with the

    component analyzer in t he sam e

    configur at ion th at is used for

    laser measurements.

    However, a significant difference

    exists due to the modulator being

    a thr ee-port device. While the

    frequency response of a m odula-

    tor is often independent of th e

    input optical power, th e respon-

    sivity is not. Th e conver sionefficiency of th e modu lat or is

    not only a function of th e elec-

    tr ical inpu t, but also the level of

    th e optical inpu t.

    The LCA measu rement compar es

    the output modulation power to

    the input modulat ion current .

    A responsivity in Wat ts per Ampis then computed an d displayed.

    If the inpu t optical power is

    increased, th e output modulation

    will typically also increase. Th us,

    the a ppar ent r esponsivity will

    increase. This means th at t he

    modulator responsivity mea-

    sur ement is valid only for the

    specific optical inpu t power t ha t

    existed when the measu rement

    was performed. Th e frequency

    resp onse is t ypically valid over

    a wide ra nge of input powers.

    Figure 18 is a measu rement of a

    wide bandwidth external modu-

    lator. The unu sua l response at

    the low frequency ra nge is due

    to the efficiency of the electrical

    impedance ma tching circuitry.

    Similar t o the process used for

    laser measurements, the phase

    response an d electrical input

    impedan ce can a lso be cha ra c-terized. The frequency domain

    informa tion can also be used to

    predict the step and impulse

    responses.

    Lasers are typically described

    by an input current versus output

    power relationship. The preferred

    description for a modulat or is

    often a n inpu t voltage versus out -

    put power relat ionsh ip. Becau se

    LCA measur ements assum e a

    50 ohm m easurement environ-ment , the LCA modulator mea-

    sur ement in Watts per Amp can

    be convert ed to Watts per volt by

    scaling (dividing) the measure-

    ment by 50. With th e HP 8703,

    th is can be achieved by setting

    th e nu mer at or K (gain ) term of

    th e coefficient model t o 50, load-

    ing the model into memory, and

    dividing th e dat a by memory.

    These functions are under the

    Display key.

    HP 8703

    CW LWSource

    DUT

    RF in

    LW out

    Figu re 17. E/Omodulator mea-surement setup

    Figure 18.Modulatorbandwidth

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    electr ical r eceiver. Normally th e

    frequency of the modulation is

    swept to allow examination of

    the photodiode over a wide ran geof modula tion frequen cies.

    Measurement Results

    and Interpretation

    The instru ment display of Figure

    19 shows the conversion efficiency

    of th e ph otodiode as a fun ction

    of modu lat ion frequ ency. The

    vertical axis display un its ar e

    Amps per Watt an d th e horizon-

    tal axis is modulation frequency.

    In t his case, the vertical axis is

    in a logarith mic format where0 dB (the center line of the dis-

    play) represent s 1 Amp per Wat t.

    12

    Lightwave ReceiverMeasurements(O/E)

    The measurements that t he LCAmakes on lightwave receivers

    are in m any ways similar to those

    ma de on lightwa ve sources. In

    th is case, th e stimulus will be

    modulated light an d the response

    will be demodulat ed electrical

    signals. Measurements include:

    photodiode responsivity an d

    modulation bandwidth

    step and impulse response

    char acterization and improve-

    ment of the electrical outpu timpedance

    As with the laser source, band-

    width m easurements a re relevant

    to pulse rise and fall times, while

    impedance measurements ar e

    important to minimize signal

    reflections and maximize elec-

    tr ical power tr an sfer. Optical

    power reflections are discussed

    in Optical components: Reflec-

    tion measurement s.

    Photodiode ModulationBandwidth, FrequencyResponse , andConversion Efficiency

    As discussed ea rlier, photodiode

    conversion efficiency refers to

    how a change in optical power is

    convert ed to a change in output

    electr ical curr ent. As th e fre-

    quen cy of modula tion increases,

    eventually the receiver conver-

    sion efficiency will rolloff. Thus,

    th e device ha s a limited modu-

    lation bandwidth.

    The m easurement of modulation

    band width consists of stimulat -

    ing the photodiode with a source

    of modulated light a nd mea sur-

    ing the outpu t r esponse (RF or

    microwave) curren t with a n

    Figu re 19. O/Ebandwidth andresponsivi tymeasurement

    The photodiode under test h as a

    modulation bandwidth of appr oxi-

    ma tely 1.5 to 2 GHz. The fre-

    quency response a lso shows some

    distinct resonances that will

    impact th e time-doma in (step

    or impulse) performa nce, as

    shown in Figures 22 and 23.Measurement Procedu re

    The measu remen t process is

    virtua lly identical t o the laser

    measur ement . An accura te

    measurement r equires a user

    calibration. This will allow the

    LCA to remove the response of

    the test system including the

    electrical cables, optical fiber,

    and the instr ument i tself. Prior

    to the actua l calibration step,th e LCA needs to be configured.

    This in cludes:

    start and st op frequencies

    sweep type (linear or

    logarithmic)

    number of measurement

    points

    measurement sweep t ime

    sour ce power level

    Note: LCAs have a Guided

    Setup featur e tha t leads the

    user th rough all the steps tha tar e described here. This is the

    recommended measurement pro-

    cedur e. Guided setup is a ccessed

    by pressing the SYSTEM key

    an d th e Guided Set up softkey.

    The following text discusses th e

    processes that the guided setup

    executes.

    To perform a s imple frequency

    response calibration, th e con-

    nections in Figur e 20 must be

    made. The analyzer then mea-sures the appr opriate path s. The

    frequency an d pha se responses

    of th e un kn own pat h(s) is/are

    then characterized. The analyzer/

    system u ses this inform ation in

    conjunction with the internal

    calibration data to generate an

    error ma tr ix. (The light wave

    source and receiver chara cteris-

    tics are predetermined and stored

    in m emory. The st orage meth od

    depends on t he t ype of LCA used.)

    The end resul t i s that the f re-quency and pha se responses of

    the ent ire test system are removed

    from the measurement so that

    th e displayed response is only

    that of the ph otodiode under t est.

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    13

    After complet ion of the calibra -

    tion, one might expect to see a

    flat response at 0 dB indicat ing

    the test system response has

    been removed. When u sing anHP 8702, th e display seen u pon

    completion of the response cal-

    ibra tion pr ocess will not neces-

    sar ily be a flat l ine. The O/E

    receiver used in th e calibrat ion,

    which is sti l l in th e measu re-

    ment path , has become the DUT.

    Thu s its response is now dis-

    played. When th e HP 8703 cali-

    bra tion is completed, no response

    other th an n oise is displayed

    until an O/E test device is con-

    nected between t he electr icaland optical measur ement planes.

    In a ddition to the simple response

    calibrat ion, ther e are also the

    response plus isolation and t he

    response plus ma tch calibrations.

    The isolation calibrat ion is used

    for high-inser tion loss (low con-

    version efficiency) devices, where

    an y signal leakage within t he

    instr u-ment m ay be significant

    relat ive to the actua l signa ls

    measu red. The ma tch calibration

    is used to rem ove th e effects of

    reflections between the instrument

    electrical test port a nd t he ph o-

    todiode under test. (The response

    an d ma tch calibrat ion is only

    available with the HP 8703 LCA.)

    Once th e setup an d calibrations

    have been completed, the instr u-

    ment is now ready to make accur-

    ate m easur ements. The receiver

    to be tested is placed in the m ea-surement path and its response

    can be seen, as in F igure 19

    O/E bandwidth and responsivity

    measurement, previously

    shown.

    Response an d

    Match Calibration

    The response and ma tch calibra-

    tion is used to impr ove measu re-

    ment u ncertainty when t he O/E

    test device ha s a poor outpu t

    mat ch. Impedan ce mismat ch

    leads to s tan ding waves tha t

    degrade th e measurement of

    device responsivity. Typically,

    th is problem is m ore pronounced

    at higher modulation frequencies.

    The response and match calibra-

    tion uses network an alysis error

    correction techniques to minimize

    th e effects of misma tch. The cali-

    brat ion requires a 1-port electr ical

    reflection calibration in addition

    to the thru tra nsm ission calibra-

    tion for t he optical and electr icalpaths.

    Figure 21 is a composite m easur e-

    ment of a high-speed photodiode.

    The lower tra ce is a measur ement

    with only th e normal responsecalibrat ion. The upper trace, which

    ha s lower ripple, is ma de using

    the response and match calibra-

    tion. The tr aces are intent iona lly

    offset for cla rit y.

    HP 8702 HP 8703

    HP 8340XSource

    HP 8341XReceiver

    Figu re 20. O/Ecal ibration con-figuration

    Figure 21. Responseand match cal ibration

    The r esponse m atch calibration

    can be executed by following

    the steps in the Guided Setup

    procedure.

    Photodiode PulseMeasurements

    To see what implications th e

    device bandwidth and frequency

    response have on the t ime domain

    performa nce, the time domain

    tra nsform can be used. This trans-

    form uses t he measured frequency

    response data t o predict the small

    signal st ep and impulse responses

    of the photodiode. (See Appendix 2,

    "Operat ion in th e time domain;"

    Basic considerations. )

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    14

    Figu re 22. O/Estep response

    gat ing removes t he effects of

    reflections and is discussed in

    deta il in Appendix 2, "Opera tion

    in th e time domain ;"Improvingmeasurement accuracy through

    gating.

    It is interestin g to compare th e

    predicted time-domain response

    with a tr ue time domain mea-

    sur ement . Figur e 24 shows a

    composite of the step response

    generat ed by an LCA in com-

    parison with the step response

    when measured using a sharp

    optical pu lse and a h igh-speed

    HP 54120 oscilloscope.

    The two measur ements agree very

    well. It is importan t t o remember

    that the oscilloscope measurement

    displays the combined response

    of the optical pulse, the oscillo-

    scope, an d th e photodiode. The

    LCA measurement can calibrat e

    out the response of the test system

    in order t o isolat e th e response

    of th e DUT. The tr ace magnitu de

    differences are du e to unequa l

    instr um ent vertical scales.

    Figure 22 shows the predicted step

    response of th e sam e photodiode

    whose bandwidth was measured

    in Figure 19. There are severalpoints of interest. Th e tr an sition

    from off to on or risetime (on

    the order of 180 ps) is dependent

    upon th e device ban dwidth

    (roughly 2 GHz). There is some

    ringing in the step response.

    The frequen cy of th e ringing

    corr elates d irectly to th e fre-

    quency response resona nce at

    3.2 GHz. Anoth er inter esting

    chara cteristic is the seconda ry

    step th at occur s roughly 600 ps

    after th e initial step. This is dueto reflections with in th e device,

    and is easier to understand by

    viewing the impulse response.

    Figure 23 shows the pr edicted

    impulse response of the photodi-

    ode using t he low-pass impulse

    data tran sform. This measure-

    ment provides several pieces of

    informa tion. First, we see the

    impulse width. The t ime between

    the m ark ers is 123 ps at th e full-width ha lf-maximum points.

    (This is due not only to the ph o-

    todiode bandwidth , but a lso th e

    finite bandwidth of th e instru -

    men t its elf. The net pulsewidt his th e effective pulsewidth of th e

    photodiode alone after r emoving

    th e effect of th e inst ru men ts

    bandwidth.) Another importan t

    data point is noted by mar ker 1

    at the pea k of th e response. This

    value is 621 ps a nd is t he effec-

    tive delay of th e ph otodiode or

    in other words, the a verage

    propagation t ime experienced

    by the modulation signal from

    the optical input to the electrical

    outpu t. A second impulse is notedby mark er 2. This response is

    due to an intern al reflection and

    re-reflection. Th e r e-reflected

    signal tra vels a longer distance

    than the primary impulse, and

    ther efore shows up with a rela-

    tive delay.

    Figu re 23. O/Eimpulse response

    Figure 24. Compos ite

    t ime domain mea-surements

    The reflection in the photo-

    diode has an adverse affect on

    the frequency response of the

    device. If this reflection could beremoved, the r esponse would be

    improved. A technique called

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    16

    The dat a can a lso be displayed

    simply as Retu rn Loss, th e ratio

    of reflected to incident power

    (10 Log (P re fl/ P inc).

    Figu re 28. O/Ereturn lossmagnitude

    Figure 29. Timedomain display of electrical reflec-t ions

    Figu re 27. O/Ereturn loss inSmith chartformat

    Measurement Procedu re

    and Interpretation

    The setup and measur ement

    of photodiode ret ur n loss ar eidentical to th e procedure u sed

    in characterizing laser r eturn loss.

    See Laser inpu t impedan ce

    on page 9. Figure 27 sh ows the

    ret ur n loss of an optical receiver

    measured with the component

    an alyzer, displayed on a Smith

    Char t. A Smith Ch ar t is a form

    of an impedance map . The dis-

    play shows the outpu t impedan ce

    as a fun ction of frequen cy. For

    this receiver, an electrical amp-

    lifier follows the photodiode, sothe measur ed impedan ce is essen-

    tially that of the amplifier. Over

    the 6 GHz measurement ran ge,

    the impedance stays reasonably

    close to 50 Ohms (th e center of

    the Sm ith Cha rt). The ideal case

    would be for the impeda nce to

    be a consta nt 50 (or 75) Ohms.

    The Smith Chart data presenta-

    tion is selected u nder the Format

    key menu.

    Using the time domain feature

    of th e LCA can help to determine

    the locations of any discontinu-

    ities in the electr ical pat h of theph otodiode as sembly. Figur e 29

    is a t ime/distance represent ation

    looking back int o a ph otodiode

    assembly. (This is the same pho-

    todiode measu red on pa ges 12

    to 14, where it wa s shown in a

    tra nsmission measurement th at

    there were significant reflections.)

    SMAConnector

    Joint50 Ohm

    Transmission Line

    PhotodiodeAssembly

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    17

    Optical Componen ts(O/O): Tran sm iss ionand Re f lect ion

    Measurements

    Consistent, accurate measure-

    ments of multi-mode fiber band-

    width ar e difficult to achieve using

    an LCA, principally due to th e

    fibers inherent instability in m ode

    stru ctur e and distribution. How-

    ever, frequency response data can

    be used in a time domain forma t

    to yield pr ecision length an d

    propagation delay tra nsm ission

    measurements and high-resolu-

    tion reflection measu remen ts.

    TransmissionMeasurements

    Fiber Leng th andPropagat ion Delay

    In the following example we want

    to determine the length of a sec-

    tion of singlemode fiber. The mea-

    surement will be made by using

    a modulated optical signa l with

    a swept modulation frequency.

    The ran ge and resolut ion a redirectly dependent upon the m od-

    ulation frequency bandwidth and

    the nu mber of measur ement

    point s. A useful tool built into the

    HP 8702 and HP 8703 that assists

    in making time domain measure-

    ments is th e tra nsform param -

    eter s function. See Appendix 2,

    Operat ion in th e time domain;"

    Transform Param eters.

    Measurement Results

    and InterpretationFigure 30 shows the result

    of th e fiber tr an smission m ea-

    surem ent displayed in th e time-

    domain. The frequency-domain

    data has been t ran sformed to

    predict t he impu lse response of

    th e fiber.

    Figure 30. Impulseresponse of a lengthof fiber

    Placing a marker a t the peak

    of the pulse indicat es th e propa-gation time th rough th e fiber,

    24.429 ns. If we know the index

    of refraction, we can calculat e th e

    physical length of th e fiber. Con-

    versely, if we kn ow the p hysical

    length , we can calculat e th e fibers

    index of refraction. The impulse

    width is due t o the finite ban d-

    width of the LCA and not th e

    fiber itself.

    Measurement Procedu re

    The measurement setup is

    stra ightforwar d. The swept m od-

    ula ted optical source is connected

    th rough a short piece of fiber to

    the inst ru ment s light wave

    receiver. A mea sur ement cali-

    bration is required to remove the

    tra nsmission path length an d

    frequency response er rors of theLCA sour ce and receiver.

    Care must be tak en in setting

    the instrum ent sweeptime and

    IF ba ndwidth , part icular ly for

    long devices. This is because

    th e LCA tun ed receiver cont in-

    ues to sweep while the stimu lus

    signal is delayed through th e

    fiber. The m inimum sweeptime

    for a given device delay is det er-

    mined by the combination of IF

    bandwidth, number of measure-ment point s, and th e frequen cy

    span . There are no simple rules

    to follow in set tin g th e critical

    parameters. The best procedure

    is to set th e sweeptime to a large

    value, such a s 10 seconds, with

    th e DUT conn ected, prior to per-

    form ing a calibra tion. (If th ere is

    no response, the sweeptime may

    need to be increased furt her ). The

    sweeptime is sequent ially reduced

    un til the response cha nges. The

    sweeptime is then increased backto a level giving a st able mea-

    surement .

    Figu re 31. O/Ocal ibration s etup

    HP 8702 HP 8703

    HP 8340XSource

    HP 8341XReceiver

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    18

    Once th e measur ement calibra-

    tion h as been performed, th e test

    fiber can be conn ected between

    th e short fiber and th e test sys-tem. The initial measurement is

    ma de in the frequency domain.

    Actual length measur ements are

    determined through t he t ime-

    domain t ran sform. Measurement

    accuracy is discussed in Appen-

    dix 2, Operat ion in th e time-

    domain.

    Fiber ModulationPhase Stabil i ty

    In cert ain fiber optic microwave

    link applications, it is importan t

    for t he m icrowave signal to ha ve

    a very stable phase response

    relative to other signals propaga-

    ting on different fibers or through

    different media. If the index of

    refraction varies with temper a-

    tur e, or some other environmen tal

    parameter, the carrier (l ight)

    velocity an d th us t he m odulat ion

    envelope will experience a rela -

    tive phase sh ift.

    Because we ar e attempt ing to

    measure a change in the fiber

    char acter is t ics , the setup a nd

    calibra tion procedur es ar e dif-

    ferent t han for m ost measu re-

    ment s. In th is case, we calibrate

    the instru ment with the fiber

    un der test conn ected to the

    instrument .

    HP 8703

    Figure 32. Pha sestability calibration

    With th e fiber under t est in

    place during th e calibrat ion, we

    effectively rem ove an y respons e

    present in an ambient environ-ment. Care must be taken th at

    effects other tha n th e param eter

    of interest (for example t emper-

    ature) do not impact the measure-

    ment. For instance, any bending

    of th e cable after calibrat ion can

    cause a change in the pha se

    response.

    For this measurement, the

    device un der test is a 10 km

    spool of fiber. The mea sur emen t

    is made with a CW modulat ionfrequen cy of 10 GHz. In stea d of

    sweeping frequency, th e m easur e-

    ment is ma de over a 16 minute

    time span. It can be seen t hat

    the modulation phase response

    does vary significantly with time.

    In this measurement , the rela-

    tive phase response begins a t

    roughly 60 degrees (some phase

    change ha s already occurred

    between the time the calibration

    was completed and t he measu re-

    ment began). The pha se contin-ues t o cha nge to 180 degrees,

    where th e an alyzer rolls over

    to +180 degrees. For the given

    time span , the total variation is

    appr oximately 150 degrees.

    As shorter lengths of fiber ar e

    examined, the phase response

    variance versus time will become

    sma ller. However, other pa ra m-eters such as temperatu re or

    physical stress can cause ph ase

    variat ion, even over short ru ns

    of cab le.

    Reflection Measurements

    In a high-speed fiber optic

    system, reflected light can cause

    a variety of problems and come

    from several different sources.

    Both distributed feedback (DFB)

    and Fabry-Perot lasers are sen-sitive to light reflecting back int o

    their resonant structures. Both

    noise an d modulation chara cter-

    istics can be degraded. In a com-

    munication system, re-reflected

    light can arr ive at th e receiver

    an d potentia lly cause bit errors.

    To minim ize th ese effects, it is

    importa nt to char acter ize the

    am ount of light th at is reflected

    off of optical componen ts an d

    determ ine where t he r eflections

    occur.

    Methods for Measu ringLightwave Reflectionsvs. Distance

    In component development it is

    often n ecessary to determine t he

    physical location of the r eflection.

    If ther e ar e mu ltiple reflections,

    we mu st determine which reflec-

    tions contribute significantly to

    the total a mount of reflected light.

    There are a variety of methods for

    measu ring reflected light versu s

    distance or position. Among t hesemethods are optical time-domain

    reflectomet ers (OTDR), optical

    coher ence-domain reflectometer s

    (such as the HP 8504A precision

    reflectomet er), and optical fre-

    quency domain reflectometers

    (OFDR). The LCA uses the OFDR

    Figu re 33. O/Ophase measure-ment vs. t ime

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    19

    HP 8702

    Test Port

    HP 8341XReceiver

    HP 8340XSource

    HP 8703

    TestPort

    HP 11890/1 Figure 34.OFDR setup

    technique. Each technique has

    advanta ges an d disadvant ages.

    (When m easur ements of total

    retur n loss are required, withoutspatial informa tion, a power m eter

    solut ion su ch as the H P 8153A

    is used.)

    Determining both th e ma gnitude

    an d locat ion of reflections in light-

    wave components require t ech-

    niques beyond th e capabilities

    of a multimet er or conventional

    OTDR.

    The LCA is well suited for

    ma king h igh resolution reflec-

    tion measu remen ts of light wavecomponen ts. Th e LCA does not

    use a pu lse techn ique and con-

    sequently does not suffer from

    deadzone problems typical of

    OTDRs. Instead, a wide band-

    width swept frequency technique

    is used, which leads to precision

    location a nd resolut ion of each

    reflection.

    The set up for a r eflection

    measurement requires that

    th e light wave source be rout edto th e input of a dir ectional cou-

    pler. The DUT is conn ected to

    the coupler output a rm. The

    coupled ar m is connected t o the

    LCA receiver.

    The r esolution of th e LCA in

    OFDR mode is dependen t u pon

    the modulation frequency range.

    The wider the bandwidth, thehigher is the two-event r esolution.

    The closest t ha t t wo reflections

    can be and st ill be resolved is refer-

    red to as response resolution. (See

    Appendix 2, Operation in the

    time domain;Basic considera-

    tions.) A 20 GHz instr umen t band-

    width can pr ovide 5 mm of two-

    event resolution wh ile a 3 GH z

    bandwidth can provide 33 mm

    (in fiber). If higher resolut ion is

    required, th e HP 8504 precision

    reflectometer offers better tha n25 micron 2-event resolution. Mea-

    surement sensitivity is enhan ced

    thr ough trace averaging and set-

    ting the LCA IF bandwidth to a

    low value, su ch as 30 H z. This

    usually slows the measurement

    rate, but will reduce the effects

    of noise. Sm aller reflections can

    then be seen.

    Once the frequency range ha s

    been set, a calibration must be

    perform ed. The simplest cali-brat ion is achieved by using th e

    open-ended test port a s a Fresn el

    reflection stan dard. This assu mes

    tha t t he port is polished, clean,

    an d in good condit ion. With t his

    calibrat ion sta nda rd in pla ce,

    the a nalyzer measur es the light

    reflected off the test port as th e

    frequency of modulation is sweptover th e selected bandwidth.

    Thu s, the frequency response

    imper fections of th e LCA are

    ma th emat ically removed from

    the measurement .

    Figure 35 shows the reflections

    from a light wave cable consisting

    of th ree pa tchcords with simple

    PC conn ectors. The ma gnitude

    of th e r eflection for each conn ec-

    tor is easily seen. Settin g the

    index of refra ction t o 1.46, an dusing the marker functions, the

    length of each pa tchcord can be

    determ ined, at 1.514m, 1.761m,

    an d 1.756m r espectively.

    Figure 35. Multipleref lect ion measu rement

    Measur ement accur acy is dis-

    cussed in Appendix 2, Opera tion

    in the time domain.

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    (The sweeptime considerations

    discussed in O/O tr an smission

    measurements are even more

    critical here, since the signal istr aversing the length of the fiber

    twice before being detected.)

    98.513 s of electr ical dela y is

    added, and while in t he t ime

    mode, the spa n is reduced to

    show two reflections very close

    together. These are th e Fr esnel

    reflections at the two coupler

    outpu ts, which ar e measured to

    ha ve a different ial path length

    of 18 mm . The t wo-pass mea -

    surement technique has pr o-

    vided m illimeter resolut ion atth e end of a 10 km cable.

    Note: This technique is sus-

    ceptible to alias r esponses. The

    reflection a t t he inst ru men ts

    test port, or where t he coupler

    is conn ected to the fiber spool, can

    potentially show up in a nother

    region du e to th e limitations of

    th e tr an sform. To determine if a

    response is real or an alias, the

    num ber of measurement pointsshould be chan ged and th e mea-

    surement repeated. True events

    will ma intain their locat ion, wh ile

    alias events will move.

    20

    There are l imitations in the

    OFDR technique. The higher

    th e two-event resolution, the

    smaller th e overal l measur e-ment range. For instance, the

    20 GHz configuration with 201

    measu remen t point s offers th e

    best two-event resolution (5 mm

    in fiber), but t he one-way ran ge

    is only 1 meter. The mea sure-

    ment ran ge can be increased by

    increasing the nu mber of mea-

    sur ement p oint s, or decreasing

    the instruments frequency range,

    which will in tur n degrade t he

    two-event resolution. (See

    Appendix 2, Operat ing in t hetime domain.)

    Achieving Both HighResolut ion an d Long Range

    Some measurement scenarios

    require both high r esolution and

    long range. This can be achieved

    using t he LCA in a 2-pass

    measurement technique. The

    ana lyzer is first set up in a nar -

    row bandwidth mode that pro-

    vides a long enough ra nge to

    locate th e region of inter est. Thepropagation time to the ar ea of

    interest is deter mined. The LCAs

    frequency range is then widened

    to provide the two-event resolu-

    tion required t o isolat e th e indi-

    vidua l reflections. The electrical

    delay equal to th e propagation

    time t o the r eflections is added

    to the measurement (using the

    electrical delay function under

    th e Scale Referen ce key). This

    effectively pu lls th e r eflections

    of inter est into the instr um ent sreduced range.

    A High-resolution Measurem ent

    of Differential L ength

    To demonst ra te th is procedure,

    a long s pool of fiber with a 1X2coupler at t he end was m easured.

    The different ial length of the two

    arm s of the coupler is t he desired

    measurement.

    The first ta sk is to locate the

    coupler a t t he end of the fiber. The

    spool is estimated to be 10 km

    in length. The measurement span

    is configured t o provide 12 k m of

    ran ge. This requires a frequency

    spa n of only 2.5 MHz. After a

    response calibrat ion similar totha t described above, th e spool

    an d coupler a re th en conn ected

    to the test port, and the measur e-

    ment of Figure 36 is generat ed.

    Two reflections a re seen . One

    at time 0, corr esponding to th e

    fiber connection to the instrument,

    and another over 98.513 s (two-

    way) or 10.114 km (one way), at

    the cable end.

    The t ask is now to zoom in on

    the cable end an d examine the

    reflections in high resolution

    mode. The an alyzer ban dwidth

    is increased to 20 GHz an d placed

    in set freq low pass mode. The

    ana lyzer is then recal ibrat ed

    with t he DUT disconnected.

    Figure 36. OFDRmeasurement inwide span

    Figure 37. Zoomin gin on the cable end

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    21

    Electrical Compone ntMeasurements (E/E)

    Lightwave component analyzershave t he capability to operate a s

    RF an d microwave network ana -

    lyzers. They can th en be used t o

    chara cterize the electr ical compo-

    nent s used in lightwa ve systems

    including amplifiers, filters, coup-

    lers etc. For tu torial informa tion

    on RF an d microwave network

    an alysis please refer to the HP

    "Vector Semina r" booklet (HP lit-

    erature number 5954-8355.)

    Appen dix 1:Signal Relat ionships inOpto-electric Device s

    Signal Relationsh ipsUsed in ComponentMeasurements

    The LCA measurement technique

    is built upon concepts u sed in

    cha racterizing RF and m icrowave

    devices. S-para met er or s cat-

    tering matr ix techniques have

    proven to be convenient ways to

    chara cterize device per form an ce.

    The following section will discuss

    how similar techniques ar e usedin char acterizing devices in t he

    lightwave domain. This is intended

    to show the basis on which E/O

    an d O/E responsivity measu re-

    ments are defined.

    Figure 38 is a general represen-

    ta tion of a l ightwa ve system,

    showing input and output signals

    in term s of term inal voltages,

    input and output currents, and

    optical modulat ion power.

    S-para meters are used todescribe the tran smitted and

    reflected s ignal flow with in a

    device or network . For the model,

    the following S-par am eters a re

    defined:

    S11=b1 (a2= 0)a1

    S22

    =b2 (a

    1

    = 0)a2

    where:

    a1 =V1 incident on E/O deviceZ0

    = I1 Z0

    b1 =V1 reflected from E/O deviceZ0

    a2 =V2 incident on O/E deviceZ0

    b2 = V2 transmitted from O/E device

    Z0

    = I2 Z0

    It is interesting to note tha t

    delta volta ges and curren ts

    ar e used a s opposed to RMS

    values. Th is is done because we

    deal with m odulation signals in

    describing lightwa ve tra nsdu c-

    ers, where a cha nge in optical

    power is proportional to a change

    in electrical current or voltage.The overall system forwar d gain

    is defined as:

    S21 =b2

    (a2= 0)a1

    S12 = 0 (no reverse transmission

    is assumed)

    5050

    PI

    50

    PO P

    2

    I2

    II

    PO

    E/O O/E

    PO

    f

    Rr(A)

    WR

    s(W)

    A

    50

    Figure 38. Signaldefini t ions

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    Data Subject to ChangeCopyright 1992Hewlett-Packard CompanyPrinted in U.S.A. 4/975091 6478E

    With the t ime-domain tra nsform

    turned off, the gate function may

    rema in a ctive. The frequency

    response is now shown, butwith th e effect of th e reflection

    removed. It is apparent th at t he

    reflection has a significant effect

    on the frequency response. Thus,

    gating p rovides a useful tool to

    simulat e the resu lts of actu ally

    removing unwanted responses.

    The t ime-doma in gat ing function

    acts a s a time ban dpass filter

    tha t passes the primary response

    an d removes the responses dueto r eflections. Once t he reflec-

    tions ha ve been gated out , th e

    measurement can be returned

    to the frequency doma in. The

    frequency response displayed is

    as if th e reflected signals wer e

    no longer presen t.

    Figure 39 shows a photodiode

    response th at is degraded due

    to int erna l reflections.

    Analyzing the r esponse in t he

    time domain, the secondary

    impulse is determined t o be

    du e to a reflection.

    Using th e gating function (part

    of the tra nsform m enu), the time

    gate or filter is centered an dthe spa n a djusted to reject a ll

    but th e primary response. The

    gate center is noted by the T

    an d width by the two flag ma rk -

    ers. The gate is turned on, and

    the reflection response is

    removed.

    Figure 39.Degraded fre-quency response

    Figure 40. Timedomain response(with ref lect ions)

    Figure 42.Frequency responsewi th and wi thoutgating act ive (gatedtrace is offset)

    Figu re 41. "Gated "time domainresponse

    For more information aboutHewlett-Packard test and measure-ment products, and for a cu rrentsales office l isting, visit our website, http:www.hp.com/go/tmdir.