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    Misure di compatibilita

    Elettromagnetica

    Roberto Sacch i

    Electronic Measurements GroupAgilent Technologies

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    Agenda Introduzione alle misure EMI

    Terminologia;

    Sistema di misura (antenna, LISN, ricevitore, etc.);

    Detectors;

    Normative europee ed internazionali

    Misure di compatibilita elettromagnetica Misure di emissioni radiate

    Misure di emissioni condotte Misure di immunita(EMS)

    Setup di misura

    Camere anecoiche vs. OATS (Open Area Test Site)

    Soluzioni Agilent Introduzione al nuovo ricevitore EMI Full Compliance Agilent MXE

    Uso degli analizzatori Agilent della Serie-X per misure EMI pre-compliance.

    Sorgenti per i test di immunita

    Software applicativo

    Soluzioni complete tramite i nostri partners

    Page 2

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    Pre-compliance vs. Full compliance measurements

    Page 3

    Pre-compliance measurements

    Evaluate the conducted and radiatedemissions of a device using correct

    detectors and bandwidths before going

    to a test house for compliance testing

    Full Compliance measurementsFull compliance testing requires a receiver

    that meets all the requirements of CISPR

    16-1-1 (response to a CISPR pulse gen), aqualified open area test site or semi

    anechoic chamber and an antenna tower

    and turntable to maximize EUT signals.

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    What is EMC?

    Electromagnetic Compatibility (EMC): The ability of equipment to function

    satisfactorily in its electromagnetic environment without introducing intolerabledisturbances into that environment or into other equipment.

    Combination of Interference and Immunity.

    Electromagnetic Interference (EMI):Electromagnetic energy emanating from one device which causes another device to

    have degraded performance.

    Electromagnetic Immunity (Susceptibility, EMS): Tolerance in the presenceof electromagnetic energy (Performance degradation due to electromagnetic energy).

    Compliance measurements require a receiver that meets the requirements of

    CISPR part 16 (for commercial) or MIL-STD-461 (for military).

    All EMI receivers require a pre-selector at lower frequencies to limit the input energy

    and maintain sufficient dynamic range to meet the CISPR 16 requirements.

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    Definitions

    EMCElectroMagnetic Compatibility

    EMIElectroMagneticInterference

    EMS

    ElectroMagneticSusceptibility

    (aka Immunity)

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    EMI measurement system

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    Compliance EMI receiver requirements

    A CISPR 16-1-1 receiver must have the following functionality in

    the range 9 kHz - 18 GHz:

    A normal +/- 2 dB absolute accuracy

    CISPR-specified resolution bandwidths (-6 dB)

    Peak, quasi-peak, EMI average, and RMS average detectors

    Specified input impedance with a nominal value of 50 ohms; deviations

    specified as VSWR

    Be able to pass product immunity in a 3 V/m field

    Be able to pass the CISPR pulse test (implies pre-selector below 1 GHz)

    Other specific harmonic and intermodulation requirements

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    Receiver requirements above 1 GHz

    Above 1 GHz regulations require:

    1 MHz bandwidth for measurements

    No quasi-peak detector

    No CISPR pulse test, meaning no additional pre-selector required

    excellent sensitivity

    According to current FCC regulations, the maximum test frequency is the

    fifth harmonic of the highest clock frequency for an unintentional radiator(for example, computers without wireless connectivity) and the tenth

    harmonic for an intentional radiator (such as a cellular phone or wireless

    LAN).

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    What is an EMI Receiver?Lets begin with a spectrum analyzer

    Page 9

    Display and measure amplitude versus frequency for RF & MW signals

    Separate or demodulate complex signals into their base components (sine waves)

    Spectrum Analysis

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    OverviewTypes of Tests Made

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    Modulation

    Noise

    Distortion

    EMC

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    Architecture of Modern Spectrum/Signal Analyzers

    What does Modern mean?

    Digitize the IF output, not detector output

    FFT and swept capability (neither one is optimum for everything)

    Data output available

    Connectivity

    Automated measurement features Ability to use new features and duplicate or expand necessary old ones

    Complete spectrum analyzer & vector signal analyzer

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    Theory of OperationSwept Spectrum Analyzer Block Diagram

    Page 12

    Pre-Selector

    Or Low PassInput Filter

    Crystal

    Reference

    Oscillator

    Log

    Amp

    RF inputattenuator

    mixer

    IF filter

    (RBW)envelope

    detector

    videofilter

    local

    oscillator

    sweep

    generator

    IF gain

    Input

    signal

    ADC, Display

    & Video

    Processing

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    Traditional Spectrum Analyzer

    Scalar analysis

    Digitizing the video signal

    Classic superheterodyne swept spectrum analyzer

    Product detector

    loss of phaseinformation

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    Digital IF Spectrum/Signal Analyzer

    Vector data CAN be preserved (mag/phase or I/Q)

    Digitizing the IF Signal

    Some troublesome operations

    and conversions are now

    fast, accurate DSP

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    OverviewDifferent Types of Analyzers

    Page 15

    Parallel filters measured

    simultaneouslyA

    ff1 f2

    FFT Analyzer

    A

    ff1 f2

    Filter 'sweeps' over

    range of interest

    Swept Analyzer

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    SpecificationsResolution: RBW Type Determines Sweep Time

    280 sec134 sec

    13.5 sec

    8563E Analog RBW

    PSA Digital RBW

    PSA FFT RBW

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    Speed Improvements

    Useful comparisons highly specific, many factors

    PXA mode switching typically faster than PSA

    Where speed is critical, consider modifying measurement routines to

    include features such as list sweep

    Benchmark PXA PSA Speedimprovement

    Preset (*RST) 28 ms 168 ms 6x

    Marker peak search 6.5 ms 78 ms 12x

    Local Update 13 ms 17 ms 1.3x

    CF Tune and Transfer (4 - 5GHz) 109 ms 186 ms 1.7xRemote sweep and trace transfer 18 ms 30 ms 1.67x

    Nominal speed comparison, PSA example:

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    Modern spectrum analyzer

    Resolution BW Selectivity or Shape Factor

    Page 18

    3 dB

    60 dB

    60 dBBW

    60 dB BW3 dB BW

    3 dB BW

    Selectivity =

    Determines resolvability of unequal amplitude signals

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    Specifications

    Resolution: RBW Type and Selectivity

    Page 19

    DIGITAL FILTER

    ANALOG FILTER

    SPAN 3 kHzRES BW 100 Hz

    Typical

    Selectivity

    Analog 15:1

    Digital 5:1

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    Digital Filter Shape

    Better shape factor, biggest selectivity benefit for different signal levels

    Equivalent selectivity at a wider, faster-sweeping RBW

    digital filters swept an additional 3-4x faster

    30 kHz Digital Filter

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    MIL-STD-461 Bandwidth Requirements

    Measurement Range -6dB Bandwidth

    30Hz - 1 KHz 10 Hz

    1 KHz -10 KHz 100 Hz

    10 KHz - 150 KHz 1 KHz150 KHz - 30MHz 10 KHz

    30 MHz - GHz 100 KHz

    > 1GHz 1 MHz

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    Some modern analyzers approach accuracy of power meter + sensor

    Even better for low-level signals, with narrower noise bandwidth andthe benefit of frequency selectivity

    Some factors determining uncertainty:

    Input connector (mismatch)

    RF input attenuator

    Mixer and input filter (flatness)

    IF gain/attenuation (reference level)

    RBW filters

    Display scale fidelity

    Calibrator

    Modern Spectrum Analyzer Accuracy

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    Modern Spectrum Analyzer Accuracy Examples

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    Line Impedance Stabilization Networks (LISN)

    Page 25

    Purpose of a LISN:

    1. Isolates the power mains from theequipment under test. The power

    supplied to the EUT must be as clean as

    possible. Any noise on the line will be

    coupled to the X-Series signal analyzer

    and interpreted as noise generated by

    the EUT.

    2. Isolates any noise generated by the EUT

    from being coupled to the power mains.

    Excess noise on the power mains can

    cause interference with the proper

    operation of other devices on the line.

    3. The signals generated by the EUT are

    coupled to the X-Series analyzer using a

    high-pass filter, which is part of the LISN.

    Signals that are in the pass band of the

    high-pass filter see a 50- load.

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    LISN

    Page 26

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    LISN

    Page 27

    @ Electrical Network Frequency

    @ 150 kHz to 30 MHz

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    Transient Limiter

    The purpose of the limiter is to protect the input of the EMC analyzer from

    large transients when connected to a LISN. Switching EUT power on or offcan cause large spikes generated in the LISN.

    The Agilent 11947A transient limiter incorporates a limiter, high-pass filter,

    and an attenuator. It can withstand 10 kW for 10 sec and has a frequencyrange of 9 kHz to 200 MHz. The high-pass filter reduces the line frequencies

    coupled to the EMC analyzer.

    Page 28

    DUT

    LimiterLISN

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    Field Strength and Antenna factors

    Radiated EMI emissions tests measure the electric field. The

    field strength is calibrated in dBV/m.

    Antenna factors is the ratio of the electric field (V/m) present

    at the plane of the antenna versus the voltage out of the

    antenna connector.

    Log units:

    AF(dB/m) = E(dBV/m) - V(dBV)E(dBV/m) = V(dBV) + AF(dB/m)

    Notes:

    Antenna factors are not the same as antenna gain.

    dBV = dBm + 107

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    Detectors: Convert IF Samples to Display Bins or

    Buckets

    Multiple simultaneous detectors

    Screen Shot Detector 3types

    Time

    Volts

    Peak

    Neg Peak

    Sample

    Display points or

    buckets

    Normal, Average, Neg Peak

    Peak, Neg Peak, Sample

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    Detectors

    Page 33

    Most radiated and conducted limits are based on quasi-peak

    detection mode.

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    Peak QP AveragePeak Detector

    Initially used

    Faster than QP and Average modes

    If all signals fall below the limit, then the product passes and no futuretesting is needed.

    QP

    For CW signal, Peak = QP

    Much slowerby 2 or 3 order magnitude compared to using Peak detector

    Charge rate much faster than discharge rate

    the higher repetition rate of the signal, the higher QP reading

    Average

    Radiated emissions measurements above 1 GHz are performed usingaverage detection

    Page 35

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    Close field probe

    Page 36

    Measures the magnetic field H strength at the centerof its sense loop. The plane of the probe tip loops

    must be perpendicular to the radiating magnetic field

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    Test example

    Page 37

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    International emissions regulations (summary)

    Page 38

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    CISPR changes

    RMS-Average

    Preselector-less testing: enables use of spectrum analyzer for specific

    test cases.(no emissions with PRF < 20 Hz)

    CISPR 22 to 6 GHz

    Time Domain: sometimes required for the automotive market

    APD: soon to be required by CISPR11

    Page 39

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    G l P f M ki EMI M t

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    General Process for Making EMI Measurements

    Page 42

    Determine the country or countries in which the productwill be sold which in turn identifies the regulator agency.

    Select the limit lines to be tested to (conducted/radiated).

    Select the band to be used.

    Correct for transducer loses and amplifiers gains.

    Identify signals above the limit that must be evaluated.

    Zoom in on failed signal and perform quasi-peak or

    average measurements.

    C d t d E i i M t

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    Conducted Emissions Measurements

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    1. Connect DUT to the test system

    2. Set the proper frequency range3. Load limit lines and correction factors for LISN and limiter

    4. View the ambient emissions with DUT OFF

    5. Switch on the DUT and find signals above limits by using peak detector

    6. Measure all signals above limits with quasi-peak and average detectors

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    R di t d E i i M t

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    Radiated Emissions Measurements

    Page 46

    1. Connect the antenna

    to the EMI receiver and

    separate the antenna fromthe DUT as specified by the

    regulation requirements

    2. Set the proper frequency

    range and bandwidth

    3. Load limit lines and

    correction factors for

    antenna and cable.

    4. With DUT OFF, measure the ambient emissions and store them

    5. Switch on the DUT and find signals above limits by using peak detector (only those

    not present during the ambient scan). Rotate the DUT to maximize the emissions.

    6. Measure all signals above limits with quasi-peak and average detectors

    O A T t Sit (OATS)

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    Open Area Test Site (OATS)

    EUTs are measured in an open area test site (OATS) or anechoic chamber.

    ANSI C63.4 and CISPR 16-1-1 specify the requirements for an OATS, including: Preferred measurement distances

    of 3, 10, and 30 meters

    Antenna positioning at 1 to 4 meter

    Heights

    An area called the CISPR ellipseof major diameter 2X and minor

    diameter 3 X, where X is themeasurement distance; the ellipse

    must be free of any reflecting objects

    A metal ground plane for the measurement area

    Page 47

    Note: 10 meter anecho ic ch ambers and GTEM cel ls can also be used fo r radiated

    com pl iance measurements.

    1 Select the measurement range

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    1. Select the measurement range

    Page 48

    2 Load Corrections factors

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    2. Load Corrections factors

    Page 49

    Amplitude at

    point circled

    Amplitude

    referenced toblue line

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    Troubleshooting

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    Troubleshooting

    Page 53

    Use the close-field probe to locate the sources of the radiated signals

    exceeding the limit lines

    Immunity test setup

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    Immunity test setup

    Conducted Immunity

    100 kHz 1 GHz

    Amplifiers

    HF-Switch

    Radiated Immunity

    30 MHz 18 GHz

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    Agilent Solutions

    Page 55

    What is a CISPR 16-1-1 Compliant Receiver

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    What is a CISPR 16-1-1 Compliant Receiver

    CISPR 16-1-1 is the document that defines the

    functionality of an EMI receiver

    Detectors

    N9038A MXE EMI receiver is CISPR 16-1-1 2010 Compliant

    Frequencyresponse

    CISPR is a subcommittee of the IEC

    What is the MXE EMI Receiver?

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    X-Series

    signalanalyzer

    CISPR 16

    compliantEMI receiver

    What is the MXE EMI Receiver?

    The Agilent MXE is more than a CISPR 16-1-1 compliant EMI

    receiver

    It is also an X-Series signal analyzer that can run a variety of

    measurement applications

    The MXE can evolve as technology changes

    N9038A MXE EMI Recei er

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    20 Hz to 1 GHz forConducted Emissions

    (built-in limiter)

    20 Hz to 26.5GHz for

    Radiated

    Emissions

    CompliantPreselection 20 Hz

    to 3.6 GHz in both

    EMI Receiver

    Mode and SA

    Mode on

    Both Inputs

    CISPR 16-1-1 2010Compliant EMI Receiver

    N9038A MXE EMI Receiver

    in 30 seconds

    Run X-Seriesapplications

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    L

    CF

    RF

    IN

    DDS

    Noise Source

    20 Hz -1GHz

    Agilent X-Series Signal Analyzers

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    Agilent X-Series Signal Analyzers

    Multiple instruments in one box: Swept spectrum analyzer;

    FFT analyzer;

    RF and Baseband Vector Signal analyzer;

    Noise Figure analyzer. Fastest signal analysis measurements

    Broadest set of applications and demodulation capabilities

    Upgradeable HW

    Most advanced user interface & world-class connectivity

    Instrument Architecture

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    Instrument ArchitectureModern Spectrum Analyzers Architecture (PSA, X-Series)

    RF Section IF Section BB Section

    AttenuationFiltering

    Downconversion RBW Filtering Envelope Detection Log Conversion VBW Filtering

    Peak/sample/rmsdetection

    Averaging

    ADCIF/BB Section

    on ASIC

    All Digital IF Architecture

    Modern Spectrum Analyzer Block Diagram

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    Modern Spectrum Analyzer Block Diagram

    YIG ADC

    Analog IFFilter

    Digital IF Filter

    Digital Log Amp

    Digital Detectors

    FFT

    Swept vs. FFTAttenuation

    Pre-amp

    Replaced

    by

    All Digital IF Advantages

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    All Digital IF Advantages

    RF Section ADC IF/BB Sectionon ASIC

    Flexibility:

    RBW filtering in 10% steps

    Filters with better selectivity Multiple operation modes (Swept, FFT, VSA, NFA)

    Accuracy:

    Log conversion practically ideal

    No drift errors; increased repeatability

    Speed:

    When Swept mode is slow, go FFT

    FFT

    Techniques for Reducing DANL, Improving Dynamic

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    q g , p g y

    Range

    Reduce attenuation

    Add preamp

    Reduce RBW

    Add external filtering

    Better/shorter cables, connectors

    Move analyzer closer

    Time averaging (where possible, not measurement avg.)

    Measurement processing (take advantage of Moores Law)

    Noise power subtraction/noise correction/NNC

    Noise floor extension (NFE) leverages deep knowledge ofanalyzer/circuit behavior

    CW Signal Measured Near Analyzer Noise Floor

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    g y

    Actual S/NDisplayed

    S/N

    CW Signal

    Apparent

    Signal

    This is

    fundamental, and

    often missedAmpl & Freq

    Axes Expanded

    Example: No noise subtraction or near noise correction

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    Noise Subtraction, Noise Floor Extension

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    ,

    New technique NFE improves D.A.N.L.

    analyzer noise power calculated/subtracted real time

    3 dB error

    without NFE

    No error

    Improved noise floor

    or displayed averagenoise level

    Analyzer Noise Floor with NFE

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    Source still off, green trace shows analyzer noise level with NFE

    Other measurement conditions unchanged

    Note high variance result from subtraction of small, noisy numbers

    Analyzer DANL now far enough below source for minimal(0.2 - 0.4 dB) error

    A Closer Look

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    Pink trace adds to blue trace; result is yellow trace (NFE not used)

    Green trace is included in blue trace but resulting error very small

    Source noise Level, no NFE

    Source Noise Level, with NFE

    Analyzer Noise, no NFE

    Analyzer Noise with NFE

    EMC Features standard in all X-Series Spectrum

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    EMI Roadmap

    6/28/2011Page 70

    p

    analyzers

    Limit Lines(2000 pts)

    Amplitude correction (2000 pts) 40001 sweep points

    Option EMC in X-Series spectrum analyzer

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    Page 71

    p p y

    CISPR 16-1-1 detectors

    (to latest spec)Quasi Peak

    EMI Average (CISPR-AVG)RMS Average (CISPR-RMS)

    EMI Bandwidths (CISPR & MIL STD)

    EMI Presets

    Tune & Listen

    Measure at Marker

    EMI Peak, EMI Average, and

    Quasi Peak measurements

    displayed together

    W/N6141A EMC measurement application

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    Page 72

    Full Featured Pre-compliance Application

    Available in all X-Series models

    pp

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    N6141A measurement: Frequency Scan w ith Log Display

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    - same functionality as E7400 Signal List

    Meters tune

    to selected

    signal

    N6141A measurement: Str ip Chart Patent

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    EMI Roadmap

    6/28/2011Page 77

    p

    Time recordof zero span

    data scrolls

    to left Up to three

    different

    detectors

    Can be usedto make

    click

    measure-

    ments

    Click measurements are made on home appliances

    Patent

    Applied

    For

    Option EDP (Enhanced Display Package) for the SA

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    Spectrogram

    Trace Zoom

    Zone Span

    Group/Presentation Title

    Agilent RestrictedPage 78

    N6141A EMI Measurement Application

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    Pre-complianceCompliance

    PXA

    MXA

    CXAAgilent MXE N9038A

    EXA

    Agilent products for Immunity test (EMS)

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    Signal

    generator

    9 kHz 3 GHz, AM, FM, Phase, Pulse IQ Modulator,

    40 MHz Mod.-BW

    Signal

    generator

    N5182, N5182, N5183

    100 kHz- 1,3, 6, 20, 40 GHz, AM, FM, Phase, Pulse,

    optional vector, 120 MHz Mod.-BW, step , sweep,

    USB-Power meter included

    Power meter/

    Power sensors

    E441x, E191x, N8262, U200x

    100 kHz 40 GHzsingle channel, dual channel, USB, peak, envelope,

    pulse

    Accessories Directional Couplers, cables, Adapters, Switches etc.

    Solution partners for EMC

    http://www.home.agilent.com/agilent/product.jspx?nid=-35560.695944.00&cc=US&lc=enghttp://www.home.agilent.com/agilent/product.jspx?nid=-536902901.899991.00&cc=US&lc=enghttp://www.home.agilent.com/agilent/product.jspx?nid=-536902903.689086.00&cc=US&lc=eng
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    EMC seminar

    Complete solution:

    1. Automation software

    2. Chambers

    3. GTEM

    4. Antennas

    5. Power amplifiers

    6. Accessories

    Page 81

    Per documentazione su prodotti ed applicazioni EMI/EMC

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    visitare il sito

    http://www.agilent.com/find/EMC

    Contatti:

    Agilent Technologies ItaliaRoberto Sacchi

    Application EngineerE-mail: [email protected]

    Giuseppe SavoiaSignal Analysis and Generation Sales SpecialistE-mail: [email protected]

    Agilent Contact CenterE-mail: [email protected]: 02 9260 8484

    http://www.agilent.com/find/EMCmailto:[email protected]:[email protected]:[email protected]:[email protected]:[email protected]:[email protected]:[email protected]:[email protected]:[email protected]:[email protected]:[email protected]:[email protected]:[email protected]:[email protected]://www.agilent.com/find/EMC