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Berkeley Nucleonics Corporation
ICX-FieldHawk application noteBNC-AN-109 Rev BOctober 2026 | dc-62022201
A semi-anechoic chamber: absorber on the walls and ceiling, a metal ground plane, an equipment enclosure on a turntable and a log-periodic antenna on a mast at 3 m. No real site is depicted.
IllustrationA semi-anechoic chamber: absorber on the walls and ceiling, a metal ground plane, an equipment enclosure on a turntable and a log-periodic antenna on a mast at 3 m. No real site is depicted.
Application note

EMC pre-compliance testing on your own bench

What CISPR 16-1-1 specifies, which parts of it a general-purpose analyzer reproduces, and how to make a bench scan that predicts a chamber result.

CISPR 16-1-1Bands, 6 dB bandwidths, detectors and overload factor
CorrectionsFrom an indicated level to a field strength, per point
Observation timeDwell, max hold and a gap-free window
Option 74CISPR detectors, bandwidths and limit lines on the bench

EMC pre-compliance testing on your own bench

What CISPR 16-1-1 specifies, which parts of it a general-purpose analyzer reproduces, and how to make a bench scan that predicts a chamber result.

Abstract

The cost of a failed radiated emissions test is the loop between the failure and the retest, not the chamber day itself. This paper sets out what CISPR 16-1-1 specifies for a scan: five bands, four resolution bandwidths defined at 6 dB rather than 3 dB, detector time constants that govern dwell, and an overload factor that governs headroom. It derives the corrections that turn an indicated level into a field strength, works the noise floor and common-mode current arithmetic for one stated bench, quantifies the observation time a stepped scan needs to catch an intermittent emission, and states what a bench result can and cannot establish. It then sets the requirements against the published ICX-FieldHawk figures, including the CISPR detectors, bandwidths and limit lines published as option 74 on the ICX-045, ICX-060 and ICX-090.

Who this paper is for

Hardware and compliance engineers who own a product's first emissions test and want the failures found before the chamber is booked. Test engineers building a repeatable pre-compliance scan. Engineering managers comparing the cost of a bench, a chamber day, or both.

David Brown, President, Berkeley Nucleonics Corp.

Key results
22.5 dB
Error in a broadband emission scanned at the band B bandwidth of 9 kHz instead of the band C bandwidth of 120 kHz.
30 min
Max hold needed for 99 percent confidence on a 5 ms burst every 2 s with a one second sweep over 30 MHz to 1 GHz; one burst period gap-free.
3.6 µA
Common-mode current on a 1 m cable at 200 MHz that reaches the FCC Class B limit of 150 µV/m at 3 m.
5.9 dB
Expanded uncertainty (k = 2) of the careful bench worked here, against 12.1 dB for the casual one.
Contents
  1. 1What a failed emissions test costs
  2. 2What the standard specifies
  3. 3Why a scan finds nothing and reports it as a pass
  4. 4Requirements for a pre-compliance bench
  5. 5Meeting the requirements, and what it costs
  6. 6Measurement practice
  7. 7What a bench result cannot establish
  8. 8Summary and selection
  9. 9Definitions, symbols and further reading

1What a failed emissions test costs

The worked case in this paper takes an accredited 3 m semi-anechoic chamber day at 2,000 to 4,000 US dollars and a first radiated scan at two or three days (the bench and cost assumptions are collected in Table 3). The larger cost is the loop: the product fails at 240 MHz, a ferrite is fitted, and the chamber is rebooked three weeks out. Two loops put a launch about two months late.

A bench is not a chamber, and a bench scan does not produce a number a certification body accepts. It answers the three questions that set the loop count: which frequencies lie close to a limit, what is radiating them, and whether the latest change helped. None of the three needs an accredited site. All three need the measurement made as the standard defines it, because a scan at the wrong bandwidth is not conservative; it is wrong by a computable amount, and section 2 computes it.

2What the standard specifies

CISPR 16-1-1 describes a measuring receiver, not a spectrum analyzer, and it fixes what an analyzer leaves to the operator: band boundaries, resolution bandwidth, detector time constants and overload factor. Table 1 collects them, and Figure 2 draws the bands on one frequency axis.

Bandwidth enters a bench scan twice. CISPR specifies it at the −6 dB points; analyzers specify it at the −3 dB points, a narrower filter for the same number. And a narrowband carrier reads the same at any bandwidth wide enough to hold it, while a clock edge does not, because a broadband emission follows bandwidth in volts rather than power:

B3 = B6 / √2     ΔL = 20 log10(B2 / B1)
(1)

where

B3, B6
filter width at the 3 dB and 6 dB points, in hertz, for a Gaussian filter
B1, B2
the bandwidth used and the bandwidth the standard specifies, in hertz; 9 kHz and 120 kHz for the band B and band C settings, so ΔL is the correction to add and Figure 1 plots its negative, the error made
ΔL
change in indicated level of a broadband emission, in dB
The 22.5 dB error

Scan band C at the band B bandwidth, which happens when the conducted setup is reused unchanged, and a broadband emission reads 20 log10(120 kHz / 9 kHz) = 22.5 dB low. A product 12 dB over the limit is displayed 10.5 dB under it. The error reverses the verdict rather than widening its uncertainty.

-60-40-2002040200 Hz1 kHz9 kHz120 kHz1 MHz10 MHz9 kHz in band C: 22.5 dBlowBand C, correct3 dB RBW at 120 kHz: 3.0 dB highResolution bandwidth, at the 6 dB pointsError in indicated level (dB)Broadband emissionNarrowband carrierIllustrative. Curves are computed from the stated model, not measured data.
DerivedFigure 1. Bandwidth error is signed, and it falls only on broadband emissions: too narrow and a failing product passes, too wide and a passing one fails, while the narrowband carrier reads the same at every setting wide enough to hold it. Entering the CISPR 6 dB number into a 3 dB field over-reads by 3.0 dB.

Figure 1 plots the error against bandwidth, and the error is signed. Table 1 gives the settings the standard specifies, band by band, with the 3 dB equivalents an analyzer without CISPR bandwidths is set to.

Table 1. Columns three, seven and eight are from CISPR 16-1-1; the rest are derived from equation (1). CISPR 16-1-1 defines band E to 18 GHz; CISPR 32 measures in it only to the ceiling of Table 1. An analyzer set to 84.9 kHz at 3 dB has the band C and D bandwidth of a CISPR receiver; set to any other value, its broadband readings differ from a receiver's by equation (1), which is why the resolution bandwidth is the first setting a bench scan records.
BandRange6 dB RBW3 dB equiv.StepPointsτc/τd/meter (ms)Overload
A9 to 150 kHz200 Hz141 Hz100 Hz1,41045 / 500 / 16024 dB
B0.15 to 30 MHz9 kHz6.4 kHz4.5 kHz6,6331 / 160 / 16030 dB
C, D30 MHz to 1 GHz120 kHz84.9 kHz60 kHz16,1671 / 550 / 10043.5 dB
E1 to 18 GHz1 MHz707 kHz500 kHz10,000 to 6 GHz; 34,000 to 18 GHznonen/a

The highest frequency a radiated scan reaches is set by CISPR 32 from the highest frequency generated or used inside the product, as Table 2 lists; the bands of Table 1 say how each decade is measured, and Table 2 says where the scan stops.

Table 2. The CISPR 32 upper measurement frequency. A product with a 1.2 GHz processor clock is scanned to 6 GHz; a product whose fastest clock is 25 MHz is scanned to 1 GHz. The rule, not the band table, decides whether band E is needed.
Highest internal source frequencyRadiated scan reachesBands scanned
below 108 MHz1 GHzC and D
108 to 500 MHz2 GHzC, D and E
500 MHz to 1 GHz5 GHzC, D and E
above 1 GHzfive times the highest frequency, or 6 GHz, whichever is lowerC, D and E
CISPR 16-1-1 bands, 6 dB bandwidth, charge / discharge / meter time constants, overload factorBand A200 Hz at 6 dB45 / 500 / 160 msoverload 24 dBBand B9 kHz at 6 dB1 / 160 / 160 msoverload 30 dBBand C, D120 kHz at 6 dB1 / 550 / 100 msoverload 43.5 dBBand E1 MHz at 6 dBpeak, averageoverload n/a9 kHz150 kHz30 MHz1 GHz6 GHz18 GHzCISPR 32 radiated scan, by the highest internal source frequencybelow 108 MHzto 1 GHz108 to 500 MHzto 2 GHz500 MHz to 1 GHzto 5 GHzabove 1 GHzto 5 x f, 6 GHz at most
SchematicFigure 2. The five CISPR 16-1-1 bands on one logarithmic axis, each with its 6 dB bandwidth, its quasi-peak charge, discharge and meter time constants and its overload factor, and below them the CISPR 32 rule that sets where a radiated scan stops. Band E runs to 18 GHz in CISPR 16-1-1; a CISPR 32 scan uses at most the first 6 GHz of it.

The bench assumed for the worked examples

Every number in the worked examples that is a property of the bench rather than of the standard is stated once, in Table 3, and used from there. None is a published ICX-FieldHawk specification except the analyzer noise figure, which is derived from one.

Table 3. The bench the worked examples use. Substitute your own antenna factor table, cable loss and preamplifier figures; the arithmetic is unchanged.
ItemValue assumedWhere it enters
Antenna factor12 dB/m at 30 MHz, 17.5 dB/m at 240 MHz, 25 dB/m at 1 GHz, 33 dB/m at 6 GHz, on a straight line against log frequency between those pointsequations (2) and (4)
Cable and pad loss0.8 dB at 30 MHz, 2.2 dB at 240 MHz, 4.0 dB at 1 GHz, scaling with the square root of frequency above 1 GHzequations (2) and (4)
Preamplifier30 dB gain, 3 dB noise figure, +10 dBm output-referred 1 dB compressionsection 5
Analyzer noise figure15 dB from the connector to the display, consistent with the published displayed noise level of −159.9 dBm/Hz at 1 GHz in a 1 kHz resolution bandwidth at a −50 dBm reference level (ICX-400 family)equation (4)
Current probe transfer impedance15 dBΩsection 6
Search sweepone second over 30 MHz to 1 GHz at 120 kHzequation (3)
Chamber2,000 to 4,000 US dollars a day; two or three days for a first radiated scansection 1

From an indicated level to a field strength

An analyzer displays the level at its connector; a limit is field strength at a distance. Everything between is a signed correction:

E = Vind + AF + Lc − Gp
(2)

where

E
field strength at the measurement distance, in dBµV/m
Vind
level indicated at the analyzer input, in dBµV
AF
antenna factor, in dB/m; 17.5 at 240 MHz and 25 at 1 GHz for the assumed antenna
Lc
cable and pad loss, in dB; 2.2 and 4.0 at the same two frequencies
Gp
preamplifier gain, in dB; 30 for the assumed preamplifier

The conducted case has the same shape, with the mains network's voltage division factor replacing the antenna factor (Figure 3). Three of the terms vary with frequency, so a mid-band constant is decibels wrong at the band edges.

fieldEquipmentmains portMainsnetworkdivision factorPad andcablelossAnalyzerband B, 9 kHz at 6 dB or 6.4 kHz at 3 dBEquipmentradiatedAntennaantenna factorCable andpadlossPreamplifiergainAnalyzerband C, 120 kHz at6 dB or 84.9 kHzat 3 dBThe preamplifier buys sensitivity and spends headroom; section 5 prices both.
SchematicFigure 3. The conducted chain above and the radiated chain below, each term a signed correction between the equipment and the display. Four frequency-dependent corrections at each of the 16,167 points of bands C and D are applied in the instrument from its antenna-factor and amplitude-offset tables, or in the script that drives it.

3Why a scan finds nothing and reports it as a pass

The second failure has nothing to do with amplitude: the emission was not present while the analyzer was tuned to it. A stepped scan visits each cell for the fraction of the sweep set by bandwidth over span:

td = Tsweep · B / S,   p = (td + te) / Te,   Pn = 1 − (1 − p)n
(3)

where

td, S, n
cell dwell; span, 970 MHz; sweeps held in max hold
te, Te
event duration and period, 5 ms and 2 s for the worked commutation burst

Across 30 MHz to 1 GHz at 120 kHz with the one second search sweep of Table 3, td = 1 s × 120 kHz / 970 MHz = 124 µs, so p = (124 µs + 5 ms) / 2 s = 2.562 × 10−3. One sweep finds a 5 ms commutation burst a quarter of one percent of the time. Figure 4 draws the geometry and Figure 5 computes its consequence.

020406080100Emitter5 ms burst, 2 s periodStepped scan124 us in the affected cell, once per sweepburst missedmissed againGap-free windowparked, 100 MHz at onceboth bursts measured wholeTime, 100 units = 4 sThe scan is in the right cell for 124 microseconds of every second, and the burst lasts 5 milliseconds onceevery two.
SchematicFigure 4. The geometry behind the arithmetic. The stepped scan is not slow; it is elsewhere. It visits the affected cell once a second for 124 microseconds, and the burst arrives while it is in another cell. A faster sweep shortens the dwell in the same proportion as the revisit, so the single-sweep probability does not change. Drawn for legibility rather than to scale: the true ratio of 124 microseconds to one second against a 5 millisecond burst cannot be drawn, and the arithmetic carries it.
0204060801001 s10 s1 min5 min15 min60 min14.2% at 1 min53.7% at 5 min99.0% at 30 minElapsed max hold timeProbability of capture (%)Gap-free captureStepped, 5 ms burstStepped, 200 us burst99 percentIllustrative. Curves are computed from the stated model, not measured data.
DerivedFigure 5. Thirty minutes of max hold reaches 99 percent confidence on a 5 ms emission that repeats every two seconds, against a single pass of one burst period with gap-free capture. A one minute max hold finds the 5 ms burst 14 percent of the time; a 200 microsecond burst on the same period reaches 44 percent after a full hour and needs 7.9 hours for 99 percent. A scan that reports nothing has established only that nothing occurred during the time it spent in each cell, and the confidence that supports is the curve's value at the time the scan ran.

4Requirements for a pre-compliance bench

None of the above names an instrument. Table 4 converts it into six requirements, each with the number and the equation or table it comes from.

Table 4. Six requirements, derived rather than asserted. R1 and R4 are properties of the receiver; R3 and R5 are properties of the scan script; R2 is set by the product; R6 is the difference between a stepped scan and a gap-free window.
RequirementThe numberFrom
R1Bandwidth at the CISPR values, or at their 3 dB equivalents with the correction recorded200 Hz, 9 kHz, 120 kHz, 1 MHz at 6 dB; 141 Hz, 6.4 kHz, 84.9 kHz, 707 kHz at 3 dBTable 1, Eq. (1)
R2Coverage of the bands the product's clocks require9 kHz to 1 GHz for every product; to 2, 5 or 6 GHz by the CISPR 32 ruleTables 1 and 2
R3Step at half bandwidth, dwell at the meter constant16,167 points at 60 kHz over bands C and D; 100 ms a pointTable 1
R4Headroom for the overload factor43.5 dB in bands C and DTable 1
R5Corrections applied per pointantenna factor, cable and pad loss, preamplifier gain, each against frequencyEq. (2)
R6Observation that measures a 5 ms event whole on the first passprobability 1 within one event period, against 1,795 sweeps for 0.99Eq. (3)

5Meeting the requirements, and what it costs

The ICX-FieldHawk is a general-purpose real-time analyzer. Two routes meet R1 on it, and which one applies depends on the model.

R1 on the ICX-045, ICX-060 and ICX-090. Option 74, EMI pre-compliance measurement, is published on the handheld datasheet for these three models: CISPR 16-1-1 Peak, Quasi-Peak, Average and RMS detectors run in parallel, so one scan serves every detector; the CISPR resolution bandwidths by band, 200 Hz, 9 kHz, 120 kHz and 1 MHz; a preloaded limit-line library covering FCC Part 15 Class A and B, CISPR 11, 22 and 32 and IEC limits with automated margin and pass or fail against the selected line; segmented sweeps with a one-touch sequence of initial peak scan, automatic peak finding and quasi-peak and average final measurement, which SpectraCore runs and flags against the selected limit line; and export of the raw and pass or fail data as CSV. With option 74 the bandwidth of R1 is the CISPR value itself, equation (1) is not needed, and the quasi-peak reading is made by the detector the limit is written for. Figure 6 draws the published sequence.

Initial peakscanCISPR bandwidthper band,segmented sweepsAutomaticpeak findingevery point withinreach of the limitlineQuasi-peakand averagefinaldwell at eachfound peakMarginagainst thelimit linelimit-linelibrary; pass orfailCSV exportraw readings andpass or failPeak scan: the search of section 3. Final measurement: the confirmation, only where the search found something.
SchematicFigure 6. The option 74 sequence as published: a peak scan over the selected bands, automatic peak finding, a quasi-peak and average final measurement at each peak, margin against the chosen limit line, and a CSV export. It is the search-then-confirm structure that the dwell arithmetic of section 3 asks for, with the four detectors run in parallel so no band is scanned twice.
Two spectrum traces about 20 dB apart with the amplitude offset menu showing 20 dB

The offset is one term of equation (2) applied as a constant; the antenna-factor function applies the frequency-dependent term from a table. Together they are R5, and the screen then reads in the unit the limit is written in.

MeasuredFigure 7. Two clear-write traces of one carrier near 1 GHz in a 5 MHz span, 3 kHz resolution bandwidth, 300 Hz video bandwidth, peak detector, reference level 20 dBm, preamplifier auto on. The amplitude menu beside the display reads an AmpOffset of 20 dB, and the two traces differ by about 20 dB: the orange trace is the yellow trace with the offset applied to every point, noise floor included. A scan that enters its cable loss, pad and antenna factor as an offset reads field strength at the antenna rather than level at the connector.

R1 on the ICX-095, ICX-200 and ICX-400, the ICX-FieldHawk-R and the modules. Option 74 is not published for these models. Their datasheets publish a swept resolution bandwidth of 1 Hz to 10 MHz, so the 3 dB equivalents of 141 Hz, 6.4 kHz, 84.9 kHz and 707 kHz fall inside the range. The scan sets the nearest available bandwidth to each equivalent and records it, and equation (1) gives the correction for the ratio used; a bandwidth within 10 percent of the equivalent is within 0.8 dB on a broadband emission. A quasi-peak detector is not published on these models, so the scan uses the peak detector, and section 7 says what a peak reading establishes.

R2. The three option 74 handhelds reach 4.5, 6 and 9 GHz, so the ICX-060 and ICX-090 cover every ceiling in Table 2 and the ICX-045 covers products whose highest internal source frequency is below 500 MHz. The ICX-095, ICX-200 and ICX-400 handhelds, the ICX-095R, ICX-200R and ICX-400R tablets and the ICX-200U and ICX-400U modules reach 9.5, 20 or 40 GHz, so the 20 and 40 GHz models cover band E to its 18 GHz edge for a standard that asks for it.

R3 and R5. On any model the scan can be built in a script. SCPI is standard, with C, C++, C#, Python, MATLAB, Qt and LabVIEW on Windows and Linux: the script steps center frequency in 60 kHz increments across band D, 300 MHz to 1 GHz, holds 100 ms and records the peak. Antenna Factor, Amplitude Offset and amplitude correction are published functions on every ICX-FieldHawk datasheet, so SpectraCore applies equation (2) point by point from the antenna-factor table and the measured cable loss, and Figure 7 shows the amplitude offset applied to a trace. At 100 ms a point, a confirmation pass over bands C and D takes 27 minutes. The one second sweep of Table 3 is the search; the 100 ms dwell is the confirmation of what the search found, and a confirmation pass run as a search costs the 27 minutes at every iteration of the loop.

R6. The published engine is an FPGA transform with no missing samples across the analysis bandwidth, and its relation is published with it: 100 percent probability of intercept equals 2 × N × D × 8 ns on the ICX-095, ICX-200 and ICX-400 family, or 32.768 µs at 2,048 points, and 2 × N × D × 16 ns on the ICX-045, ICX-060 and ICX-090 as standard, or 131.072 µs at 4,096 points. A 5 ms burst is 150 times the first figure and 38 times the second, so it is measured at true amplitude on the first pass with either. The window is 100 MHz wide on the ICX-095, ICX-200 and ICX-400 family and 50 MHz as standard on the other three, so band D, 300 MHz to 1 GHz, takes seven or fourteen placements. Put equation (3) to the seven-placement case: parked for one event period each, the placements cover the band in 14 seconds at a probability of one, against the 1,795 sweeps and thirty minutes the stepped scan needs for 99 percent. Figure 8 is a time-domain record of that kind, and Figure 9 shows the other case the bandwidth table does not cover: a narrowband emission, which reads the same at any bandwidth wide enough to hold it.

Power against time record of a bursting emitter with a zoomed section
MeasuredFigure 8. Power against time at 1 GHz in a 62.5 MHz analysis bandwidth, reference level 0 dBm: a 16 ms record of a bursting emitter, every burst captured whole at about −10 dBm with the floor at about −50 dBm and below between bursts, and a zoom from 5.49 to 11.66 ms beneath it. Bursts about 0.5 ms long at 2 ms intervals are held in one record; a stepped scan dwelling 124 microseconds in the cell would catch each one with a probability of 0.31 per sweep.
Harmonics measurement of a 1 GHz source with a four-row result table
MeasuredFigure 9. Harmonics of a 1 GHz source measured in a 10 MHz span at each harmonic, 10 kHz resolution and video bandwidth, reference level 10 dBm: fundamental −6.01 dBm, second harmonic −88.12 dBm (82.11 dBc), third −73.08 dBm (67.06 dBc), fourth −62.64 dBm (56.62 dBc), total harmonic distortion 0.154 percent or −56.24 dBc. Each line is narrowband, so its level does not change with the resolution bandwidth; the noise floor between them does, by 10 log of the bandwidth ratio.

Worked example: what the bench can see

Referred to field strength, the noise floor is:

En = −174 + NF + 10 log10B + 107 + AF
(4)

where

−174
thermal noise density at 290 K, in dBm/Hz; 107 converts dBm to dBµV across 50 Ω
NF
noise figure from the antenna terminals to the display, cable included; 15 dB for the analyzer alone from Table 3
B
the 3 dB resolution bandwidth, in hertz; 84,900 in bands C and D

In band D at 240 MHz, 10 log10(84,900) = 49.3 dB. With 2.2 dB of cable ahead of a 15 dB analyzer the system noise figure is 17.2 dB, so En = −174 + 17.2 + 49.3 + 107 + 17.5 = 17.0 dBµV/m against a 46 dBµV/m FCC Class B limit at 3 m: 29 dB of clearance. The assumed preamplifier, 3 dB noise figure and 30 dB gain, takes the system noise factor to 1.66 × (1.995 + 30.62/1000) = 3.362, or 5.3 dB, which is 11.9 dB better than the 17.2 dB bare figure. Put the preamplifier at the antenna instead of at the analyzer and the cable loss follows the gain rather than preceding it: 3.1 dB, which is 14.1 dB better.

It also spends headroom, which is R4. At +10 dBm output-referred 1 dB compression the preamplifier compresses at −20 dBm in, or 87 dBµV. Band C asks for 43.5 dB of overload factor, so the highest level the chain measures without compressing an impulse is 43.5 dBµV at the preamplifier input, or 63.2 dBµV/m at the antenna, 17 dB above the limit. A product failing by more than that is measured with the preamplifier out. That ceiling assumes the preamplifier at the analyzer; at the antenna it sees the extra 2.2 dB, so the ceiling falls to 61.0 dBµV/m. The antenna position gains 2.2 dB of noise figure and spends 2.2 dB of headroom, the same trade in both directions. Figure 10 draws floor, ceiling and limit across the radiated bands.

02040608030 MHz100 MHz240 MHz1 GHz6 GHz17.0 at 240 MHz, bare63.2 ceiling at 240 MHz35.5 at 1 GHz, bareFrequencyField strength at 3 m (dBµV/m)Class B limitCeiling, with preampFloor, bareFloor, with preampIllustrative. Curves are computed from the stated model, not measured data.
DerivedFigure 10. The assumed bench of Table 3 against the FCC Part 15 Class B radiated limit at 3 m, 30 MHz to 6 GHz. The bare noise floor is 23 to 29 dB under the limit across bands C and D and 18 dB under it at 1 GHz, where the bandwidth widens to 707 kHz; the preamplifier lowers the floor by about 12 dB and caps the measurable level at 17 dB above the limit in bands C and D. Sensitivity is not what fails this bench; headroom and the corrections of R5 decide whether a reading is right.

Figure 10 extends the two worked points across the bands. The same arithmetic in band E at 1 GHz gives 35.5 dBµV/m bare against a 54 dBµV/m limit, and the conducted noise floor is nearly 60 dB below the conducted limit. Sensitivity rarely sets the result of a pre-compliance bench built this way; R4 and R5 decide whether a reading can be trusted.

6Measurement practice

  1. Start with the conducted scan. A mains network, a 10 dB pad and 150 kHz to 30 MHz find much of what fails a mains-powered product. For a mains-powered box with no radio and one short cable, that scan and a limit line may be all the pre-compliance needed.
  2. Use a current probe before an antenna. Cable common mode dominates radiated emissions below 1 GHz. Rearranging the short-radiator relation, ICM = 2rE / (μ0fL): at 200 MHz on a 1 m cable against the Class B limit of 150 µV/m at 3 m, that is (2 × 3 × 150 × 10−6) / (1.2566 × 10−6 × 2 × 108) = 3.6 µA, or 11.1 dBµA. Through the 15 dBΩ transfer impedance of Table 3 that is 26.1 dBµV, well clear of the noise floor. Four microamps of common mode on a one meter cable fails Class B, and a clamp finds it.
  3. Hold the near-field probe still. Loop field falls as the cube of distance, so 5 mm to 10 mm changes the reading by 60 log10(2) = 18.1 dB, more than any margin being chased. Near-field probing ranks sources; it does not measure them.
  4. Take the dwell from Table 1 and the max hold from Figure 5, with the peak detector for both. Thirty minutes if anything intermittent is suspected. Quasi-peak never exceeds peak, so a peak scan that clears the limit clears it under any detector. Keep one scan with the equipment off, and give the analyzer its published 10 minutes at 25 °C first.
  5. Record the bandwidth, detector, dwell, corrections and limit line with every scan. Two scans are comparable only when all five match, and a change between them is the first thing to look for when a reading moves.

7What a bench result cannot establish

Uncertainty separates a bench result from a certificate; Table 5 compares the budgets of two benches.

Table 5. Two illustrative bench budgets, combined in quadrature and expanded at k = 2: the careful bench is 6.2 dB tighter than the casual one. The site term dominates both columns, so a ground plane and a fixed geometry improve the budget more than an instrument upgrade does. A certificate carries the accredited site's own budget, computed under CISPR 16-4-2.
ContributionCareful ±dBuiCasual ±dBui
Receiver accuracy, antenna factor2.0, 1.31.382.0, 3.52.32
Cable loss and mismatch0.6, 1.20.922.0, 2.52.12
Site, height and polarization3.01.737.04.04
Preamplifier and repeatability1.0, 1.61.702.0, 3.03.21
Expanded, k = 2U = 5.9U = 12.1

Limitations

Field evidence

No chamber correlation has yet been scored against a bench built as described here, so this paper reports no measured agreement between a bench prediction and an accredited result. Every requirement is derived from CISPR 16-1-1, every instrument figure is a published one, and the arithmetic of sections 2 to 4 does not depend on any option.

8Summary and selection

Nothing above is a compliance measurement. The scan is shaped like CISPR's, the bench is not an accredited site, and the certificate still comes from one. Table 6 collects the published values with their conditions, by model family.

Table 6. Published values with their conditions, from the ICX-FieldHawk handheld, ICX-FieldHawk-R and USB/LAN module datasheets.
QuantityICX-045, ICX-060, ICX-090ICX-095, ICX-200, ICX-400; ICX-095R, ICX-200R, ICX-400R; ICX-200U, ICX-400UCondition
Frequency coverage9 kHz to 4.5, 6 or 9 GHz9 kHz to 9.5, 20 or 40 GHz
Swept resolution bandwidth0.1 Hz to 10 MHz1 Hz to 10 MHzstandard spectrum analysis
CISPR bandwidths and detectorsoption 74: 200 Hz, 9 kHz, 120 kHz, 1 MHz; Peak, Quasi-Peak, Average, RMS in parallel; limit-line library; CSV exportnot published; 3 dB equivalents by script, peak detectoroption 74 is a software option
Amplitude accuracy±1.0 dB typical, 20 to 30 °C; ±1.5 dB over the full temperature range and all conditions±2.0 dB to 9.5 GHz; ±3.0 dB above10 minute warm-up, 25 °C ambient; spur reject standard on for the second family
Maximum continuous input+23 dBm, 50 MHz and above, preamplifier off+23 dBm, 50 MHz and above, preamplifier off+10 dBm below 50 MHz or with the preamplifier on
Analysis bandwidth; 100 percent intercept50 MHz, 100 MHz with option 50; 2 × N × D × 16 ns, 131.072 µs at N = 4,096 (8 ns and 65.536 µs with option 50)100 MHz; 2 × N × D × 8 ns, 32.768 µs at N = 2,048D = 1
CorrectionsAntenna Factor, Amplitude Offset, amplitude correctionAntenna Factor, Amplitude Offset, amplitude correctionpublished functions on every model

Table 7 is the selection guide. For a bench, the ICX-045, ICX-060 or ICX-090 handheld with option 74 carries the CISPR detectors, bandwidths and limit lines on the instrument; by Table 2, the ICX-060 reaches the 6 GHz CISPR 32 ceiling and the ICX-090 reaches 9 GHz. For band E beyond 6 GHz, which CISPR 16-1-1 defines to 18 GHz, the ICX-200 and ICX-400 handhelds, the ICX-200R and ICX-400R tablets and the ICX-200U and ICX-400U modules reach 20 or 40 GHz with the 3 dB-equivalent bandwidths of Table 1 set by script. The modules run the scripted scan beside a host in a rack; the handhelds and the ICX-FieldHawk-R tablet take the same script to a product in the field.

Table 7. Selection by product. The option 74 handhelds carry the CISPR measurement on the instrument; the other models carry the scan in a script, with the bandwidth correction of equation (1) recorded beside each reading.
Product under testModelOptions and settingsWhy
Mains-powered, clocks below 108 MHz, conducted and radiated to 1 GHzICX-045 with option 7474; antenna-factor table loaded; peak scan then quasi-peak confirmation4.5 GHz covers the 1 GHz ceiling with room for harmonics; CISPR bandwidths and detectors on the instrument
Digital product with clocks above 108 MHz, radiated to 2, 5 or 6 GHzICX-060 or ICX-090 with option 7474; option 50 for 100 MHz placements in the gap-free check6 or 9 GHz covers every CISPR 32 ceiling
Band E to 18 GHz, or a product that also needs microwave measurementsICX-200 or ICX-400; ICX-200R or ICX-400R in the field3 dB equivalents by script; peak detector; 71 if demodulation is also needed20 or 40 GHz coverage; no quasi-peak detector published, so the peak scan bounds the result
Scripted bench in a rack, host-drivenICX-200U or ICX-400U, LAN interface3 dB equivalents by script; CSV from the hostno display; the API drives the 60 kHz step, the 100 ms dwell and the corrections

9Definitions, symbols and further reading

Overload factor
The margin in dB by which an impulse peak may exceed the indicated level without any stage compressing. CISPR 16-1-1 specifies it per band for a measuring receiver.
Quasi-peak detector
A detector with defined charge, discharge and meter time constants, so its reading depends on repetition rate as well as amplitude. It never exceeds a peak detector.
Pre-compliance
A measurement made as the standard defines it, on a site that is not accredited, to find and rank emissions before the accredited test.
Probability of intercept
The minimum event duration an analyzer measures at its true amplitude, as distinct from merely detecting it.
Symbols used in this document.
SymbolMeaningUnits
EField strength at the measurement distancedBµV/m
EnNoise floor referred to field strengthdBµV/m
VindLevel indicated at the analyzer inputdBµV
B1, B2Bandwidth used; bandwidth the standard specifiesHz
AF, Lc, Gp, NF, FAntenna factor; cable loss; preamplifier gain; noise figure and factordB/m, dB
B3, B6, S, τc, τd, td, te, Te, r, LBandwidth at 3 dB and 6 dB; span; quasi-peak constants; dwell; event duration and period; distance and radiator lengthHz, s, m
ICM, ZT, μ0Common-mode current; transfer impedance; permeability of free spacedBµA, dBΩ, H/m
p, Pn, n, N, D, ui, U, kIntercept probability and cumulative form; sweeps; transform size; decimation; standard uncertainty; expanded uncertainty; coverage factordimensionless, dB
AF  Antenna factor
AMN  Artificial mains network
CISPR  Comité International Spécial des Perturbations Radioélectriques
EMC  Electromagnetic compatibility
FPGA  Field-programmable gate array
RBW, VBW  Resolution bandwidth, video bandwidth
SCPI  Standard commands for programmable instruments

Further reading

If you are building a pre-compliance bench and want the bandwidth, dwell and headroom arithmetic worked against your own product, our application engineers would be glad to help.