Lesson 8/1080%
MODULE 08

Test Setup, Measurement & Detectors

From the seven-step measurement procedure to the four detector types and the distance a lab actually places the antenna from the EUT — this module ties the environment and equipment from Module 07 into a repeatable, animated test process, with a real EUT test setup diagram and interactive Plotly charts.

Every accredited RE test follows the same repeatable sequence, regardless of product type or standard. The steps below are shown alongside a live animation of what actually happens on the test-site turntable while each one runs.

Typical Measurement Procedure

  1. Configure the EUT in its highest emission operating mode (worst-case cables, peripherals, clock speeds, and duty cycle).
  2. Position the EUT on the non-conductive test table at the specified height and orientation.
  3. Rotate the EUT through 360° on the turntable, pausing to capture the azimuth with the highest emission at each frequency of interest.
  4. Sweep the antenna height (typically 1–4 m) at each azimuth to find the height that maximizes coupling to the EUT.
  5. Measure both horizontal and vertical antenna polarizations, since a given source may radiate more strongly in one plane.
  6. Record the maximum emission level found across all azimuth/height/polarization combinations at each frequency.
  7. Compare the recorded maxima against the applicable standard's limit line and flag any exceedances.

Animated: Turntable Rotation & Antenna Height/Polarization Sweep

The active step is highlighted on the left as the diagram cycles through rotation, height sweep, and polarization change — the three physical motions a lab actually performs while chasing the worst-case reading.

Rotating EUT through 360°…
A pre-scan is usually run with a fast Peak detector across all azimuths and heights to identify candidate frequencies, then only those specific frequency/azimuth/height combinations are re-measured with the slower Quasi-Peak or Average detector the standard actually requires for compliance — saving significant test time without missing a failing frequency.

The receiver's detector determines how it converts a raw, rapidly fluctuating RF signal into the single displayed emission level. The same noisy pulse train can produce four very different readings depending on which detector is selected — which is why standards mandate a specific detector for compliance rather than leaving it to the tester's choice.

Detector How It Responds Purpose
Peak Captures and holds the single highest instantaneous amplitude in the measurement window. Fast pre-scan — always reads at or above the true compliance level, so nothing failing is ever missed.
Quasi-Peak Weights repetitive pulses by how often they occur using standardized charge/discharge time constants, mimicking human annoyance perception. CISPR compliance — the detector actually named in most commercial limit lines.
Average Averages the signal envelope over the measurement time, smoothing out short transients. Continuous / narrowband emissions such as clock harmonics.
RMS Reads the true root-mean-square power of the signal over the measurement time. Broadband measurements where total energy content matters more than any single peak.

Animated: Four Detectors, One Pulse Train

A repetitive noisy pulse (typical of a switching power supply) scrolls across the top trace. Each colored needle below shows what that specific detector would report for the same signal in real time — notice how Peak always sits highest and Average/RMS settle lower and steadier.

Interactive: Detector Reading vs. Pulse Repetition Rate

Quasi-Peak and Average readings rise as the same pulse repeats more often per second, while Peak stays essentially flat because it only ever tracks the single highest excursion — hover any trace to compare. This is why a product with a very low pulse-repetition clock can sometimes pass Peak/QP but still be worth checking against Average.

In the far field, radiated field strength falls off roughly as 1/d, so moving the antenna from 3 m to 10 m alone would drop the reading by about 10.5 dB even if the EUT emitted nothing differently — this is exactly why the standard specifies both a limit and a fixed measurement distance together, and why results at one distance can't be casually compared to results at another without a correction factor.

Distance Typical Application
1 m Automotive (component-level, small chamber footprint)
3 m Medical, Industrial, Consumer
10 m Large equipment, OATS (Open Area Test Site)
The selected distance depends on the applicable standard and the physical size of the Equipment Under Test (EUT). Larger EUTs need more distance to reach the far field and to physically fit inside the antenna's beamwidth.

Animated: Same EUT at 1 m, 3 m, and 10 m

The radiating field rings expand and fade identically from the EUT in all three panels — only the antenna position differs, which is exactly why the raw reading (right-hand bar) drops at greater distance for the same physical emission.

Interactive: Field Strength Falloff vs. Distance (1/d)

Log-log trace of the theoretical far-field 1/d falloff, with the three standard test distances marked. Hover to read the exact predicted dB drop relative to 1 m.

Putting it all together: the EUT sits on an insulating turntable at a fixed height above the ground plane, cabled with its worst-case peripheral harness draped per the standard's cable-routing rules, while a mast-mounted antenna at the specified test distance feeds the receiver through low-loss coax and an optional LNA. This is a realistic illustration of that full chain since a licensed stock photo of a live test setup isn't available to embed here.

The measurement chain from Section 4 is built from a small, well-defined set of equipment, each piece contributing a known gain or loss that must be accounted for in the final reading.

Biconical Antenna
Log-Periodic Antenna
Horn Antenna
Loop Antenna
LNA (Preamp)
Low-Loss Coax
RF Switch Matrix
EMI Receiver
Spectrum Analyzer
Antenna Mast
Turntable
Calibration Kit
KNOWLEDGE CHECK

Module 8 Quiz

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