Why a correct, traceable, signed survey of a 5G site can be low by 28.6 dB, and what has to be measured instead.
Human exposure limits are written against the maximum time-averaged field an installation can produce. A traffic-dependent transmitter almost never radiates that maximum while a surveyor is standing under it. This paper derives the conversion from a receiver reading to an incident field strength, sets out the exposure-ratio sum that compliance turns on, works a 3.5 GHz extrapolation in full, and shows a rooftop moving from 49 percent to 81 percent of the limit on the strength of a carrier that contributed less than one part in ten thousand of the measured budget. It closes with an uncertainty budget, six checkable instrument requirements, and the field practice that keeps a report defensible.
RF safety officers and survey engineers who sign compliance reports and have to defend them. System integrators building EMF measurement products around a receive module, their own antennas and their own software. Regulators and network operators specifying what a survey must contain before they will accept it.
The deliverable is a document saying, with a signature on it, that a location is below a published exposure limit. A rooftop, a tower base, a schoolyard sixty meters from a macro cell. Someone who wants it to be wrong will read it.
Three things go wrong and only one is an instrument fault. Max-hold on a burst without duty correction over-reads by 10 log(1/δ), where δ is the duty cycle: 30 dB on a radar at one part in a thousand. A cable loss read at the wrong frequency row loses 2.4 dB. And most often the survey answers the wrong question.
That last failure is the subject here, because it does not look like one. Instrument calibrated, operator careful, every number traceable, and the answer still low by several hundredfold.
A more sensitive probe does not fix this. The quantity the limit is written against is not the field on the meter: on the carrier worked in section 4 the two differ by 28.6 dB, and they differ in kind.
Standards work in two layers. Basic restrictions, the dosimetric reference limits of IEEE C95.1-2019, are in-body quantities not measurable in the field: whole-body average SAR over 30 minutes, local SAR in a 10 g cube over 6, absorbed surface power density above 6 GHz. Reference levels are external field quantities derived conservatively from them, and are what a survey measures.
A template written for the 1998 guidelines is therefore wrong twice over. The whole-body window moved from 6 minutes to 30, and a higher local-exposure surface appeared where none existed. Neither error is visible in the final percentage.
A frequency-selective survey can prove compliance but not non-compliance. A reference level exceeded triggers escalation to dosimetry; it is not a finding.
In the far field E and H are locked together by the impedance of free space, so power density follows from either alone:
Equation (1) is illegal in the reactive near field, where a power-density readout reports a quantity that does not exist. One check to carry: √3770 is 61.4 V/m, exactly the FCC occupational limit from 30 to 300 MHz.
Figure 1 shows where each term enters. Written out, the chain is:
Antenna factor is the ratio of incident field strength to the voltage across a 50 Ω load, a property of the terminated antenna. With the aperture relation, equation (1) gives the identity every certificate implies:
Check it: a half-wave dipole at 100 MHz gives 40.00 − 2.15 − 29.77, or 8.08 dB(1/m), against a published figure near 8.1. Back the implied gain out of any certificate and ask whether it is plausible for that aperture. One implying 15 dBi from a biconical is a typing error, caught before the survey rather than after it.
Everything adds in power, never in field, and every source in every band is a term:
Ratios are squared before summing, so three sources each at 60 percent of their own reference level total 1.08 and the site fails with no reading above 60 percent. Every unmeasured band is a term set to zero.
Limits are on the maximum time-averaged exposure, 1800 s whole body and 360 s local. A traffic-dependent transmitter radiates what demand asks of it, and roof access is granted when it is granted. IEC 62232 and ITU-R SM.2452-1 resolve that by scaling an always-on component:
A 3.5 GHz macro cell: 100 MHz channel, 30 kHz spacing, 3276 subcarriers, an eight-beam burst set every 20 ms, a DDDSU frame, a declared 6 dB traffic-to-broadcast ratio. All values are illustrative.
The receiver reads −33.2 dBm on the strongest secondary synchronization resource element, with antenna factor 35.10 dB(1/m) and 2.0 dB of cable loss. Equation (2): −33.2 + 107.0 = 73.8 dBµV, then 73.8 + 35.10 + 2.0 = 110.9 dBµV/m, or 0.35 V/m. Equation (3) puts the implied gain at 6.01 dBi, so the certificate stands, and equation (1) gives 3.249 × 10−4 W/m².
Then the factors. 98.28 MHz over 30 kHz is 3276. Downlink duty is (3 × 14 + 10)/70 = 0.743, taken as 0.75. No limiter is declared, and 6 dB is a factor of 4. The product is 9828, so equation (5) gives 3.193 W/m²: 31.9 percent of the 10 W/m² limit above 2 GHz.
The raw reading would have said 0.0032 percent. A shaped broadband probe integrates the whole burst instead: all 240 subcarriers are on during a synchronization symbol, giving a 5.42 V/m burst, and at 5.71 percent duty the 30-minute average is 0.045 percent. Section 5 takes up what that number can and cannot support.
Figure 2 shows why: the probe integrates across a window in which the burst is present for a small fraction of the time. Table 1 decomposes the gap term by term, and every term in it is a property of the network rather than of the instrument.
| Term | dB |
|---|---|
| Subcarriers not seen, kBW | +35.15 |
| Traffic beam not entered, kbeam | +6.02 |
| TDD downlink duty, kDC | −1.25 |
| Burst power spread over 240 resource elements, not one | −23.80 |
| Burst duty cycle of 5.71 percent | +12.43 |
| Net | +28.55 |
Put that carrier on a rooftop with three others: FM at 15.0 V/m against 27.7, GSM 900 at 12.0 against 42.32, LTE 1800 at 20.0 against 59.01. The squared ratios with the 5G term raw sum to 0.489. Extrapolating that term takes it to 0.808, and Figure 3 shows where the budget then sits.
At 80.8 percent with an expanded uncertainty of 3.0 dB the 95 percent upper bound is 161 percent, so the site cannot be declared compliant. It was declared compliant an hour earlier, by the same crew, with the same instrument.
The antagonist is an architecture: the shaped isotropic broadband probe read as one percent-of-limit number. It deserves its place. Shaped to the reciprocal of the reference-level curve, it implements the exposure sum in hardware, and if the question is only whether a rooftop has a hot spot it wins. It fails for four structural reasons, none fixable by a better probe.
Take that claim at its least flattering to us. Grant the probe a perfect true-RMS detector, a shaping curve with zero error, isotropy to a hundredth of a decibel and unlimited sensitivity, none of which any real probe has. It still cannot produce the number the standard asks for, because every one of those improvements makes the same scalar more accurate and the standard needs the terms that went into it. The broadband probe does not fail because it is imprecise. It fails because it has already added up.
The complementary failure belongs in the same breath: without a preceding broadband scan, nine tripod points are nine samples of a field with maxima every 43 mm. The architecture is both, in that order.
Table 2 converts the physics into requirements a reader can score any receiver against, including ones we do not make.
| Requirement and number | Why not looser | |
|---|---|---|
| R1 | RBW at or below the reference-signal subcarrier spacing, 15 or 30 kHz | Adjacent subcarrier energy is multiplied by 3276 too, so 100 kHz over-reads by 5.2 dB. |
| R2 | True-RMS detector, integration settable from 500 µs to 360 s | 577 µs is one GSM timeslot; longer dilutes it by up to 9 dB. |
| R3 | Phase noise at or below −105 dBc/Hz at 10 kHz offset, 60 dB of linear range | A rooftop spans 57.5 dB, from an FM carrier at −5 dBm to a resource element at −62.5 dBm; an attenuator change injects 0.3 to 0.5 dB. |
| R4 | Documented amplitude budget, U at or below 3.0 dB at k = 2 | 3.0 dB sets a 50 percent decision threshold; 6.0 dB doubles the compliance radius. |
| R5 | Isotropic total field from three orthogonal axes, matched within 1.0 dB | Reference levels assume maximum coupling; a linear antenna 45° off under-reads 3 dB. |
| R6 | Continuous coverage in one calibrated chain, 100 kHz to at least 6 GHz | An unmeasured band is a term set to zero; two instruments sum two traffic states. |
Table 3 shows where the 3.0 dB in R4 comes from, and the row worth staring at is the last one, which is not an instrument term at all.
| Contribution | Half-width (dB) | Distribution | ui2 |
|---|---|---|---|
| Receiver amplitude accuracy | ±1.5 | rectangular | 0.750 |
| Antenna factor certificate | 1.0 at k = 2 | normal | 0.250 |
| Antenna directivity, isotropy imbalance | ±1.0 | rectangular | 0.333 |
| Operator and tripod scattering | ±1.0 | rectangular | 0.333 |
| Detector response to modulation | ±0.6 | rectangular | 0.120 |
| Cable, mismatch, linearity, drift, repeatability | combined | mixed | 0.409 |
| Undeclared traffic-beam ratio | ±3.0 | rectangular | 3.000 |
| The instrument chain alone sums to 2.196, giving U = 2.96 dB at k = 2. Adding the traffic-beam term gives 5.196 and U = 4.56 dB, moving the threshold from 50.6 to 35.0 percent of the limit. Half-widths are illustrative. | |||
An exposure measurement system at scale is assembled rather than bought whole. An integrator pairs a receive module with a calibrated antenna set and software of their own, so the receiver has to hold its amplitude accuracy across the band, cover that band in one calibrated chain, take commands from someone else's software, and fit a mast or a case. The ICX-FieldHawk family covers that on one engine in three form factors: handheld, rugged tablet, and a USB or LAN module under 305 g. Each requirement below carries its published value and its condition, and the summary table in section 9 collects them.
R3. Published single-sideband phase noise at a 1 GHz carrier and 10 kHz offset is −107.5 dBc/Hz for the ICX-400 family and −101.6 dBc/Hz for the ICX-090 family, at 25 °C after 10 minutes of warm-up with spur reject standard on. An adjacent carrier at −10 dBm throws a skirt of −10 − 107.5 + 10 log(30 000) = −72.7 dBm into 30 kHz, so a resource element at −60 dBm sits 12.7 dB clear and takes 0.23 dB of error. On the 090 tier the margin is 6.8 dB and the error 0.82 dB.
R4, and the honest limitation. Published amplitude accuracy is ±2.0 dB from 9 kHz to 9.5 GHz and ±3.0 dB from 9.5 to 40 GHz, at 25 °C after 10 minutes of warm-up with spur reject standard on. Substitute ±2.0 dB into the budget for the ±1.5 dB illustrative term and the sum becomes 2.778, so U is 3.3 dB. That is above the 3.0 dB target set in R4, and above 9.5 GHz it reaches 4.2 dB. Meeting R4 needs a site amplitude correction against a calibrated reference, which is why the published amplitude correction and Amplitude Offset functions belong in the method. Any receiver quoting one ex-factory figure has the same problem; what differs is whether the correction path exists.
R5, honestly. The published antennas are an omnidirectional element and an active directional antenna, neither a three-axis isotropic probe, so total field comes from three sequential orientations in quadrature, exact only for a stationary field. Power detection, in Figure 4, is one of six published measurement functions a survey uses at every point, Channel Power and Antenna Factor among them, included rather than licensed.
R7. Antenna factor correction belongs inside the chain, not in a spreadsheet afterwards. The correction table is applied at the instrument, so the logged value is already a field strength. The host application, SpectraCore, drives that over SCPI with published bindings for C, Python, MATLAB and LabVIEW, and an integrator whose survey software is the product can bypass SpectraCore and drive the module directly.
Figure 5 is worth setting beside the practice list below, because every item on it exists to make that one number defensible.
Most of what makes a survey defensible has nothing to do with which receiver is in the case.
One limit of the state of the art belongs in every report. Where the point lies outside the synchronization beam sweep, SM.2452-1 requires the measurement to be made in a traffic beam and says plainly that methods for attracting one are still under development. A survey assuming the easy case is non-conservative by up to 9 dB, and no instrument closes that gap. Theoretical-maximum extrapolation also runs 5 to 9 dB above the actual-maximum assessment IEC 62232:2022 permits, so say which convention was used.
The instrument a safety officer carries is increasingly an integrator's product with a general-purpose receiver inside it, built with the integrator's own antennas and software. That arrangement puts the arithmetic of sections 4 and 5 on the integrator rather than on the officer, and it is why this paper spends its length there. The failure reported from the field is not a sensitivity failure. It is a survey that was correct, traceable and signed, and answered the wrong question by 28.6 dB.
Table 4 collects the governing relations and published values with conditions.
| Requirement | Relation or published value | Condition |
|---|---|---|
| R6 coverage | 9 kHz to 9.5 GHz (090); 9 kHz to 40 GHz (400) | one calibrated chain, all three form factors |
| R1, R2 | RBW 1 Hz to 10 MHz swept; PosPeak, NegPeak, Sample, Average, RMS, MaxPower | VBW 1 Hz to 10 MHz; power detection at 8 ns resolution |
| R3 phase noise, 1 GHz | −107.5 dBc/Hz (400); −101.6 dBc/Hz (090) | 10 kHz offset, 25 °C, 10 min warm-up, spur reject standard on |
| R4 amplitude accuracy | ±2.0 dB; ±3.0 dB | 9 kHz to 9.5 GHz; 9.5 to 40 GHz; 25 °C, 10 min warm-up |
| Source: the ICX-FieldHawk handheld, rugged and USB datasheets. Values on preliminary pages should be verified before quotation. | ||
| Symbol | Meaning | Units |
|---|---|---|
| Einc, Hinc | Incident rms electric, magnetic field | V/m, A/m |
| Sinc | Incident power density | W/m² |
| Z0, AF | Free-space impedance, antenna factor | Ω, dB(1/m) |
| Lc, Gpre | Cable loss, preamplifier gain | dB |
| kBW, kDC, kbeam | Extrapolation factors | dimensionless |
| U, TER | Expanded uncertainty, total exposure ratio | dB, dimensionless |
If you are building an exposure product around a receive module, or specifying what a survey report must contain, our application engineers would be glad to work through the chain and the budget with you.
The following values in this paper are not yet confirmed against a published Berkeley Nucleonics datasheet and are marked verify in the text. They must be confirmed before this paper is released.