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Berkeley Nucleonics Corporation
ICX-FieldHawk application noteBNC-AN-103 Rev BOctober 2026 | dc-62022201
A site perimeter: a fence line, a slim mast carrying two panel antennas and a dome, an equipment cabinet, and a small quadcopter in the distance. No real site is depicted.
IllustrationA site perimeter: a fence line, a slim mast carrying two panel antennas and a dome, an equipment cabinet, and a small quadcopter in the distance. No real site is depicted.
Application note

Detecting unmanned aircraft, and finding the operator

Why the emission that matters most is the one that is hardest to hear.

Two emittersThe downlink is loud; only the uplink finds the operator
InterceptCoincidence, computed: 89 s against 0.6 s
Link budgetWhy the controller is fourteen times harder to hear
Finding the operatorBearing, fix geometry and the legal boundary

Detecting unmanned aircraft, and finding the operator

Why the emission that matters most is the one that is hardest to hear.

Abstract

Radio detection of small unmanned aircraft is often specified as a sensitivity problem. The arithmetic in this paper shows it to be a probability-of-intercept problem: against a burst lasting 645 microseconds once every 600 milliseconds, a scanning receiver needs about ninety seconds to reach ninety percent confidence while a gap-free receiver needs the emitter's own repetition interval. The paper derives that result, works the link budget for both ends of the link, sets out what each direction-finding method delivers, and states where radio detection is blind.

Who this paper is for

Counter-UAS system integrators designing or specifying an RF sensing layer. Security and site-protection engineers evaluating what an RF sensor can and cannot deliver. Spectrum enforcement staff working unauthorized flight cases.

David Brown, President, Berkeley Nucleonics Corp.

Key results
89 s
Time for a 1 MHz scanning receiver to reach 90 percent confidence against a 645 µs identification burst every 600 ms; 0.6 s for a gap-free receiver.
20 dB
Sensitivity forfeited by a scanner dwelling 1 ms in a 100.8 ms revisit, under integrating detection.
14:1
Ratio of aircraft to controller detection range on a 127 dB budget at 2.44 GHz: about 20 km in clear air against 1.4 km through urban clutter.
247 m
Circular error probable of two 3-degree bearings crossing at 25 degrees at 2 km, against 124 m at a right angle.
Contents
  1. 1Two emitters, two geometries
  2. 2Why detection is a timing problem, not a sensitivity problem
  3. 3The link budget, and the asymmetry it creates
  4. 4Finding the operator
  5. 5The legal boundary, which is also a design boundary
  6. 6Measurement practice
  7. 7Where radio detection is blind
  8. 8Summary, definitions and further reading

1Two emitters, two geometries

A small unmanned aircraft flown over a radio link is a pair of radios. The controller sends a narrow, low-duty-cycle uplink. The aircraft returns a wide, high-duty-cycle video downlink. They occupy the same bands and belong to the same system, and for the purpose of finding the person flying they differ in every property that matters.

A scanning detector sold as a drone-band monitor is the least expensive sensor for the band, and it detects traffic. What it cannot do is report how much it missed: section 2 shows that such a receiver hears a hopping link about one percent of the time, so what it reports is a sparse and unrepeatable sample of the traffic, and an operator cannot tell a quiet sky from a missed one. Adding receivers does not change the fraction: three receivers each hearing the band one percent of the time are still hearing it one percent of the time, and the false alarms triple. The constraint is neither sensitivity nor channel count. It is coincidence, and coincidence can be computed. Figure 1 draws the two links.

uplink: narrow, low dutydownlink: wide, high dutythe emission that locates the operatorController1.5 m, in clutter, directionalAircraft20 to 400 m, clear line of sightGap-free receiverwhole hop band at once, feeds DFThe downlink is loud, wide and unobstructed. The uplink is quiet, narrow and buried in ground clutter, and only the uplink leads to the operator.
SchematicFigure 1. Two emitters, two geometries, two problems. Detection is usually won on the downlink and the operator is found only on the uplink, which is the harder of the two by twenty to forty decibels of geometry alone.

Figure 1 is the difficulty in one picture. The aircraft is in clear air with a quasi-omnidirectional antenna, transmitting tens of megahertz at high duty cycle. The controller is a meter and a half above the ground, behind whatever the ground has on it, with an antenna pointed at the aircraft rather than at the sensor, transmitting a short slot.

There is a third emission, and it is the easiest of all: the mandated Remote ID broadcast. Under ASTM F3411 and 14 CFR Part 89 a compliant aircraft transmits its identity, its position and its control station position in the clear over Bluetooth or Wi-Fi, at least once per second. The European requirement under Regulation (EU) 2019/945 is equivalent and explicitly names the remote pilot's position. That broadcast is designed to be received by anyone, and by construction it is present only on aircraft whose operators chose to comply.

2Why detection is a timing problem, not a sensitivity problem

Control links hop. Regulation requires it: a frequency-hopping device in the 2.4 GHz band must use at least fifteen channels and may not occupy any one of them for more than 0.4 seconds within a defined period. The practical result is a set of emitters that are on a given frequency for a millisecond or less at a time.

Table 1 gives representative figures for the link classes a sensor meets.

Table 1. Representative hopping behavior for control and identification links. Figures are drawn from open-source implementations and published reverse engineering rather than vendor datasheets, and should be treated as representative rather than exact.
Link classBandChannelsRF on per hopHop rate
Consumer RC, 16-channel2.4 GHz47about 3 msabout 111 /s
Long-range RC, 500 Hz mode2.4 GHzabout 80about 0.25 ms500 /s
Long-range RC, sub-GHz868 / 915 MHzabout 50about 1.5 ms150 /s
Proprietary video link identifier2.4 / 5.8 GHzwide OFDM645 us burstabout 1.7 /s

Set a scanning receiver against that. If it covers a hop band of width Bh in steps of its instantaneous bandwidth Bi, dwelling d at each step with a retune time tr, its revisit period is the product of the number of steps and the time per step. The probability of catching any one burst is the fraction of the revisit period during which the dwell and the burst overlap by at least the detector's minimum observation:

P1 = min[1, (d + τ − 2tmin) / T],   T = Ns(d + tr)
(1)

where

d
the dwell at each tuning step, in seconds; 1 ms is representative of a fast scanner
τ
the burst duration, in seconds; 645 µs for the identification burst worked below
tmin
the shortest contiguous observation the detector needs; 50 µs here
Ns
the number of tuning steps across the hop band; 84 at 1 MHz across 83.5 MHz
tr
the retune and settling time, in seconds; 0.2 ms

Detection over many bursts follows a geometric law, so the number of bursts needed for ninety percent confidence is the log of one tenth over the log of one minus the single-burst probability. Working that through for a 645 microsecond identification burst repeating every 600 milliseconds gives the numbers in Table 2.

Table 2. Time to ninety percent confidence against a 645 microsecond burst repeating every 600 milliseconds, computed from equation (1) across an 83.5 MHz hop band in 84 steps, with a 1 ms dwell, a 0.2 ms retune and a 50 microsecond minimum observation. Change any of those five and the column changes with it. The gap-free figure is set by the emitter's repetition interval, not by the receiver.
ReceiverInstantaneous BWRevisitP per burstTime to 90 percent
Narrow scanner1 MHz100.8 ms0.01589 seconds
Mid scanner20 MHz6.0 ms0.264.6 seconds
Gap-free captureat least 100 MHzcontinuous1.000.6 seconds
Eighty-nine seconds against six tenths of a second

An aircraft traveling at fifteen meters per second covers 1.3 kilometers while the narrow scanner is still accumulating confidence: the difference between a warning while the aircraft is in range and a report after it has left.

There is a second, quieter penalty, and it carries a condition. A scanner observes any given channel for only the fraction of wall-clock time given by dwell over revisit. For a detector that integrates energy over the whole revisit period, it forfeits ten times the logarithm of that ratio in sensitivity: for the narrow scanner in Table 2 that is 20 dB, which at the free-space path-loss exponent is a factor of ten in range. A burst that falls entirely inside the dwell suffers no such penalty; the scanner's problem with that burst is the one percent chance of being tuned there when it arrives. Under integrating detection the scanning receiver is slower and 20 dB less sensitive at once.

0255075100125150175200Control link47 channels, 111 hops/sScanning receiver1 MHz steps, 100 ms revisit, 1 ms dwellmissedmissedGap-free capturewhole band, continuouslyevery hop capturedTime (milliseconds)The scanner is tuned to the right channel at the right instant only by coincidence, and coincidence is whatequation 1 computes.
SchematicFigure 2. A hopping link fills the time-frequency plane with short marks while a scanner traces a single line through it. What determines detection is coincidence, not coverage.

Figure 2 shows where the twenty decibels go. Both the scanner's marks and the link's marks are sparse, and the receiver hears the link only where the two coincide, which for a narrow scanner is about one percent of wall-clock time. Figure 3 draws the time to ninety percent confidence against the receiver's instantaneous bandwidth, with the same dwell, retune and minimum observation as Table 2.

0204060801001251020501001 MHz: 89 s20 MHz: 4.6 s83.5 MHz and above: 0.6 s, one burstReceiver instantaneous bandwidth (MHz)Time to 90 percent (seconds)Illustrative. Curves are computed from the stated model, not measured data.
DerivedFigure 3. Time to ninety percent confidence against the 645 microsecond burst of Table 2, from equation (1) with a 1 ms dwell, a 0.2 ms retune and a 50 microsecond minimum observation across the 83.5 MHz band. The steps are the integer number of tuning steps the band needs. Below about 42 MHz the receiver needs more than two bursts; from 83.5 MHz the band is held whole and the time is the emitter's own repetition interval.

Sections 1 and 2 define a criterion, not yet a specification. Table 3 states it as four requirements a reader can score any receiver against; it is placed here so that it can be read with the derivation beside it.

Table 3. Four requirements, and the third is the one to ask about. R1 and R2 are published and answer sections 1 and 2 directly. R4 is published, but read it with section 4: the instrument is not what limits a time-difference fix. R3 is the requirement a direction-finding system is built on, and the ICX-FieldHawk datasheets publish the synchronization and trigger figures rather than a matched multi-channel specification, which is why section 4 spends its length there.
#RequirementDerived valuePublished
R1Instantaneous bandwidth covering the whole hop band at once≥ 83.5 MHz for the 2.4 GHz band, from §2100 MHz on the 9.5, 20 and 40 GHz models in every enclosure; 50 MHz standard and 100 MHz with option 50 on the 4.5, 6 and 9 GHz handhelds, so this band needs the option there
R2Probability of intercept published as a guarantee with its transform size≤ 645 µs to catch an identification burst whole0.512 µs at N = 32; 32.768 µs at N = 2048, D = 1
R3Coherent channels on one time base for a bearing≥ 2 for an interferometer, ≥ 4 for an arrayNot published as a matched multi-channel figure; GNSS 1PPS synchronization ±100 ns standard and ±75 or ±50 ns with options, external trigger input and output, and Multiple Unit Display are published
R4Time tagging fine enough that the instrument is not the limit≤ 10 ns, since 1 ns is 30 cm8 ns power detection time resolution
The 2.4 GHz band captured whole, max hold against a single instant, with spectrogram
MeasuredFigure 4. The 2.4 GHz control band held whole: 2.39 to 2.49 GHz in one 100 MHz window at 30 kHz resolution bandwidth, 300 kHz video bandwidth, peak detector, reference level −20 dBm, with max hold (T1) and a single sweep (T2) overlaid in the center pane, a spectrogram above, and a 31.67 MHz zoom below on one video downlink. The gap between the two overlaid traces is what a receiver that visits this band rather than holding it would report as empty, and the spectrogram is what a hopping link looks like before anything has been identified.

Figure 4 is the band this paper is about. Read the spectrogram rather than the spectrum: the marks are short, they move, and none of them is where it was a moment ago, which is the whole of the detection problem in one picture. Note what the figure cannot prove. A max-hold trace and a spectrogram look much the same behind a fast swept receiver as behind a gap-free one, so R1 is not settled by a screenshot. It is settled by the published frame rate in R2, which is why that row carries a transform size.

3The link budget, and the asymmetry it creates

Free-space path loss sets the floor for both directions:

Lfs = 32.44 + 20 log10(fMHz) + 20 log10(dkm)
(2)

where

fMHz
the frequency, in megahertz; 2440 for the control band and 5800 for the video downlink
dkm
the path length, in kilometers

At 2.44 GHz that is 100.2 dB at one kilometer and 109.7 dB at three. At 5.8 GHz it is 7.5 dB worse at every range, which is one reason long-range control links migrate down to 900 MHz, where the same geometry costs 8.5 dB less than 2.4 GHz.

The asymmetry does not come from transmit power, which is similar at both ends and capped by the same rules. It comes from geometry. The aircraft path is essentially free space. The controller path leaves a transmitter a meter and a half above the ground, so beyond a crossover of roughly 1.5 kilometers the loss follows a fourth-power law rather than a square law, and urban clutter adds 20 to 35 dB on top. For a sensor budget allowing 127 dB of path loss, the aircraft is detectable to around twenty kilometers in clear air while the controller is detectable to about 1.4 kilometers through urban clutter. Figure 5 plots both.

Limitation

That fourteen-to-one range ratio reverses in three common cases. A split link with a 900 MHz uplink and a 5.8 GHz downlink hands the uplink a 16 dB path-loss advantage plus better clutter penetration. Photogrammetry and waypoint missions often fly with video off entirely. And an aircraft directly overhead is in its own antenna null. Detection range is a distribution, not a number.

801001201401601800.10.3131025controller: 1.4 kmaircraft: about 20 kmRange (kilometers)Path loss (dB)Aircraft, 2.44 GHz free spaceAircraft, 5.8 GHz free spaceController, two-ray plus 25 dB clutterIllustrative. Curves are computed from the stated model, not measured data.
DerivedFigure 5. At identical transmit power the aircraft is detectable roughly fourteen times further than its controller. The difference comes from ground reflection and clutter between the sensor and the controller, not from transmit power.

Figure 5 plots both against a 127 dB budget. The crossing points are the whole planning problem: a sensor sited for the aircraft is not sited for the operator.

4Finding the operator

A bearing is not a position, and received power is not a range. The methods available differ by an order of magnitude in what they deliver, and two of the classical ones are structurally unsuited to hopping links. Table 4 sets them out.

Table 4. Direction-finding methods and what each delivers. Pseudo-Doppler needs milliseconds of continuous carrier, which a 250 microsecond hop does not provide, and interferometry and time-difference methods both require the same burst captured coherently, which a scanning front end cannot supply.
MethodAchievable accuracyWhat it needsWhere it fails
Received signal strengthrange to plus or minus 30 to 60 percentamplitude onlyunknown emitter power is indistinguishable from range
Amplitude comparison, 4 to 8 sectors5 to 15 degreesone burst, amplitude onlymultipath ripple
Pseudo-Doppler2 to 10 degreesa continuous carrier for several millisecondsshort bursts and fast hopping, structurally
Multi-baseline interferometry1 to 3 degrees clear, 5 to 15 urbancoherent, gap-free, multi-channel capturecoherent multipath
Time difference of arrival10 to 50 m inside the arraythe same burst at three or more synchronized sitesemitter outside the array

For a phase interferometer the geometry sets both the accuracy and the ambiguity. Bearing follows from the phase difference across a baseline, and unambiguous coverage of the hemisphere requires the baseline to be no more than half a wavelength:

σθ = λ σφ / (2πD cos θ),   unambiguous if D ≤ λ/2
(3)

where

λ
the wavelength, in meters; 0.1229 m at 2.44 GHz
D
the baseline length, in meters; 0.5 m in the worked case
σφ
the phase measurement error, in radians, roughly the reciprocal square root of linear SNR; 0.1 rad at 20 dB
θ
the angle from broadside, in degrees; the relation degrades as 1/cos θ and is written for boresight

The tension is immediate. A half-meter baseline at 2.44 GHz gives about 0.2 degrees of bearing accuracy at 20 dB signal to noise, and eight ambiguous bearings across the hemisphere, one for every half wavelength of baseline. Resolving them takes a ladder of baselines, the shortest at half a wavelength and the longest to refine, which is why direction-finding systems use arrays rather than pairs.

Whatever produces the bearing, two bearings produce a fix, and the error follows from range and cut angle. Cross-range error is range times bearing error: three degrees at two kilometers is 105 meters. Taking circular error probable as 0.5887 times the sum of the two semi-axes, two such bearings crossing at right angles give about 124 meters. The same two bearings crossing at twenty-five degrees stretch the ellipse to 343 by 76 meters and give 247, with no change in the sensors at all. Figure 6 plots the whole curve.

010020030040050060010203045607590right angle: 124 m25 degrees: 247 m10 degrees: 545 mAngle at which the two bearings cross (degrees)Circular error probable (meters)Illustrative. Curves are computed from the stated model, not measured data.
DerivedFigure 6. Circular error probable of a fix from two bearings each 3 degrees in error at 2 km range, against the angle at which the bearings cross. Each bearing contributes 105 m of cross-range error; at a right angle the fix is 124 m, at 25 degrees 247 m, and at 10 degrees 545 m. Nothing in the sensors changed between those numbers; the geometry of the two sites did.

Figure 6 is the site-selection argument in one curve. Time-difference methods trade the bearing problem for a timing problem, and the conversion is simple: one nanosecond is thirty centimeters. The estimator floor for a 645 microsecond burst across 10 MHz at 10 dB signal to noise is about 0.15 nanoseconds, which is four and a half centimeters, and field systems do not reach it. Real accuracy is set by inter-site clock synchronization, 10 to 50 nanoseconds for a satellite-disciplined oscillator, and by multipath leading-edge bias in urban settings, which is a bias rather than noise and therefore does not average away.

Signal track measurement with the marker menu open
MeasuredFigure 7. Marker signal track holding a drifting carrier at 999.90 MHz: 1 MHz to 2 GHz span, 300 kHz resolution bandwidth, 3 MHz video bandwidth, peak detector, reference level 0 dBm, with the marker menu open. This is the limit of what one channel can prove about one emitter. A bearing needs the same burst on several channels at once, and no single-channel display can show that.

Figure 7 is the front-end requirement rather than the answer: every method in Table 4 below the first two rows needs the same burst, captured coherently and timestamped.

5The legal boundary, which is also a design boundary

Radio detection of unmanned aircraft is lawful. Demodulating the communications those aircraft carry generally is not, and a system specification should state the distinction.

In United States law the Wiretap Act turns on contents, meaning information concerning the substance, purport or meaning of a communication (18 U.S.C. § 2510(8)). The existence of an emission, its center frequency, its bandwidth, its timing, its hop pattern, its amplitude, its phase and its bearing are none of those things. A further provision withholds the protection of ready public accessibility from communications sent using modulation whose essential parameters have been withheld from the public (§ 2510(16)), which means a proprietary drone link can be legally protected even though it carries no encryption. Unencrypted is not the same as lawful to decode.

Design rule

A lawful radio counter-UAS sensor detects, characterizes and direction-finds an emission. It does not demodulate the communication that emission carries. The constraint costs less capability than it appears to, because bearing, timing and hop structure locate an operator and payload content does not.

There is one clean exception, and it is worth designing around. The mandated Remote ID broadcast is required by regulation to be open, documented and receivable by the general public, so a sensor may decode it. Its second use is less obvious and more valuable: correlating Remote ID against the non-cooperative detections lets a system suppress compliant traffic from the alert stream, so the one aircraft that did not announce itself is not buried under the dozens that did.

6Measurement practice

  1. Detect on the downlink, then cue onto the uplink. The downlink gives early warning cheaply. Finding the operator needs a longer dwell and more antenna gain pointed at a quieter, lower emitter; the option 35 active directional antenna published for the ICX-FieldHawk line covers 0.5 to 10 GHz, with under 5 dBi of gain with its amplifier off and under 25 dBi with it on.
  2. Do not set a detection threshold on a max-hold trace, in SpectraCore or in any other software. Max hold discards the underlying statistics, so a constant-false-alarm threshold computed against it has no characterizable false-alarm probability.
  3. Use an order-statistic false-alarm threshold, not a cell average. The 2.4 GHz reference window is full of interferers, and cell averaging collapses in their presence.
  4. Confirm before declaring. A per-burst false-classification rate of one in a thousand, confirmed four times in ten opportunities, gives a track false-alarm rate around two in ten billion. Confirmation buys seven orders of magnitude for a few hundred milliseconds of latency.
  5. Survey the site before trusting a bearing. Every reflector within a few hundred meters is a competing arrival, and interferometric bearing error in dense clutter is five to twenty degrees regardless of the array.

Field evidence

Two things show up in deployment that the arithmetic above does not predict. The first is siting. Sensors placed for the aircraft are mounted high and clear, and the same mast is the worst place from which to hear a controller a meter and a half off the ground behind a building line, so an installation that detects well and geolocates badly is a recurring outcome. The second is clutter, and it lands at the top of Table 4's urban range rather than the middle: sites with metal-clad buildings inside two hundred meters are at the fifteen-degree end, which at two kilometers is the difference between a street and a district. Both are geometry problems, and both cost less to fix before the mast goes up than after.

7Where radio detection is blind

Radio detection has blind spots, and a specification that states them is the one a buyer can plan against. Table 5 sets the modalities against the threat modes.

Table 5. Radio sensing is necessary and not sufficient. It is the only modality that offers protocol-level identification and a path to the operator, and it has a complete blind spot against three operationally significant threat modes.
Threat modeRFRadarAcousticElectro-optical
Standard aircraft, link upbest: warning, identity, operatorgoodweakconfirmation
Fiber-tethered aircraftblindbestfairconfirmation
Pre-programmed, link offblindbestfairconfirmation
Cellular-linked aircraftblindbestfairconfirmation
Locating the operatoronly sensor that cannonono
Payload and intentnononoonly sensor that can

Fiber-tethered aircraft deserve their own sentence. Spools of ten to twenty kilometers are now fielded, and the control and video links run on glass. There is no emission to detect, at any sensitivity, at any bandwidth. A radio sensor is one layer of a system that pairs radio for cue and operator geolocation with radar for track and electro-optics for identification.

Cutting the false-alarm rate with an existing decoder

A false alarm on a cooperative aircraft costs operator attention. Cooperative aircraft announce themselves continuously on 1090 MHz, and the same receiver that watches the control bands can decode that broadcast to an aircraft address, callsign, altitude and position. A track correlating with a decoded 1090ES report is cooperative traffic and can be suppressed before an operator sees it; a track with no such report stays a candidate. Watching 1090 MHz costs tuner time, and a second channel if it has to run while the control bands are being watched. No other hardware is needed: with the -SDR option, the ICX-FieldHawk presents itself through SoapySDR, the vendor-neutral hardware abstraction layer, the ADS-B 1090ES chain is one of the six documented in the SDR Integration Handbook, and an existing GNU Radio decoder runs against the instrument with its calibration already applied to the samples, while SpectraCore and every standard measurement function stay installed. Figure 8 draws where the decoder attaches.

What the integrator writesWhat it costsCounter-UAS applicationtracks, alarms, operator displayThe integrator's. Nothing below itchanges when this changes.Existing 1090ES decoderan open flowgraph, written for other hardwareNot written for this instrument, andnot modified for it.SoapySDR abstraction layerdevice discovery, tuning, IQ streamingThe boundary. Everything above isportable.Driver and calibration filesinstalled togetherThe correction arrives with thedriver, so the layers above receive ameasurement.Receiver hardwareone tuner, shared with the control bandsThe cost is tuner time, not anotherbox.
SchematicFigure 8. Why the suppression argument needs no second instrument. The decoder is an existing open flowgraph that was never written for this instrument, and it attaches at a standard boundary with the amplitude correction already applied beneath it. What a bearing solution consumes from the layer below is not a spectrum but a timestamped, corrected sample stream, which is what section 4 required of a bearing and what a scanning front end cannot deliver.

Figure 8 draws the attachment point. The fourth layer is what distinguishes this from a development board: the calibration files install with the driver, so the flowgraph above is handed a measurement rather than samples.

8Summary, definitions and further reading

Table 6 collects the governing relations and published values with their conditions.

Table 6. Governing relations and published values with their conditions.
QuantityRelation or valueCondition
Single-burst intercept(d + τ − 2tmin) / Tunsynchronized timing
Bursts to 90 percentln(0.1) / ln(1 − P1)independent looks
Scanner sensitivity penalty10 log10(dwell / revisit)integrating detection over the revisit; 20 dB for 1 ms in 100.8 ms
Free-space path loss32.44 + 20 log fMHz + 20 log dkm
Interferometer ambiguityunambiguous if D ≤ λ/2full hemisphere
Timing to distance1 ns = 0.30 mc = 299,792,458 m/s
Cross-range errorrange × bearing error3 degrees at 2 km is 105 m
Fix errorCEP = 0.5887 (a + b)124 m at a right angle, 247 m at 25 degrees
Gap-free bandwidth100 MHz9.5, 20 and 40 GHz models in every enclosure; 50 MHz standard and 100 MHz with option 50 on the 4.5, 6 and 9 GHz handhelds
Published POI0.512 µs at N = 32full amplitude accuracy, D = 1
GNSS 1PPS synchronization±100 ns standard±75 or ±50 ns with the high-precision GNSS options
Instrument values are from the ICX-FieldHawk handheld, ICX-FieldHawk-R and ICX-Series USB/LAN datasheets. Link parameters are representative rather than exact and should be confirmed per target.
Circular error probable
The radius of the circle, centered on the estimate, containing the true position half the time.
Probability of intercept
The minimum duration a signal must be present for the analyzer to measure its amplitude correctly. A stronger claim than the duration required merely to detect it.
Remote ID
A mandated broadcast identifying an unmanned aircraft, its position and its control station, sent in the clear.
Symbols used in this document.
SymbolMeaningUnits
P1Single-burst intercept probabilitydimensionless
d, trDwell, retune times
TRevisit periods
τBurst durations
D, λBaseline, wavelengthm
σθ, σφBearing error, phase errorrad
a, bSemi-axes of the fix error ellipsem
ADS-B  automatic dependent surveillance, broadcast
CEP  circular error probable
CFAR  constant false alarm rate
DF  direction finding
OFDM  orthogonal frequency-division multiplexing
POI  probability of intercept
SDR  software-defined radio
SNR  signal-to-noise ratio
TDOA  time difference of arrival
UAS  unmanned aircraft system

Further reading

If you are specifying a sensing layer and want the intercept and link-budget arithmetic run against your own site geometry, our application engineers would be glad to help.