Why the emission that matters most is the one that is hardest to hear.
Radio detection of small unmanned aircraft is usually described as a sensitivity problem. It is not. It is a probability-of-intercept problem, and the arithmetic is unforgiving: 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. This paper derives that result, works the link budget for both ends of the link, sets out what each direction-finding method can actually deliver, and states plainly where radio detection is blind.
Counter-UAS system integrators designing or specifying an RF sensing layer. Security and site-protection engineers evaluating what an RF sensor can and cannot promise. Spectrum enforcement staff working unauthorized flight cases.
Almost every small unmanned aircraft in service 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 live in the same bands, they belong to the same system, and for the purpose of finding the person flying, they could hardly be less alike.
The instinct at this point is to reach for a cheap scanning detector, the kind sold as a drone-band monitor, and see what it finds. It will find something, which is the problem. 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. Buying a second and a third does not fix it either: three receivers each blind ninety-nine percent of the time are still blind, and now the false alarms triple. The constraint is not sensitivity or channel count. It is coincidence, and coincidence is arithmetic.
Figure 1 is the whole difficulty in one picture. The aircraft sits in clear air with a quasi-omnidirectional antenna, transmitting tens of megahertz at high duty cycle. The controller sits 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 you, 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. It is also, by construction, only present on aircraft whose operators intended to comply.
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 actually meets.
| Link class | Band | Channels | RF on per hop | Hop rate |
|---|---|---|---|---|
| Consumer RC, 16-channel | 2.4 GHz | 47 | about 3 ms | about 111 /s |
| Long-range RC, 500 Hz mode | 2.4 GHz | about 80 | about 0.25 ms | 500 /s |
| Long-range RC, sub-GHz | 868 / 915 MHz | about 50 | about 1.5 ms | 150 /s |
| Proprietary video link identifier | 2.4 / 5.8 GHz | wide OFDM | 645 us burst | about 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:
Detection over many bursts follows a geometric law, so the 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.
| Receiver | Instantaneous BW | Revisit | P per burst | Time to 90 percent |
|---|---|---|---|---|
| Narrow scanner | 1 MHz | 100.8 ms | 0.015 | 89 seconds |
| Mid scanner | 20 MHz | 6.0 ms | 0.26 | 4.6 seconds |
| Gap-free capture | at least 100 MHz | continuous | 1.00 | 0.6 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. That is the difference between a warning and a report written afterward.
There is a second, quieter penalty. A scanner observes any given channel for only the fraction of wall-clock time given by dwell over revisit, so it forfeits ten times the logarithm of that ratio in sensitivity. For the narrow scanner in Table 2 that is 20 dB, which at a free-space path-loss exponent is a factor of ten in range. The scanning receiver is not merely slower. It is also deaf by twenty decibels while it is being slow.
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.
Sections 1 and 2 are a criterion, not yet a specification. Table 3 states it as four requirements a reader can score any receiver against, and the reason they are stated here rather than at the end is that a reader who stops at this table should still be able to buy correctly.
| # | Requirement | Derived value | Published |
|---|---|---|---|
| R1 | Instantaneous bandwidth covering the whole hop band at once | ≥ 83.5 MHz for the 2.4 GHz band, from §2 | 100 MHz; 50 MHz standard on the 9.5 GHz module |
| R2 | Probability of intercept published as a guarantee with its transform size | ≤ 645 µs to catch an identification burst whole | 0.512 µs at N = 32; 32.768 µs at N = 2048 |
| R3 | Coherent channels on one time base for a bearing | ≥ 2 for an interferometer, ≥ 4 for an array | Not published as a matched multi-channel figure (verify) |
| R4 | Time tagging fine enough that the instrument is not the limit | ≤ 10 ns, since 1 ns is 30 cm | 8 ns power detection resolution |
Figure 3 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.
Free-space path loss sets the floor for both directions:
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.
That fourteen-to-one range ratio reverses more often than counter-UAS marketing admits. 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 sits in its own antenna null. Detection range is a distribution, not a number.
Figure 4 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.
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.
| Method | Achievable accuracy | What it needs | Where it fails |
|---|---|---|---|
| Received signal strength | range to plus or minus 30 to 60 percent | amplitude only | unknown emitter power is indistinguishable from range |
| Amplitude comparison, 4 to 8 sectors | 5 to 15 degrees | one burst, amplitude only | multipath ripple |
| Pseudo-Doppler | 2 to 10 degrees | a continuous carrier for several milliseconds | short bursts and fast hopping, structurally |
| Multi-baseline interferometry | 1 to 3 degrees clear, 5 to 15 urban | coherent, gap-free, multi-channel capture | coherent multipath |
| Time difference of arrival | 10 to 50 m inside the array | the same burst at three or more synchronized sites | emitter 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:
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 serious direction finding uses 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 simply 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 degradation in the sensors at all. Geometry does that, not equipment.
Time-difference methods trade the bearing problem for a timing problem, and the conversion is brutal in its simplicity: 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 no field system has ever achieved it. Real accuracy is set by inter-site clock synchronization, which for a satellite-disciplined oscillator is 10 to 50 nanoseconds, and by multipath leading-edge bias in urban settings, which is a bias rather than noise and therefore does not average away.
Figure 5 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.
Radio detection of unmanned aircraft is lawful. Demodulating the communications those aircraft carry generally is not, and the distinction is sharper than most system specifications acknowledge.
In United States law the Wiretap Act turns on contents, meaning information concerning the substance, purport or meaning of a communication. 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, 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.
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. Parsing it is not interception in any meaningful sense. 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.
Two things show up in deployment that the arithmetic above does not predict. The first is siting. Sensors placed for the aircraft sit 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 installations that detect well and geolocate badly are the common failure rather than the rare one. 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 sit at the fifteen-degree end, which at two kilometers is the difference between a street and a district. Both are geometry problems, and both are cheaper to fix before the mast goes up than after.
This is the section most counter-UAS material omits, and omitting it is why buyers lose confidence in the category.
Table 5 sets the modalities against the threat modes.
| Threat mode | RF | Radar | Acoustic | Electro-optical |
|---|---|---|---|---|
| Standard aircraft, link up | best: warning, identity, operator | good | weak | confirmation |
| Fibre-tethered aircraft | blind | best | fair | confirmation |
| Pre-programmed, link off | blind | best | fair | confirmation |
| Cellular-linked aircraft | blind | best | fair | confirmation |
| Locating the operator | only sensor that can | no | no | no |
| Payload and intent | no | no | no | only sensor that can |
Fibre-tethered aircraft deserve their own sentence. Spools of ten to twenty kilometers are now fielded at scale, and the control and video links run on glass. There is no emission to detect, at any sensitivity, at any bandwidth. Any radio sensor sold as a complete answer is being oversold, and a serious system pairs radio for cue and operator geolocation with radar for track and electro-optics for identification.
The failure mode that erodes operator trust fastest is not a missed drone, it is an alarm on a helicopter. 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, because the ICX-FieldHawk presents itself through SoapySDR, the vendor-neutral hardware abstraction layer, so an existing GNU Radio decoder runs against it with the instrument calibration already applied to the samples. The capability is demonstrated rather than specified; see the verification note.
Figure 6 draws the attachment point. The layer worth staring at is the fourth: the calibration files install with the driver, so the flowgraph above is handed a measurement rather than samples, and that is the whole difference between this and a development board.
Table 6 collects the governing relations and published values with their conditions.
| Quantity | Relation or value | Condition |
|---|---|---|
| Single-burst intercept | (d + τ − 2tmin) / T | unsynchronized timing |
| Bursts to 90 percent | ln(0.1) / ln(1 − P1) | independent looks |
| Free-space path loss | 32.44 + 20 log fMHz + 20 log dkm | |
| Interferometer ambiguity | unambiguous if D ≤ λ/2 | full hemisphere |
| Timing to distance | 1 ns = 0.30 m | c = 299,792,458 m/s |
| Cross-range error | range × bearing error | 3 degrees at 2 km is 105 m |
| Gap-free bandwidth | 100 MHz | 50 MHz standard on the 9.5 GHz module |
| Published POI | 0.512 us at N = 32 | full amplitude accuracy |
| Instrument values are from the ICX-FieldHawk datasheets. Link parameters are representative rather than exact and should be confirmed per target. | ||
| Symbol | Meaning | Units |
|---|---|---|
| P1 | Single-burst intercept probability | dimensionless |
| d, tr | Dwell, retune time | s |
| T | Revisit period | s |
| τ | Burst duration | s |
| D, λ | Baseline, wavelength | m |
| σθ, σφ | Bearing error, phase error | rad |
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.
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.