Coverage Prediction
How a Coverage Prediction Is Built
A coverage prediction starts with the physical environment. A digital elevation model (DEM) supplies terrain heights, and a land-use raster classifies each pixel as water, open land, suburban, dense urban, or forest so the engine can apply morphology-dependent clutter loss. For macrocell studies, 30 m terrain and 5 to 20 m clutter resolution are common; microcell and millimeter-wave work demands 1 to 5 m 3D building vectors. The transmitter is defined by its location, antenna height above ground, EIRP, and the antenna's horizontal and vertical patterns with electrical and mechanical downtilt. The engine then walks radials or pixels outward, summing free-space loss, terrain diffraction, and clutter attenuation to produce a path-loss surface.
The second half of the workflow is the link budget. Received signal level equals EIRP minus path loss plus receive antenna gain minus feeder and connector losses. Wherever the predicted median received power exceeds the receiver sensitivity (or the threshold set by the required signal-to-interference-plus-noise ratio), the location is counted as covered. Because shadow fading scatters real measurements around the median by a log-normal distribution, planners do not design to the median alone; they add a fade margin sized to the desired area or cell-edge reliability, so the served region is the area where signal exceeds threshold with the target probability.
Modern tools blend methods. Empirical models such as Okumura-Hata and COST 231-Hata are fast and adequate for wide-area screening, while deterministic ray-tracing resolves individual reflection, diffraction, and waveguiding paths through street canyons at the cost of compute time and data quality. Calibrating any model against drive-test measurements for the local morphology is the single most effective way to cut prediction error.
Governing Equations
RSL (dBm) = EIRP − Lpath + Grx − Lfeeder
Coverage Condition (per pixel):
RSL ≥ Srx + Mfade → covered
Path Loss (Okumura-Hata, urban):
Lpath ≈ 69.55 + 26.16 log f − 13.82 log hb − a(hm) + (44.9 − 6.55 log hb) log d
Fade Margin (log-normal shadowing):
Mfade = Q−1(1 − Pedge) × σSF
Where f = frequency in MHz, hb = base height (m), hm = mobile height (m), d = distance (km), Srx = receiver sensitivity, σSF = shadow-fade standard deviation (≈ 6 to 10 dB). Example: σSF = 8 dB, 90% cell-edge → Mfade ≈ 10 dB.
Propagation Model Comparison
| Model / Method | Frequency Range | Best Environment | Typical Std. Error | Compute Cost |
|---|---|---|---|---|
| Okumura-Hata | 150 to 1500 MHz | Urban / suburban macrocell | 8 to 12 dB | Very low |
| COST 231-Hata | 1500 to 2000 MHz | Urban macrocell | 8 to 12 dB | Very low |
| Longley-Rice (ITM) | 20 MHz to 20 GHz | Irregular terrain, P2P | 7 to 10 dB | Low |
| ITU-R P.1546 | 30 MHz to 4 GHz | Broadcast, coordination | 7 to 10 dB | Low |
| Erceg (SUI) | ~1.9 GHz | Fixed wireless access | 7 to 9 dB | Low |
| Ray-tracing (3D) | 0.3 to 100 GHz | Dense urban / mmWave | 4 to 6 dB | High |
Frequently Asked Questions
Which propagation model should I choose for coverage prediction?
Choice depends on frequency, environment, and cell radius. Okumura-Hata (150 to 1500 MHz) and COST 231-Hata (to 2000 MHz) suit urban and suburban macrocells; Longley-Rice handles irregular terrain from 20 MHz to 20 GHz; deterministic ray-tracing over 3D building data is required for dense urban microcells and millimeter-wave 5G. Calibrating any model with drive-test data cuts the standard error from 8 to 12 dB down to 6 to 8 dB.
How accurate is RF coverage prediction compared to drive-test measurements?
Untuned empirical models such as Okumura-Hata show an 8 to 12 dB location-variability standard deviation versus measured received signal level. Calibrating against drive-test data for the local clutter usually drops the residual error to 6 to 8 dB, and ray-tracing in surveyed urban areas can reach 4 to 6 dB. Because shadow fading is log-normal, planners add a fade margin of 8 to 10 dB for 90% area reliability on top of the median.
What input data does a coverage prediction need?
It needs a digital elevation model for terrain, a land-use or clutter layer for morphology-dependent loss, transmitter location and antenna height, the antenna horizontal and vertical patterns with tilt, EIRP after feeder losses, the operating frequency, and the receiver sensitivity or required threshold. Macrocells commonly use 30 m DEM and 5 to 20 m clutter; microcell and millimeter-wave studies need 1 to 5 m 3D building vectors.