Near-vertical incidence skywave
Steep-angle HF for reliable regional contacts.
Steep-angle HF for reliable regional contacts.
Near-vertical incidence skywave (NVIS) sends an HF signal almost straight up so the ionosphere returns it steeply, landing within a few hundred miles. It fills the gap that ordinary low-angle skip leaves around the transmitter, and gives reliable regional coverage with no dependence on line of sight, which is why it is a staple of emergency and disaster communications.
Normal HF contacts use low takeoff angles, so the signal lands far away and leaves a skip zone around you: too far for the ground wave, too close for the sky wave. Aim the signal steeply and the same layer returns it close by instead. The ground wave covers the first few miles, NVIS the rest of the region, and the two overlap.
Sending a signal straight up has a hard rule: it returns only if its frequency is below the layer's critical frequency, which is typically a few MHz to around 10 MHz depending on the time and the solar cycle. Higher, and it passes through into space. Lower, and the D layer absorbs it in daytime. That leaves a narrow window, so the right band changes through the day.
| Time | Typical NVIS band |
|---|---|
| Daytime | 40 m; 60 m or 80 m when the critical frequency is low |
| Evening and night | 80 m, sometimes 160 m |
These are rough guides: check which band the signals from your area actually favour. The MUF and LUF window for a near-vertical path is simply narrow and low.
A horizontal dipole close to the ground radiates mostly straight up, because the ground reflection cancels the low-angle radiation and reinforces the overhead lobe. A tenth to a quarter wavelength high works well; higher, and more energy goes out at low angles, the opposite of what you want. A vertical has a null straight up, so it is a poor NVIS choice, while a low inverted-V or dipole is a good one.