Propagation prediction tools
Forecasts and real-time maps.
Forecasts and real-time maps.
Propagation tools help you decide which band to try and when, instead of tuning around hoping. They fall into three families, which answer different questions. This article describes the categories, not any one product: features and availability change, so check each tool's own documentation.
| Kind | Answers | Typical examples |
|---|---|---|
| Space weather data | How active is the sun, and how disturbed is Earth's magnetic field? | solar flux, A and K indices, X-ray and solar wind readings, published by space-weather agencies |
| Prediction models | Between these two places at this time, which frequencies should work? | HF prediction programs (many built on the VOACAP engine), usually run on your computer or on a website |
| Live reports | What is actually being heard right now? | maps built from spotting networks, beacons and WSPR |
For VHF and UHF, the idea is the same, but the inputs are weather rather than the sun: forecasts that show where tropospheric ducting is likely, and Sporadic E or Aurora propagation alerts. See Tropospheric ducting and scatter.
Space weather data are inputs, not answers. In general, a higher solar flux means stronger ionisation and better support for the higher HF bands, while a high K or A index means a disturbed field and degraded paths, especially near the poles. The solar cycle and propagation indices explains each one, and Space weather explains what drives them.
A prediction model takes a path, a date and time, transmit power, antennas and a smoothed sunspot figure, and returns an estimate of the MUF (see MUF, LUF and the best frequency) and the likelihood a signal will get through. Predictions are statistical: they describe a typical day in that month, not today.
When a forecast and a live report disagree, believe the live report: it is the measurement, while the forecast is an average.