Read the indicator before choosing a band
Use the solar and propagation indicators as planning inputs rather than guarantees of band openings. Compare the indicators with current on-air reports and your own observations.
Current-source solar/propagation observations, band-condition guidance and links to real-time observation maps.
The image below is fetched live from HamQSL / N0NBH when the network is available. Everything else on this page (band-behaviour tables, interpretation notes) is static reference material that does not update automatically.
Embeds and links from public sources (N0NBH / HamQSL, NOAA). Refresh the page for latest images.
Live image could not be loaded (CORS or offline).
Open HamQSL Solar Page| Band | Day | Night | Notes |
|---|---|---|---|
| 160 / 80 m | Poor–Fair | Good–Excellent | Night DX, high noise by day |
| 40 m | Fair | Excellent | Workhorse regional + DX |
| 30 / 20 m | Good–Excellent | Good | Prime DX bands |
| 17 / 15 m | Excellent (high SFI) | Fair | Solar-cycle dependent |
| 12 / 10 m | Excellent (high SFI) | Poor | Daytime only when open |
| 6 m | Es / F2 openings | Rare | Sporadic-E summer, F2 peak cycle |
These are generalizations. Real openings depend on path, time, power and antennas.
Live digital-mode reception reports worldwide.
CW & RTTY skimmer spots in near real-time.
Weak-signal beacon paths and heatmaps.
Classic path-prediction engine.
MUF / foF2 maps and effective SSN.
Full solar panels, MUF tools and banners.
Propagation is often enhanced along the gray-line (terminator). Check a gray-line map at sunrise/sunset for long-path or unusual openings on the lower bands.
Use the solar and propagation indicators as planning inputs rather than guarantees of band openings. Compare the indicators with current on-air reports and your own observations.
Propagation depends on time, location, path geometry, season, geomagnetic conditions and the ionosphere. A single index cannot describe every path.
Combine forecasts with cluster reports, beacons and recent operating experience before making a band-choice decision.
Propagation indicators are useful because they describe the state of the ionosphere rather than the performance of one particular antenna. Solar flux, sunspot activity and geomagnetic indices can help explain broad HF trends, but none of them directly guarantees a good path between two stations. Frequency selection matters: a band that works well for one path can be poor for another because the ionosphere changes with latitude, local time and solar illumination. Treat indices as context and combine them with current reception reports, beacon observations and your own measurements. A strong signal report can also be misleading if local noise is low at one station but high at the other. When planning a contact, choose a likely band, check the current conditions, test the path and move between bands when the first choice is weak. The calculator and reference material are therefore best used as a decision aid rather than as a promise of propagation.
A useful habit is to record the band, UTC time, signal report and propagation indicators for successful and unsuccessful contacts. Over time those observations become more informative than any single index because they show how your own station behaves under changing conditions.
Use the calculation as a starting point, then move to the tool that answers the next practical question.