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Ham Stats

HF propagation predictions trained on 14 billion real observations — not theory, not opinions.

Ham Stats provides live HF propagation intelligence for amateur radio operators. Everything on this site is derived from measured radio observations — WSPR beacons, Reverse Beacon Network skimmers, PSK Reporter reception reports, and contest QSOs — combined with real-time solar conditions from NOAA.

  • Predictions — Which bands and modes can reach your target right now
  • Band Activity — What's actually being heard across the HF spectrum
  • Solar Conditions — Current SFI, Kp, and their impact on propagation
  • Historical Data — Band-by-band trends, contest schedules, and DXpedition tracking

The predictions are powered by IONIS — a physics-constrained neural network trained on one of the largest curated amateur radio propagation datasets we are aware of. For technical details on the model and methodology, see ionis-ai.com.

SFI Kp Conditions

Updated 03:00 UTC · NOAA SWPC


Band Activity (Last 24 Hours)

Which bands had propagation in the last 24 hours, based on spots from all sources. RBN archives lag ~24 hours; zeroes indicate no data in the window, not band closure.

Band WSPR Spots RBN Spots PSKR Spots Peak SNR Status
10m 0 0 3.0M +62 dB Strong
12m 0 0 1.1M +54 dB Strong
15m 0 0 6.1M +69 dB Strong
17m 0 0 3.5M +57 dB Strong
20m 0 0 10.2M +87 dB Strong
30m 0 0 2.5M +56 dB Strong
40m 0 0 5.9M +87 dB Strong
80m 0 0 1.2M +55 dB Strong
160m 0 0 133,972 +50 dB Strong

Data Pipeline

Source Latest Date Total Rows Status
WSPR 2026-04-05 11.21B 2 days behind
RBN 2026-04-05 2.28B 2 days behind
PSK Reporter 2026-04-07 1.89B Live
Contest Archive 234.3M Static
Solar 2026-04-05 76,968 2 days behind

About This Site

Ham Stats is generated every 3 hours from a self-hosted ClickHouse database containing 14+ billion amateur radio propagation observations — one of the largest curated datasets of its kind. No cloud services. No third-party APIs. Every query runs against data we collected and maintain.

The data comes from four independent networks, each measuring a different layer of HF propagation:

  • WSPR (11.21B spots, 2008–present) — the SNR floor at minimum power
  • Reverse Beacon Network (2.28B spots, 2009–present) — CW/RTTY measured signals
  • PSK Reporter (1.89B spots, live since Feb 2026) — FT8/digital operational contacts
  • Contest Logs (234.3M QSOs, 2005–present) — the SSB/RTTY ceiling at contest power

Solar indices (SFI, Kp, SSN) are joined at 3-hour resolution so every propagation measurement has its solar context.

This site is a product of the IONIS Project — the Ionospheric Neural Inference System.

The logs were speaking for decades, but nobody was listening. Now we're listening — and we're publishing what we hear.