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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 21:00 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 11,441 512 1.3M +90 dB Strong
12m 6,906 142 388,429 +87 dB Strong
15m 25,120 1,702 6.0M +87 dB Strong
17m 42,770 2,840 4.7M +87 dB Strong
20m 243,605 17,587 12.6M +74 dB Strong
30m 112,952 3,818 2.1M +63 dB Strong
40m 259,194 8,511 3.7M +87 dB Strong
80m 53,067 1,308 363,468 +52 dB Strong
160m 11,956 515 30,528 +51 dB Open

Data Pipeline

Source Latest Date Total Rows Status
WSPR 2026-05-22 11.48B Current
RBN 2026-05-22 2.31B Current
PSK Reporter 2026-05-23 3.46B Live
Contest Archive 234.3M Static
Solar 2026-05-23 77,604 Live

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 (11.48B spots, 2008–present) — the SNR floor at minimum power
  • Reverse Beacon Network (2.31B spots, 2009–present) — CW/RTTY measured signals
  • PSK Reporter (3.46B 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.