Drop your station on the map and see where a shortwave signal comes back down — the near-in reach, the dead skip zone, and the hop rings out to DX. It predicts the ionospheric bounce with the ITU-R P.533 method (the physics behind VOACAP), then folds in your actual antenna — its height, type and orientation — so the map is yours, not a best-case guess. Runs on your device; works offline.
Where your shortwave signal comes back down
This maps where an HF (shortwave) signal launched from your station returns to earth — the near-in reach, the dead skip zone, and the hop rings out to DX. It runs entirely on your device, so it works with the internet down.
The shading is the predicted signal-to-noise at each spot — brighter is stronger:
Because your antenna’s elevation gain is in the calculation, coverage responds to it: a low dipole is strong close-in (NVIS) but weak for DX, while a vertical is weaker close-in and reaches farther. Raise or lower the antenna and the reach changes.
Ionospheric MUF from the ITU-R P.533 F2-layer method over the CCIR monthly maps (the physics behind VOACAP), then a P.533-style link budget for each spot: free-space spreading + D-region absorption + ground-reflection loss, minus your antenna’s elevation gain, against an HF noise floor — giving a signal-to-noise the map colors by. The MUF and skip geometry are rigorous; the field-strength and noise terms are faithful approximations (the full P.533 uses absorption and noise tables we don’t bundle offline), so treat the exact SNR edges as relative, not absolute.