How Satellite Coverage Works
A satellite's coverage footprint is the area on the ground from which it can be seen above a minimum elevation angle. For a typical LEO satellite at 400 km altitude, the footprint is a circle roughly 5,000 km in diameter (at 0° minimum elevation). At a more practical 10° minimum elevation — where signals are strong enough for reliable communication — the footprint shrinks to about 3,600 km diameter.
Why Grid Squares Matter
The Maidenhead grid square system divides the Earth into a hierarchy of rectangles. A 4-character grid (e.g. IO91) covers roughly 100 × 200 km. A 6-character subsquare (e.g. IO91wm) covers about 5 × 10 km. For satellite work, 4-character grids are the standard exchange — they give enough precision to confirm that two stations shared the same pass while being short enough to transmit quickly during a brief satellite window.
Using the Heatmap
Select a satellite and pass from the controls above, then click "Compute Coverage". The heatmap shows every grid square that can see the satellite during the pass, colour-coded by maximum elevation — brighter colours indicate stronger potential signals. Use this to find operators in other grids who could hear the same pass and coordinate contacts in advance.
Contest & DX Planning
For satellite contests (AMSAT Field Day, ARRL VHF+), the heatmap is invaluable for planning. Identify which passes cover rare grid squares, find time windows where multiple high-value grids overlap with your own footprint, and prioritise passes that give you access to grids you haven't worked yet. The grid search tool below the map tells you instantly whether a specific grid is workable on a given pass.
For pass predictions with Doppler-corrected frequencies, visit the ham radio pass predictor. Listen to recordings from other operators in the audio archive. Learn more about orbital mechanics in the Orbital Academy.