Geography is the constraint
An optical downlink needs clear sky at a specific place at a specific minute, which makes the map the most load-bearing view of this registry. Five lenses draw onto the same geography: where the stations are, which longitudes have nobody, how much of the geostationary arc is in reach, how many genuinely independent sites the station count represents, and which of those sites have a second site that could take the same pass under different sky.
Longitude coverage
A direct-to-Earth station only sees a satellite when the pass crosses its sky, so a constellation's contact rate depends on how evenly stations are spread in longitude — not on how many exist. The longitude lens stripes the map into 24 one-hour bands and counts operational stations in each.
Most empty bands are open ocean, where the absence is physics rather than a market gap.
A 15° bin is narrower than the longitude a single station actually works: at mid-latitudes a low-Earth pass stays usable across roughly ±20–25°, so an empty band flanked by occupied ones is generally covered by its neighbours and only a run of consecutive empty bands is a real hole. The bins also say nothing about latitude — two stations one band apart but 60° apart north to south see quite different passes. Read the bands as a distribution, not as a coverage model.
Stations per 15° band
| Band | Operational | Land | Where |
|---|
The GEO arc is already covered
GEO feeder links are the opposite story. A GEO satellite sits at a fixed longitude, so a station's usefulness is fixed too: it can reach the slots where the satellite stays above a workable elevation. The GEO lens draws each operational GEO-capable station's reach as a fan down to the arc, taking 20° elevation as the floor — where fans overlap, more than one station can work the same slot.
Reach per station
| Station | Site longitude | Reach ± | Slots in view above 20° |
|---|
Fewer independent sites than stations
Cloud cover is correlated over a few hundred kilometres, so two stations at the same site are one weather bet, not two. The sites lens collapses operational stations within 100 km of each other into a single marker, numbered by how many stations it holds.
Backup exists on the map, not on paper
A station has a weather backup only if a second site can take the same pass under different sky. That means a partner roughly 500 to 2,000 km away: far enough that one frontal system rarely covers both, close enough that a single LEO pass crosses both horizons. The weather lens draws every operational pair that qualifies, and marks the few an operator has actually documented.
Both distances are stated assumptions, not measurements: 500 km is a mid-range figure for how far cloud cover stays correlated, 2,000 km approximates where a low-Earth pass stops being mutually visible. Neither is isotropic, and the lens treats them as if they were. Cloud decorrelates over tens of kilometres in convective tropical air and over well beyond a thousand in a North Atlantic frontal system, so a single 500 km threshold is generous at low latitudes and tight in the storm tracks. Separation is also measured as plain great-circle distance, which ignores how a pair is oriented: a near-polar ground track runs north–south, so two sites on that axis share a pass quite differently from two the same distance apart east–west. See how weather is handled. A documented pair is drawn whatever its separation, because an operator's stated arrangement outranks our geometry. And an undocumented pair is possibility only: nothing here says those two operators have agreed, scheduled or ever tested a handover.
Hemispheres
Coordinate precision varies and is recorded per station. Markers are drawn at the best published position; a marker is never more precise than the location.precision field on the record, and none should be read as a survey coordinate. Where an operator runs several telescopes at one site, the registry holds one record per station as published — which is why the site count is lower than the station count.
Coverage figures are computed from the plotted coordinates at page load. Elevation geometry assumes a spherical Earth and a nominal geostationary radius of 42,164 km, ignores terrain masking, and takes no account of cloud statistics, licensing or actual scheduling access — it is an upper bound on where a link is geometrically possible, not a claim that one has been made. Fans are drawn as straight lines in the map projection, so their edges are schematic; the longitude figures behind them are computed spherically. Demonstrated links are recorded per station in the tracker.