The trig pillar network Data study · 2026
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Data study2026

The trig pillar network: how Britain was measured

Every station in the Ordnance Survey's list for Great Britain, 24,433 in all, coloured by order. Lines join each primary station, and each secondary and third-order pillar, to its nearest neighbour of the same order: blue where the terrain model says they can see each other, red where it says they cannot. Drag the timeline; tap a dot or a line.

    Station order
    primary (1)
    secondary (2)
    third order (3)
    fourth order and later
    recorded destroyed (hollow)
    in sight over the terrain model
    blocked in the model
    Pillars shown; spires, bolts and other marks in Layers
    Great Britain only (the OS list has no Northern Ireland)
    1936 to 1995

    On hilltops all over Britain stand squat concrete pillars about four feet (1.2 m) high, each with a brass mounting on top. They were the Ordnance Survey's survey stations for the Retriangulation of Great Britain, whose first pillar went up in 1936 and which gave Britain its National Grid. The OS list of its old triangulation stations holds 24,433 stations in Great Britain, 6,573 of them pillars. I mapped every one and asked four questions: how the network was laid out, when it was built, how much has been lost, and whether a modern open terrain model can still see the rule the surveyors worked to, that a station must be in sight of its neighbours.

    Dr Tristan Hotham · Independent researcher · 2026 · Data: Ordnance Survey legacy triangulation station list (Contains OS data © Crown copyright and database right 2018, Open Government Licence v3.0, via the trigpoints R package), Terrain Tiles (AWS Open Data; Mapzen), OpenStreetMap contributors (ODbL) · Base map: OpenFreeMap Positron
    95%of nearest-neighbour primary lines clear over the terrain model (228 of 240)
    11%of random pairs of points on land at the same distances
    99%of pillars dated 1936 to 1962
    415of 6,573 pillars recorded destroyed (6.3%)

    01 · The meshA net inside a net

    The network was built in orders. 347 primary stations carry the big triangles; secondary and third-order stations fill them in, and fourth-order marks (often bolts on buildings, church spires and flagstaffs) fill in the towns. The median distance from a primary station to its nearest primary neighbour is 19.6 km (95% interval 18.5 to 20.6). For secondary pillars it is 7.1 km, and for third-order pillars 4.3 km.

    The stations are also far more evenly spaced than chance. A Clark and Evans ratio measures this: 1 for random points, higher for more even spacing. The primaries score 1.54, while random points scattered on the same land score 1.02 to 1.17. Joining neighbouring primaries into triangles, 71% of the 582 triangles have every angle at least 30 degrees, the kind of well-shaped triangle surveyors aim for, against 48% for random points.

    Histograms of the distance to the nearest station of the same order: primary stations about 20 km apart, secondary pillars about 7 km, third-order pillars about 4 km; and dot charts showing each order more evenly spaced than random points

    Nearest same-order neighbour by order, and evenness compared with random points on the same land.

    02 · The buildOne generation of concrete

    The first pillar was used in 1936. Of the 6,573 pillars, 6,510 (99%) carry a commissioning date between 1936 and 1962, the years of the Retriangulation. The busiest year in the list is 1948, with 744 pillars. Work stopped for the war: no station in the list is dated 1940 or 1941. Many primary stations carry the date of their whole block of the network rather than their own, so single years should be read loosely.

    Bar chart of trig pillars by commissioning year from 1936 to 1995: a small pre-war build of primaries, a gap in 1940 and 1941, a peak in the late 1940s and 1950s, and almost nothing after 1962

    Pillars by commissioning year in the OS station list, coloured by order.

    03 · Line of sightDo the hills still see each other?

    Triangulation needs every station to see its neighbours. So I drew a line from each primary station to its nearest primary neighbour and checked it over a modern open terrain model, Terrain Tiles at zoom 9 (pixels about 190 m across), with the Earth's curvature and the usual allowance for light bending in the air. The ends sit at the surveyed height of the station plus 1.5 m for the instrument. I wrote down the test, and what would count against it, before running it.

    Of 240 nearest-neighbour primary lines, 228 (95.0%, 95% interval 91.5 to 97.1%) are clear. Every side of the primary triangle net up to 80 km: 95.6%. Secondary pillars: 97.1%; third-order pillars: 91.9%. For comparison, the same lines with both ends moved 1 km in a random direction are clear only 17% of the time, and random pairs of points on land at the same distances 11% of the time. That fits stations sited for what they could see.

    Dot chart: about 95% of primary, 97% of secondary and 92% of third-order nearest-neighbour lines are clear, against 17% when the ends are moved 1 km and 11% for random land pairs

    Share of lines with a clear line of sight, with 95% intervals.

    The 12 primary lines that fail are telling. 8 involve a cathedral, an observatory, a lighthouse, a water tower or a castle whose height is not recorded in the list, so the test puts the observer on the ground rather than up the tower. 3 are pillar to pillar in flat country in Norfolk, Suffolk and Lincolnshire, blocked by a few metres. Every one of those 3 has an end at a station where the surveyors put up a steel observing tower (often about 30 m tall), and with a 30 m tower added, 3 of 3 clear.

    Three terrain profiles: Fair Isle to Foula clear over the sea; Crimplesham to Walpole St Peters blocked by a few metres but clear from 30 m towers; West Hills to Buddon blocked by rising ground

    Three lines as the test sees them. The terrain is lowered for the curvature of the Earth less refraction.

    The result does not hang on the details: with no refraction allowance, with more, with a finer profile, with the two nearest neighbours instead of one, or leaving out one region at a time, the share stays between 93.2% and 96.6%. With no instrument height at all it is 90%; from a 5 m signal, 98%. One choice matters a lot. The zoom 9 terrain rounds off summits: at pillars it sits a median 22 m below the surveyed height. Using the terrain model's own heights at the ends, only 67% of primary lines are clear, though that is still far above the placebo lines. So the 95% figure rests on the surveyed heights. The last failure, West Hills to Buddon near Dundee, a ground mark with no recorded height behind rising ground, I cannot explain.

    04 · What survivesPillars outlast spires and bolts

    The OS list flags stations known to be destroyed. 6.3% of pillars are flagged, against 26% of spires, towers, masts and other intersected stations, and 36% of ground marks such as bolts and buried blocks. In a model that also allows for order, region, decade and whether the station is in the lowlands, intersected stations had 3.3 times the odds of being flagged destroyed (95% interval 2.8 to 3.8) and ground marks 5.5 times; stations below 100 m had 1.47 times the odds of upland ones. By region, Scotland's pillars are the least often flagged (2.3%).

    Bar chart: 6% of pillars, 26% of intersected stations and 36% of ground marks flagged destroyed; and a dot chart of pillars flagged destroyed by region, lowest in Scotland

    Share flagged destroyed, by kind of station and, for pillars, by region.

    OS no longer maintains the list, so "not destroyed" means only "not known to be destroyed". As a rough check, 29% of the surviving pillars have a survey point mapped in OpenStreetMap within 50 m, against 2.9% of the destroyed ones.

    05 · How I did thisStations, lines and a terrain model

    Stations. The OS legacy list, as packaged in the trigpoints R package, has 31,521 rows. A station can have several rows (a pillar, a bolt beneath it, a refixed mark), so I grouped rows with the same station code within 100 m into 24,433 stations, and called a station a pillar if any of its rows is one.

    Lines of sight. For each line I sampled the terrain every 100 m, lowered it for the curvature of the Earth less refraction (coefficient 0.13), ignored the first and last 250 m, and called the line clear if no sample rose above it. The placebos use the same terrain and the ground height plus 1.5 m at each end.

    What this cannot say. The terrain model has no trees or buildings and rounds off hilltops; the OS list does not record which lines were actually observed, so nearest neighbours stand in for them; and the destroyed flag is out of date. The St Kilda stations lie just outside the terrain tiles, so the one line to St Kilda is treated as open sea, which it mostly is.

    Sources and licences
    Read the paperData and codeBlog post