GNSS Sky Plots

Live C/N0

Anomaly vs 1 hour

Anomaly vs 1 day

Anomaly vs 1 week

Cumulative anomalies

Centre = zenith, edge = horizon. With 1°×1° cells the 1-hour view is usually sparse (a cell is rarely revisited within an hour); the 1-day and 1-week views are the meaningful ones. Gray = no baseline yet for that direction.

Cumulative anomalies aggregates every stored observation: for each direction it counts how many readings fell at least the threshold (default 6 dB) below that direction's own median, then groups the counts into coarser cells. Deep red = a direction where the signal repeatedly drops — a persistent obstruction, multipath, or antenna issue. Gray = seen, but never anomalous. Unlike the live views above, this accumulates over all retained history, so a real problem direction stands out even though any single pass looks fine.

Direction finding — biggest anomalies on a map

Bearings of the strongest anomalies in the selected window, drawn from the antenna () outward along each satellite's azimuth at the moment of the drop — the compass direction the obstruction or reflector most likely lies in. Use the controls to pick the time window and how many rays to show. Thicker / redder = larger drop; ray length is fixed (direction only, not distance). Click a ray for details; zoom and pan freely. Map data © OpenStreetMap contributors.

Anomaly lists — strongest first

Each table lists the individual anomalous readings in that period, ordered by how far below the direction's own median they fell — from the threshold (default 6 dB) up to the worst. Δ dB = size of the drop; Sat and C/N0 are added for context. Tables scroll; only the strongest per period are listed.

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