Where do the sightlines meet?
Combine timed angular observations from different locations to estimate a moving object’s 3D position and velocity, with residuals and explicit uncertainty limits.
triangulate_tracksTry the real call 01 / UNDERSTAND THE METHOD
ILLUSTRATION · NOT A CALCULATIONMake sight lines tangible.
INPUT SIGHT LINES · NO FIT YETPerspective
Preparing the interactive view…
Drag to orbit · pinch or scroll to zoom · right-drag to pan. Camera rotation does not advance time. The input preview sweeps through each supplied angle sequence independently. It does not align clocks or fit a trajectory. Ray lengths are illustrative; no range is estimated here. Observer markers are enlarged for visibility.
Teaching animation only · no MCP request
KNOW WHAT THE RESULT MEANS
Useful evidence needs boundaries.
- Stationary observers and constant velocity on a 6371.0088 km spherical Earth are explicit assumptions. These are supplied angle measurements, not automatic video or photo analysis.
- Refraction is not modelled; low-elevation samples are flagged. Clock offsets must be supplied, and systematic biases can be partly absorbed by a two-observer fit.
- Reported standard deviations are local, model-based approximations using the declared errors. They do not include unmodelled refraction, sensor bias or clock error and are not independently calibrated accuracy guarantees.
- The reduced chi-square cutoff of 9 is an explicit screening convention. Inconsistent concerns the supplied single-object motion model, never an accusation or a conclusion about origin.